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	<title>cluster - 用户贡献 [zh-cn]</title>
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	<updated>2026-04-29T17:46:24Z</updated>
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		<title>Colloquium</title>
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		<updated>2019-05-10T05:51:42Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* The Lecture Hall, The Third Floor of Astronomy Building */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== &#039;&#039;&#039;SHAO Astrophysics Colloquium&#039;&#039;&#039; ==&lt;br /&gt;
=== Thursdays 3:00 - 4:00 pm ===&lt;br /&gt;
=== The Lecture Hall, The Third Floor of Astronomy Building ===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This is the wiki page for Astrophysics Colloquium at Shanghai Astronomical Observatory. The colloquium language is usually English, unless otherwise stated (often due to some special reasons). If you would like to give a colloquium or invite someone to give a colloquium at SHAO, please contact one of the current members of the colloquium committee: Fulai Guo, Hong Guo, Minfeng Gu, Zhenya Zheng, Ling Zhu.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&#039;&#039;&#039;Spring 2019&#039;&#039;&#039;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Date&lt;br /&gt;
! Speaker &lt;br /&gt;
! Topic&lt;br /&gt;
! Host&lt;br /&gt;
|-&lt;br /&gt;
| March 7&lt;br /&gt;
|  Wenda Zhang (Czech Academy of Sciences)&lt;br /&gt;
|  Self-consistent calculations of Comptonised spectra of extended AGN coronae in Kerr spacetime&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| March 14&lt;br /&gt;
| Zigao Dai (Nanjing Univ)&lt;br /&gt;
| Neutron Star Mergers   &lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| March 21&lt;br /&gt;
| Sowgat Muzahid (Leiden Observatory)&lt;br /&gt;
| MUSEQuBES CGM Surveys: From Low-z Star-forming Galaxies to High-z Lyman-alpha Emitters [[File:Sowgat.pdf]]&lt;br /&gt;
|  Shiyin Shen&lt;br /&gt;
|-&lt;br /&gt;
| March 28&lt;br /&gt;
|  Binbin Zhang (Nanjing)&lt;br /&gt;
|  Data-Oriented GRB Research and the Gravitational Wave GRBs&lt;br /&gt;
|  Minfeng Gu&lt;br /&gt;
|-&lt;br /&gt;
| April 4&lt;br /&gt;
|  Cosimo Bambi (Fudan Univ.)&lt;br /&gt;
|  Testing general relativity using X-ray reflection spectroscopy&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| April 11&lt;br /&gt;
|  Xiao-Jun Bi (IHEP)&lt;br /&gt;
|   Geminga周围介质性质及对宇宙线正电子超出的影响&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| April 18&lt;br /&gt;
|   Cheng Li (Tsinghua)&lt;br /&gt;
|    Mapping the stars, gas and dust in nearby galaxies  &lt;br /&gt;
| Ling Zhu&lt;br /&gt;
|-&lt;br /&gt;
| April 19&lt;br /&gt;
|   Xun Shi (Yunnan Univ) at 10 am&lt;br /&gt;
|   Turbulence and non-thermal pressure in galaxy clusters&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| April 25&lt;br /&gt;
|  Shude Mao (Tsinghua)&lt;br /&gt;
|  What have we learned about extrasolar planets with microlensing? &lt;br /&gt;
|  Ling Zhu&lt;br /&gt;
|-&lt;br /&gt;
| May 2&lt;br /&gt;
| &lt;br /&gt;
| No colloquium:  Labor Day holidays  &lt;br /&gt;
| &lt;br /&gt;
|-&lt;br /&gt;
| May 9&lt;br /&gt;
|   Chris Reynolds and Andy Fabian (Univ of Cambridge)&lt;br /&gt;
|    Special colloquium at 9-11:30 am&lt;br /&gt;
|  Feng Yuan&lt;br /&gt;
|-&lt;br /&gt;
| May 9&lt;br /&gt;
|   Tim Beers (Notre Dame)&lt;br /&gt;
|   The Origin of the Astrophysical r-Process. Slides for his two talks are available here: [[:File:Beers_CEMP_Beijing_2019.pptx| Monday]] and [[:File:Beers_rproc_Shanghai_2019.pptx|Thursday]].&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| May 16&lt;br /&gt;
| Dandan Xu (Tsinghua) &lt;br /&gt;
|   &lt;br /&gt;
|   Ling Zhu&lt;br /&gt;
|-&lt;br /&gt;
| May 23&lt;br /&gt;
|  Bin Hu (Beijing Normal Univ)&lt;br /&gt;
|    Stochastic Gravitational Wave Background&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| May 28&lt;br /&gt;
| Tao Wang (Univ of Tokyo) *Tuesday*&lt;br /&gt;
|   New insights into the formation of the most massive galaxies in the early Universe&lt;br /&gt;
|  Zhenya Zheng&lt;br /&gt;
|-&lt;br /&gt;
| May 30&lt;br /&gt;
| Daniel Wang (University of Massachusetts) &lt;br /&gt;
|  Probing Astrophysics of Galactic Feedback in Nearby Disk Galaxies&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| June 6&lt;br /&gt;
|  Ran Wang (KIAA/PKU)&lt;br /&gt;
|  &lt;br /&gt;
| Minfeng Gu&lt;br /&gt;
|-&lt;br /&gt;
| June 13&lt;br /&gt;
|  Zuhui Fan (Peking Univ /Yunnan Univ)&lt;br /&gt;
|   &lt;br /&gt;
|  Zhenya Zheng&lt;br /&gt;
|-&lt;br /&gt;
| June 20&lt;br /&gt;
| Fukun Liu (PKU)  &lt;br /&gt;
|   &lt;br /&gt;
|Zhenya Zheng   &lt;br /&gt;
|-&lt;br /&gt;
| June 27&lt;br /&gt;
|  Zhiyuan Li (Nanjing)&lt;br /&gt;
|   &lt;br /&gt;
|  Minfeng Gu&lt;br /&gt;
|-&lt;br /&gt;
| July 4&lt;br /&gt;
|  Jie Jiang (Beihang University)&lt;br /&gt;
|   The solar cycle: its variability and prediction&lt;br /&gt;
|   Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| July 11&lt;br /&gt;
|  Hugh  Jones (University of Hertfordshire)&lt;br /&gt;
|   &lt;br /&gt;
|  Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&#039;&#039;&#039;Fall 2018&#039;&#039;&#039;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Date&lt;br /&gt;
! Speaker &lt;br /&gt;
! Topic&lt;br /&gt;
! Host&lt;br /&gt;
|-&lt;br /&gt;
| Sep 25&lt;br /&gt;
| Chi-Kwan Chan (Univ of Arizona)  &lt;br /&gt;
|  special colloquium: Imaging Event Horizons&lt;br /&gt;
|  Fulai Guo &lt;br /&gt;
|-&lt;br /&gt;
| Sep 27&lt;br /&gt;
| Wei Wang (Wuhan Univ)  &lt;br /&gt;
|   Probe of Supernova Progenitors with Gamma-rays&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Oct 4&lt;br /&gt;
| No colloquium (Holidays)&lt;br /&gt;
| &lt;br /&gt;
|  &lt;br /&gt;
|-&lt;br /&gt;
| Oct 11&lt;br /&gt;
|  Jiaxin Han (SJTU)&lt;br /&gt;
|  The small scale distribution of dark matter--from simulations to observations &lt;br /&gt;
|  Hong Guo&lt;br /&gt;
|-&lt;br /&gt;
| Oct 18&lt;br /&gt;
|  Yao Chen (Shandong Univ-Weihai)&lt;br /&gt;
|   Initiation and Energy Release of Solar Coronal Mass Ejections and Relevant Solar Radio Bursts &lt;br /&gt;
| Juntai Shen  &lt;br /&gt;
|-&lt;br /&gt;
| Oct 25&lt;br /&gt;
|   Piero Madau (UCSC)&lt;br /&gt;
|  Connecting the Dark and Light Side of Galaxy Formation&lt;br /&gt;
|   Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 1&lt;br /&gt;
|  John Kormendy (Univ of Texas at Austin)&lt;br /&gt;
|   Special: STRUCTURE AND FORMATION OF S0 AND SPHEROIDAL GALAXIES [[file:Parallel-Shanghai.pdf|pdf]]&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| Nov 1&lt;br /&gt;
|  Yu Dai (NAOC)&lt;br /&gt;
|    Is there a relationship between AGN and star formation in IR-bright AGNs?&lt;br /&gt;
|  Hong Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 8&lt;br /&gt;
|Yi Mao (Tsinghua)   &lt;br /&gt;
|  Reionization science and 21-cm cosmology in the era of SKA&lt;br /&gt;
| Juntai Shen  &lt;br /&gt;
|-&lt;br /&gt;
| Nov 15&lt;br /&gt;
|  Subo Dong (Peking Univ)  &lt;br /&gt;
|  The Full Transient Sky at &amp;lt;17 mag&lt;br /&gt;
|  Zhenya Zheng&lt;br /&gt;
|-&lt;br /&gt;
| Nov 22&lt;br /&gt;
| &lt;br /&gt;
|  No colloquium due to the annual CAS key lab meeting &lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
| Nov 29&lt;br /&gt;
|Yongquan Xue (USTC)       &lt;br /&gt;
|  Probing AGN Physics with Variability Studies&lt;br /&gt;
|  Minfeng Gu   &lt;br /&gt;
|-&lt;br /&gt;
| Dec 6&lt;br /&gt;
|   Jing Wang (Peking Univ)&lt;br /&gt;
|   An HI view of the nearby galaxies&lt;br /&gt;
|   Hong Guo&lt;br /&gt;
|-&lt;br /&gt;
| Dec 13&lt;br /&gt;
| Lulu Fan (Shandong Univ-Weihai)  &lt;br /&gt;
| WISE-selected, luminous dust-obscured quasars and their host galaxies&lt;br /&gt;
| Zhenya Zheng&lt;br /&gt;
|-&lt;br /&gt;
| Dec 20&lt;br /&gt;
|Weimin  Gu (Xiamen Univ)   &lt;br /&gt;
|   Accretion disks and outflows: theories and applications to ULXs and GRBs&lt;br /&gt;
|   Minfeng Gu&lt;br /&gt;
|-&lt;br /&gt;
| Dec 21&lt;br /&gt;
|Dong Lai (Cornell Univ)   &lt;br /&gt;
|   Circumbinary Accretion: From Supermassive Binary Black Holes to Circumbinary Planets&lt;br /&gt;
|   Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Dec 27&lt;br /&gt;
|  Qingwen Wu (HUST)&lt;br /&gt;
|  black holes and jets in the Universe&lt;br /&gt;
|  Minfeng Gu&lt;br /&gt;
|-&lt;br /&gt;
| Jan 3&lt;br /&gt;
| Jianfeng Wu (Xiamen Univ)&lt;br /&gt;
|    X-ray Emission of High-Redshift Jetted Active Galactic Nuclei&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Jan 8&lt;br /&gt;
| Niel Brandt (Penn State)&lt;br /&gt;
|   special colloq 3pm, A Good Hard Look at Cosmic Supermassive Black Hole Growth&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Jan 10&lt;br /&gt;
|   Hongyan Zhou &lt;br /&gt;
|  Hydrogen and Helium Absorption-Lines in Quasars&lt;br /&gt;
|  Zhenya Zheng&lt;br /&gt;
|-&lt;br /&gt;
| Jan 17&lt;br /&gt;
|  Kohei Inayoshi (KIAA)&lt;br /&gt;
|   Black hole accretion in the present-day and early universe&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Jan 21&lt;br /&gt;
|  Xiangcheng Ma (UC Berkeley)&lt;br /&gt;
|   special colloquium&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&#039;&#039;&#039;Spring 2018&#039;&#039;&#039;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Date&lt;br /&gt;
! Speaker &lt;br /&gt;
! Topic&lt;br /&gt;
! Host&lt;br /&gt;
|-&lt;br /&gt;
| March 8&lt;br /&gt;
| Alex Pettitt (Hokudai)&lt;br /&gt;
| What drives the morphological features of disc galaxies?&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| March 15&lt;br /&gt;
|Lei Hao (SHAO)&lt;br /&gt;
|   Galaxy Evolution via 2D Spectroscopy&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| March 22&lt;br /&gt;
| Pengjie Zhang (SJTU)&lt;br /&gt;
| ABS, CMB foreground removal, weak lensing reconstruction by counting galaxies, and beyond&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| March 29&lt;br /&gt;
| Andrzej Zdziarski (Copernicus Astronomical Center) &lt;br /&gt;
|  Jets in black-hole binaries&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| April 5&lt;br /&gt;
| No Colloquium&lt;br /&gt;
| Holiday&lt;br /&gt;
| &lt;br /&gt;
|-&lt;br /&gt;
| April 11&lt;br /&gt;
| Jerry Sellwood (University of Arizona)&lt;br /&gt;
|  The Origin of Spirals in Galaxies / time: 2 pm (Wednesday)&lt;br /&gt;
| Juntai Shen  &lt;br /&gt;
|-&lt;br /&gt;
| April 19&lt;br /&gt;
|  S. Peng Oh (Univ of California, Santa Barbara)&lt;br /&gt;
|  Make it, Shake it, Bake it: Warm Gas in the Circumgalactic Medium&lt;br /&gt;
| Fulai Guo &lt;br /&gt;
|-&lt;br /&gt;
| April 26&lt;br /&gt;
| Xinwen Shu (Anhui Normal University)&lt;br /&gt;
|  Supersoft AGNs: signature of super Eddington accretion, IMBH, TDE or new AGN spectral state?&lt;br /&gt;
| Fulai Guo &lt;br /&gt;
|-&lt;br /&gt;
| May 4&lt;br /&gt;
| Tinggui Wang (USTC)  Friday 3 pm&lt;br /&gt;
|  超大质量黑洞撕裂恒星事件&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| May 10&lt;br /&gt;
|  Zhenya Zheng (SHAO)&lt;br /&gt;
|  Probing Cosmic Reionization with Lyman Alpha Galaxies&lt;br /&gt;
| Fulai Guo &lt;br /&gt;
|-&lt;br /&gt;
| May 17&lt;br /&gt;
| Jian-Min Wang (IHEP)  &lt;br /&gt;
|  Reverberation Mapping of AGNs&lt;br /&gt;
| Fulai Guo &lt;br /&gt;
|-&lt;br /&gt;
| May 24&lt;br /&gt;
|  Ying Zu (SJTU)&lt;br /&gt;
|   Galaxy-Halo Connection for Next Generation Galaxy Surveys&lt;br /&gt;
|  Hong Guo&lt;br /&gt;
|-&lt;br /&gt;
| May 31&lt;br /&gt;
| Tong Liu (Xiamen University)  &lt;br /&gt;
|  伽玛暴中心的黑洞超吸积&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| June 7&lt;br /&gt;
|  Qi Guo (NAOC)&lt;br /&gt;
|  Galaxy formation in the context of concordance cosmology: confront theory with observations &lt;br /&gt;
|Hong Guo  &lt;br /&gt;
|-&lt;br /&gt;
| June 14&lt;br /&gt;
| Guilin Liu (USTC)&lt;br /&gt;
|  Star formation and quasar feedback on galactic scales&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| June 21&lt;br /&gt;
|  Jifeng Liu (NAOC) &lt;br /&gt;
|  司天工程&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| June 28&lt;br /&gt;
| Jingwen Wu (NAOC)&lt;br /&gt;
|  Hot dust-obscured galaxies: Catching the maximum SMBH accretion during galaxy evolution&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&#039;&#039;&#039;Fall 2017&#039;&#039;&#039;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Date&lt;br /&gt;
! Speaker &lt;br /&gt;
! Topic&lt;br /&gt;
! Host&lt;br /&gt;
|-&lt;br /&gt;
| Sep 7&lt;br /&gt;
|  Mousumi Das (Indian Institute of Astrophysics)&lt;br /&gt;
|  Low Surface Brightness Galaxies - their morphological classes and disk evolution&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Sep 14&lt;br /&gt;
|  Stijn Wuyts (Univ. of Bath)&lt;br /&gt;
|  The Growth of Disks and Bulges&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Sep 18&lt;br /&gt;
|  Mike Rich (UC Los Angeles)&lt;br /&gt;
|  New Observational Perspectives on the Galaxy&#039;s Central Bulge/Bar System&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| Sep 21&lt;br /&gt;
|  Sandra Faber (UCSC)&lt;br /&gt;
|  Toy model for the growth of black holes and galaxy quenching&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| Sep 28&lt;br /&gt;
|  Ji-Wei Xie (Nanjing Univ)&lt;br /&gt;
| The scientific impact of the LAMOST on exoplanet research&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Oct 5&lt;br /&gt;
| No colloquium (Holidays)&lt;br /&gt;
| &lt;br /&gt;
|  &lt;br /&gt;
|-&lt;br /&gt;
| Oct 12&lt;br /&gt;
| Xiaowei Liu (PKU)&lt;br /&gt;
|  The LAMOST Spectroscopic Survey of the Galactic Anti-center&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Oct 19&lt;br /&gt;
| E. (Lia) Athanassoula (LAM)&lt;br /&gt;
|   Dynamical and chemical modeling of Milky Way-type galaxies&lt;br /&gt;
|  Martin Smith&lt;br /&gt;
|-&lt;br /&gt;
| Oct 26&lt;br /&gt;
|  Xian Chen (PKU)&lt;br /&gt;
| Retrieving the true mass of gravitational-wave sources&lt;br /&gt;
|  Hong Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 2&lt;br /&gt;
|  Yifu Cai (USTC)&lt;br /&gt;
|  Probing the Very Early Universe with CMB Experiments&lt;br /&gt;
| Hong Guo &lt;br /&gt;
|-&lt;br /&gt;
| Nov 9&lt;br /&gt;
|  Tong Liu (Xiamen Univ)&lt;br /&gt;
| cancelled&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 16&lt;br /&gt;
|   Bernhard Brandl (Leiden)&lt;br /&gt;
|  Science Goals of the Mid-Infrared Imager and Spectrograph (METIS) at ESO&#039;s Extremely Large Telescope (ELT)&lt;br /&gt;
|   Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 23&lt;br /&gt;
|   Xu Kong (USTC)&lt;br /&gt;
|  Star formation quenching and mass assembly of galaxies&lt;br /&gt;
|  Hong Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 30&lt;br /&gt;
|   Xiaohu Yang (SJTU)&lt;br /&gt;
| Mapping the real space distribution of galaxies&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| Dec 7&lt;br /&gt;
|  Jinlin Han (NAOC)&lt;br /&gt;
|  银河系结构与磁场研究的新结果&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| Dec 13&lt;br /&gt;
|  Jian Ge (Univ of Florida) &lt;br /&gt;
| Searching for Habitable Worlds Using Artificial Intelligence (special time: 10:30 am)&lt;br /&gt;
|  Fulai  Guo &lt;br /&gt;
|-&lt;br /&gt;
| Dec 14&lt;br /&gt;
|  Yong Shi (Nanjing Univ) &lt;br /&gt;
| Star Formation Across Cosmic Time&lt;br /&gt;
|  Hong Guo &lt;br /&gt;
|-&lt;br /&gt;
| Dec 21&lt;br /&gt;
|   &lt;br /&gt;
|  note: cancelled due to SKA meeting&lt;br /&gt;
|   &lt;br /&gt;
|-&lt;br /&gt;
| Dec 28&lt;br /&gt;
| Liang Gao (NAOC)&lt;br /&gt;
| 暗物质天文学研究&lt;br /&gt;
|  Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| Jan 4&lt;br /&gt;
| Daniel Wang (Univ of Massachusetts)&lt;br /&gt;
|  The Galactic Center Ecosystem&lt;br /&gt;
|  Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Jan 11&lt;br /&gt;
|  Hua Feng (Tsinghua) &lt;br /&gt;
| Ultraluminous X-ray Sources&lt;br /&gt;
| Fulai Guo  &lt;br /&gt;
|-&lt;br /&gt;
| Jan 18&lt;br /&gt;
|  Zheng Zheng (Univ of Utah)&lt;br /&gt;
|  The Curious Case of Lyman-alpha Emitting Galaxies&lt;br /&gt;
| Hong Guo &lt;br /&gt;
|-&lt;br /&gt;
| Jan 25&lt;br /&gt;
| Shiyin Shen (SHAO) &lt;br /&gt;
| The dust along the line-of-sight to extra-galactic objects&lt;br /&gt;
| Fulai Guo &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&#039;&#039;&#039;Spring 2017&#039;&#039;&#039;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Date&lt;br /&gt;
! Speaker &lt;br /&gt;
! Topic&lt;br /&gt;
! Host&lt;br /&gt;
|-&lt;br /&gt;
| Feb 16&lt;br /&gt;
|  Christine Wilson (McMaster)&lt;br /&gt;
|  Observing Galaxies with the Atacama Large Millimeter Array (ALMA)&lt;br /&gt;
|  Ting Xiao, Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Feb 23&lt;br /&gt;
|  &lt;br /&gt;
| &lt;br /&gt;
|  No Colloquium&lt;br /&gt;
|-&lt;br /&gt;
| March 2&lt;br /&gt;
| James Stone (Princeton)&lt;br /&gt;
|  cancelled&lt;br /&gt;
| Feng Yuan, Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| March 9&lt;br /&gt;
| Di Li (NAOC)&lt;br /&gt;
| An Unprecedented Commensal Drift-Scan Survey with FAST&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| March 16&lt;br /&gt;
| Yipeng Jing (SJTU)&lt;br /&gt;
|  星系红移巡天 &lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| March 23&lt;br /&gt;
| Alok Gupta (ARIES/SHAO)&lt;br /&gt;
| Multi-wavelength Time Domain Astronomy: &lt;br /&gt;
To Probe the Environs of Central Super Massive Black Hole of Blazars&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| March 30&lt;br /&gt;
| Pengfei Chen (NJU)&lt;br /&gt;
|  Observations and Modeling of Solar Coronal Waves&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
|-&lt;br /&gt;
| April 6&lt;br /&gt;
| Jun Lin (Yunnan Observatories)&lt;br /&gt;
| Lin-Forbes Model for the Solar Eruption and the CME/Flare Current Sheet&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| April 11&lt;br /&gt;
| James Binney (Oxford)&lt;br /&gt;
|  Special Colloquium: How did our Galaxy form?&lt;br /&gt;
| Martin Smith&lt;br /&gt;
|-&lt;br /&gt;
| April 13&lt;br /&gt;
| Martin Bureau (Oxford)&lt;br /&gt;
| 3D Observations of Molecular Gas in Galaxies: From Global Dynamics to Supermassive Black Holes&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| April 20&lt;br /&gt;
| Xiaofeng Wang (Tsinghua)&lt;br /&gt;
| Supernova Zoo: Obervations and Theories&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| April 27&lt;br /&gt;
| Xi Kang (PMO)&lt;br /&gt;
|  Galaxy formation and spatial alignment&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
|-&lt;br /&gt;
| May 4&lt;br /&gt;
| Wei Cui (Tsinghua/Purdue)&lt;br /&gt;
| Probing Missing Baryons with X-ray Spectroscopy&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| May 11&lt;br /&gt;
| Xuefeng Wu (PMO)&lt;br /&gt;
| Testing Fundamental Physics With Fast Radio Bursts&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
|-&lt;br /&gt;
| May 18&lt;br /&gt;
|  Zigao Dai (NJU)&lt;br /&gt;
| Models for Fast Radio Bursts and Future Astrophysical Tests &lt;br /&gt;
|  Fu-guo Xie&lt;br /&gt;
|-&lt;br /&gt;
| May 25&lt;br /&gt;
| Zhanwen Han (Yunnan Observatories)&lt;br /&gt;
| Binary population synthesis and the formation of binary-related objects &lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| June 1&lt;br /&gt;
| Jin Chang (PMO)&lt;br /&gt;
| 空间探测暗物质粒子 &lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| June 8&lt;br /&gt;
| Linhua Jiang (KIAA/PKU)&lt;br /&gt;
| Properties of Spectroscopically-Confirmed Galaxies at z &amp;gt;= 6&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
|-&lt;br /&gt;
| June 15&lt;br /&gt;
| Qiang Yuan (PMO)&lt;br /&gt;
| Cosmic ray physics and dark matter searches with AMS-02&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| June 22&lt;br /&gt;
| Junxian Wang (USTC)&lt;br /&gt;
| The UV/Optical Variation in Active Galactic Nuclei&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| June 29&lt;br /&gt;
| Xiang-Yu Wang (NJU)&lt;br /&gt;
| Multi-messenger approach to study the origin of high-energy cosmic rays&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
|}&lt;br /&gt;
 &lt;br /&gt;
----&lt;br /&gt;
&#039;&#039;&#039;Fall 2016&#039;&#039;&#039;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Date&lt;br /&gt;
! Speaker &lt;br /&gt;
! Topic&lt;br /&gt;
! Host&lt;br /&gt;
|-&lt;br /&gt;
| Oct 20&lt;br /&gt;
| Weiguang Cui (ICRAR/UWA)&lt;br /&gt;
| The MACRO simulated galaxy cluster project: The final chapter&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
|-&lt;br /&gt;
| Oct 27&lt;br /&gt;
| Jun Zhang (CAA/SJTU)&lt;br /&gt;
| Recent Progress in Weak Lensing Measurement&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
|-&lt;br /&gt;
| Oct 28 &lt;br /&gt;
| Sandra Faber (UCSC)&lt;br /&gt;
| Fast vs. Slow: Galaxy Death at z ~ 2 vs. z ~ 0 (NEW TIME: 10 am)&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 3&lt;br /&gt;
| Neal Evans (UT Austin)&lt;br /&gt;
| What Determines Star Formation Rates?&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 10&lt;br /&gt;
| Richard (Dick) Manchester (CSIRO)&lt;br /&gt;
| Pulsars and FRBs: Recent Developments&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Nov 17&lt;br /&gt;
| Houjun Mo (Tsinghua/UMass)&lt;br /&gt;
| Reconstructing the initial conditions to simulate the formation of the local universe&lt;br /&gt;
| Juntai Shen&lt;br /&gt;
|-&lt;br /&gt;
| Nov 24&lt;br /&gt;
| Bin Luo (Nanjing Univ.)&lt;br /&gt;
| Cosmic Supermassive Black Hole Growth in the 7 Ms CDF-S&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Dec 1&lt;br /&gt;
| Youjun Lu (NAOC)&lt;br /&gt;
| A short introduction to gravitational wave and gravitational wave astrophysics&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Dec 8&lt;br /&gt;
| Peter Scicluna (ASIAA)&lt;br /&gt;
| Comparing radiative transfer models and observations of astrophysical dust&lt;br /&gt;
| Lei Hao&lt;br /&gt;
|-&lt;br /&gt;
| Dec 15&lt;br /&gt;
| Siming Liu (PMO)&lt;br /&gt;
| Acceleration of high-energy particles in supernova remnants&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Dec 22&lt;br /&gt;
| Shuang-Nan Zhang (IHEP)&lt;br /&gt;
| Testing Einstein’s Equivalent Principle with Fast Radio Bursts and &lt;br /&gt;
the Problem of Detecting Electromagnetic Waves from Merging Black Holes&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Dec 29&lt;br /&gt;
| Xiang-Dong Li (Nanjing Univ)&lt;br /&gt;
| Formation of Galactic Black Hole Low-Mass X-ray Binaries&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Jan 5, 2017&lt;br /&gt;
| Shude Mao (Tsinghua/NAOC)&lt;br /&gt;
|  Is the IMF Universal in Galaxies? A MaNGA View&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Jan 12, 2017&lt;br /&gt;
| Luis Ho (KIAA/Peking)&lt;br /&gt;
| Some Unsolved Problems in Black Hole - Galaxy Coevolution&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|-&lt;br /&gt;
| Jan 19, 2017&lt;br /&gt;
| Richard de Grijs (KIAA)  TIME: 1:30 pm&lt;br /&gt;
| Not-so-simple stellar populations in nearby, resolved massive star clusters&lt;br /&gt;
| Fulai Guo&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Beers_CEMP_Beijing_2019.pptx&amp;diff=3073</id>
		<title>文件:Beers CEMP Beijing 2019.pptx</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Beers_CEMP_Beijing_2019.pptx&amp;diff=3073"/>
		<updated>2019-05-09T10:18:16Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​Tim Beers&amp;#039; seminar from Monday 6th May.&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Tim Beers&#039; seminar from Monday 6th May.&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Beers_rproc_Shanghai_2019.pptx&amp;diff=3072</id>
		<title>文件:Beers rproc Shanghai 2019.pptx</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Beers_rproc_Shanghai_2019.pptx&amp;diff=3072"/>
		<updated>2019-05-09T10:17:24Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​Tim&amp;#039;s colloquium from 9th May.&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Tim&#039;s colloquium from 9th May.&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=3069</id>
		<title>Students</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=3069"/>
		<updated>2019-05-05T08:25:55Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* 张燕琼 Yanqiong Zhang */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== João Antonio Amarante ==&lt;br /&gt;
&lt;br /&gt;
 [[File:joao.jpg|145px|right|João]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email:  amarante@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: Milky Way structure &amp;amp; evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Martin C. Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2020&lt;br /&gt;
&lt;br /&gt;
==冯帅 Shuai  Feng==&lt;br /&gt;
&lt;br /&gt;
 [[File:照片 049.1.jpg|100px|right|Feng]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5322&lt;br /&gt;
&lt;br /&gt;
Email:  fengsh@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: Galaxy pairs, galaxy evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2019&lt;br /&gt;
&lt;br /&gt;
[http://cluster.shao.ac.cn/~sfeng Personal Page]&lt;br /&gt;
&lt;br /&gt;
[[Shuai Feng&#039;s Wiki Main Page]]&lt;br /&gt;
&lt;br /&gt;
==居梦婷 Mengting Ju==&lt;br /&gt;
[[File:Jumengting.JPG  |150px|right|jumengting]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: mtju@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Jun Yin&lt;br /&gt;
&lt;br /&gt;
Expected graduation:2020&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[ MTJU Wiki Main Page]]&lt;br /&gt;
&lt;br /&gt;
==李璐 Lu Li==&lt;br /&gt;
[[File:IMG 5036.jpg|150px|right|lilu]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: lilu@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  Star clusters, Astrostatistics&lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao , Chen Li&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2020&lt;br /&gt;
&lt;br /&gt;
==刘蓉蓉 Rongrong Liu==&lt;br /&gt;
[[File:Liurongrong.jpg|115px|right|liurongrong]]&lt;br /&gt;
Office: &lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email: lrongr@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
== 卢家风 Jiafeng Lu ==&lt;br /&gt;
&lt;br /&gt;
 [[File:jiafenglu.jpg|100px|right|jflu]]&lt;br /&gt;
&lt;br /&gt;
Office:  1513&lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email:  jflu@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: &lt;br /&gt;
&lt;br /&gt;
Supervisor: Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张书会  Shuhui Zhang ==&lt;br /&gt;
 [[File:Shuhui Zhang.JPG|200px|right|Zhang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510  &lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email:  shzhang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: Galaxies, Stars and Milk way &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao, Ruixiang Chang, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2018&lt;br /&gt;
&lt;br /&gt;
==张燕琼 Yanqiong Zhang==&lt;br /&gt;
 [[File:yanqiong.jpg|150px|right|yanqiong]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email: zhangyq@shao.ac.cn  &lt;br /&gt;
&lt;br /&gt;
Research interests:  Galactic formation and kinematics, Hyper-velocity stars&lt;br /&gt;
&lt;br /&gt;
Supervisor：Martin Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2019&lt;br /&gt;
&lt;br /&gt;
==郑云亮 Yunliang Zheng==&lt;br /&gt;
&lt;br /&gt;
[[File:|100px|right|zhengyunliang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: ylz@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==钟文心 Wenxin Zhong==&lt;br /&gt;
&lt;br /&gt;
 [[File:钟文心.JPG|100px|right|zhongwenxin]]&lt;br /&gt;
&lt;br /&gt;
Office:  1513&lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email:  zhongwenxin@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Jian Fu , Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation: &lt;br /&gt;
----&lt;br /&gt;
==黄轶琦  Yiqi Huang==&lt;br /&gt;
&lt;br /&gt;
Office:   &lt;br /&gt;
 &lt;br /&gt;
Email:  hyq@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: &lt;br /&gt;
&lt;br /&gt;
Supervisor：Jinliang Hou, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==胡国真 Guozhen Hu==&lt;br /&gt;
 [[File:1536673757543.jpeg|150px|right|guozhen]]&lt;br /&gt;
&lt;br /&gt;
Office:  &lt;br /&gt;
&lt;br /&gt;
Tel:  &lt;br /&gt;
&lt;br /&gt;
Email: hgz@shao.ac.cn  &lt;br /&gt;
&lt;br /&gt;
Research interests:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao&lt;br /&gt;
&lt;br /&gt;
Expected graduation: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[已毕业学生|Graduated students]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2895</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2895"/>
		<updated>2018-10-28T08:59:44Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* Coauthours */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;The Lives of Stars: Insights from the TGAS-RAVE-LAMOST Data Set&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;, 2018, ApJ, 860, 91 ([http://adsabs.harvard.edu/abs/2018ApJ...860...91V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Galactic extinction and reddening from the South Galactic Cap U-band Sky Survey: u band galaxy number counts and u−r color distribution&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Linlin Li, Shiyin Shen, Jinliang Hou, Fangting Yuan, Jing Zhong&#039;&#039;&#039; et al., 2017, AJ, 153， 88([http://adsabs.harvard.edu/abs/2017AJ....153...88L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039; et al., 2017, MNRAS, 467, 208 ([http://adsabs.harvard.edu/abs/2017MNRAS.467..208O ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Why do disk galaxies present a common gas-phase metallicity gradient?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Chang, R., Zhang, Shuhui, Shen, Shiyin, Yin, Jun, and Hou, Jinliang&#039;&#039;&#039; , 2017, IAUS 321, 134 ([http://adsabs.harvard.edu/abs/2017IAUS..321..134C ADS])&lt;br /&gt;
#&#039;&#039;The atomic gas in outer disks in semi-analytic models of galaxy formation, 2017IAUS..321..131F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu Jian&#039;&#039;&#039;, Luo, Yu&lt;br /&gt;
#&#039;&#039;Cold gas in the models of galaxy formation and evolution, 2017SSPMA..47d9802F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
#&#039;&#039;Bayesian Inference of Kinematics and Mass Segregation of Open Cluster?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shao, Z.,Xie, X.,Chen, L.,Zhong, J.,Hou, J.,Lin, C.-C.&#039;&#039;&#039; , 2017, IAUS 316, 265 ([http://adsabs.harvard.edu/abs/2017IAUS..316..265S ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;StarGO: A New Method to Identify the Galactic Origins of Halo Stars&#039;&#039;&lt;br /&gt;
#:Yuan, Zhen; Chang, Jiang; Banerjee, Projjwal; Han, Jiaxin; Kang, Xi; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, 2018, ApJ, 863, 26 ([http://adsabs.harvard.edu/abs/2018ApJ...863...26Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST DR1: Stellar Parameters and Chemical Abundances with SP_Ace&#039;&#039;&lt;br /&gt;
#:Boeche, C.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Grebel, E. K.; &#039;&#039;&#039;Zhong, J.&#039;&#039;&#039;; &#039;&#039;&#039;Hou, J. L.&#039;&#039;&#039;; &#039;&#039;&#039;Chen, L.&#039;&#039;&#039;; Stello, D., 2018, AJ, 155, 181 ([http://adsabs.harvard.edu/abs/2018AJ....155..181B ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The velocity ellipsoid in the Galactic disc using Gaia DR1&#039;&#039;&lt;br /&gt;
#:Anguiano, Borja; Majewski, Steven R.; Freeman, Kenneth C.; Mitschang, Arik W.; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;, 2018, MNRAS, 474, 854 ([http://adsabs.harvard.edu/abs/2018MNRAS.474..854A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Structure of the Milky Way stellar halo out to its outer boundary with blue horizontal-branch stars&#039;&#039;&lt;br /&gt;
#:Fukushima, Tetsuya; Chiba, Masashi; Homma, Daisuke; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;; et al., 2018, PASJ, 70, 69 ([http://adsabs.harvard.edu/abs/2018PASJ...70...69F ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III&#039;&#039;&lt;br /&gt;
#:Homma, Daisuke; Chiba, Masashi; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039; et al., 2018, PASJ, 70, 18 ([http://adsabs.harvard.edu/abs/2018PASJ...70S..18H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Hyper Suprime-Cam SSP Survey: Overview and survey design&#039;&#039;&lt;br /&gt;
#:Aihara, Hiroaki et al. (incl. &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;), 2018, PASJ, 70, 4 ([http://adsabs.harvard.edu/abs/2018PASJ...70S...4A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Spectral classification and composites of galaxies in LAMOST DR4&#039;&#039;&lt;br /&gt;
#: Wang, Li-Li, Luo, A.-Li, &#039;&#039;&#039;Shen, Shi-Yin&#039;&#039;&#039;, et al.,, MNRAS, 2018, 474, 1873 ([http://adsabs.harvard.edu/abs/2018MNRAS.474.1873W ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Identification of the White Dwarf Companion to the Millisecond Pulsar J2317+1439&#039;&#039;&lt;br /&gt;
#:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Wang, S.; &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;; Xu, R. X.; Yue, Y. L.; Liu, J. F., 2017, ApJ, 842, 105&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Star formation history of the galaxy merger Mrk848 with SDSS-IV MaNGA&#039;&#039;&lt;br /&gt;
#:Yuan, Fang-Ting, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, Hao, Lei, and Fernandez, Maria Argudo, 2017, IAUS, 321, 304 ([http://adsabs.harvard.edu/abs/2017IAUS..321..304Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;球状动力学系统的基本面——从椭圆星系到球状星团&#039;&#039;&lt;br /&gt;
#:庞晓莹，&#039;&#039;&#039;沈世银&#039;&#039;&#039;,《天文学进展》，2017, 4, 389 [http://center.shao.ac.cn/twxjz/abstract/2017/20170401.pdf pdf]  &lt;br /&gt;
#&#039;&#039;Integrated HI emission in galaxy groups and clusters, 2017RAA....17..101A&#039;&#039;&lt;br /&gt;
#: Ai, Mei; Zhu, Ming; &#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2016 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2894</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2894"/>
		<updated>2018-10-28T08:58:55Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;The Lives of Stars: Insights from the TGAS-RAVE-LAMOST Data Set&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;, 2018, ApJ, 860, 91 ([http://adsabs.harvard.edu/abs/2018ApJ...860...91V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Galactic extinction and reddening from the South Galactic Cap U-band Sky Survey: u band galaxy number counts and u−r color distribution&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Linlin Li, Shiyin Shen, Jinliang Hou, Fangting Yuan, Jing Zhong&#039;&#039;&#039; et al., 2017, AJ, 153， 88([http://adsabs.harvard.edu/abs/2017AJ....153...88L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039; et al., 2017, MNRAS, 467, 208 ([http://adsabs.harvard.edu/abs/2017MNRAS.467..208O ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Why do disk galaxies present a common gas-phase metallicity gradient?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Chang, R., Zhang, Shuhui, Shen, Shiyin, Yin, Jun, and Hou, Jinliang&#039;&#039;&#039; , 2017, IAUS 321, 134 ([http://adsabs.harvard.edu/abs/2017IAUS..321..134C ADS])&lt;br /&gt;
#&#039;&#039;The atomic gas in outer disks in semi-analytic models of galaxy formation, 2017IAUS..321..131F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu Jian&#039;&#039;&#039;, Luo, Yu&lt;br /&gt;
#&#039;&#039;Cold gas in the models of galaxy formation and evolution, 2017SSPMA..47d9802F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
#&#039;&#039;Bayesian Inference of Kinematics and Mass Segregation of Open Cluster?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shao, Z.,Xie, X.,Chen, L.,Zhong, J.,Hou, J.,Lin, C.-C.&#039;&#039;&#039; , 2017, IAUS 316, 265 ([http://adsabs.harvard.edu/abs/2017IAUS..316..265S ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;StarGO: A New Method to Identify the Galactic Origins of Halo Stars&#039;&#039;&lt;br /&gt;
#:Yuan, Zhen; Chang, Jiang; Banerjee, Projjwal; Han, Jiaxin; Kang, Xi; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, 2018, ApJ, 863, 26 ([http://adsabs.harvard.edu/abs/2018ApJ...863...26Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST DR1: Stellar Parameters and Chemical Abundances with SP_Ace&#039;&#039;&lt;br /&gt;
#:Boeche, C.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Grebel, E. K.; &#039;&#039;&#039;Zhong, J.&#039;&#039;&#039;; &#039;&#039;&#039;Hou, J. L.&#039;&#039;&#039;; &#039;&#039;&#039;Chen, L.&#039;&#039;&#039;; Stello, D., 2018, AJ, 155, 181 ([http://adsabs.harvard.edu/abs/2018AJ....155..181B ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The velocity ellipsoid in the Galactic disc using Gaia DR1&#039;&#039;&lt;br /&gt;
#:Anguiano, Borja; Majewski, Steven R.; Freeman, Kenneth C.; Mitschang, Arik W.; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;, 2018, MNRAS, 474, 854&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Structure of the Milky Way stellar halo out to its outer boundary with blue horizontal-branch stars&#039;&#039;&lt;br /&gt;
#:Fukushima, Tetsuya; Chiba, Masashi; Homma, Daisuke; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;; et al., 2018, PASJ, 70, 69 ([http://adsabs.harvard.edu/abs/2018PASJ...70...69F ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III&#039;&#039;&lt;br /&gt;
#:Homma, Daisuke; Chiba, Masashi; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039; et al., 2018, PASJ, 70, 18 ([http://adsabs.harvard.edu/abs/2018PASJ...70S..18H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Hyper Suprime-Cam SSP Survey: Overview and survey design&#039;&#039;&lt;br /&gt;
#:Aihara, Hiroaki et al. (incl. &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;), 2018, PASJ, 70, 4 ([http://adsabs.harvard.edu/abs/2018PASJ...70S...4A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Spectral classification and composites of galaxies in LAMOST DR4&#039;&#039;&lt;br /&gt;
#: Wang, Li-Li, Luo, A.-Li, &#039;&#039;&#039;Shen, Shi-Yin&#039;&#039;&#039;, et al.,, MNRAS, 2018, 474, 1873 ([http://adsabs.harvard.edu/abs/2018MNRAS.474.1873W ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Identification of the White Dwarf Companion to the Millisecond Pulsar J2317+1439&#039;&#039;&lt;br /&gt;
#:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Wang, S.; &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;; Xu, R. X.; Yue, Y. L.; Liu, J. F., 2017, ApJ, 842, 105&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Star formation history of the galaxy merger Mrk848 with SDSS-IV MaNGA&#039;&#039;&lt;br /&gt;
#:Yuan, Fang-Ting, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, Hao, Lei, and Fernandez, Maria Argudo, 2017, IAUS, 321, 304 ([http://adsabs.harvard.edu/abs/2017IAUS..321..304Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;球状动力学系统的基本面——从椭圆星系到球状星团&#039;&#039;&lt;br /&gt;
#:庞晓莹，&#039;&#039;&#039;沈世银&#039;&#039;&#039;,《天文学进展》，2017, 4, 389 [http://center.shao.ac.cn/twxjz/abstract/2017/20170401.pdf pdf]  &lt;br /&gt;
#&#039;&#039;Integrated HI emission in galaxy groups and clusters, 2017RAA....17..101A&#039;&#039;&lt;br /&gt;
#: Ai, Mei; Zhu, Ming; &#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2016 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2893</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2893"/>
		<updated>2018-10-28T08:56:19Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* Coauthours */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;The Galactic extinction and reddening from the South Galactic Cap U-band Sky Survey: u band galaxy number counts and u−r color distribution&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Linlin Li, Shiyin Shen, Jinliang Hou, Fangting Yuan, Jing Zhong&#039;&#039;&#039; et al., 2017, AJ, 153， 88([http://adsabs.harvard.edu/abs/2017AJ....153...88L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039; et al., 2017, MNRAS, 467, 208 ([http://adsabs.harvard.edu/abs/2017MNRAS.467..208O ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Why do disk galaxies present a common gas-phase metallicity gradient?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Chang, R., Zhang, Shuhui, Shen, Shiyin, Yin, Jun, and Hou, Jinliang&#039;&#039;&#039; , 2017, IAUS 321, 134 ([http://adsabs.harvard.edu/abs/2017IAUS..321..134C ADS])&lt;br /&gt;
#&#039;&#039;The atomic gas in outer disks in semi-analytic models of galaxy formation, 2017IAUS..321..131F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu Jian&#039;&#039;&#039;, Luo, Yu&lt;br /&gt;
#&#039;&#039;Cold gas in the models of galaxy formation and evolution, 2017SSPMA..47d9802F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
#&#039;&#039;Bayesian Inference of Kinematics and Mass Segregation of Open Cluster?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shao, Z.,Xie, X.,Chen, L.,Zhong, J.,Hou, J.,Lin, C.-C.&#039;&#039;&#039; , 2017, IAUS 316, 265 ([http://adsabs.harvard.edu/abs/2017IAUS..316..265S ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;StarGO: A New Method to Identify the Galactic Origins of Halo Stars&#039;&#039;&lt;br /&gt;
#:Yuan, Zhen; Chang, Jiang; Banerjee, Projjwal; Han, Jiaxin; Kang, Xi; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, 2018, ApJ, 863, 26 ([http://adsabs.harvard.edu/abs/2018ApJ...863...26Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST DR1: Stellar Parameters and Chemical Abundances with SP_Ace&#039;&#039;&lt;br /&gt;
#:Boeche, C.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Grebel, E. K.; &#039;&#039;&#039;Zhong, J.&#039;&#039;&#039;; &#039;&#039;&#039;Hou, J. L.&#039;&#039;&#039;; &#039;&#039;&#039;Chen, L.&#039;&#039;&#039;; Stello, D., 2018, AJ, 155, 181 ([http://adsabs.harvard.edu/abs/2018AJ....155..181B ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The velocity ellipsoid in the Galactic disc using Gaia DR1&#039;&#039;&lt;br /&gt;
#:Anguiano, Borja; Majewski, Steven R.; Freeman, Kenneth C.; Mitschang, Arik W.; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;, 2018, MNRAS, 474, 854&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Structure of the Milky Way stellar halo out to its outer boundary with blue horizontal-branch stars&#039;&#039;&lt;br /&gt;
#:Fukushima, Tetsuya; Chiba, Masashi; Homma, Daisuke; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;; et al., 2018, PASJ, 70, 69 ([http://adsabs.harvard.edu/abs/2018PASJ...70...69F ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III&#039;&#039;&lt;br /&gt;
#:Homma, Daisuke; Chiba, Masashi; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039; et al., 2018, PASJ, 70, 18 ([http://adsabs.harvard.edu/abs/2018PASJ...70S..18H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Hyper Suprime-Cam SSP Survey: Overview and survey design&#039;&#039;&lt;br /&gt;
#:Aihara, Hiroaki et al. (incl. &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;), 2018, PASJ, 70, 4 ([http://adsabs.harvard.edu/abs/2018PASJ...70S...4A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Spectral classification and composites of galaxies in LAMOST DR4&#039;&#039;&lt;br /&gt;
#: Wang, Li-Li, Luo, A.-Li, &#039;&#039;&#039;Shen, Shi-Yin&#039;&#039;&#039;, et al.,, MNRAS, 2018, 474, 1873 ([http://adsabs.harvard.edu/abs/2018MNRAS.474.1873W ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Identification of the White Dwarf Companion to the Millisecond Pulsar J2317+1439&#039;&#039;&lt;br /&gt;
#:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Wang, S.; &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;; Xu, R. X.; Yue, Y. L.; Liu, J. F., 2017, ApJ, 842, 105&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Star formation history of the galaxy merger Mrk848 with SDSS-IV MaNGA&#039;&#039;&lt;br /&gt;
#:Yuan, Fang-Ting, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, Hao, Lei, and Fernandez, Maria Argudo, 2017, IAUS, 321, 304 ([http://adsabs.harvard.edu/abs/2017IAUS..321..304Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;球状动力学系统的基本面——从椭圆星系到球状星团&#039;&#039;&lt;br /&gt;
#:庞晓莹，&#039;&#039;&#039;沈世银&#039;&#039;&#039;,《天文学进展》，2017, 4, 389 [http://center.shao.ac.cn/twxjz/abstract/2017/20170401.pdf pdf]  &lt;br /&gt;
#&#039;&#039;Integrated HI emission in galaxy groups and clusters, 2017RAA....17..101A&#039;&#039;&lt;br /&gt;
#: Ai, Mei; Zhu, Ming; &#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2016 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2892</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2892"/>
		<updated>2018-10-28T08:53:43Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* Coauthours */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;The Galactic extinction and reddening from the South Galactic Cap U-band Sky Survey: u band galaxy number counts and u−r color distribution&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Linlin Li, Shiyin Shen, Jinliang Hou, Fangting Yuan, Jing Zhong&#039;&#039;&#039; et al., 2017, AJ, 153， 88([http://adsabs.harvard.edu/abs/2017AJ....153...88L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039; et al., 2017, MNRAS, 467, 208 ([http://adsabs.harvard.edu/abs/2017MNRAS.467..208O ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Why do disk galaxies present a common gas-phase metallicity gradient?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Chang, R., Zhang, Shuhui, Shen, Shiyin, Yin, Jun, and Hou, Jinliang&#039;&#039;&#039; , 2017, IAUS 321, 134 ([http://adsabs.harvard.edu/abs/2017IAUS..321..134C ADS])&lt;br /&gt;
#&#039;&#039;The atomic gas in outer disks in semi-analytic models of galaxy formation, 2017IAUS..321..131F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu Jian&#039;&#039;&#039;, Luo, Yu&lt;br /&gt;
#&#039;&#039;Cold gas in the models of galaxy formation and evolution, 2017SSPMA..47d9802F&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
#&#039;&#039;Bayesian Inference of Kinematics and Mass Segregation of Open Cluster?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shao, Z.,Xie, X.,Chen, L.,Zhong, J.,Hou, J.,Lin, C.-C.&#039;&#039;&#039; , 2017, IAUS 316, 265 ([http://adsabs.harvard.edu/abs/2017IAUS..316..265S ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;StarGO: A New Method to Identify the Galactic Origins of Halo Stars&#039;&#039;&lt;br /&gt;
#:Yuan, Zhen; Chang, Jiang; Banerjee, Projjwal; Han, Jiaxin; Kang, Xi; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, 2018, ApJ, 863, 26 ([http://adsabs.harvard.edu/abs/2018ApJ...863...26Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST DR1: Stellar Parameters and Chemical Abundances with SP_Ace&#039;&#039;&lt;br /&gt;
#:Boeche, C.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Grebel, E. K.; &#039;&#039;&#039;Zhong, J.&#039;&#039;&#039;; &#039;&#039;&#039;Hou, J. L.&#039;&#039;&#039;; &#039;&#039;&#039;Chen, L.&#039;&#039;&#039;; Stello, D., 2018, AJ, 155, 181 ([http://adsabs.harvard.edu/abs/2018AJ....155..181B ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Structure of the Milky Way stellar halo out to its outer boundary with blue horizontal-branch stars&#039;&#039;&lt;br /&gt;
#:Fukushima, Tetsuya; Chiba, Masashi; Homma, Daisuke; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;; et al., 2018, PASJ, 70, 69 ([http://adsabs.harvard.edu/abs/2018PASJ...70...69F ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III&#039;&#039;&lt;br /&gt;
#:Homma, Daisuke; Chiba, Masashi; &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039; et al., 2018, PASJ, 70, 18 ([http://adsabs.harvard.edu/abs/2018PASJ...70S..18H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Hyper Suprime-Cam SSP Survey: Overview and survey design&#039;&#039;&lt;br /&gt;
#:Aihara, Hiroaki et al. (incl. &#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;), 2018, PASJ, 70, 4 ([http://adsabs.harvard.edu/abs/2018PASJ...70S...4A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Spectral classification and composites of galaxies in LAMOST DR4&#039;&#039;&lt;br /&gt;
#: Wang, Li-Li, Luo, A.-Li, &#039;&#039;&#039;Shen, Shi-Yin&#039;&#039;&#039;, et al.,, MNRAS, 2018, 474, 1873 ([http://adsabs.harvard.edu/abs/2018MNRAS.474.1873W ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Identification of the White Dwarf Companion to the Millisecond Pulsar J2317+1439&#039;&#039;&lt;br /&gt;
#:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Wang, S.; &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;; Xu, R. X.; Yue, Y. L.; Liu, J. F., 2017, ApJ, 842, 105&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Star formation history of the galaxy merger Mrk848 with SDSS-IV MaNGA&#039;&#039;&lt;br /&gt;
#:Yuan, Fang-Ting, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, Hao, Lei, and Fernandez, Maria Argudo, 2017, IAUS, 321, 304 ([http://adsabs.harvard.edu/abs/2017IAUS..321..304Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;球状动力学系统的基本面——从椭圆星系到球状星团&#039;&#039;&lt;br /&gt;
#:庞晓莹，&#039;&#039;&#039;沈世银&#039;&#039;&#039;,《天文学进展》，2017, 4, 389 [http://center.shao.ac.cn/twxjz/abstract/2017/20170401.pdf pdf]  &lt;br /&gt;
#&#039;&#039;Integrated HI emission in galaxy groups and clusters, 2017RAA....17..101A&#039;&#039;&lt;br /&gt;
#: Ai, Mei; Zhu, Ming; &#039;&#039;&#039;Fu, Jian&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2016 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2454</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2454"/>
		<updated>2017-08-25T07:08:59Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* Coauthours */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;The Galactic extinction and reddening from the South Galactic Cap U-band Sky Survey: u band galaxy number counts and u−r color distribution&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Linlin Li, Shiyin Shen, Jinliang Hou, Fangting Yuan, Jing Zhong&#039;&#039;&#039; et al., 2017, AJ, 153， 88([http://adsabs.harvard.edu/abs/2017AJ....153...88L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039; et al., 2017, MNRAS, 467, 208 ([http://adsabs.harvard.edu/abs/2017MNRAS.467..208O ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A Global Correction to PPMXL Proper Motions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, J.J&#039;&#039;&#039; et al., 2016, AJ, 151, 99 ([http://adsabs.harvard.edu/abs/2016AJ....151...99V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The effect of local and large-scale environments on nuclear activity and star formation&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Argudo-Fernández, M.&#039;&#039;&#039;; &#039;&#039;&#039;Shen, S.&#039;&#039;&#039;; Sabater, J.; Duarte Puertas, S.; Verley, S.; Yang, X., 2016, A&amp;amp;A, 592,30 ([http://adsabs.harvard.edu/abs/2016A%26A...592A..30A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&amp;quot;The Luminosity Dependence of Quasar UV Continuum Slope: Dust Extinction Scenario&amp;quot;&lt;br /&gt;
#:&#039;&#039;&#039;Xie, Xiaoyi&#039;&#039;&#039;; &#039;&#039;&#039;Shao, Zhengyi&#039;&#039;&#039;; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;; Liu, Hui; &#039;&#039;&#039;Li, Linlin&#039;&#039;&#039;, 2016, ApJ, 824, 38([http://adsabs.harvard.edu/abs/2016ApJ...824...38X ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA, 16, 72 ([http://adsabs.harvard.edu/abs/2016RAA....16...43S  ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA, 16, 43 ([http://adsabs.harvard.edu/abs/2016RAA....16...43S ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2016 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [http://adsabs.harvard.edu/abs/2016ASSL..420..113S ADS], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|PDF]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;The Identification of the White Dwarf Companion to the Millisecond Pulsar J2317+1439&#039;&#039;&lt;br /&gt;
#:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Wang, S.; &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;; Xu, R. X.; Yue, Y. L.; Liu, J. F., 2017, ApJ, 842, 105&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The star formation history of low-mass disk galaxies: A case study of NGC 300&#039;&#039;&lt;br /&gt;
#:Kang, Xiaoyu; Zhang, Fenghui; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;; Wang, Lang; Cheng, Liantao, 2016, A&amp;amp;A, 585,20&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The evolution of the spiral galaxy M51a&#039;&#039;&lt;br /&gt;
#:Kang, Xiaoyu; Zhang, Fenghui; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;,  2016IAUS..319..129K&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Halo Mass Estimation for Galaxy Groups: The Role Of Magnitude Gaps&#039;&#039;&lt;br /&gt;
#:Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2016, 317,332 &lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;South Galactic Cap u-band Sky Survey (SCUSS): Project Overview&#039;&#039;&lt;br /&gt;
#:Zhou, Xu et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;), RAA, 16, 69&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;South Galactic Cap u-band Sky Survey (SCUSS): Data Release&#039;&#039;&lt;br /&gt;
#:Zhou, Hu et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;), 2016AJ....151...37Z&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Large Sky Area Multi-object Fiber Spectroscopic Telescope Quasar Survey: Quasar Properties from the First Data Release&#039;&#039;&lt;br /&gt;
#:Ai, Y.L. et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;), 2016AJ....151...24A&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;,2016A&amp;amp;A...585A..50R&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2453</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2453"/>
		<updated>2017-08-25T07:05:17Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;The Galactic extinction and reddening from the South Galactic Cap U-band Sky Survey: u band galaxy number counts and u−r color distribution&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Linlin Li, Shiyin Shen, Jinliang Hou, Fangting Yuan, Jing Zhong&#039;&#039;&#039; et al., 2017, AJ, 153， 88([http://adsabs.harvard.edu/abs/2017AJ....153...88L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039; et al., 2017, MNRAS, 467, 208 ([http://adsabs.harvard.edu/abs/2017MNRAS.467..208O ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A Global Correction to PPMXL Proper Motions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, J.J&#039;&#039;&#039; et al., 2016, AJ, 151, 99 ([http://adsabs.harvard.edu/abs/2016AJ....151...99V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The effect of local and large-scale environments on nuclear activity and star formation&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Argudo-Fernández, M.&#039;&#039;&#039;; &#039;&#039;&#039;Shen, S.&#039;&#039;&#039;; Sabater, J.; Duarte Puertas, S.; Verley, S.; Yang, X., 2016, A&amp;amp;A, 592,30 ([http://adsabs.harvard.edu/abs/2016A%26A...592A..30A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&amp;quot;The Luminosity Dependence of Quasar UV Continuum Slope: Dust Extinction Scenario&amp;quot;&lt;br /&gt;
#:&#039;&#039;&#039;Xie, Xiaoyi&#039;&#039;&#039;; &#039;&#039;&#039;Shao, Zhengyi&#039;&#039;&#039;; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;; Liu, Hui; &#039;&#039;&#039;Li, Linlin&#039;&#039;&#039;, 2016, ApJ, 824, 38([http://adsabs.harvard.edu/abs/2016ApJ...824...38X ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA, 16, 72 ([http://adsabs.harvard.edu/abs/2016RAA....16...43S  ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA, 16, 43 ([http://adsabs.harvard.edu/abs/2016RAA....16...43S ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2016 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [http://adsabs.harvard.edu/abs/2016ASSL..420..113S ADS], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|PDF]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;The star formation history of low-mass disk galaxies: A case study of NGC 300&#039;&#039;&lt;br /&gt;
#:Kang, Xiaoyu; Zhang, Fenghui; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;; Wang, Lang; Cheng, Liantao, 2016, A&amp;amp;A, 585,20&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The evolution of the spiral galaxy M51a&#039;&#039;&lt;br /&gt;
#:Kang, Xiaoyu; Zhang, Fenghui; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;,  2016IAUS..319..129K&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Halo Mass Estimation for Galaxy Groups: The Role Of Magnitude Gaps&#039;&#039;&lt;br /&gt;
#:Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2016, 317,332 &lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;South Galactic Cap u-band Sky Survey (SCUSS): Project Overview&#039;&#039;&lt;br /&gt;
#:Zhou, Xu et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;), RAA, 16, 69&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;South Galactic Cap u-band Sky Survey (SCUSS): Data Release&#039;&#039;&lt;br /&gt;
#:Zhou, Hu et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;), 2016AJ....151...37Z&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Large Sky Area Multi-object Fiber Spectroscopic Telescope Quasar Survey: Quasar Properties from the First Data Release&#039;&#039;&lt;br /&gt;
#:Ai, Y.L. et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;), 2016AJ....151...24A&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A et al.(including &#039;&#039;&#039;Shiyin Shen&#039;&#039;&#039;,2016A&amp;amp;A...585A..50R&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2320</id>
		<title>Students</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2320"/>
		<updated>2017-01-18T03:14:21Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== João Antonio Amarante ==&lt;br /&gt;
&lt;br /&gt;
 [[File:joao.jpg|145px|right|João]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email:  amarante@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: Milky Way structure &amp;amp; evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Martin C. Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2020&lt;br /&gt;
&lt;br /&gt;
==冯帅 Shuai  Feng==&lt;br /&gt;
&lt;br /&gt;
 [[File:照片 049.1.jpg|100px|right|Feng]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5322&lt;br /&gt;
&lt;br /&gt;
Email:  fengsh@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: Galaxy pairs, galaxy evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
[http://cluster.shao.ac.cn/~sfeng Personal Page]&lt;br /&gt;
&lt;br /&gt;
[[Shuai Feng&#039;s Wiki Main Page]]&lt;br /&gt;
&lt;br /&gt;
==居梦婷 Mengting Ju==&lt;br /&gt;
[[File:Jumengting.JPG  |150px|right|jumengting]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: mtju@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Jun Yin&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李琳琳 Linlin Li==&lt;br /&gt;
[[File:Linlin Li.JPG|200px|right|Li]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5321&lt;br /&gt;
&lt;br /&gt;
Email: lilin@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: Galactic structure &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen, Jinliang Hou&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李璐 Lu Li==&lt;br /&gt;
[[File:IMG 5036.jpg|150px|right|lilu]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: lilu@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  Star clusters, Astrostatistics&lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao , Chen Li&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==刘蓉蓉 Rongrong Liu==&lt;br /&gt;
[[File:Liurongrong.jpg|115px|right|liurongrong]]&lt;br /&gt;
Office: &lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email: lrongr@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==杨丽 Li Yang==&lt;br /&gt;
[[File:IMG.jpeg |90px|right|Yangli]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: liyang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  Star clusters&lt;br /&gt;
&lt;br /&gt;
Supervisor：Chen Li, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张书会  Shuhui Zhang ==&lt;br /&gt;
 [[File:Shuhui Zhang.JPG|200px|right|Zhang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510  &lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email:  shzhang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests: Galaxies, Stars and Milk way &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao, Ruixiang Chang, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张燕琼 Yanqiong Zhang==&lt;br /&gt;
 [[File:yanqiong.jpg|150px|right|yanqiong]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email: zhangyq@shao.ac.cn  &lt;br /&gt;
&lt;br /&gt;
Research interests:  Galactic formation and kinematics, Hyper-velocity stars&lt;br /&gt;
&lt;br /&gt;
Supervisor：Martin Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2017&lt;br /&gt;
&lt;br /&gt;
==郑云亮 Yunliang Zheng==&lt;br /&gt;
&lt;br /&gt;
[[File:DSC9459-2.jpg|100px|right|zhengyunliang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: ylz@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interests:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
[[已毕业学生|Graduated students]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2319</id>
		<title>Students</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2319"/>
		<updated>2017-01-18T03:10:49Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* João Antonio Amarante */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== João Antonio Amarante ==&lt;br /&gt;
&lt;br /&gt;
 [[File:joao.jpg|160px|right|João]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email:  amarante@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Milky Way structure &amp;amp; evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Martin C. Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2020&lt;br /&gt;
&lt;br /&gt;
==冯帅 Shuai  Feng==&lt;br /&gt;
&lt;br /&gt;
 [[File:照片 049.1.jpg|100px|right|Feng]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5322&lt;br /&gt;
&lt;br /&gt;
Email:  fengsh@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxy pairs, galaxy evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
[http://cluster.shao.ac.cn/~sfeng Personal Page]&lt;br /&gt;
&lt;br /&gt;
[[Shuai Feng&#039;s Wiki Main Page]]&lt;br /&gt;
&lt;br /&gt;
==居梦婷 Mengting Ju==&lt;br /&gt;
[[File:Jumengting.JPG  |150px|right|jumengting]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: mtju@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Jun Yin&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李琳琳 Linlin Li==&lt;br /&gt;
[[File:Linlin Li.JPG|200px|right|Li]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5321&lt;br /&gt;
&lt;br /&gt;
Email: lilin@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galactic structure &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen, Jinliang Hou&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李璐 Lu Li==&lt;br /&gt;
[[File:IMG 5036.jpg|150px|right|lilu]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: lilu@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, Astrostatistics&lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao , Chen Li&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==刘蓉蓉 Rongrong Liu==&lt;br /&gt;
[[File:Liurongrong.jpg|115px|right|liurongrong]]&lt;br /&gt;
Office: &lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email: lrongr@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==杨丽 Li Yang==&lt;br /&gt;
[[File:IMG.jpeg |90px|right|Yangli]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: liyang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, &lt;br /&gt;
&lt;br /&gt;
Supervisor：Chen Li, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张书会  Shuhui Zhang ==&lt;br /&gt;
 [[File:Shuhui Zhang.JPG|200px|right|Zhang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510  &lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email:  shzhang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxies, Stars and Milk way &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao, Ruixiang Chang, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张燕琼 Yanqiong Zhang==&lt;br /&gt;
 [[File:yanqiong.jpg|150px|right|yanqiong]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email: zhangyq@shao.ac.cn  &lt;br /&gt;
&lt;br /&gt;
Research interest:  Galactic formation and kinematics, Hyper-velocity stars&lt;br /&gt;
&lt;br /&gt;
Supervisor：Martin Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2017&lt;br /&gt;
&lt;br /&gt;
==郑云亮 Yunliang Zheng==&lt;br /&gt;
&lt;br /&gt;
[[File:DSC9459-2.jpg|100px|right|zhengyunliang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: ylz@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
[[已毕业学生|Graduated students]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2318</id>
		<title>Students</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2318"/>
		<updated>2017-01-18T03:08:42Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== João Antonio Amarante ==&lt;br /&gt;
&lt;br /&gt;
 [[File:joao.jpg|150px|right|João]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email:  amarante@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Milky Way structure &amp;amp; evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Martin C. Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2020&lt;br /&gt;
&lt;br /&gt;
==冯帅 Shuai  Feng==&lt;br /&gt;
&lt;br /&gt;
 [[File:照片 049.1.jpg|100px|right|Feng]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5322&lt;br /&gt;
&lt;br /&gt;
Email:  fengsh@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxy pairs, galaxy evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
[http://cluster.shao.ac.cn/~sfeng Personal Page]&lt;br /&gt;
&lt;br /&gt;
[[Shuai Feng&#039;s Wiki Main Page]]&lt;br /&gt;
&lt;br /&gt;
==居梦婷 Mengting Ju==&lt;br /&gt;
[[File:Jumengting.JPG  |150px|right|jumengting]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: mtju@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Jun Yin&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李琳琳 Linlin Li==&lt;br /&gt;
[[File:Linlin Li.JPG|200px|right|Li]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5321&lt;br /&gt;
&lt;br /&gt;
Email: lilin@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galactic structure &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen, Jinliang Hou&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李璐 Lu Li==&lt;br /&gt;
[[File:IMG 5036.jpg|150px|right|lilu]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: lilu@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, Astrostatistics&lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao , Chen Li&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==刘蓉蓉 Rongrong Liu==&lt;br /&gt;
[[File:Liurongrong.jpg|115px|right|liurongrong]]&lt;br /&gt;
Office: &lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email: lrongr@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==杨丽 Li Yang==&lt;br /&gt;
[[File:IMG.jpeg |90px|right|Yangli]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: liyang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, &lt;br /&gt;
&lt;br /&gt;
Supervisor：Chen Li, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张书会  Shuhui Zhang ==&lt;br /&gt;
 [[File:Shuhui Zhang.JPG|200px|right|Zhang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510  &lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email:  shzhang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxies, Stars and Milk way &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao, Ruixiang Chang, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张燕琼 Yanqiong Zhang==&lt;br /&gt;
 [[File:yanqiong.jpg|150px|right|yanqiong]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email: zhangyq@shao.ac.cn  &lt;br /&gt;
&lt;br /&gt;
Research interest:  Galactic formation and kinematics, Hyper-velocity stars&lt;br /&gt;
&lt;br /&gt;
Supervisor：Martin Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2017&lt;br /&gt;
&lt;br /&gt;
==郑云亮 Yunliang Zheng==&lt;br /&gt;
&lt;br /&gt;
[[File:DSC9459-2.jpg|100px|right|zhengyunliang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: ylz@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
[[已毕业学生|Graduated students]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Joao.jpg&amp;diff=2317</id>
		<title>文件:Joao.jpg</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Joao.jpg&amp;diff=2317"/>
		<updated>2017-01-18T03:02:02Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2316</id>
		<title>Students</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2316"/>
		<updated>2017-01-18T02:59:27Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== João Antonio Amarante ==&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email:  amarante@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Milky Way structure &amp;amp; evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Martin C. Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2020&lt;br /&gt;
&lt;br /&gt;
==冯帅 Shuai  Feng==&lt;br /&gt;
 [[File:照片 049.1.jpg|100px|right|Feng]]&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5322&lt;br /&gt;
&lt;br /&gt;
Email:  fengsh@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxy pairs, galaxy evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
[http://cluster.shao.ac.cn/~sfeng Personal Page]&lt;br /&gt;
&lt;br /&gt;
[[Shuai Feng&#039;s Wiki Main Page]]&lt;br /&gt;
&lt;br /&gt;
==居梦婷 Mengting Ju==&lt;br /&gt;
[[File:Jumengting.JPG  |150px|right|jumengting]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: mtju@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Jun Yin&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李琳琳 Linlin Li==&lt;br /&gt;
[[File:Linlin Li.JPG|200px|right|Li]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5321&lt;br /&gt;
&lt;br /&gt;
Email: lilin@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galactic structure &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen, Jinliang Hou&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==李璐 Lu Li==&lt;br /&gt;
[[File:IMG 5036.jpg|150px|right|lilu]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: lilu@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, Astrostatistics&lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao , Chen Li&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==刘蓉蓉 Rongrong Liu==&lt;br /&gt;
[[File:Liurongrong.jpg|115px|right|liurongrong]]&lt;br /&gt;
Office: &lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email: lrongr@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==杨丽 Li Yang==&lt;br /&gt;
[[File:IMG.jpeg |90px|right|Yangli]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: liyang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, &lt;br /&gt;
&lt;br /&gt;
Supervisor：Chen Li, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张书会  Shuhui Zhang ==&lt;br /&gt;
 [[File:Shuhui Zhang.JPG|200px|right|Zhang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510  &lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email:  shzhang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxies, Stars and Milk way &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao, Ruixiang Chang, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
==张燕琼 Yanqiong Zhang==&lt;br /&gt;
 [[File:yanqiong.jpg|150px|right|yanqiong]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email: zhangyq@shao.ac.cn  &lt;br /&gt;
&lt;br /&gt;
Research interest:  Galactic formation and kinematics, Hyper-velocity stars&lt;br /&gt;
&lt;br /&gt;
Supervisor：Martin Smith&lt;br /&gt;
&lt;br /&gt;
Expected graduation: 2017&lt;br /&gt;
&lt;br /&gt;
==郑云亮 Yunliang Zheng==&lt;br /&gt;
[[File:DSC9459-2.jpg  |100px|right|zhengyunliang]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: ylz@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
Expected graduation:&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
[[已毕业学生|Graduated students]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2315</id>
		<title>Students</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Students&amp;diff=2315"/>
		<updated>2017-01-18T02:48:44Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​Alphabetised&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==冯帅 Shuai  Feng==&lt;br /&gt;
 [[File:照片 049.1.jpg|100px|right|Feng]]&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5322&lt;br /&gt;
&lt;br /&gt;
Email:  fengsh@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxy pairs, galaxy evolution&lt;br /&gt;
&lt;br /&gt;
Supervisor: Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
[http://cluster.shao.ac.cn/~sfeng Personal Page]&lt;br /&gt;
&lt;br /&gt;
[[Shuai Feng&#039;s Wiki Main Page]]&lt;br /&gt;
&lt;br /&gt;
==居梦婷 Mengting Ju==&lt;br /&gt;
[[File:Jumengting.JPG  |150px|right|jumengting]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: mtju@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Jun Yin&lt;br /&gt;
&lt;br /&gt;
==李琳琳 Linlin Li==&lt;br /&gt;
[[File:Linlin Li.JPG|200px|right|Li]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5321&lt;br /&gt;
&lt;br /&gt;
Email: lilin@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galactic structure &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen, Jinliang Hou&lt;br /&gt;
&lt;br /&gt;
==李璐 Lu Li==&lt;br /&gt;
[[File:IMG 5036.jpg|150px|right|lilu]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: lilu@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, Astrostatistics&lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao , Chen Li&lt;br /&gt;
&lt;br /&gt;
==刘蓉蓉 Rongrong Liu==&lt;br /&gt;
[[File:Liurongrong.jpg|115px|right|liurongrong]]&lt;br /&gt;
Office: &lt;br /&gt;
&lt;br /&gt;
Tel: &lt;br /&gt;
&lt;br /&gt;
Email: lrongr@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao&lt;br /&gt;
&lt;br /&gt;
==杨丽 Li Yang==&lt;br /&gt;
[[File:IMG.jpeg |90px|right|Yangli]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: liyang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  Star clusters, &lt;br /&gt;
&lt;br /&gt;
Supervisor：Chen Li, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
==张书会  Shuhui Zhang ==&lt;br /&gt;
 [[File:Shuhui Zhang.JPG|200px|right|Zhang]]&lt;br /&gt;
&lt;br /&gt;
Office: 1510  &lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email:  shzhang@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest: Galaxies, Stars and Milk way &lt;br /&gt;
&lt;br /&gt;
Supervisor：Zhengyi Shao, Ruixiang Chang, Jing Zhong&lt;br /&gt;
&lt;br /&gt;
==张燕琼 Yanqiong Zhang==&lt;br /&gt;
 [[File:yanqiong.jpg|150px|right|yanqiong]]&lt;br /&gt;
&lt;br /&gt;
Office:  1510&lt;br /&gt;
&lt;br /&gt;
Tel:  5322&lt;br /&gt;
&lt;br /&gt;
Email: zhangyq@shao.ac.cn  &lt;br /&gt;
&lt;br /&gt;
Research interest:  Galactic formation and kinematics, Hyper-velocity stars&lt;br /&gt;
&lt;br /&gt;
Supervisor：Martin Smith&lt;br /&gt;
&lt;br /&gt;
==郑云亮 Yunliang Zheng==&lt;br /&gt;
[[File:DSC9459-2.jpg  |100px|right|zhengyunliang]]&lt;br /&gt;
Office: 1510&lt;br /&gt;
&lt;br /&gt;
Tel: 5532&lt;br /&gt;
&lt;br /&gt;
Email: ylz@shao.ac.cn&lt;br /&gt;
&lt;br /&gt;
Research interest:  &lt;br /&gt;
&lt;br /&gt;
Supervisor：Shiyin Shen&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
[[已毕业学生|Graduated students]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2314</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2314"/>
		<updated>2017-01-18T02:39:46Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039; et al., 2017, MNRAS, in press ([https://arxiv.org/abs/1701.04422 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A Global Correction to PPMXL Proper Motions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, J.J&#039;&#039;&#039; et al., 2016, AJ, 151, 99 ([http://adsabs.harvard.edu/abs/2016AJ....151...99V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2016 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [http://adsabs.harvard.edu/abs/2016ASSL..420..113S ADS], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|PDF]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2313</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2313"/>
		<updated>2017-01-18T02:37:31Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;A Global Correction to PPMXL Proper Motions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, J.J&#039;&#039;&#039; et al., 2016, AJ, 151, 99 ([http://adsabs.harvard.edu/abs/2016AJ....151...99V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2016 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [http://adsabs.harvard.edu/abs/2016ASSL..420..113S ADS], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|PDF]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2312</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2312"/>
		<updated>2017-01-18T02:37:05Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;A Global Correction to PPMXL Proper Motions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, J.J&#039;&#039;&#039; et al., 2016, AJ, 151, 99 ([http://adsabs.harvard.edu/abs/2016AJ....151...99V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2016 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [http://adsabs.harvard.edu/abs/2016ASSL..420..113S ADS], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|preprint]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2311</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2311"/>
		<updated>2017-01-18T02:36:41Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;A Global Correction to PPMXL Proper Motions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, J.J&#039;&#039;&#039; et al., 2016, AJ, 151, 99 ([http://adsabs.harvard.edu/abs/2016AJ....151...99V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2015 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [http://adsabs.harvard.edu/abs/2016ASSL..420..113S ADS], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|preprint]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2310</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2310"/>
		<updated>2017-01-18T02:31:35Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;A Global Correction to PPMXL Proper Motions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, J.J&#039;&#039;&#039; et al., 2016, AJ, 151, 99 ([http://adsabs.harvard.edu/abs/2016AJ....151...99V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2308</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2308"/>
		<updated>2017-01-18T02:29:51Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* Coauthours */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey&#039;&#039;&lt;br /&gt;
#:Homma, D. et al. (including &#039;&#039;&#039;Okamoto, S.&#039;&#039;&#039;), 2016, ApJL, 832, 21 ([http://adsabs.harvard.edu/abs/2016ApJ...832...21H ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2306</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2306"/>
		<updated>2017-01-18T02:21:36Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2016 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [http://adsabs.harvard.edu/abs/2016ASSL..420..113S ADS], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|preprint]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2305</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2305"/>
		<updated>2017-01-18T02:19:11Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2016 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|preprint]])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_publications&amp;diff=2304</id>
		<title>2015 publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_publications&amp;diff=2304"/>
		<updated>2017-01-18T02:18:02Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
&lt;br /&gt;
#&#039;&#039;Isolated Galaxies versus Interacting Pairs with MaNGA&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Argudo-Fernández, María&#039;&#039;&#039;; Yuan, Fangting; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;; &#039;&#039;&#039;Yin, Jun&#039;&#039;&#039;; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;; &#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;, 2015, Galaxies, 3, 156([http://adsabs.harvard.edu/abs/2015Galax...3..156F ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Catalogues of isolated galaxies, isolated pairs, and isolated triplets in the local Universe&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Argudo-Fernández, María&#039;&#039;&#039;; et al., 2015, A&amp;amp;A, 578A, 110A([http://adsabs.harvard.edu/abs/2015A%26A...578A.110A ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Reconstructing the Accretion History of the Galactic Stellar Halo from Chemical Abundance Ratio Distributions&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Lee, Duane M.&#039;&#039;&#039;; et al. 2015, ApJ, 802, 48 ([http://adsabs.harvard.edu/abs/2015ApJ...802...48L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Searching for classical Be stars in LAMOST DR1&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Lin, Chien-Cheng; Hou, Jin-Liang; Chen, Li; Shao, Zheng-Yi; Zhong, Jing;&#039;&#039;&#039; Yu, Po-Chieh, 2015, RAA, 15, 1325 ([http://adsabs.harvard.edu/abs/2015RAA....15.1325L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A Hyper Suprime-Cam View of the Interacting Galaxies of the M81 Group&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039; et al.; 2015, ApJL, 809, L1 ([http://ads.nao.ac.jp/abs/2015ApJ...809L...1O ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Red Runaways: Hypervelocity Stars, Hills Ejecta and Other Outliers in the F-M Star Regime&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Grebel, Eva K.; 2015, AJ, 150, 77 ([http://adsabs.harvard.edu/abs/2015arXiv150603153V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Apparent Redshift Dependence of Quasar Continuum: Implication for Cosmic Dust Extinction?&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Xie, Xiaoyi&#039;&#039;&#039;; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;; &#039;&#039;&#039;Shao, Zhengyi&#039;&#039;&#039;; &#039;&#039;&#039;Yin, Jun&#039;&#039;&#039;, 2015, ApJL, 802,16 ([http://adsabs.harvard.edu/abs/2015ApJ...802L..16X ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;M-giant star candidates identified in LAMOST DR 1&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhong, Jing&#039;&#039;&#039;;  Lépine, Sébastien; &#039;&#039;&#039;Li, Jing&#039;&#039;&#039;; &#039;&#039;&#039;Chen, Li&#039;&#039;&#039;; &#039;&#039;&#039;Hou, Jin-Liang&#039;&#039;&#039;, et al., 2015, RAA, 15, 1154([http://adsabs.harvard.edu/abs/2015RAA....15.1154Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#Automated Identification of 2612 Late-K and M Dwarfs in the LAMOST Commissioning Data Using Classification Template Fits&lt;br /&gt;
#:&#039;&#039;&#039;Zhong, Jing&#039;&#039;&#039;; Lépine, Sébastien; &#039;&#039;&#039;Hou, Jinliang&#039;&#039;&#039;; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al., 2015, AJ, 150, 42([http://adsabs.harvard.edu/abs/2015AJ....150...42Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#双城记—星系并合和星系对&lt;br /&gt;
#:&#039;&#039;&#039;沈世银，袁方婷，侯金良&#039;&#039;&#039;， 2015,《物理》，4, 152  ([http://www.cnki.com.cn/Article/CJFDTotal-WLZZ201504004.htm cnki])&lt;br /&gt;
&lt;br /&gt;
==Coauthors==&lt;br /&gt;
# &#039;&#039;Gravitational Microlensing by Neutron Stars and Radio Pulsars: Event Rates, Timescale Distributions, and Mass Measurements&#039;&#039;&lt;br /&gt;
#:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Lin, M. X.; Yue, Y. L.; Hobbs, G.; Xu, R. X.; 2015, ApJ, 802, 120 ([http://adsabs.harvard.edu/abs/2015ApJ...802..120D ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;3D cluster members and near-infrared distance of open cluster NGC 6819&#039;&#039;&lt;br /&gt;
#:Gao Xin-Hua; Xu, Shou-Kun; &#039;&#039;&#039;Chen, Li&#039;&#039;&#039;, 2015, RAA, 15, 2193 ([http://adsabs.harvard.edu/abs/2015RAA....15.2193G ADS]) &lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Discovery of high-velocity EHB stars in the globular cluster ω Centauri (NGC 5139)&#039;&#039;&lt;br /&gt;
#:Gao Xin-Hua; Xu, Shou-Kun; &#039;&#039;&#039;Chen, Li&#039;&#039;&#039;, 2015, RAA, 15, 1639, ([http://adsabs.harvard.edu/abs/2015RAA....15.1639G ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;The evolution of interacting spiral galaxy NGC 5194&#039;&#039;&lt;br /&gt;
#:Kang, Xiaoyu; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414 ([http://adsabs.harvard.edu/abs/2015MNRAS.449..414K ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;The star formation history of low-mass disk galaxies: A case study of NGC 300&#039;&#039;&lt;br /&gt;
#:Kang, Xiaoyu; Zhang, Fenghui; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;;  Wang,Lang; Cheng, Liantao; 2015, A&amp;amp;A, 585, 20 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..20K ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Using member galaxy luminosities as halo mass proxies of galaxy groups&#039;&#039; &lt;br /&gt;
#:Lu, Yi; Yang, Xiaohu; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, 2015, ApJL, 804, 55 ([http://adsabs.harvard.edu/abs/2015ApJ...804...55L ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Resonant Orbits and the High Velocity Peaks Towards the Bulge&#039;&#039;&lt;br /&gt;
#:Molloy, Matthew; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Evans, N. Wyn; Shen, Juntai; 2015, ApJ, in press ([http://adsabs.harvard.edu/abs/2015arXiv150504245M ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Resonant Clumping and Substructure in Galactic Disks&#039;&#039;&lt;br /&gt;
#:Molloy, Matthew; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Shen, Juntai; Wyn Evans, N.; 2015, ApJ, 804, 80 ([http://adsabs.harvard.edu/abs/2015ApJ...804...80M ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;An extended view of the Pisces Overdensity from the SCUSS survey&#039;&#039;&lt;br /&gt;
#:Nie, J.D.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; et al; 2015, ApJ, 810, 153 ([http://adsabs.harvard.edu/abs/2015arXiv150801272N ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Fixing the reference frame for PPMXL proper motions using extragalactic sources&#039;&#039;&lt;br /&gt;
#:Grabowski, Kathleen et al.; 2015, RAA, 15, 849 ([http://adsabs.harvard.edu/abs/2015RAA....15..849G ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Photometric metallicity calibration with SDSS and SCUSS and its application to distant stars in the south Galactic cap&#039;&#039;&lt;br /&gt;
#:Gu, J. et al., 2015, MNRAS, 452, 3092([http://adsabs.harvard.edu/abs/2015MNRAS.452.3092G ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;The discovery of 64 luminous infrared galaxies in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap&#039;&#039;&lt;br /&gt;
#:Lam, M. et al., 2015, RAA, 15, 1424 ([http://adsabs.harvard.edu/abs/2015RAA....15.1424L ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;The first data release (DR1) of the LAMOST regular survey&#039;&#039;&lt;br /&gt;
#:Luo, A., et al. (including: &#039;&#039;&#039;Chen, Li; Hou, Jinliang; Lin, Chien-Cheng; Shen, Shiyin&#039;&#039;&#039;), 2015, RAA, 15, 1095([http://adsabs.harvard.edu/abs/2015RAA....15.1095L ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;An Investigation of the Absolute Proper Motions of the SCUSS Catalog&#039;&#039;&lt;br /&gt;
#:Peng, Xiyan et al., 2015, PASP, 127, 250 ([http://adsabs.harvard.edu/abs/2015PASP..127..250P ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Rings and Radial Waves in the Disk of the Milky WAY&#039;&#039;&lt;br /&gt;
#:Xu, Yan et al.; 2015, ApJ, 801, 105([http://adsabs.harvard.edu/abs/2015ApJ...801..105X ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;A sample of E+A galaxy candidates in the Second Data Release of LAMOST Survey&#039;&#039;&lt;br /&gt;
#:Yang, H. et al., 2015, 15,1414 RAA ([http://adsabs.harvard.edu/abs/2015RAA....15.1414Y ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Capability of Quasar Selection by Combining SCUSS and SDSS Observations&#039;&#039; &lt;br /&gt;
#:Zhou, H. et al., 2015,PASP,127,94 ([http://adsabs.harvard.edu/abs/2015PASP..127...94Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
# &#039;&#039;Searching for Be Stars in the Open Cluster NGC 663&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2015, AJ, 149, 43 ([http://adsabs.harvard.edu/abs/2015AJ....149...43Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;An H I view of galaxy conformity: H I-rich environment around H I-excess galaxies&#039;&#039;&lt;br /&gt;
#:Wang, Jing et al., 2015, 453, 2399W MNRAS ([http://adsabs.harvard.edu/abs/2015MNRAS.453.2399W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Galaxy Formation &amp;amp; Dark Matter Modelling in the Era of the Square Kilometre Array&#039;&#039;&lt;br /&gt;
#:Power, C et al., 2015aska.confE.133P ([http://adsabs.harvard.edu/abs/2015aska.confE.133P ADS])&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2303</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2303"/>
		<updated>2017-01-18T02:16:51Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, 832, 10 ([http://adsabs.harvard.edu/abs/2016ApJ...832...10Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2177</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=2177"/>
		<updated>2016-11-03T08:53:06Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
#&#039;&#039;Red Runaways II: Low mass Hills stars in SDSS Stripe 82&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Zhang, Y.&#039;&#039;&#039;, &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;, Carlin, J.L., 2016, ApJ, in press ([http://adsabs.harvard.edu/abs/2016arXiv160804053Z ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;基于LAMOST光谱巡天的Be星搜寻&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;林建争; 陈力; 锺靖&#039;&#039;&#039;, 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;An Isolated Compact Galaxy Triplet&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Feng, Shuai&#039;&#039;&#039;; &#039;&#039;&#039;Shao Zhengyi&#039;&#039;&#039;, &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, &#039;&#039;&#039;Fernández, María&#039;&#039;&#039; et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;LAMOST 1: A Disrupted Satellite in the Constellation Draco&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039; et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])&lt;br /&gt;
#:&lt;br /&gt;
#&#039;&#039;New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars&#039;&#039;&lt;br /&gt;
#:&#039;&#039;&#039;Li, Jing.&#039;&#039;&#039;; &#039;&#039;&#039;Liu, Chao.&#039;&#039;&#039; et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthours==&lt;br /&gt;
#&#039;&#039;The Gaia-ESO survey: Metal-rich bananas in the bulge&#039;&#039;&lt;br /&gt;
#:Williams, A.A. et al. (including &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])&lt;br /&gt;
# &#039;&#039;Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST&#039;&#039;&lt;br /&gt;
#:Lee, Chien-Hsiu and &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;, 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE&#039;&#039;&lt;br /&gt;
#:Tang, Baitian; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2016arXiv161006763T ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST&#039;&#039;&lt;br /&gt;
#:Hou, Wen; et al. (including &#039;&#039;&#039;Lin, Chien-Cheng&#039;&#039;&#039;), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])&lt;br /&gt;
#: &lt;br /&gt;
#&#039;&#039;The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant&#039;&#039;&lt;br /&gt;
#:Raichoor, A. et al., 2016, A&amp;amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])&lt;br /&gt;
#: &lt;br /&gt;
# &#039;&#039;Be Stars in the Open Cluster NGC 6830&#039;&#039;&lt;br /&gt;
#:Yu, Po-Chieh; &#039;&#039;&#039;Lin, Chien-Cheng;&#039;&#039;&#039; et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])&lt;br /&gt;
#: &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2015 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;br /&gt;
----&lt;br /&gt;
*ADS custom format，%A,%T,%J,%y,%v,%p&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:20151125-martin.pdf&amp;diff=1767</id>
		<title>文件:20151125-martin.pdf</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:20151125-martin.pdf&amp;diff=1767"/>
		<updated>2015-11-26T08:11:17Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​Group meeting talk for 25th Nov.&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Group meeting talk for 25th Nov.&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Seminar_Plan&amp;diff=1766</id>
		<title>Seminar Plan</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Seminar_Plan&amp;diff=1766"/>
		<updated>2015-11-26T08:04:19Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Date !! Speaker !! Title&lt;br /&gt;
|-&lt;br /&gt;
| 2014.09.03 ||	Lin, Chien-Cheng || [[Media:20140903-roger.pdf|Searching for and Characterization of Galactic Open Clusters toward the Galactic Anti-Center with Pan-STARRS1]]&lt;br /&gt;
|-&lt;br /&gt;
| 2014.09.10 ||	Lee, Duane || [[Media:duane_talk091014.pdf|A next-generation program for chemical enrichment evolution of dwarf satellite galaxy models]]&lt;br /&gt;
|-&lt;br /&gt;
| 2014.09.17 ||	Chen, Li || [[Media:ngc6791_chenli.pdf|WIYN OPEN CLUSTER STUDY. LIX. RADIAL-VELOCITY MEMBERSHIP OF THE EVOLVED population OF THE OLD OPEN CLUSTER NGC6791 &amp;lt;br /&amp;gt;(ref.arXiv:1408.3117)]]&lt;br /&gt;
|-&lt;br /&gt;
|2014.09.24 ||	Mamen Argudo||  [[Media:Mamen.pdf|Characterisation of an Isolated Galaxy Sample and the Influence of the Environment]]&lt;br /&gt;
|-&lt;br /&gt;
|2014.10.01 ||	National Day || none&lt;br /&gt;
|-&lt;br /&gt;
|2014.10.08 ||	National Day || none&lt;br /&gt;
|-&lt;br /&gt;
|2014.10.15 ||	Li, Linlin ||  [[Media:Linlin Li2014.10.15.pdf|Star Count Method to Study Galactic Structure]]  &lt;br /&gt;
&lt;br /&gt;
|-&lt;br /&gt;
|2014.10.22 ||	Molloy, Matthew (KIAA) || Resonant Clumping and Substructure in Galaxy Disks&lt;br /&gt;
|-&lt;br /&gt;
|2014.10.29 ||	Annual Meeting of Astronomy || none&lt;br /&gt;
|-&lt;br /&gt;
|2014.11.05 ||	No Meeting || none&lt;br /&gt;
|-&lt;br /&gt;
|2014.11.12 ||	Li, Jiangtao || [[Media:201411_NJU_PMO_XMU_KIAA_v3.pptx|Circum-galactic Medium Around Local Spiral Galaxies -- A New Window to Understand Galaxy Evolution]] &lt;br /&gt;
|-&lt;br /&gt;
|2014.11.19 ||	No Meeting || none&lt;br /&gt;
|-&lt;br /&gt;
|2014.11.26 ||	Shen, Shiyin || [[Media:The_galaxy_pairs.pdf|The galaxy pairs]]&lt;br /&gt;
|-&lt;br /&gt;
|2014.12.03 ||	Conference in Barcelona || The Milky Way Unravelled. The GREAT-ITN Closing Conference&lt;br /&gt;
|-&lt;br /&gt;
|2014.12.10 ||	Shao, Zhengyi ||Mixture-model of open clusters and the contemplation of LAMOST   &lt;br /&gt;
|-&lt;br /&gt;
|2014.12.17 ||	Liu, Chengze ||UCD in the Virgo Cluster&lt;br /&gt;
|-&lt;br /&gt;
|2014.12.24 ||	Christmas Day || none&lt;br /&gt;
|-&lt;br /&gt;
|2014.12.31 ||	New Year&#039;s Day || none&lt;br /&gt;
|-&lt;br /&gt;
|2015.02.11 ||	Winter Holiday||&lt;br /&gt;
|-&lt;br /&gt;
|2015.03.04 ||	Jing, Zhong/ Xiaoying, Pang|| Discussions on NSFC application&lt;br /&gt;
|-&lt;br /&gt;
|2015.03.05 ||	Fu, Jian/ Liu, Chengze|| Discussions on NSFC application&lt;br /&gt;
|-&lt;br /&gt;
|2015.03.11 ||	Shiyin, Shen|| Discussions on NSFC application&lt;br /&gt;
|-&lt;br /&gt;
|2015.03.25 ||	Meeting in Xiamen|| none&lt;br /&gt;
|-&lt;br /&gt;
|2015.04.02 ||	Boeche, Corrado||SP_Ace: a new code to derive stellar parameters and chemical abundances from stellar spectra&lt;br /&gt;
|-&lt;br /&gt;
|2015.04.08 ||	Yuan, Fang-Ting||Exploring Star formation properties of mergers using multiwavelength data&lt;br /&gt;
|-&lt;br /&gt;
|2015.04.15 ||	Lin, Chien-Cheng||Newly Discovered B-type Emission Stars in the LAMOST DR1&lt;br /&gt;
|-&lt;br /&gt;
|2015.04.22 ||	Chang, Rui-Xiang||A simple model of the evolution of local spiral galaxies&lt;br /&gt;
|-&lt;br /&gt;
|2015.04.29 ||	Meeting at Jiading||[[LAMOST和SDSS-IV数据讨论会]]&lt;br /&gt;
|-&lt;br /&gt;
|2015.05.06 ||	Xie, Xiao-Yi||The redshift and luminosity dependence of the quasar continuum slope&lt;br /&gt;
|-&lt;br /&gt;
|2015.05.13 ||	Pang, Xiaoying||GalevNB: conversion from simulations to observations&lt;br /&gt;
|-&lt;br /&gt;
|2015.05.20 ||	KIAA-SHAO meeting in Beijing&amp;lt;br /&amp;gt;Young Astronomer Forum in Nanjing||None&lt;br /&gt;
|-&lt;br /&gt;
|2015.05.27 ||	Wang, Youfen||L dwarfs  discovered in LAMOST low flux spectra&lt;br /&gt;
|-&lt;br /&gt;
|2015.06.03 ||	Li, Zhiyuan||Not-so-simple stellar populations in massive star clusters&lt;br /&gt;
|-&lt;br /&gt;
|2015.06.10 ||	Meeting in Nanjing || None&lt;br /&gt;
|-&lt;br /&gt;
|2015.06.17 ||	John, Vicker||Hypervelocity Stars, Hills Ejecta, and Other Runaways&lt;br /&gt;
|-&lt;br /&gt;
|2015.06.24 ||	Carlin, Jeff||What can LAMOST tell us about halo substructure&lt;br /&gt;
|-&lt;br /&gt;
|2015.07.01 ||	Fu, Jian||The environment and ram pressure on satellite galaxies in semi-analytic models of galaxy formation&lt;br /&gt;
|-&lt;br /&gt;
|2015.07.08 ||	Meeting in Xinglong|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.07.16-31 ||Summer Holiday|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.08.01-15 ||IAU Meeting in Hawaii|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.08.21-28 ||Meetings in Delingha, Qinghai|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.09.02||Advanced Telescope and Instrument &amp;lt;br /&amp;gt;Techonlogy Conference in Taiwan|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.09.09|| Zhong, Jing|| Open cluster study in the LAMOST DR2&lt;br /&gt;
|-&lt;br /&gt;
|2015.09.16|| Feng, Shuai|| Isolated galaxy triplet&lt;br /&gt;
|-&lt;br /&gt;
|2015.09.23|| Yin, Jun|| How could we recover the SFH from the integrated-light and spectrum?&lt;br /&gt;
|-&lt;br /&gt;
|2015.09.30|| Meeting in Weihai|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.10.07|| National Day Holidays|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.10.14|| Vicker, John|| Searching for Substructure in the Milky Way Halo&lt;br /&gt;
|-&lt;br /&gt;
|2015.10.21|| Annual Meeting of Chinese &amp;lt;br /&amp;gt;astronomical society in PKU|| None&lt;br /&gt;
|-&lt;br /&gt;
|2015.10.28|| None||None&lt;br /&gt;
|-&lt;br /&gt;
|2015.11.04|| Pang, Xiaoying|| Starburst-like dust found in Galactic star cluster NGC 3603&lt;br /&gt;
|-&lt;br /&gt;
|2015.11.11|| Argudo-Fernandez, Maria|| Evolution of spiral isolated galaxies with MaNGA&lt;br /&gt;
|-&lt;br /&gt;
|2015.11.18|| None||None&lt;br /&gt;
|-&lt;br /&gt;
|2015.11.25|| Smith, Martin||[[Media:20151125-martin.pdf| The life and times of the Milky Way as viewed by LAMOST]]&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&amp;diff=1663</id>
		<title>Lunch talks</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&amp;diff=1663"/>
		<updated>2015-09-28T05:22:57Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.&lt;br /&gt;
&lt;br /&gt;
If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:&lt;br /&gt;
http://eepurl.com/bomK-9&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Date !! Speaker !! Title !! Poll&lt;br /&gt;
|-&lt;br /&gt;
| 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||&lt;br /&gt;
|-&lt;br /&gt;
| 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||&lt;br /&gt;
|-&lt;br /&gt;
| 05.10.2015&lt;br /&gt;
| colspan=&amp;quot;3&amp;quot;| No talk due to National Day vacation&lt;br /&gt;
|-&lt;br /&gt;
| 12.10.2015 || Prashanth Mohan (SHAO) || TBA || http://doodle.com/poll/dqupmrgby739nztk&lt;br /&gt;
|-&lt;br /&gt;
| 26.10.2015 || TBA || TBA ||&lt;br /&gt;
|-&lt;br /&gt;
| 09.11.2015 || TBA || TBA ||&lt;br /&gt;
|-&lt;br /&gt;
| 23.10.2015 || TBA || TBA ||&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1651</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1651"/>
		<updated>2015-09-02T10:02:29Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;A Hyper Suprime-Cam View of the Interacting Galaxies of the M81 Group&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Okamoto, Sakurako&#039;&#039;&#039;; et. al.; 2015, ApJL, 809, L1 ([http://ads.nao.ac.jp/abs/2015ApJ...809L...1O ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Red Runaways: Hypervelocity Stars, Hills Ejecta and Other Outliers in the F-M Star Regime&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Grebel, Eva K.; 2015, AJ, 150, 77 ([http://adsabs.harvard.edu/abs/2015arXiv150603153V ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2015 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|preprint]])&lt;br /&gt;
&lt;br /&gt;
*Automated Identification of 2612 Late-K and M Dwarfs in the LAMOST Commissioning Data Using Classification Template Fits&lt;br /&gt;
:&#039;&#039;&#039;Zhong, Jing&#039;&#039;&#039;; Lépine, Sébastien; &#039;&#039;&#039;Hou, Jinliang&#039;&#039;&#039;; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039; et al., 2015, AJ, 150, 42([http://adsabs.harvard.edu/abs/2015AJ....150...42Z ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;An Apparent Redshift Dependence of Quasar Continuum: Implication for Cosmic Dust Extinction?&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Xie, Xiaoyi&#039;&#039;&#039;; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;; &#039;&#039;&#039;Shao, Zhengyi&#039;&#039;&#039;; Yin, Jun, 2015, ApJL, 802,16 ([http://adsabs.harvard.edu/abs/2015ApJ...802L..16X ADS])&lt;br /&gt;
&lt;br /&gt;
*&amp;quot;Reconstructing the Accretion History of the Galactic Stellar Halo from Chemical Abundance Ratio Distributions&amp;quot;&lt;br /&gt;
:&#039;&#039;&#039;Lee, Duane M.&#039;&#039;&#039;; et al. 2015, ApJ, 802, 48 ([http://adsabs.harvard.edu/abs/2015ApJ...802...48L ADS])&lt;br /&gt;
&lt;br /&gt;
==Coauthors==&lt;br /&gt;
*&#039;&#039;The evolution of interacting spiral galaxy NGC 5194&#039;&#039;&lt;br /&gt;
:Kang, Xiaoyu; &#039;&#039;&#039;Chang, Ruixiang&#039;&#039;&#039;; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414 ([http://adsabs.harvard.edu/abs/2015MNRAS.449..414K ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;An extended view of the Pisces Overdensity from the SCUSS survey&#039;&#039;&lt;br /&gt;
:Nie, J.D.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; et al; 2015, ApJ, in press ([http://adsabs.harvard.edu/abs/2015arXiv150801272N ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Resonant Orbits and the High Velocity Peaks Towards the Bulge&#039;&#039;&lt;br /&gt;
:Molloy, Matthew; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Evans, N. Wyn; Shen, Juntai; 2015, ApJ, in press ([http://adsabs.harvard.edu/abs/2015arXiv150504245M ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Resonant Clumping and Substructure in Galactic Disks&#039;&#039;&lt;br /&gt;
:Molloy, Matthew; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Shen, Juntai; Wyn Evans, N.; 2015, ApJ, 804, 80 ([http://adsabs.harvard.edu/abs/2015ApJ...804...80M ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Gravitational Microlensing by Neutron Stars and Radio Pulsars: Event Rates, Timescale Distributions, and Mass Measurements&#039;&#039;&lt;br /&gt;
:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Lin, M. X.; Yue, Y. L.; Hobbs, G.; Xu, R. X.; 2015, ApJ, 802, 120 ([http://adsabs.harvard.edu/abs/2015ApJ...802..120D ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Using member galaxy luminosities as halo mass proxies of galaxy groups&#039;&#039; &lt;br /&gt;
:Lu, Yi; Yang, Xiaohu; &#039;&#039;&#039;Shen, Shiyin&#039;&#039;&#039;, 2015, ApJL, 804, 55 ([http://adsabs.harvard.edu/abs/2015ApJ...804...55L ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Capability of Quasar Selection by Combining SCUSS and SDSS Observations&#039;&#039; &lt;br /&gt;
:Zhou H. et al., 2015,PASP,127,94 ([http://adsabs.harvard.edu/abs/2015PASP..127...94Z ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;An Investigation of the Absolute Proper Motions of the SCUSS Catalog&#039;&#039;&lt;br /&gt;
:Peng, Xiyan et al., 2015, PASP, 127, 250[http://adsabs.harvard.edu/abs/2015PASP..127..250P ADS]&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Fixing the reference frame for PPMXL proper motions using extragalactic sources&#039;&#039;&lt;br /&gt;
:Grabowski, Kathleen et al.; 2015, RAA, 15, 849 ([http://adsabs.harvard.edu/abs/2015RAA....15..849G ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;The first data release (DR1) of the LAMOST regular survey&#039;&#039;&lt;br /&gt;
:Luo A. et al., 2015, RAA, 15, 1095([http://adsabs.harvard.edu/abs/2015RAA....15.1095L ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Photometric metallicity calibration with SDSS and SCUSS and its application to distant stars in the south Galactic cap&#039;&#039;&lt;br /&gt;
:Gu, J. et al., 2015, MNRAS, 452, 3092([http://adsabs.harvard.edu/abs/2015MNRAS.452.3092G ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;The discovery of 64 luminous infrared galaxies in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap&#039;&#039;&lt;br /&gt;
:Lam, M. et al., 2015, RAA, 15, 1424 ([http://adsabs.harvard.edu/abs/2015RAA....15.1424L ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;A sample of E+A galaxy candidates in the Second Data Release of LAMOST Survey&#039;&#039;&lt;br /&gt;
:Yang H. et al., 2015, 15,1414 RAA ([http://adsabs.harvard.edu/abs/2015RAA....15.1414Y ADS])&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1626</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1626"/>
		<updated>2015-08-20T03:17:47Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Red Runaways: Hypervelocity Stars, Hills Ejecta and Other Outliers in the F-M Star Regime&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Grebel, Eva K.; 2015, AJ, 150, 77 ([http://adsabs.harvard.edu/abs/2015arXiv150603153V ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2015 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|preprint]])&lt;br /&gt;
&lt;br /&gt;
*Automated Identification of 2612 Late-K and M Dwarfs in the LAMOST Commissioning Data Using Classification Template Fits[http://adsabs.harvard.edu/abs/2015AJ....150...42Z]&lt;br /&gt;
:Zhong, Jing; Lépine, Sébastien; Hou, Jinliang; Shen, Shiyin; Yuan, Haibo; Huo, Zhiying; Zhang, Huihua; Xiang, Maosheng; Zhang, Huawei; Liu, Xiaowei&lt;br /&gt;
&lt;br /&gt;
*An Apparent Redshift Dependence of Quasar Continuum: Implication for Cosmic Dust Extinction? [http://adsabs.harvard.edu/abs/2015ApJ...802L..16X]&lt;br /&gt;
:Xie, Xiaoyi; Shen, Shiyin; Shao, Zhengyi; Yin, Jun, 2015, ApJL, 802,16&lt;br /&gt;
&lt;br /&gt;
*The evolution of interacting spiral galaxy NGC 5194[http://adsabs.harvard.edu/abs/2015MNRAS.449..414K]&lt;br /&gt;
:Kang, Xiaoyu; Chang, Ruixiang; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414&lt;br /&gt;
&lt;br /&gt;
==Coauthors==&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;An extended view of the Pisces Overdensity from the SCUSS survey&#039;&#039;&lt;br /&gt;
:Nie, J.D.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; et al; 2015, ApJ, in press ([http://adsabs.harvard.edu/abs/2015arXiv150801272N ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Resonant Orbits and the High Velocity Peaks Towards the Bulge&#039;&#039;&lt;br /&gt;
:Molloy, Matthew; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Evans, N. Wyn; Shen, Juntai; 2015, ApJ, submitted ([http://adsabs.harvard.edu/abs/2015arXiv150504245M ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Resonant Clumping and Substructure in Galactic Disks&#039;&#039;&lt;br /&gt;
:Molloy, Matthew; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Shen, Juntai; Wyn Evans, N.; 2015, ApJ, 804, 80 ([http://adsabs.harvard.edu/abs/2015ApJ...804...80M ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Gravitational Microlensing by Neutron Stars and Radio Pulsars: Event Rates, Timescale Distributions, and Mass Measurements&#039;&#039;&lt;br /&gt;
:Dai, S.; &#039;&#039;&#039;Smith, M. C.&#039;&#039;&#039;; Lin, M. X.; Yue, Y. L.; Hobbs, G.; Xu, R. X.; 2015, ApJ, 802, 120 ([http://adsabs.harvard.edu/abs/2015ApJ...802..120D ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Fixing the reference frame for PPMXL proper motions using extragalactic sources&#039;&#039;&lt;br /&gt;
:Grabowski, Kathleen et al.; 2015, RAA, 15, 849 ([http://adsabs.harvard.edu/abs/2015RAA....15..849G ADS])&lt;br /&gt;
&lt;br /&gt;
*Using member galaxy luminosities as halo mass proxies of galaxy groups [http://adsabs.harvard.edu/abs/2015ApJ...804...55L]&lt;br /&gt;
:Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2015ApJ...804...55L&lt;br /&gt;
&lt;br /&gt;
*Capability of Quasar Selection by Combining SCUSS and SDSS Observations [http://adsabs.harvard.edu/abs/2015PASP..127...94Z]&lt;br /&gt;
:Zhou H. et al., 2015,PASP,127,94&lt;br /&gt;
&lt;br /&gt;
*An Investigation of the Absolute Proper Motions of the SCUSS Catalog[http://adsabs.harvard.edu/abs/2015PASP..127..250P]&lt;br /&gt;
:Peng, Xiyan et al., 2015, PASP, 127, 250[]&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1625</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1625"/>
		<updated>2015-08-20T03:08:46Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Red Runaways: Hypervelocity Stars, Hills Ejecta and Other Outliers in the F-M Star Regime&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Grebel, Eva K.; 2015, AJ, 150, 77 ([http://adsabs.harvard.edu/abs/2015arXiv150603153V ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2015 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], [[Media:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf|preprint]])&lt;br /&gt;
&lt;br /&gt;
*Automated Identification of 2612 Late-K and M Dwarfs in the LAMOST Commissioning Data Using Classification Template Fits[http://adsabs.harvard.edu/abs/2015AJ....150...42Z]&lt;br /&gt;
:Zhong, Jing; Lépine, Sébastien; Hou, Jinliang; Shen, Shiyin; Yuan, Haibo; Huo, Zhiying; Zhang, Huihua; Xiang, Maosheng; Zhang, Huawei; Liu, Xiaowei&lt;br /&gt;
&lt;br /&gt;
*An Apparent Redshift Dependence of Quasar Continuum: Implication for Cosmic Dust Extinction? [http://adsabs.harvard.edu/abs/2015ApJ...802L..16X]&lt;br /&gt;
:Xie, Xiaoyi; Shen, Shiyin; Shao, Zhengyi; Yin, Jun, 2015, ApJL, 802,16&lt;br /&gt;
&lt;br /&gt;
*The evolution of interacting spiral galaxy NGC 5194[http://adsabs.harvard.edu/abs/2015MNRAS.449..414K]&lt;br /&gt;
:Kang, Xiaoyu; Chang, Ruixiang; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414&lt;br /&gt;
&lt;br /&gt;
==Coauthors==&lt;br /&gt;
*Using member galaxy luminosities as halo mass proxies of galaxy groups [http://adsabs.harvard.edu/abs/2015ApJ...804...55L]&lt;br /&gt;
:Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2015ApJ...804...55L&lt;br /&gt;
*Capability of Quasar Selection by Combining SCUSS and SDSS Observations [http://adsabs.harvard.edu/abs/2015PASP..127...94Z]&lt;br /&gt;
:Zhou H. et al., 2015,PASP,127,94&lt;br /&gt;
*An Investigation of the Absolute Proper Motions of the SCUSS Catalog[http://adsabs.harvard.edu/abs/2015PASP..127..250P]&lt;br /&gt;
:Peng, Xiyan et al., 2015, PASP, 127, 250[]&lt;br /&gt;
----&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf&amp;diff=1624</id>
		<title>文件:Smith2015Kinematically Detected Halo Streams1-28.pdf</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Smith2015Kinematically_Detected_Halo_Streams1-28.pdf&amp;diff=1624"/>
		<updated>2015-08-20T03:05:31Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​Springer chapter preprint&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Springer chapter preprint&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1623</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1623"/>
		<updated>2015-08-20T03:04:14Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​/* First author */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Red Runaways: Hypervelocity Stars, Hills Ejecta and Other Outliers in the F-M Star Regime&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Grebel, Eva K.; 2015, AJ, 150, 77 ([http://adsabs.harvard.edu/abs/2015arXiv150603153V ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2015 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library ([http://www.springer.com/us/book/9783319193359 webpage], preprint)&lt;br /&gt;
&lt;br /&gt;
*Automated Identification of 2612 Late-K and M Dwarfs in the LAMOST Commissioning Data Using Classification Template Fits[http://adsabs.harvard.edu/abs/2015AJ....150...42Z]&lt;br /&gt;
:Zhong, Jing; Lépine, Sébastien; Hou, Jinliang; Shen, Shiyin; Yuan, Haibo; Huo, Zhiying; Zhang, Huihua; Xiang, Maosheng; Zhang, Huawei; Liu, Xiaowei&lt;br /&gt;
&lt;br /&gt;
*An Apparent Redshift Dependence of Quasar Continuum: Implication for Cosmic Dust Extinction? [http://adsabs.harvard.edu/abs/2015ApJ...802L..16X]&lt;br /&gt;
:Xie, Xiaoyi; Shen, Shiyin; Shao, Zhengyi; Yin, Jun, 2015, ApJL, 802,16&lt;br /&gt;
&lt;br /&gt;
*The evolution of interacting spiral galaxy NGC 5194[http://adsabs.harvard.edu/abs/2015MNRAS.449..414K]&lt;br /&gt;
:Kang, Xiaoyu; Chang, Ruixiang; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414&lt;br /&gt;
&lt;br /&gt;
==Coauthors==&lt;br /&gt;
*Using member galaxy luminosities as halo mass proxies of galaxy groups [http://adsabs.harvard.edu/abs/2015ApJ...804...55L]&lt;br /&gt;
:Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2015ApJ...804...55L&lt;br /&gt;
*Capability of Quasar Selection by Combining SCUSS and SDSS Observations [http://adsabs.harvard.edu/abs/2015PASP..127...94Z]&lt;br /&gt;
:Zhou H. et al., 2015,PASP,127,94&lt;br /&gt;
*An Investigation of the Absolute Proper Motions of the SCUSS Catalog[http://adsabs.harvard.edu/abs/2015PASP..127..250P]&lt;br /&gt;
:Peng, Xiyan et al., 2015, PASP, 127, 250[]&lt;br /&gt;
----&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1622</id>
		<title>Publications</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=Publications&amp;diff=1622"/>
		<updated>2015-08-20T03:03:44Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==First author==&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Red Runaways: Hypervelocity Stars, Hills Ejecta and Other Outliers in the F-M Star Regime&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Vickers, John J.&#039;&#039;&#039;; &#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; Grebel, Eva K.; 2015, AJ, 150, 77 ([http://adsabs.harvard.edu/abs/2015arXiv150603153V ADS])&lt;br /&gt;
&lt;br /&gt;
*&#039;&#039;Kinematically Detected Halo Streams&#039;&#039;&lt;br /&gt;
:&#039;&#039;&#039;Smith, Martin C.&#039;&#039;&#039;; 2015 in Newberg H. J., Carlin J. L. (eds), Tidal Streams in the Local Group and Beyond, vol. 420 of Astrophysics and Space Science Library &lt;br /&gt;
([http://www.springer.com/us/book/9783319193359 webpage], &lt;br /&gt;
(preprint)&lt;br /&gt;
&lt;br /&gt;
*Automated Identification of 2612 Late-K and M Dwarfs in the LAMOST Commissioning Data Using Classification Template Fits[http://adsabs.harvard.edu/abs/2015AJ....150...42Z]&lt;br /&gt;
:Zhong, Jing; Lépine, Sébastien; Hou, Jinliang; Shen, Shiyin; Yuan, Haibo; Huo, Zhiying; Zhang, Huihua; Xiang, Maosheng; Zhang, Huawei; Liu, Xiaowei&lt;br /&gt;
&lt;br /&gt;
*An Apparent Redshift Dependence of Quasar Continuum: Implication for Cosmic Dust Extinction? [http://adsabs.harvard.edu/abs/2015ApJ...802L..16X]&lt;br /&gt;
:Xie, Xiaoyi; Shen, Shiyin; Shao, Zhengyi; Yin, Jun, 2015, ApJL, 802,16&lt;br /&gt;
&lt;br /&gt;
*The evolution of interacting spiral galaxy NGC 5194[http://adsabs.harvard.edu/abs/2015MNRAS.449..414K]&lt;br /&gt;
:Kang, Xiaoyu; Chang, Ruixiang; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414&lt;br /&gt;
&lt;br /&gt;
==Coauthors==&lt;br /&gt;
*Using member galaxy luminosities as halo mass proxies of galaxy groups [http://adsabs.harvard.edu/abs/2015ApJ...804...55L]&lt;br /&gt;
:Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2015ApJ...804...55L&lt;br /&gt;
*Capability of Quasar Selection by Combining SCUSS and SDSS Observations [http://adsabs.harvard.edu/abs/2015PASP..127...94Z]&lt;br /&gt;
:Zhou H. et al., 2015,PASP,127,94&lt;br /&gt;
*An Investigation of the Absolute Proper Motions of the SCUSS Catalog[http://adsabs.harvard.edu/abs/2015PASP..127..250P]&lt;br /&gt;
:Peng, Xiyan et al., 2015, PASP, 127, 250[]&lt;br /&gt;
----&lt;br /&gt;
[[2014 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2013 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2012 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2011 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2010 publications]]&lt;br /&gt;
&lt;br /&gt;
[[2009 publications]]&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1421</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1421"/>
		<updated>2015-05-09T11:54:49Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;11&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| -&lt;br /&gt;
| Professor&lt;br /&gt;
| Group overview&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;7&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Guo-bin Mou&lt;br /&gt;
| Student&lt;br /&gt;
| Feng&lt;br /&gt;
| The Accretion Wind Model of the Fermi Bubbles&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Numerical simulation of hot accretion flow: where can outflow be produced?&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 350&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1420</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1420"/>
		<updated>2015-05-07T12:29:16Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;11&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| -&lt;br /&gt;
| Professor&lt;br /&gt;
| Group overview&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;7&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Guo-bin Mou&lt;br /&gt;
| Student&lt;br /&gt;
| Feng&lt;br /&gt;
| The Accretion Wind Model of the Fermi Bubbles&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 350&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1419</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1419"/>
		<updated>2015-05-07T12:27:33Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;7&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Guo-bin Mou&lt;br /&gt;
| Student&lt;br /&gt;
| Feng&lt;br /&gt;
| The Accretion Wind Model of the Fermi Bubbles&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 350&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1418</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1418"/>
		<updated>2015-05-05T13:32:38Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 350&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1417</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1417"/>
		<updated>2015-05-05T13:29:38Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;9&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Emma Small&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 350&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1416</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1416"/>
		<updated>2015-05-04T15:41:33Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;9&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1415</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1415"/>
		<updated>2015-05-04T15:20:10Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;9&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY FERMI&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1414</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1414"/>
		<updated>2015-05-04T15:14:18Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;9&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY FERMI&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1413</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1413"/>
		<updated>2015-05-04T15:10:19Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;9&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY FERMI&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Liang Chen&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhaoyu Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jinliang Hou&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1397</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1397"/>
		<updated>2015-05-04T02:33:28Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;9&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY FERMI&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Liang Chen&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1363</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1363"/>
		<updated>2015-04-20T16:54:48Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;9&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Morphology and Kinematics of the Peanut/X-shaped Galactic Bulge: Insights from a Self-consistent N-body Model&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY FERMI&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Liang Chen&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yujing Qin&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1362</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1362"/>
		<updated>2015-04-20T15:15:37Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;8&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| Student&lt;br /&gt;
| Lei&lt;br /&gt;
| Feeding and Feedback in Nearby Active Galaxies of VENGA&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY FERMI&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Liang Chen&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Rongxin Luo&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Weizhe Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1361</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1361"/>
		<updated>2015-04-20T08:16:37Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;8&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;5&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY FERMI&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Liang Chen&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
	<entry>
		<id>http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1360</id>
		<title>2015 KIAA-SHAO workshop</title>
		<link rel="alternate" type="text/html" href="http://cluster.shao.ac.cn/wiki/index.php?title=2015_KIAA-SHAO_workshop&amp;diff=1360"/>
		<updated>2015-04-20T08:07:40Z</updated>

		<summary type="html">&lt;p&gt;Msmith：​&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Registration information for KIAA-SHAO 2015 meeting. Website [http://kiaa.pku.edu.cn/kiaashao2015 here].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO speakers&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Topic&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Group&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Position&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Talk Title&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Hotel&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;1&amp;quot;|1. Planetary systems, planets, and exoplanets&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;8&amp;quot;|2. Stars and stellar populations: evolution and dynamics&lt;br /&gt;
&lt;br /&gt;
| Duane M. Lee&lt;br /&gt;
| Jinliang/Martin&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Martin C. Smith&lt;br /&gt;
|Jinliang/Martin&lt;br /&gt;
|Prof.&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Zhao-Yu Li&lt;br /&gt;
|Juntai&lt;br /&gt;
|Assoc. prof.&lt;br /&gt;
|Mapping the &amp;quot;X-shaped Structure&amp;quot; in the Galactic Bulge Bar&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|Yanqiong Zhang&lt;br /&gt;
|Martin&lt;br /&gt;
|Student&lt;br /&gt;
|Finding low-mass Hills stars in Stripe 82&lt;br /&gt;
|Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chien-Cheng Lin&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| The Identification of Be Stars from LAMOST&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Li Lu&lt;br /&gt;
| Li Chen&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| Juntai&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| The study of Milky Way bulge with APOGEE data&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;5&amp;quot;|3. Supermassive black holes and AGNs&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| Student&lt;br /&gt;
| Zhi-qiang Shen&lt;br /&gt;
| Measuring the Hubble Constant, Black hole mass and beyond with H20 Megamasers&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Recent progresses in black hole accretion and jet formation&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xiaoyi Xie&lt;br /&gt;
| Student&lt;br /&gt;
| Zhengyi&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| Feng&lt;br /&gt;
| Photon index (Gamma) and X-ray luminosity correlation in AGNs and black hole X-ray binaries&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Lei&lt;br /&gt;
| Investigating Low Surface Brightness Galaxies using MaNGA IFU Survey&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|4. Large-scale structure, galaxy formation and evolution&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| Postdoc&lt;br /&gt;
| Triggering AGN on isolated galaxy pairs&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Research Assistant&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| Student&lt;br /&gt;
| SPECTRAL PROPERTIES OF GALAXIES IN VOID REGIONS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| CHILI Sciences and Instrumentation -- How Do We Collaborate&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| Shiyin&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhaozhou Li&lt;br /&gt;
| Donghai&lt;br /&gt;
| Student&lt;br /&gt;
| -&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Shiyin Shen&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| The galaxy pairs in LAMOST survey and SDSS&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li &lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| Hydrodynamical simulations of nuclear rings in barred galaxies&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Du Min&lt;br /&gt;
| Juntai&lt;br /&gt;
| Student&lt;br /&gt;
| FORMING DOUBLE-BARRED GALAXIES FROM DYNAMICALLY COOL INNER DISKS&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fangting Yuan&lt;br /&gt;
| Jinliang&lt;br /&gt;
| Assis. research fellow&lt;br /&gt;
| Exploring the star formation properties of mergers using MaNGA data&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|rowspan=&amp;quot;10&amp;quot;|5. High-energy astrophysics and compact objects&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc&lt;br /&gt;
| X-ray Studies of Transient Sources in NGC 55&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| Postdoc. prof.&lt;br /&gt;
| White dwarfs with debris disks&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Defu Bu&lt;br /&gt;
| Feng&lt;br /&gt;
| Assoc. prof.&lt;br /&gt;
| Hot accretion flow around the boundary of an AGN&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Student&lt;br /&gt;
| Predictions for reverberating spectral lines from a newly formed black hole accretion disk: case of tidal disruption flares&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Qi-Xiang Yang &lt;br /&gt;
| Feng&lt;br /&gt;
| Student&lt;br /&gt;
| Correlation between photon index and X-ray luminosity of BHBs &amp;amp; AGNs: observations and interpretation&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenfei Yu &lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| Observational High Energy Astrophysics of Galactic and Extra-galactic X-ray Transients: Group Overview&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Prof.&lt;br /&gt;
| X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| -&lt;br /&gt;
| Prof.&lt;br /&gt;
| -&lt;br /&gt;
| Yes&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Hui Zhang&lt;br /&gt;
| On the episodic jet power in black hole transients&lt;br /&gt;
| Wenfei&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Xing Yi&lt;br /&gt;
| SUPERNOVA REMNANT KESTEVEN 27: INTERACTION WITH A NEIGHBOR HI CLOUD VIEWED BY&lt;br /&gt;
FERMI&lt;br /&gt;
| Zhongxiang&lt;br /&gt;
| Assoc. Research Fellow&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SHAO hotel requests&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;Name&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Arr.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Date of Dept.&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Room (420/396RMB)&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Shared?&#039;&#039;&#039;&lt;br /&gt;
|&#039;&#039;&#039;Notes&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Maria Argudo-Fernandez&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 396&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jianling Gan&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Liang Chen&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhao-Yu Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Jithesh Vadakkumthani&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yes (TBD)&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Wenda Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Feng Gao&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Anestis Tziamtzis&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Lei Hao&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Juntai&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Chenxu Liu&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yingying Zhou&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Min Du&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Min Du&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 420&lt;br /&gt;
| Zhi Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Ramya&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Ramya Sethuram&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Sarah Bird&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Linlin Li&lt;br /&gt;
| 17&lt;br /&gt;
| 20&lt;br /&gt;
| 396&lt;br /&gt;
| Yanqiong Zhang&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhongxiang Wang&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Feng Yuan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| No&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Fu-Guo Xie&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
| Zhen Yan&lt;br /&gt;
| 17&lt;br /&gt;
| 19&lt;br /&gt;
| 420&lt;br /&gt;
| Fu-Guo&lt;br /&gt;
| -&lt;br /&gt;
|-&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Msmith</name></author>
	</entry>
</feed>