http://cluster.shao.ac.cn/wiki/api.php?action=feedcontributions&feedformat=atom&user=Increaselin cluster - 用户贡献 [zh-cn] 2026-05-13T00:52:46Z 用户贡献 MediaWiki 1.38.1 http://cluster.shao.ac.cn/wiki/index.php?title=Photos&diff=2347 Photos 2017-02-22T05:09:15Z <p>Increaselin：​</p> <hr /> <div> 2017.02.22 party<br /> [[file:Party.png|800px]]<br /> <br /> 2016.10.26 seminar<br /> [[file:WechatIMG21.JPG|480px]]<br /> <br /> 2014 seminar <br /> [[file:P1160140.JPG|480px]]<br /> <br /> [[SHAO logo]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Party.png&diff=2346 文件:Party.png 2017-02-22T05:08:28Z <p>Increaselin：​</p> <hr /> <div></div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Photos&diff=2345 Photos 2017-02-22T05:07:58Z <p>Increaselin：​</p> <hr /> <div> 2017.02.22 party<br /> [[file:WechatIMG21.JPG|480px]]<br /> <br /> 2016.10.26 seminar<br /> [[file:WechatIMG21.JPG|480px]]<br /> <br /> 2014 seminar <br /> [[file:P1160140.JPG|480px]]<br /> <br /> [[SHAO logo]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&diff=2280 Lunch talks 2017-01-03T13:00:27Z <p>Increaselin：​</p> <hr /> <div>The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.<br /> <br /> If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:<br /> http://eepurl.com/bomK-9<br /> <br /> == 2016 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 16.01.2017 || TBD (SJTU)|| || <br /> |-<br /> | 19.12.2016 || Chao Liu 刘超 (NAOC)|| [[The stellar density of the Milky Way with LAMOST RGB stars]] || http://doodle.com/poll/75cgz2xv9zitz54z<br /> |-<br /> | 28.11.2016 || Yun Li 李云 (SJTU)|| [[The dynamical evolution of disc-fragmented multiple systems]] || http://doodle.com/poll/74naw9nkumr45bcwwvsx2hrm/admin#table<br /> |-<br /> |}<br /> <br /> == 2016 Spring ==<br /> 11.04.2016 discussion summarized by Martin: <br /> We decided to keep the discussion series going for a few weeks, but we will try and get PhD students to give talks. Unfortunately not many people turned up today - only around 8 people - so we worry that it may not be enough to sustain it. However, let’s see if the new strategy works. We decided to shift to Wednesday morning, because that works better for some people and it’s my time in 701 so I am happy to “donate” it. We also decided to do this every two weeks. Our current plan is to have 1000-1030 at coffee, then 1030-1130 for the talk, then people can go for lunch. <br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 20.04.2016 || Zhen Yuan (SJTU)|| [[A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv<br /> |-<br /> | 04.05.2016 || TBA || TBA || <br /> |-<br /> | 18.05.2016 || TBA || TBA || <br /> |-<br /> | 08.06.2016 || Zhongli Zhang (SHAO) || TBA || <br /> |-<br /> | 15.06.2016 || Shijie Li (SJTU)|| TBA || <br /> |-<br /> | 29.06.2016 || TBA || TBA || <br /> |-<br /> | 13.07.2016 || TBA || TBA || <br /> |}<br /> <br /> == 2015 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||<br /> |-<br /> | 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||<br /> |-<br /> | 05.10.2015<br /> | colspan=&quot;3&quot;| No talk due to National Day vacation<br /> |-<br /> | 12.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || postponed to 26.10 http://doodle.com/poll/dqupmrgby739nztk<br /> |-<br /> | 26.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || http://doodle.com/poll/dqupmrgby739nztks8pq3x56/admin#table<br /> |-<br /> | 09.11.2015 || Fu-Guo Xie (SHAO) || Radio/X-ray correlation in black hole accreting systems || postpone<br /> |-<br /> | 17.11.2015 || Xiaohu Li (NAOC) || Indicators of N2 ultraviolet shielding in AGB stars || Tuesday http://doodle.com/poll/qyebmhgd8d683ev3<br /> |-<br /> | 07.12.2015 || TBA || TBA ||<br /> |-<br /> | 21.12.2015 || TBA || TBA ||<br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2275 Publications 2016-12-30T07:01:25Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==First author==<br /> #''Red Runaways II: Low mass Hills stars in SDSS Stripe 82''<br /> #:'''Zhang, Y.''', '''Smith, M. C.''', Carlin, J.L., 2016, ApJ, in press ([http://adsabs.harvard.edu/abs/2016arXiv160804053Z ADS])<br /> #:<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> #''Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream''<br /> #:'''Li, Jing.'''; '''Smith, Martin C.''' et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])<br /> #:<br /> #''New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars''<br /> #:'''Li, Jing.'''; '''Liu, Chao.''' et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])<br /> <br /> ==Coauthours==<br /> #''The Gaia-ESO survey: Metal-rich bananas in the bulge''<br /> #:Williams, A.A. et al. (including '''Smith, M. C.'''), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])<br /> #: <br /> # ''Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST''<br /> #:Lee, Chien-Hsiu and '''Lin, Chien-Cheng''', 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])<br /> #: <br /> # ''Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE''<br /> #:Tang, Baitian; et al. (including '''Lin, Chien-Cheng'''), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])<br /> #: <br /> # ''A catalog of early-type emission-line stars and Hα line profiles from LAMOST DR2''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2274 Publications 2016-12-30T06:33:34Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==First author==<br /> #''Red Runaways II: Low mass Hills stars in SDSS Stripe 82''<br /> #:'''Zhang, Y.''', '''Smith, M. C.''', Carlin, J.L., 2016, ApJ, in press ([http://adsabs.harvard.edu/abs/2016arXiv160804053Z ADS])<br /> #:<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> #''Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream''<br /> #:'''Li, Jing.'''; '''Smith, Martin C.''' et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])<br /> #:<br /> #''New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars''<br /> #:'''Li, Jing.'''; '''Liu, Chao.''' et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])<br /> <br /> ==Coauthours==<br /> #''The Gaia-ESO survey: Metal-rich bananas in the bulge''<br /> #:Williams, A.A. et al. (including '''Smith, M. C.'''), 2016, ApJL, 824, L29 ([http://adsabs.harvard.edu/abs/2016ApJ...824L..29W ADS])<br /> #: <br /> # ''Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST''<br /> #:Lee, Chien-Hsiu and '''Lin, Chien-Cheng''', 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])<br /> #: <br /> # ''Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE''<br /> #:Tang, Baitian; et al. (including '''Lin, Chien-Cheng'''), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2017MNRAS.465...19T ADS])<br /> #: <br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&diff=2214 Lunch talks 2016-12-12T05:48:33Z <p>Increaselin：​</p> <hr /> <div>The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.<br /> <br /> If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:<br /> http://eepurl.com/bomK-9<br /> <br /> == 2016 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 28.11.2016 || Yun Li 李云 (SJTU)|| [[The dynamical evolution of disc-fragmented multiple systems]] || http://doodle.com/poll/74naw9nkumr45bcwwvsx2hrm/admin#table<br /> |-<br /> | 19.12.2016 || Chao Liu 刘超 (NAOC)|| [[The stellar density of the Milky Way with LAMOST RGB stars]] || http://doodle.com/poll/75cgz2xv9zitz54z<br /> |-<br /> |}<br /> <br /> == 2016 Spring ==<br /> 11.04.2016 discussion summarized by Martin: <br /> We decided to keep the discussion series going for a few weeks, but we will try and get PhD students to give talks. Unfortunately not many people turned up today - only around 8 people - so we worry that it may not be enough to sustain it. However, let’s see if the new strategy works. We decided to shift to Wednesday morning, because that works better for some people and it’s my time in 701 so I am happy to “donate” it. We also decided to do this every two weeks. Our current plan is to have 1000-1030 at coffee, then 1030-1130 for the talk, then people can go for lunch. <br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 20.04.2016 || Zhen Yuan (SJTU)|| [[A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv<br /> |-<br /> | 04.05.2016 || TBA || TBA || <br /> |-<br /> | 18.05.2016 || TBA || TBA || <br /> |-<br /> | 08.06.2016 || Zhongli Zhang (SHAO) || TBA || <br /> |-<br /> | 15.06.2016 || Shijie Li (SJTU)|| TBA || <br /> |-<br /> | 29.06.2016 || TBA || TBA || <br /> |-<br /> | 13.07.2016 || TBA || TBA || <br /> |}<br /> <br /> == 2015 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||<br /> |-<br /> | 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||<br /> |-<br /> | 05.10.2015<br /> | colspan=&quot;3&quot;| No talk due to National Day vacation<br /> |-<br /> | 12.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || postponed to 26.10 http://doodle.com/poll/dqupmrgby739nztk<br /> |-<br /> | 26.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || http://doodle.com/poll/dqupmrgby739nztks8pq3x56/admin#table<br /> |-<br /> | 09.11.2015 || Fu-Guo Xie (SHAO) || Radio/X-ray correlation in black hole accreting systems || postpone<br /> |-<br /> | 17.11.2015 || Xiaohu Li (NAOC) || Indicators of N2 ultraviolet shielding in AGB stars || Tuesday http://doodle.com/poll/qyebmhgd8d683ev3<br /> |-<br /> | 07.12.2015 || TBA || TBA ||<br /> |-<br /> | 21.12.2015 || TBA || TBA ||<br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=The_stellar_density_of_the_Milky_Way_with_LAMOST_RGB_stars&diff=2213 The stellar density of the Milky Way with LAMOST RGB stars 2016-12-12T04:47:29Z <p>Increaselin：​</p> <hr /> <div> Title: The stellar density of the Milky Way with LAMOST RGB stars<br /> <br /> Abstract: <br /> We present a statistical method to derive the stellar density profiles of the Milky Way from spectroscopic survey data taking into account the selection effect. We assume that the selection function of the spectroscopic survey is only in color-magnitude diagram. If no other quantities, e. g., metallicity, proper motion, and age etc., are get involved in the spectroscopic targeting, the underlying selection function can be well recovered by comparing the distribution of the spectroscopic stars in a color-magnitude plane with that of the photometric dataset. Subsequently, the stellar density profile along a line-of-sight can be derived from the spectroscopic stellar density profile multiplied by the selection function. The method is then validated using the Galaxia mock data. We demonstrate that the spectroscopically derived stellar density profiles can well reconstruct the true ones not only for the full targets, but also for the sub-populations selected from the full dataset. Finally, the method is applied to map the density profiles for the Galactic halo and disk, respectively, using the LAMOST RGB stars. The stellar halo is substantially oblate within 20 kpc and become relatively spherical beyond 30 kpc. On the other hand, the Galactic disk is found to extend to beyond 20\,kpc. The perfectly exponential stellar surface density profile smoothly transits to the halo at about 25 kpc without any truncation, bending, or breaking.</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=The_stellar_density_of_the_Milky_Way_with_LAMOST_RGB_stars&diff=2212 The stellar density of the Milky Way with LAMOST RGB stars 2016-12-12T04:46:21Z <p>Increaselin：​Created page with &quot;Title: The stellar density of the Milky Way with LAMOST RGB stars Abstract: We present a statistical method to derive the stellar density profiles of the Milky Way from spectr...&quot;</p> <hr /> <div>Title: The stellar density of the Milky Way with LAMOST RGB stars<br /> Abstract:<br /> We present a statistical method to derive the stellar density profiles of the Milky Way from spectroscopic survey data taking into account the selection effect. We assume that the selection function of the spectroscopic survey is only in color-magnitude diagram. If no other quantities, e. g., metallicity, proper motion, and age etc., are get involved in the spectroscopic targeting, the underlying selection function can be well recovered by comparing the distribution of the spectroscopic stars in a color-magnitude plane with that of the photometric dataset. Subsequently, the stellar density profile along a line-of-sight can be derived from the spectroscopic stellar density profile multiplied by the selection function. The method is then validated using the Galaxia mock data. We demonstrate that the spectroscopically derived stellar density profiles can well reconstruct the true ones not only for the full targets, but also for the sub-populations selected from the full dataset. Finally, the method is applied to map the density profiles for the Galactic halo and disk, respectively, using the LAMOST RGB stars. The stellar halo is substantially oblate within 20 kpc and become relatively spherical beyond 30 kpc. On the other hand, the Galactic disk is found to extend to beyond 20\,kpc. The perfectly exponential stellar surface density profile smoothly transits to the halo at about 25 kpc without any truncation, bending, or breaking.</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&diff=2211 Lunch talks 2016-12-12T04:45:52Z <p>Increaselin：​</p> <hr /> <div>The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.<br /> <br /> If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:<br /> http://eepurl.com/bomK-9<br /> <br /> == 2016 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 28.11.2016 || Yun Li 李云 (SJTU)|| [[The dynamical evolution of disc-fragmented multiple systems]] || http://doodle.com/poll/74naw9nkumr45bcwwvsx2hrm/admin#table<br /> |-<br /> | 19.12.2016 || Chao Liu 刘超 (NAOC)|| [[The stellar density of the Milky Way with LAMOST RGB stars]] || http://doodle.com/<br /> |-<br /> |}<br /> <br /> == 2016 Spring ==<br /> 11.04.2016 discussion summarized by Martin: <br /> We decided to keep the discussion series going for a few weeks, but we will try and get PhD students to give talks. Unfortunately not many people turned up today - only around 8 people - so we worry that it may not be enough to sustain it. However, let’s see if the new strategy works. We decided to shift to Wednesday morning, because that works better for some people and it’s my time in 701 so I am happy to “donate” it. We also decided to do this every two weeks. Our current plan is to have 1000-1030 at coffee, then 1030-1130 for the talk, then people can go for lunch. <br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 20.04.2016 || Zhen Yuan (SJTU)|| [[A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv<br /> |-<br /> | 04.05.2016 || TBA || TBA || <br /> |-<br /> | 18.05.2016 || TBA || TBA || <br /> |-<br /> | 08.06.2016 || Zhongli Zhang (SHAO) || TBA || <br /> |-<br /> | 15.06.2016 || Shijie Li (SJTU)|| TBA || <br /> |-<br /> | 29.06.2016 || TBA || TBA || <br /> |-<br /> | 13.07.2016 || TBA || TBA || <br /> |}<br /> <br /> == 2015 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||<br /> |-<br /> | 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||<br /> |-<br /> | 05.10.2015<br /> | colspan=&quot;3&quot;| No talk due to National Day vacation<br /> |-<br /> | 12.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || postponed to 26.10 http://doodle.com/poll/dqupmrgby739nztk<br /> |-<br /> | 26.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || http://doodle.com/poll/dqupmrgby739nztks8pq3x56/admin#table<br /> |-<br /> | 09.11.2015 || Fu-Guo Xie (SHAO) || Radio/X-ray correlation in black hole accreting systems || postpone<br /> |-<br /> | 17.11.2015 || Xiaohu Li (NAOC) || Indicators of N2 ultraviolet shielding in AGB stars || Tuesday http://doodle.com/poll/qyebmhgd8d683ev3<br /> |-<br /> | 07.12.2015 || TBA || TBA ||<br /> |-<br /> | 21.12.2015 || TBA || TBA ||<br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Postdocs&diff=2203 Postdocs 2016-12-02T08:51:58Z <p>Increaselin：​/* 林建爭 Roger Chien-Cheng Lin */</p> <hr /> <div><br /> <br /> ==林建爭 Roger Chien-Cheng Lin==<br /> [[File:cclinpic2.png|right|250px|Roger]]<br /> <br /> Office: 1517 <br /> <br /> Tel: 5327 <br /> <br /> Email: cclin<br /> <br /> Research Interests: open clusters, low mass stars, kinematic of star clusters, spiral arms.<br /> <br /> Webpage：http://protostar.no-ip.org , http://cluster.shao.ac.cn/~cclin/<br /> <br /> [[Lunch talks]]<br /> <br /> [[star cluster workshop]]<br /> <br /> ==岡本桜子 Sakurako Okamoto==<br /> [[file:sakurako.jpg|right|130px|Sakurako]]<br /> <br /> Office: 1802<br /> <br /> Tel: ----<br /> <br /> Email: okamoto <br /> <br /> Research Interests: Milky Way satellites, dwarf galaxy, optical photometry<br /> <br /> <br /> ==Emma Small==<br /> [[file:Emma.jpg|right|130px|Emma]]<br /> Office: 1513<br /> <br /> Tel: 5360<br /> <br /> Email: emma <br /> <br /> Research Interests: star formation history of nearby galaxies<br /> <br /> <br /> ==John J Vickers==<br /> [[file:johnjvickers.jpg|right|130px|Emma]]<br /> Office: 1802<br /> <br /> Tel: ----<br /> <br /> Email: johnjvickers <br /> <br /> Research Interests: Galactic Archaeology<br /> <br /> <br /> [[Finished Postdocs]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Star_cluster_group&diff=2202 Star cluster group 2016-12-02T08:09:30Z <p>Increaselin：​/* in APGOEE */</p> <hr /> <div>== Discussions ==<br /> === 2016 ===<br /> ==== 2016.12.02 ====<br /> ==== 2016.11.03 ====<br /> === 2015 ===<br /> ==== 2015.11.25 ====<br /> 觀測<br /> ==== 2015.06.30 ====<br /> &lt;i&gt; Zhang: 討論paper &lt;/i&gt;<br /> * Fitting isochrones to open cluster photometric data. A new global optimization tool [http://adsabs.harvard.edu/abs/2010A%26A...516A...2M]<br /> * Shao : 文章大致翻了一下，还没仔细看，感觉CE方法的重点是如何找到最佳“拟合”，与Bayes方法不完全是一个概念。而且CE方法，或者这篇文章最好是有人精读以后讲一下，是不是可以放在明天中午的组内讨论上讲，然后再讨论。另外，我可以简单介绍一下Bayes方法的概念，这样有一个比较，可以看出各自关心的重点和方法上的特点。另外，这篇文章中值得参考的是likelihood和weighting的取法，这个与参数求解过程无关，是可以借鉴的。<br /> <br /> ==== 2015.06.23 ====<br /> &lt;i&gt; Li: 星團 IMF &lt;/i&gt;<br /> * PADOVA isochrone test<br /> <br /> &lt;i&gt; Zhong: M35 Proper Motion &lt;/i&gt;<br /> * PM+Spatial --&gt; high prob. mem. comp. with LAMOST RV. (need phot info. to support the results)<br /> <br /> ==== 2015.06.18 ====<br /> &lt;i&gt; Lin: 跟中央大學談的合作事項。&lt;/i&gt;<br /> <br /> * PTF 在星團中的變星 -- 饒兆聰，楊庭彰 (造父變星、RR Ly) [[Star_cluster_group#variable_stars]]<br /> * NGC752 科學文章 -- 陳文屏 (蒸發、潮汐的成員，動力自行成員、金屬豐度)<br /> * 星團中的 Brown Dwarfs -- 陳文屏<br /> <br /> ==== 2015.06.08 ====<br /> &lt;i&gt; Lin: 說明用密度找PS1星團，分析距離年齡的方法。 &lt;/i&gt;<br /> * 整理出[[star cluster catalog]]以及[[Be star catalog]]。<br /> <br /> &lt;i&gt; Zhong: LAMOST在星團中的觀測還不足。 &lt;/i&gt;<br /> <br /> &lt;i&gt; Li: 學習Chi-square fitting方法。 &lt;/i&gt;<br /> <br /> == Star Clusters ==<br /> === in LAMOST ===<br /> <br /> === in APGOEE ===<br /> https://trac.sdss.org/wiki/APOGEE2#ClusterstarsinAPOGEEpreviouslySpecialTargetsStarClusterCalibration<br /> DR12 APOGEE Total Survey Visits [http://www.sdss.org/]<br /> [[ File:APOGEE DR12 sky coverage nvisits galactic color.png|640px]]<br /> ==== [[SouthOpenClusters]]====<br /> ==== [[NorthOpenClusters]]====<br /> ==== NOTE ====<br /> * DR13 path [https://trac.sdss.org/wiki/APOGEE2/DR13Path]<br /> * The current plan for DR13 is to have a public data release of all of APOGEE-1 data with improvements made since DR12 in July 2016. This public release will not have any APOGEE-2 data.<br /> * ASPCAP =&gt; APOGEE Stellar Parameters and Chemical Abundances Pipeline<br /> * CORE TARGETING PLAN FOR APOGEE-2 [https://trac.sdss.org/wiki/APOGEE2/TargetingPlan]<br /> * https://data.sdss.org/sas/apogeework/apogee/spectro/redux/r6/stars/cal/clust.html<br /> <br /> === in Pan-STARRS ===<br /> *[[ps1-flags]]<br /> <br /> === in 2MASS ===<br /> <br /> === in Kepler ===<br /> <br /> == Catalogs ==<br /> === Star clusters ===<br /> ==== collections ====<br /> 1995-mel95-1756.txt Mermilliod, http://www.univie.ac.at/webda/navigation.html WEBDA Navigation<br /> 1997-har97-0157.txt Harris, VII/202 Globular Clusters in the Milky Way (Harris, 1997)<br /> 2002-dia02-2167.txt Dias, B/ocl Optically visible open clusters and Candidates (Dias+ 2002-2014)<br /> 2003-bia03-0276.txt Bica, J/A+A/397/177 IR star clusters and stellar groups catalog (Bica+, 2003)<br /> 2003-bib03-0167.txt Bica, J/A+A/404/223 2MASS IR star clusters in the Galaxy (Bica+, 2003)<br /> 2003-dut03-0179.txt Dutra, J/A+A/400/533 New infrared star clusters in southern Milky Way (Dutra+, 2003) <br /> 2007-fro07-1021.txt Froebrich, J/MNRAS/374/399 Infrared star clusters with |b|&lt;20° (Froebrich+, 2007)<br /> 2009-glu09-0194.txt Glushkova, V/132 SAI Open Clusters Catalog (Glushkova+, 2009)<br /> 2010-fro10-0269.txt Froebrich, J/MNRAS/409/1281/appena Old star clusters in the FSR catalogue (Froebrich+, 2010)<br /> 2011-buk11-0849.txt Bukowiecki, http://www.home.umk.pl/~gmac/OCS/2mass.html Open Clusters in 2MASS Photometry<br /> 2013-kha13-3006.txt Kharchenko, J/A+A/558/A53 Milky Way global survey of star clusters. II. (Kharchenko+, 2013)<br /> 2014-sch14-0139.txt Schmeja, J/A+A/568/A51 Milky Way global survey of star clusters. III. (Schmeja+, 2014)<br /> ===================================================================================================================================================<br /> 2015-lin15-all.txt 4219 Merge all star cluster catalogs<br /> <br /> === variable stars ===<br /> Star cluster sample from (186) Dias et al. 2002[http://vizier.china-vo.org/viz-bin/VizieR-3?-source=B/ocl&amp;-out.max=20&amp;-out.add=_r&amp;-out.add=_RAJ,_DEJ&amp;-sort=_r] and <br /> (320) Kharchenko et al. 2013. [http://vizier.china-vo.org/viz-bin/VizieR?-source=J/A+A/558/A53&amp;-to=3] with age &gt; 10^9 years and 0 &lt; Dec &lt; 80 deg.<br /> <br /> === Be stars ===<br /> ==== collections ====<br /> 1918-hd1catalog.fits III/135A Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989) 272150 rows<br /> 1995-hd2catalog.fits III/182 HDE Charts: positions, proper motions (Nesterov+ 1995) 88883 rows<br /> =============================================================================================================================================<br /> 1982-jas82-1159.txt III/67A Catalogue of Be stars<br /> 1997-koh97-4174.txt III/205 H-alpha Stars in Northern Milky Way<br /> 2001-yud01-0628.txt J/A+A/368/912 Polarization and rotational velocities of Be stars<br /> 2002-men02-1019.txt J/A+A/393/887 SMC Be stars candidates<br /> 2005-sab05-2446.txt J/MNRAS/361/1055 BVI photometry of LMC Be stars<br /> 2005-zha05-1185.txt J/other/NewA/10.325 2MASS observations of Be stars <br /> 2006-wis06-0530.txt J/ApJ/652/458 BVRHα photometry of candidates Be stars<br /> 2007-nei07-2072.txt http://basebe.obspm.fr/basebe/ The BeSS database contains the complete catalog of CBe stars and Herbig Ae/Be stars<br /> 2007-wis07-0368.txt J/ApJ/671/2040 Polarisation of candidates Be stars<br /> 2009-mcs09-0296.txt J/ApJ/700/1216 Spectroscopy of Be stars in open clusters<br /> 2010-sil10-0069.txt J/ApJS/187/228 Hα profiles of Be stars <br /> 2011-mat11-0150.txt J/other/BASI/39.517 Spectroscopy of classical Be stars<br /> 2012-mar12-0104.txt J/AJ/144/158 Properties of B and Be stars in h and χ Persei<br /> 2012-pau12-0102.txt J/MNRAS/421/3622/stars Candidate Be stars in the Magellanic Clouds<br /> 2013-cat13-0049.txt J/A+A/550/A79/stars Hα and Hβ lines of northern Be stars<br /> 2014-sab14-0213.txt J/PASP/126/219 Southern Galactic Be star candidates<br /> 2015-cho15-0261.txt J/AJ/149/7 SDSS-III/APOGEE. I. Be stars<br /> 2015-lin15-0180.txt 2015arXiv150507290L Searching for Classical Be Stars from the LAMOST DR1 <br /> 2015-rad15-0248.txt J/MNRAS/446/274 A deep catalogue of classical Be stars<br /> 2015-yup15-0058.txt 2015AJ....149...43Y Searching for Be Stars in the Open Cluster NGC 663<br /> =============================================================================================================================================<br /> 2015-lin15-all.txt 11266 Merge all Be star catalogs<br /> <br /> ==== APOGEE1&amp;2 ====<br /> https://trac.sdss.org/wiki/APOGEE2/BeStars<br /> <br /> ==== LAMOST DR1&amp;DR2 ====<br /> Searching for Classical Be Stars in LAMOST DR1 [http://adsabs.harvard.edu/abs/2015arXiv150507290L]<br /> We report on searching for Classical B-type emission-line (CBe) stars <br /> in the first data release of the Large Sky Area Multi-Object fiber <br /> Spectroscopic Telescope (LAMOST; also called the Guo Shou Jing Telescope). <br /> A total of 192 objects (including 12 previously known CBes) were identified as <br /> CBes with prominent He~I~$\lambda4387$, He~I~$\lambda4471$ and <br /> Mg~II~$\lambda4481$ absorption lines, as well as H$\beta$~$\lambda4861$ and <br /> H$\alpha$~$\lambda6563$ emission lines. These candidates significantly <br /> increases the currently known sample of CBes by about 8\%. Most of the CBe <br /> candidates are distributed near the Galactic Anti-Center due to the observing <br /> strategy used for LAMOST. Only two of CBes are in star clusters. These two<br /> CBes have ages of 15.8 and 398~Myr, respectively.<br /> <br /> ==== NGC 6830 ====<br /> REPORTING OF NEWLY DISCOVERED BE STARS IN THE OPEN CLUSTER NGC6830 (in prep.)<br /> ABSTRACT<br /> We discovered 2 new Be stars, and re-identified one known Be star in the open <br /> cluster NGC 6830. Eleven Hα emitters were discovered using the Hα imaging <br /> photometry of the Palomar Transient Factory Survey. Stellar membership of the <br /> candidates was verified with photometric and kinematic information using 2MASS <br /> data and proper motions. The spectroscopic confirmation was carried out by using <br /> the Shane 3-m telescope at Lick observatory. Based on their spectral types, three <br /> Hα emitters were confirmed as Be stars with the Hα equivalent widths &gt; −10A. <br /> Two objects were also observed by the new spectrograph SED-Machine on the <br /> Palomar 60 inch Telescope. The SED-Machine results show strong Hα emission <br /> lines, which are consistent with the results of the Lick observations. The high <br /> efficiency of the SED-Machine can provide rapid observations for Be stars in a <br /> comprehensive survey in the future.<br /> <br /> ==== NGC 663 ====<br /> <br /> SEARCHING FOR Be STARS IN THE OPEN CLUSTER NGC 663[http://adsabs.harvard.edu/abs/2015AJ....149...43Y]<br /> ABSTRACT<br /> We present Be star candidates in the open cluster NGC663, identified by Hα imaging <br /> photometry with the Palomar Transient Factory Survey, as a pilot program to investigate <br /> how the Be star phenomena, the emission spectra, extended circumstellar envelopes, <br /> and fast rotation, correlate with massive stellar evolution. Stellar membership of the <br /> candidates was verified by 2MASS magnitudes and colors and by proper motions (PMs). <br /> We discover four new Be stars and exclude one known Be star from being a member due <br /> to its inconsistent PMs. The fraction of Be stars to member stars [N(Be)/N(members)] in <br /> NGC663 is 3.5%. The spectral type of the 34 Be stars in NGC663 shows bimodal peaks <br /> at B0–B2 and B5–B7, which is consistent with the statistics in most star clusters. <br /> Additionally, we also discover 23 emission-line stars of different types, including <br /> non-member Be stars, dwarfs, and giants.<br /> <br /> === Brown dwarfs ===<br /> [[Candidates in the LAMOST by 王有芬]]<br /> <br /> == Bookmarks ==<br /> <br /> Local Group Astrostatistics Conference http://dept.astro.lsa.umich.edu/lgastrostatistics/<br /> <br /> == Members ==<br /> Chen Li &lt;chenli@shao.ac.cn&gt;<br /> Zhengyi Shao &lt;zyshao@shao.ac.cn&gt;<br /> Zhong Jing &lt;jzhong@shao.ac.cn&gt;<br /> Jinliang Hou &lt;houjl@shao.ac.cn&gt;<br /> Li Lu&lt;lilu@shao.ac.cn&gt;<br /> Li Yang&lt;liyang@shao.ac.cn&gt;<br /> Chaolii Zhang&lt;jackzcl@outlook.com&gt;<br /> <br /> [[Category:Internal]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Star_cluster_group&diff=2200 Star cluster group 2016-12-02T06:50:29Z <p>Increaselin：​</p> <hr /> <div>== Discussions ==<br /> === 2016 ===<br /> ==== 2016.12.02 ====<br /> ==== 2016.11.03 ====<br /> === 2015 ===<br /> ==== 2015.11.25 ====<br /> 觀測<br /> ==== 2015.06.30 ====<br /> &lt;i&gt; Zhang: 討論paper &lt;/i&gt;<br /> * Fitting isochrones to open cluster photometric data. A new global optimization tool [http://adsabs.harvard.edu/abs/2010A%26A...516A...2M]<br /> * Shao : 文章大致翻了一下，还没仔细看，感觉CE方法的重点是如何找到最佳“拟合”，与Bayes方法不完全是一个概念。而且CE方法，或者这篇文章最好是有人精读以后讲一下，是不是可以放在明天中午的组内讨论上讲，然后再讨论。另外，我可以简单介绍一下Bayes方法的概念，这样有一个比较，可以看出各自关心的重点和方法上的特点。另外，这篇文章中值得参考的是likelihood和weighting的取法，这个与参数求解过程无关，是可以借鉴的。<br /> <br /> ==== 2015.06.23 ====<br /> &lt;i&gt; Li: 星團 IMF &lt;/i&gt;<br /> * PADOVA isochrone test<br /> <br /> &lt;i&gt; Zhong: M35 Proper Motion &lt;/i&gt;<br /> * PM+Spatial --&gt; high prob. mem. comp. with LAMOST RV. (need phot info. to support the results)<br /> <br /> ==== 2015.06.18 ====<br /> &lt;i&gt; Lin: 跟中央大學談的合作事項。&lt;/i&gt;<br /> <br /> * PTF 在星團中的變星 -- 饒兆聰，楊庭彰 (造父變星、RR Ly) [[Star_cluster_group#variable_stars]]<br /> * NGC752 科學文章 -- 陳文屏 (蒸發、潮汐的成員，動力自行成員、金屬豐度)<br /> * 星團中的 Brown Dwarfs -- 陳文屏<br /> <br /> ==== 2015.06.08 ====<br /> &lt;i&gt; Lin: 說明用密度找PS1星團，分析距離年齡的方法。 &lt;/i&gt;<br /> * 整理出[[star cluster catalog]]以及[[Be star catalog]]。<br /> <br /> &lt;i&gt; Zhong: LAMOST在星團中的觀測還不足。 &lt;/i&gt;<br /> <br /> &lt;i&gt; Li: 學習Chi-square fitting方法。 &lt;/i&gt;<br /> <br /> == Star Clusters ==<br /> === in LAMOST ===<br /> <br /> === in APGOEE ===<br /> DR12 APOGEE Total Survey Visits [http://www.sdss.org/]<br /> [[ File:APOGEE DR12 sky coverage nvisits galactic color.png|640px]]<br /> ==== [[SouthOpenClusters]]====<br /> ==== [[NorthOpenClusters]]====<br /> ==== NOTE ====<br /> * DR13 path [https://trac.sdss.org/wiki/APOGEE2/DR13Path]<br /> * The current plan for DR13 is to have a public data release of all of APOGEE-1 data with improvements made since DR12 in July 2016. This public release will not have any APOGEE-2 data.<br /> * ASPCAP =&gt; APOGEE Stellar Parameters and Chemical Abundances Pipeline<br /> * CORE TARGETING PLAN FOR APOGEE-2 [https://trac.sdss.org/wiki/APOGEE2/TargetingPlan]<br /> * https://data.sdss.org/sas/apogeework/apogee/spectro/redux/r6/stars/cal/clust.html<br /> <br /> === in Pan-STARRS ===<br /> *[[ps1-flags]]<br /> <br /> === in 2MASS ===<br /> <br /> === in Kepler ===<br /> <br /> == Catalogs ==<br /> === Star clusters ===<br /> ==== collections ====<br /> 1995-mel95-1756.txt Mermilliod, http://www.univie.ac.at/webda/navigation.html WEBDA Navigation<br /> 1997-har97-0157.txt Harris, VII/202 Globular Clusters in the Milky Way (Harris, 1997)<br /> 2002-dia02-2167.txt Dias, B/ocl Optically visible open clusters and Candidates (Dias+ 2002-2014)<br /> 2003-bia03-0276.txt Bica, J/A+A/397/177 IR star clusters and stellar groups catalog (Bica+, 2003)<br /> 2003-bib03-0167.txt Bica, J/A+A/404/223 2MASS IR star clusters in the Galaxy (Bica+, 2003)<br /> 2003-dut03-0179.txt Dutra, J/A+A/400/533 New infrared star clusters in southern Milky Way (Dutra+, 2003) <br /> 2007-fro07-1021.txt Froebrich, J/MNRAS/374/399 Infrared star clusters with |b|&lt;20° (Froebrich+, 2007)<br /> 2009-glu09-0194.txt Glushkova, V/132 SAI Open Clusters Catalog (Glushkova+, 2009)<br /> 2010-fro10-0269.txt Froebrich, J/MNRAS/409/1281/appena Old star clusters in the FSR catalogue (Froebrich+, 2010)<br /> 2011-buk11-0849.txt Bukowiecki, http://www.home.umk.pl/~gmac/OCS/2mass.html Open Clusters in 2MASS Photometry<br /> 2013-kha13-3006.txt Kharchenko, J/A+A/558/A53 Milky Way global survey of star clusters. II. (Kharchenko+, 2013)<br /> 2014-sch14-0139.txt Schmeja, J/A+A/568/A51 Milky Way global survey of star clusters. III. (Schmeja+, 2014)<br /> ===================================================================================================================================================<br /> 2015-lin15-all.txt 4219 Merge all star cluster catalogs<br /> <br /> === variable stars ===<br /> Star cluster sample from (186) Dias et al. 2002[http://vizier.china-vo.org/viz-bin/VizieR-3?-source=B/ocl&amp;-out.max=20&amp;-out.add=_r&amp;-out.add=_RAJ,_DEJ&amp;-sort=_r] and <br /> (320) Kharchenko et al. 2013. [http://vizier.china-vo.org/viz-bin/VizieR?-source=J/A+A/558/A53&amp;-to=3] with age &gt; 10^9 years and 0 &lt; Dec &lt; 80 deg.<br /> <br /> === Be stars ===<br /> ==== collections ====<br /> 1918-hd1catalog.fits III/135A Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989) 272150 rows<br /> 1995-hd2catalog.fits III/182 HDE Charts: positions, proper motions (Nesterov+ 1995) 88883 rows<br /> =============================================================================================================================================<br /> 1982-jas82-1159.txt III/67A Catalogue of Be stars<br /> 1997-koh97-4174.txt III/205 H-alpha Stars in Northern Milky Way<br /> 2001-yud01-0628.txt J/A+A/368/912 Polarization and rotational velocities of Be stars<br /> 2002-men02-1019.txt J/A+A/393/887 SMC Be stars candidates<br /> 2005-sab05-2446.txt J/MNRAS/361/1055 BVI photometry of LMC Be stars<br /> 2005-zha05-1185.txt J/other/NewA/10.325 2MASS observations of Be stars <br /> 2006-wis06-0530.txt J/ApJ/652/458 BVRHα photometry of candidates Be stars<br /> 2007-nei07-2072.txt http://basebe.obspm.fr/basebe/ The BeSS database contains the complete catalog of CBe stars and Herbig Ae/Be stars<br /> 2007-wis07-0368.txt J/ApJ/671/2040 Polarisation of candidates Be stars<br /> 2009-mcs09-0296.txt J/ApJ/700/1216 Spectroscopy of Be stars in open clusters<br /> 2010-sil10-0069.txt J/ApJS/187/228 Hα profiles of Be stars <br /> 2011-mat11-0150.txt J/other/BASI/39.517 Spectroscopy of classical Be stars<br /> 2012-mar12-0104.txt J/AJ/144/158 Properties of B and Be stars in h and χ Persei<br /> 2012-pau12-0102.txt J/MNRAS/421/3622/stars Candidate Be stars in the Magellanic Clouds<br /> 2013-cat13-0049.txt J/A+A/550/A79/stars Hα and Hβ lines of northern Be stars<br /> 2014-sab14-0213.txt J/PASP/126/219 Southern Galactic Be star candidates<br /> 2015-cho15-0261.txt J/AJ/149/7 SDSS-III/APOGEE. I. Be stars<br /> 2015-lin15-0180.txt 2015arXiv150507290L Searching for Classical Be Stars from the LAMOST DR1 <br /> 2015-rad15-0248.txt J/MNRAS/446/274 A deep catalogue of classical Be stars<br /> 2015-yup15-0058.txt 2015AJ....149...43Y Searching for Be Stars in the Open Cluster NGC 663<br /> =============================================================================================================================================<br /> 2015-lin15-all.txt 11266 Merge all Be star catalogs<br /> <br /> ==== APOGEE1&amp;2 ====<br /> https://trac.sdss.org/wiki/APOGEE2/BeStars<br /> <br /> ==== LAMOST DR1&amp;DR2 ====<br /> Searching for Classical Be Stars in LAMOST DR1 [http://adsabs.harvard.edu/abs/2015arXiv150507290L]<br /> We report on searching for Classical B-type emission-line (CBe) stars <br /> in the first data release of the Large Sky Area Multi-Object fiber <br /> Spectroscopic Telescope (LAMOST; also called the Guo Shou Jing Telescope). <br /> A total of 192 objects (including 12 previously known CBes) were identified as <br /> CBes with prominent He~I~$\lambda4387$, He~I~$\lambda4471$ and <br /> Mg~II~$\lambda4481$ absorption lines, as well as H$\beta$~$\lambda4861$ and <br /> H$\alpha$~$\lambda6563$ emission lines. These candidates significantly <br /> increases the currently known sample of CBes by about 8\%. Most of the CBe <br /> candidates are distributed near the Galactic Anti-Center due to the observing <br /> strategy used for LAMOST. Only two of CBes are in star clusters. These two<br /> CBes have ages of 15.8 and 398~Myr, respectively.<br /> <br /> ==== NGC 6830 ====<br /> REPORTING OF NEWLY DISCOVERED BE STARS IN THE OPEN CLUSTER NGC6830 (in prep.)<br /> ABSTRACT<br /> We discovered 2 new Be stars, and re-identified one known Be star in the open <br /> cluster NGC 6830. Eleven Hα emitters were discovered using the Hα imaging <br /> photometry of the Palomar Transient Factory Survey. Stellar membership of the <br /> candidates was verified with photometric and kinematic information using 2MASS <br /> data and proper motions. The spectroscopic confirmation was carried out by using <br /> the Shane 3-m telescope at Lick observatory. Based on their spectral types, three <br /> Hα emitters were confirmed as Be stars with the Hα equivalent widths &gt; −10A. <br /> Two objects were also observed by the new spectrograph SED-Machine on the <br /> Palomar 60 inch Telescope. The SED-Machine results show strong Hα emission <br /> lines, which are consistent with the results of the Lick observations. The high <br /> efficiency of the SED-Machine can provide rapid observations for Be stars in a <br /> comprehensive survey in the future.<br /> <br /> ==== NGC 663 ====<br /> <br /> SEARCHING FOR Be STARS IN THE OPEN CLUSTER NGC 663[http://adsabs.harvard.edu/abs/2015AJ....149...43Y]<br /> ABSTRACT<br /> We present Be star candidates in the open cluster NGC663, identified by Hα imaging <br /> photometry with the Palomar Transient Factory Survey, as a pilot program to investigate <br /> how the Be star phenomena, the emission spectra, extended circumstellar envelopes, <br /> and fast rotation, correlate with massive stellar evolution. Stellar membership of the <br /> candidates was verified by 2MASS magnitudes and colors and by proper motions (PMs). <br /> We discover four new Be stars and exclude one known Be star from being a member due <br /> to its inconsistent PMs. The fraction of Be stars to member stars [N(Be)/N(members)] in <br /> NGC663 is 3.5%. The spectral type of the 34 Be stars in NGC663 shows bimodal peaks <br /> at B0–B2 and B5–B7, which is consistent with the statistics in most star clusters. <br /> Additionally, we also discover 23 emission-line stars of different types, including <br /> non-member Be stars, dwarfs, and giants.<br /> <br /> === Brown dwarfs ===<br /> [[Candidates in the LAMOST by 王有芬]]<br /> <br /> == Bookmarks ==<br /> <br /> Local Group Astrostatistics Conference http://dept.astro.lsa.umich.edu/lgastrostatistics/<br /> <br /> == Members ==<br /> Chen Li &lt;chenli@shao.ac.cn&gt;<br /> Zhengyi Shao &lt;zyshao@shao.ac.cn&gt;<br /> Zhong Jing &lt;jzhong@shao.ac.cn&gt;<br /> Jinliang Hou &lt;houjl@shao.ac.cn&gt;<br /> Li Lu&lt;lilu@shao.ac.cn&gt;<br /> Li Yang&lt;liyang@shao.ac.cn&gt;<br /> Chaolii Zhang&lt;jackzcl@outlook.com&gt;<br /> <br /> [[Category:Internal]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=NorthOpenClusters&diff=2198 NorthOpenClusters 2016-11-30T06:56:10Z <p>Increaselin：​</p> <hr /> <div>https://trac.sdss.org/wiki/APOGEE2/SRDOutstandingIssuesForum/NorthOpenClusters<br /> <br /> Presented are the numbers of star clusters to be found in each of the APOGEE survey plans that have been considered:<br /> <br /> <br /> ||'''Field'''||'''Targeted'''||'''++ in FOV'''||'''-- in FOV'''||'''XX near FOV'''||<br /> <br /> Here are the list of clusters APOGEE would observe with the current plan (12/1/2010)<br /> <br /> The current pointings contain:[[BR]]<br /> * 121 Cluster fully within the FOV<br /> * 54 Clusters partially within the FOV<br /> * 13 Clusters just beyond the edge of the current FOV<br /> <br /> <br /> #<br /> ## APOGEE-2 &quot;Plan&quot; Cluster sample (PMF; 1/11/2014)<br /> ##<br /> ## CLASS: ++: Cluster fully contained in FOV<br /> ## --: Cluster partially contained in FOV<br /> ## **: TARGETED CLUSTER<br /> ##<br /> TOTAL: 1830 fibers<br /> ====================<br /> 10 fibers # 034+00 <br /> 40 fibers # 049+00 <br /> 30 fibers # 064+00 <br /> 30 fibers # 064+06 <br /> 30 fibers # 064+12 <br /> 90 fibers # 079+00 <br /> 10 fibers # 079-06 <br /> 120 fibers # 094+00 <br /> 30 fibers # 094-06 <br /> 100 fibers # 109+00 <br /> 30 fibers # 109+12 <br /> 20 fibers # 109-12 <br /> 180 fibers # 116+00 <br /> 50 fibers # 124+00 <br /> 110 fibers # 131+00 <br /> 10 fibers # 139+00 <br /> 10 fibers # 146+00 <br /> 30 fibers # 146-08 <br /> 10 fibers # 146-12 <br /> 30 fibers # 154+00 <br /> 40 fibers # 161+00 <br /> 40 fibers # 169+00 <br /> 10 fibers # 169-12 <br /> 120 fibers # 176+00 <br /> 130 fibers # 206+00 <br /> 30 fibers # 199+00 <br /> 60 fibers # 191+00 <br /> 40 fibers # 184+00 <br /> 40 fibers # 020+06 <br /> 30 fibers # 025-06 <br /> 90 fibers # 100+00 <br /> 30 fibers # 100-06 <br /> 40 fibers # 120-06 <br /> 20 fibers # 160+06 <br /> 10 fibers # 160-06 <br /> 20 fibers # 180+12 <br /> ??? fibers # 180-12 <br /> 20 fibers # KEPLER <br /> 20 fibers # KEPLER <br /> 30 fibers # KEPLER <br /> 20 fibers # KEPLER <br /> 40 fibers # NGC6838_M71 <br /> #========================================================================================================================================<br /> ## Field l, b CLASS Cluster l,b Cluster Name Clust Diam DCenter(') Log(age) Dist(pc) (m-M)_H RAfld-RAcl DECfld-DECcl<br /> ##<br /> # ---------------- M67 ----------------<br /> 215.0 30.8 ++ 215.40 31.69 Chupina_1 5.00 1.009008 -99.99 0 -inf 0.0180 0.0011 <br /> 215.0 30.8 ++ 215.07 31.92 Chupina_2 2.10 1.174686 -99.99 0 -inf 0.0196 0.0072 <br /> 215.0 30.8 ++ 216.15 31.76 Chupina_3 2.90 1.421117 -99.99 0 -inf 0.0238 -0.0085 <br /> 215.0 30.8 XX 215.16 32.29 Chupina_4 5.00 1.547920 -99.99 0 -inf 0.0262 0.0086 <br /> 215.0 30.8 ++ 216.03 31.42 NGC_2678 10.00 1.128162 -99.99 0 -inf 0.0176 -0.0095 <br /> 215.0 30.8 -- 215.70 31.90 NGC_2682 25.00 1.299594 9.41 908 6.79 0.0231 -0.0015 <br /> # ---------------- 034+00 ----------------<br /> 34.0 0.0 XX 33.03 1.15 FSR_0098 1.80 1.505141 -99.99 0 -inf -0.0256 -0.0059 <br /> 34.0 0.0 ++ 33.11 0.06 Teutsch_146 1.60 0.889445 8.60 3800 9.90 -0.0079 -0.0133 <br /> # ---------------- 049+00 ----------------<br /> 49.0 0.0 ++ 50.20 0.77 Alessi_57 2.50 1.420693 -99.99 3900 9.96 -0.0020 0.0247 <br /> 49.0 0.0 XX 50.04 1.15 Berkeley_45 2.00 1.547339 8.60 2350 8.86 -0.0095 0.0254 <br /> 49.0 0.0 ++ 48.55 -0.18 FSR_0126 6.20 0.488272 -99.99 0 -inf -0.0009 -0.0085 <br /> 49.0 0.0 ++ 49.39 -1.32 FSR_0129 6.20 1.378067 -99.99 0 -inf 0.0243 -0.0049 <br /> 49.0 0.0 ++ 49.17 -0.98 Kronberger_13 1.20 0.993083 8.60 1380 7.70 0.0169 -0.0055 <br /> # ---------------- 064+00 ----------------<br /> 64.0 0.0 ++ 64.10 -1.29 FSR_0165 7.90 1.299373 -99.99 0 -inf 0.0228 -0.0102 <br /> 64.0 0.0 ++ 63.45 0.83 Turner_1 4.00 0.993176 7.46 1675 8.12 -0.0195 -0.0008 <br /> # ---------------- 064+06 ----------------<br /> 64.0 6.0 ++ 63.27 6.64 ASCC_102 21.60 0.970246 8.79 1500 7.88 -0.0183 -0.0060 <br /> # ---------------- 064+12 ----------------<br /> 64.0 12.0 ++ 64.38 12.66 ASCC_100 37.20 0.758308 8.01 350 4.72 -0.0094 0.0106 <br /> # ---------------- 064-12 ----------------<br /> 64.0 -12.0 XX 64.91 -10.74 NGC_6938 7.00 1.541837 -99.99 0 -inf -0.0095 0.0254 <br /> # ---------------- 079+00 ----------------<br /> 79.0 0.0 ++ 80.14 0.74 Bica_1 3.00 1.359120 6.60 1800 8.28 0.0018 0.0237 <br /> 79.0 0.0 -- 80.22 0.79 Bica_2 5.00 1.453801 6.60 1800 8.28 0.0022 0.0253 <br /> 79.0 0.0 ++ 78.48 1.15 Dolidze_10 3.00 1.261785 -99.99 0 -inf -0.0282 0.0044 <br /> 79.0 0.0 ++ 77.63 0.38 FSR_0213 6.40 1.423539 -99.99 0 -inf -0.0252 -0.0155 <br /> 79.0 0.0 ++ 78.47 1.36 FSR_0224 2.00 1.462889 -99.99 0 -inf -0.0323 0.0064 <br /> 79.0 0.0 XX 80.28 0.95 FSR_0236 3.90 1.590448 -99.99 0 -inf -0.0001 0.0278 <br /> 79.0 0.0 ++ 79.35 0.00 Kronberger_59 1.00 0.353337 8.00 780 6.46 0.0047 0.0050 <br /> 79.0 0.0 ++ 78.12 0.30 Roslund_6 24.00 0.927913 8.47 450 5.27 -0.0172 -0.0093 <br /> # ---------------- 079-06 ----------------<br /> 79.0 -6.0 ++ 78.12 -5.24 Dol-Dzim_11 3.00 1.159433 9.30 2545 9.03 -0.0247 -0.0033 <br /> # ---------------- 094+00 ----------------<br /> 94.0 0.0 XX 92.50 -0.28 FSR_0296 3.10 1.525589 -99.99 0 -inf -0.0244 -0.0216 <br /> 94.0 0.0 ++ 93.56 0.67 FSR_0304 8.10 0.802620 -99.99 0 -inf -0.0218 0.0031 <br /> 94.0 0.0 ++ 94.20 0.47 FSR_0306 9.00 0.513207 -99.99 0 -inf -0.0050 0.0084 <br /> 94.0 0.0 ++ 94.25 -0.77 FSR_0307 1.20 0.815510 -99.99 0 -inf 0.0198 -0.0069 <br /> 94.0 0.0 ++ 94.45 -0.74 FSR_0312 2.00 0.871066 -99.99 0 -inf 0.0233 -0.0041 <br /> 94.0 0.0 ++ 92.90 0.59 NGC_7058 7.00 1.249319 8.35 400 5.01 -0.0333 -0.0060 <br /> 94.0 0.0 ++ 94.41 0.22 NGC_7086 12.00 0.462310 8.14 1298 7.57 0.0041 0.0077 <br /> 94.0 0.0 ++ 92.74 0.46 Teutsch_144 8.40 1.339613 8.90 2280 8.79 -0.0339 -0.0095 <br /> # ---------------- 094-06 ----------------<br /> 94.0 -6.0 ++ 94.38 -5.49 IC_5146 20.00 0.632936 6.00 852 6.65 -0.0005 0.0110 <br /> # ---------------- 109+00 ----------------<br /> 109.0 0.0 ++ 108.32 -0.81 FSR_0394 1.90 1.056904 -99.99 0 -inf -0.0092 -0.0178 <br /> 109.0 0.0 ++ 109.40 -0.23 FSR_0401 1.50 0.464211 -99.99 0 -inf 0.0160 -0.0007 <br /> 109.0 0.0 ++ 108.48 -0.40 King_10 4.00 0.652280 7.45 3379 9.64 -0.0102 -0.0101 <br /> 109.0 0.0 XX 110.57 0.14 King_19 5.00 1.576548 8.56 1967 8.47 0.0482 0.0134 <br /> 109.0 0.0 ++ 110.20 0.01 Kronberger_23 2.50 1.203828 8.00 3065 9.43 0.0381 0.0089 <br /> 109.0 0.0 ++ 109.13 1.12 NGC_7419 5.00 1.127696 7.15 2300 8.81 -0.0127 0.0186 <br /> 109.0 0.0 ++ 108.96 0.27 NGC_7429 14.00 0.275513 -99.99 0 -inf -0.0054 0.0040 <br /> 109.0 0.0 ++ 109.99 -0.09 Reiland_1 1.00 0.996735 -99.99 0 -inf 0.0327 0.0058 <br /> 109.0 0.0 ++ 107.90 0.57 Teutsch_54 8.00 1.242279 8.95 2890 9.30 -0.0430 0.0005 <br /> # ---------------- 109+12 ----------------<br /> 109.0 12.0 -- 110.27 11.36 vdBergh_152 25.00 1.398239 -99.99 0 -inf 0.0707 0.0042 <br /> # ---------------- 109-12 ----------------<br /> 109.0 -12.0 ++ 109.51 -11.61 NGC_7686 14.00 0.637050 -99.99 0 -inf 0.0093 0.0093 <br /> # ---------------- 116+00 ----------------<br /> 116.0 0.0 ++ 116.21 0.34 ASCC_130 18.00 0.395204 7.03 3400 9.66 0.0047 0.0065 <br /> 116.0 0.0 XX 116.75 -1.29 Berkeley_58 11.00 1.492965 8.00 3003 9.39 -6.2462 -0.0192 <br /> 116.0 0.0 ++ 115.20 -0.98 FSR_0448 4.90 1.270715 -99.99 0 -inf -0.0199 -0.0200 <br /> 116.0 0.0 ++ 115.67 -1.17 FSR_0451 1.90 1.219312 -99.99 0 -inf -0.0020 -0.0213 <br /> 116.0 0.0 ++ 115.80 1.25 FSR_0453 4.50 1.261852 -99.99 0 -inf -0.0188 0.0203 <br /> 116.0 0.0 ++ 116.56 -0.57 Frolov_1 4.00 0.797157 7.66 2560 9.04 0.0248 -0.0075 <br /> 116.0 0.0 ++ 116.21 -0.35 Harvard_21 3.00 0.409488 -99.99 0 -inf 0.0104 -0.0052 <br /> 116.0 0.0 ++ 116.12 -0.13 King_12 3.00 0.179701 7.04 2378 8.88 0.0056 -0.0017 <br /> 116.0 0.0 ++ 115.95 0.68 King_21 4.00 0.684599 7.16 2103 8.61 -0.0079 0.0114 <br /> 116.0 0.0 ++ 116.32 0.67 Kronberger_55 1.10 0.740078 8.60 1260 7.50 0.0062 0.0126 <br /> 116.0 0.0 ++ 116.43 -0.78 NGC_7788 4.00 0.894181 7.59 2374 8.88 0.0219 -0.0116 <br /> 116.0 0.0 ++ 116.59 -1.01 NGC_7790 5.00 1.167795 7.75 2944 9.34 0.0291 -0.0150 <br /> 116.0 0.0 ++ 115.78 1.24 Negueruela_1 2.00 1.259794 -99.99 2511 9.00 -0.0191 0.0202 <br /> 116.0 0.0 ++ 115.97 0.27 Pfleiderer_4 4.00 0.272122 9.80 7900 11.49 -0.0035 0.0045 <br /> 116.0 0.0 ++ 115.12 0.32 Stock_17 1.00 0.932827 6.78 2144 8.66 -0.0346 0.0017 <br /> 116.0 0.0 ++ 115.79 1.00 Teutsch_23 8.00 1.023139 7.00 2680 9.14 -0.0166 0.0161 <br /> # ---------------- 124+00 ----------------<br /> 124.0 0.0 XX 123.14 -1.29 ASCC_4 48.00 1.552459 8.34 750 6.38 -0.0333 -0.0222 <br /> 124.0 0.0 ++ 123.98 1.10 Berkeley_62 5.00 1.097917 7.20 2320 8.83 0.0009 0.0192 <br /> 124.0 0.0 ++ 124.26 -0.06 Czernik_3 2.40 0.271299 8.00 1410 7.75 0.0100 -0.0012 <br /> 124.0 0.0 ++ 124.54 -0.81 NGC_358 3.00 0.972998 -99.99 0 -inf 0.0191 -0.0145 <br /> 124.0 0.0 ++ 124.68 -0.59 NGC_366 3.50 0.899189 7.41 1785 8.26 0.0246 -0.0109 <br /> 124.0 0.0 XX 124.94 -1.22 NGC_381 6.00 1.541609 8.51 1148 7.30 0.0328 -0.0221 <br /> 124.0 0.0 ++ 125.35 -0.44 Stock_3 5.00 1.421094 -99.99 0 -inf 0.0502 -0.0091 <br /> # ---------------- 131+00 ----------------<br /> 131.0 0.0 ++ 130.10 -0.98 Berkeley_6 8.40 1.329806 7.50 2520 9.01 -0.0407 -0.0126 <br /> 131.0 0.0 ++ 130.14 0.38 Berkeley_7 4.00 0.940590 6.60 2570 9.05 -0.0275 0.0102 <br /> 131.0 0.0 ++ 130.49 -0.60 Czernik_5 1.50 0.786943 8.85 2205 8.72 -0.0236 -0.0079 <br /> 131.0 0.0 ++ 130.89 1.06 Czernik_6 8.00 1.062570 7.00 2700 9.16 0.0065 0.0183 <br /> 131.0 0.0 ++ 131.16 0.52 Czernik_7 10.00 0.547237 8.34 3300 9.59 0.0109 0.0081 <br /> 131.0 0.0 ++ 130.07 -0.19 IC_166 7.00 0.947597 9.00 4800 10.41 -0.0350 0.0008 <br /> 131.0 0.0 ++ 130.05 -0.96 S_1 4.60 1.347254 7.40 2200 8.71 -0.0422 -0.0121 <br /> 131.0 0.0 ++ 131.43 0.62 SAI_16 5.00 0.756610 9.15 7700 11.43 0.0218 0.0084 <br /> # ---------------- 139+00 ----------------<br /> 139.0 0.0 ++ 139.43 0.22 Berkeley_66 4.00 0.485673 9.60 5000 10.49 0.0163 -0.0003 <br /> 139.0 0.0 XX 139.71 -1.34 SAI_25 7.00 1.516786 9.15 2290 8.80 -0.0005 -0.0265 <br /> # ---------------- 146+00 ----------------<br /> 146.0 0.0 ++ 147.07 -0.51 Juchert_11 5.00 1.185439 -99.99 3600 9.78 0.0161 -0.0185 <br /> # ---------------- 146-08 ----------------<br /> 146.0 -8.0 ++ 146.65 -8.93 NGC_1245 40.00 1.129895 9.02 2800 9.24 0.0014 -0.0197 <br /> # ---------------- 146-12 ----------------<br /> 146.0 -12.0 ++ 146.81 -12.16 NGC_1193 3.00 0.811120 9.70 4571 10.30 0.0149 -0.0094 <br /> # ---------------- 154+00 ----------------<br /> 154.0 0.0 ++ 153.36 0.18 NGC_1545 18.00 0.667137 8.45 711 6.26 -0.0088 0.0102 <br /> # ---------------- 161+00 ----------------<br /> 161.0 0.0 ++ 160.13 0.96 FSR_0702 0.40 1.297655 -99.99 0 -inf 0.0046 0.0224 <br /> 161.0 0.0 ++ 161.68 -0.45 NGC_1664 9.00 0.810570 8.46 1199 7.39 0.0022 -0.0141 <br /> 161.0 0.0 ++ 160.34 -0.40 Ruprecht_148 4.00 0.772965 7.72 3028 9.41 -0.0179 0.0044 <br /> # ---------------- 169+00 ----------------<br /> 169.0 0.0 ++ 169.64 0.03 Kronberger_18 4.00 0.645582 8.00 3250 9.56 0.0088 -0.0089 <br /> 169.0 0.0 ++ 168.41 1.26 NGC_1857 10.00 1.392671 -99.99 0 -inf 0.0154 0.0211 <br /> 169.0 0.0 -- 167.69 -0.63 Teutsch_132 5.00 1.458750 6.70 5370 10.65 -0.0286 0.0121 <br /> # ---------------- 169-12 ----------------<br /> 169.0 -12.0 ++ 168.29 -12.29 Czernik_18 5.00 0.753388 -99.99 0 -inf -0.0138 0.0057 <br /> # ---------------- 176+00 ----------------<br /> 176.0 0.0 ++ 176.62 0.89 Berkeley_71 6.20 1.091075 9.00 3260 9.57 0.0225 -0.0009 <br /> 176.0 0.0 ++ 176.49 -0.11 FSR_0807 8.00 0.502354 6.70 1300 7.57 0.0035 -0.0082 <br /> 176.0 0.0 ++ 176.78 0.12 FSR_0812 10.00 0.790473 7.00 3300 9.59 0.0107 -0.0104 <br /> 176.0 0.0 ++ 177.06 -0.41 FSR_0814 2.40 1.138619 -99.99 0 -inf 0.0046 -0.0195 <br /> 176.0 0.0 ++ 177.07 -0.19 FSR_0815 2.80 1.085098 -99.99 0 -inf 0.0085 -0.0175 <br /> 176.0 0.0 ++ 177.10 0.19 FSR_0816 0.80 1.114669 -99.99 0 -inf 0.0154 -0.0144 <br /> 176.0 0.0 ++ 175.56 1.21 Koposov_27 3.00 1.289307 8.65 3700 9.84 0.0163 0.0178 <br /> 176.0 0.0 ++ 177.07 -0.41 Koposov_36 9.00 1.140855 8.35 1700 8.15 0.0048 -0.0195 <br /> 176.0 0.0 ++ 175.56 1.21 Teutsch_1 2.00 1.284101 -99.99 0 -inf 0.0163 0.0178 <br /> # ---------------- 206+00 ----------------<br /> 206.0 0.0 -- 206.94 -1.12 Collinder_104 20.00 1.460576 -99.99 0 -inf -0.0098 -0.0236 <br /> 206.0 0.0 ++ 206.00 -0.46 Collinder_106 35.00 0.462546 9.90 1000 7.00 -0.0072 -0.0038 <br /> 206.0 0.0 -- 207.15 -0.89 Collinder_107 29.00 1.456263 7.00 1738 8.20 -0.0046 -0.0250 <br /> 206.0 0.0 ++ 205.34 0.33 Collinder_111 3.00 0.733890 -99.99 0 -inf -0.0002 0.0128 <br /> 206.0 0.0 ++ 206.25 -1.26 NGC_2252 18.00 1.285086 8.84 900 6.77 -0.0176 -0.0140 <br /> # ---------------- 199+00 ----------------<br /> 199.0 0.0 ++ 198.97 0.54 NGC_2224 20.00 0.544951 -99.99 0 -inf 0.0083 0.0049 <br /> 199.0 0.0 XX 197.65 0.65 Teutsch_11 4.00 1.498055 8.78 5000 10.49 -0.0010 0.0261 <br /> 199.0 0.0 ++ 197.92 0.58 Teutsch_12 6.60 1.225018 8.48 8900 11.75 0.0002 0.0214 <br /> # ---------------- 191+00 ----------------<br /> 191.0 0.0 ++ 190.78 -0.77 FSR_0900 0.60 0.804838 -99.99 0 -inf -0.0145 -0.0032 <br /> 191.0 0.0 ++ 191.01 -0.61 FSR_0903 1.30 0.612456 -99.99 0 -inf -0.0098 -0.0053 <br /> 191.0 0.0 ++ 190.04 0.48 NGC_2175 22.00 1.072020 6.95 1627 8.06 -0.0008 0.0187 <br /> 191.0 0.0 ++ 190.08 0.80 Pismis_27 4.00 1.218369 7.70 1000 7.00 0.0047 0.0208 <br /> # ---------------- 184+00 ----------------<br /> 184.0 0.0 ++ 183.35 -0.57 FSR_0849 0.80 0.862170 -99.99 0 -inf -0.0159 0.0047 <br /> 184.0 0.0 ++ 184.13 -0.41 FSR_0852 8.00 0.430404 9.00 2200 8.71 -0.0055 -0.0056 <br /> 184.0 0.0 ++ 182.74 0.48 Teutsch_51 3.60 1.345515 8.90 3300 9.59 -0.0043 0.0232 <br /> # ---------------- 020+06 ----------------<br /> 20.0 6.0 ++ 19.23 6.76 NGC_6517 4.10 1.083469 10.20 10800 12.17 -0.0183 -0.0054 <br /> 20.0 6.0 ++ 20.80 6.78 NGC_6539 21.46 1.107209 10.20 8400 11.62 -0.0053 0.0186 <br /> # ---------------- 025-06 ----------------<br /> 25.0 -6.0 ++ 25.75 -5.69 NGC_6728 15.60 0.808245 8.93 1000 7.00 0.0009 0.0141 <br /> # ---------------- 100+00 ----------------<br /> 100.0 0.0 ++ 99.49 -0.32 ASCC_116 21.60 0.597460 7.03 5000 10.49 -0.0063 -0.0098 <br /> 100.0 0.0 ++ 99.09 0.96 FSR_0336 9.90 1.323771 -99.99 0 -inf -0.0400 0.0034 <br /> 100.0 0.0 ++ 99.24 0.95 FSR_0338 2.70 1.214311 -99.99 0 -inf -0.0361 0.0049 <br /> 100.0 0.0 ++ 99.72 -0.08 NGC_7175 29.00 0.292696 -99.99 0 -inf -0.0054 -0.0040 <br /> 100.0 0.0 XX 101.40 -0.60 NGC_7226 2.00 1.525987 8.44 2616 9.09 0.0455 0.0061 <br /> # ---------------- 100-06 ----------------<br /> 100.0 -6.0 ++ 98.86 -5.52 NGC_7243 29.00 1.232921 8.06 808 6.54 -0.0329 -0.0040 <br /> # ---------------- 120-06 ----------------<br /> 120.0 -6.0 -- 120.02 -7.48 ASCC_3 25.20 1.477155 7.90 1700 8.15 0.0044 -0.0257 <br /> 120.0 -6.0 ++ 120.13 -4.83 Stock_21 4.00 1.173746 -99.99 1111 7.23 0.0012 0.0205 <br /> # ---------------- 160+06 ----------------<br /> 160.0 6.0 ++ 160.70 4.85 NGC_1798 5.00 1.346572 8.90 4571 10.30 -0.0139 -0.0216 <br /> 160.0 6.0 ++ 158.61 5.69 SAI_43 2.00 1.418982 8.95 3840 9.92 -0.0285 0.0164 <br /> # ---------------- 160-06 ----------------<br /> 160.0 -6.0 ++ 159.31 -6.87 SAI_36 3.00 1.106482 9.10 3000 9.39 -0.0255 -0.0022 <br /> # ---------------- 180+12 ----------------<br /> 180.0 12.0 ++ 179.21 11.85 NGC_2240 11.00 0.785925 9.50 450 5.27 -0.0099 0.0111 <br /> # ---------------- 180-12 ----------------<br /> 180.0 -12.0 XX 179.18 -10.70 NGC_1750 20.00 1.533242 8.30 630 6.00 0.0110 0.0248 <br /> 180.0 -12.0 -- 180.79 -10.86 Platais_4 204.00 1.379630 8.00 276 4.20 0.0260 0.0007 <br /> # ---------------- KEPLER ----------------<br /> 78.8 12.0 ++ 79.21 12.01 NGC_6811 14.00 0.407031 8.80 1215 7.42 0.0034 0.0067 <br /> # ---------------- KEPLER ----------------<br /> 79.7 8.0 ++ 79.56 6.84 NGC_6866 14.00 1.186243 8.58 1450 7.81 0.0232 -0.0124 <br /> # ---------------- KEPLER ----------------<br /> 73.2 8.6 ++ 73.98 8.48 NGC_6819 5.00 0.755281 9.17 2360 8.86 0.0112 0.0100 <br /> 73.2 8.6 ++ 72.72 7.56 Skiff_J1942p38.6 10.00 1.198051 -99.99 0 -inf 0.0160 -0.0168 <br /> # ---------------- KEPLER ----------------<br /> 70.8 10.1 ++ 69.96 10.90 NGC_6791 10.00 1.120527 9.64 5853 10.84 -0.0233 -0.0068 <br /> # ---------------- 000+12 ----------------<br /> 0.0 12.0 ++ 0.13 11.02 NGC_6287 10.51 0.985599 10.20 9300 11.84 0.0164 -0.0082 <br /> # ---------------- M5PAL5 ----------------<br /> 2.3 46.5 ++ 0.85 45.86 Pal_5 16.28 0.972675 10.20 23200 13.83 -0.0035 -0.0166 <br /> 2.3 46.5 ++ 3.86 46.80 NGC_5904 28.40 1.101860 10.20 7500 11.38 0.0073 0.0178 <br /> # ---------------- NGC6838_M71 ----------------<br /> 56.7 -4.6 ++ 56.74 -4.56 NGC_6838 8.96 0.001652 10.20 4000 10.01 -0.0000 -0.0000 <br /> 56.7 -4.6 ++ 56.28 -4.65 Harvard_20 7.00 0.473509 7.48 1540 7.94 -0.0029 -0.0078 <br /> 56.7 -4.6 ++ 56.11 -5.15 NGC_6839 6.00 0.860587 -99.99 0 -inf 0.0034 -0.0147</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=The_dynamical_evolution_of_disc-fragmented_multiple_systems&diff=2190 The dynamical evolution of disc-fragmented multiple systems 2016-11-23T08:10:33Z <p>Increaselin：​Created page with &quot;Title: The dynamical evolution of disc-fragmented multiple systems Abstract: The origin of very low-mass hydrogen-burning stars, brown dwarfs, and planetary-mass objects at...&quot;</p> <hr /> <div>Title: <br /> The dynamical evolution of disc-fragmented multiple systems<br /> <br /> Abstract:<br /> The origin of very low-mass hydrogen-burning stars, brown dwarfs, and planetary-mass objects at the low-mass end of the initial mass function is not yet fully understood. Gravitational fragmentation of circumstellar discs provides a possible mechanism for the formation of such low-mass objects. The multiple systems formed through disc fragmentation are generally dynamical unstable, and I will introduce our computational study of the dynamical evolution of such systems. And this study can help to understand more about the origin of the low-mass objects.</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&diff=2189 Lunch talks 2016-11-23T08:10:10Z <p>Increaselin：​/* 2016 Fall */</p> <hr /> <div>The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.<br /> <br /> If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:<br /> http://eepurl.com/bomK-9<br /> <br /> == 2016 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 28.11.2016 || Yun Li 李云 (SJTU)|| [[The dynamical evolution of disc-fragmented multiple systems]] || http://doodle.com/poll/74naw9nkumr45bcwwvsx2hrm/admin#table<br /> |-<br /> |}<br /> <br /> == 2016 Spring ==<br /> 11.04.2016 discussion summarized by Martin: <br /> We decided to keep the discussion series going for a few weeks, but we will try and get PhD students to give talks. Unfortunately not many people turned up today - only around 8 people - so we worry that it may not be enough to sustain it. However, let’s see if the new strategy works. We decided to shift to Wednesday morning, because that works better for some people and it’s my time in 701 so I am happy to “donate” it. We also decided to do this every two weeks. Our current plan is to have 1000-1030 at coffee, then 1030-1130 for the talk, then people can go for lunch. <br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 20.04.2016 || Zhen Yuan (SJTU)|| [[A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv<br /> |-<br /> | 04.05.2016 || TBA || TBA || <br /> |-<br /> | 18.05.2016 || TBA || TBA || <br /> |-<br /> | 08.06.2016 || Zhongli Zhang (SHAO) || TBA || <br /> |-<br /> | 15.06.2016 || Shijie Li (SJTU)|| TBA || <br /> |-<br /> | 29.06.2016 || TBA || TBA || <br /> |-<br /> | 13.07.2016 || TBA || TBA || <br /> |}<br /> <br /> == 2015 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||<br /> |-<br /> | 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||<br /> |-<br /> | 05.10.2015<br /> | colspan=&quot;3&quot;| No talk due to National Day vacation<br /> |-<br /> | 12.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || postponed to 26.10 http://doodle.com/poll/dqupmrgby739nztk<br /> |-<br /> | 26.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || http://doodle.com/poll/dqupmrgby739nztks8pq3x56/admin#table<br /> |-<br /> | 09.11.2015 || Fu-Guo Xie (SHAO) || Radio/X-ray correlation in black hole accreting systems || postpone<br /> |-<br /> | 17.11.2015 || Xiaohu Li (NAOC) || Indicators of N2 ultraviolet shielding in AGB stars || Tuesday http://doodle.com/poll/qyebmhgd8d683ev3<br /> |-<br /> | 07.12.2015 || TBA || TBA ||<br /> |-<br /> | 21.12.2015 || TBA || TBA ||<br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&diff=2188 Lunch talks 2016-11-23T08:07:30Z <p>Increaselin：​/* 2016 Fall */</p> <hr /> <div>The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.<br /> <br /> If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:<br /> http://eepurl.com/bomK-9<br /> <br /> == 2016 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 28.11.2016 || Yun Li 李云 (SJTU)|| The dynamical evolution of disc-fragmented multiple systems || http://doodle.com/poll/74naw9nkumr45bcwwvsx2hrm/admin#table<br /> |-<br /> |}<br /> <br /> == 2016 Spring ==<br /> 11.04.2016 discussion summarized by Martin: <br /> We decided to keep the discussion series going for a few weeks, but we will try and get PhD students to give talks. Unfortunately not many people turned up today - only around 8 people - so we worry that it may not be enough to sustain it. However, let’s see if the new strategy works. We decided to shift to Wednesday morning, because that works better for some people and it’s my time in 701 so I am happy to “donate” it. We also decided to do this every two weeks. Our current plan is to have 1000-1030 at coffee, then 1030-1130 for the talk, then people can go for lunch. <br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 20.04.2016 || Zhen Yuan (SJTU)|| [[A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv<br /> |-<br /> | 04.05.2016 || TBA || TBA || <br /> |-<br /> | 18.05.2016 || TBA || TBA || <br /> |-<br /> | 08.06.2016 || Zhongli Zhang (SHAO) || TBA || <br /> |-<br /> | 15.06.2016 || Shijie Li (SJTU)|| TBA || <br /> |-<br /> | 29.06.2016 || TBA || TBA || <br /> |-<br /> | 13.07.2016 || TBA || TBA || <br /> |}<br /> <br /> == 2015 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||<br /> |-<br /> | 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||<br /> |-<br /> | 05.10.2015<br /> | colspan=&quot;3&quot;| No talk due to National Day vacation<br /> |-<br /> | 12.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || postponed to 26.10 http://doodle.com/poll/dqupmrgby739nztk<br /> |-<br /> | 26.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || http://doodle.com/poll/dqupmrgby739nztks8pq3x56/admin#table<br /> |-<br /> | 09.11.2015 || Fu-Guo Xie (SHAO) || Radio/X-ray correlation in black hole accreting systems || postpone<br /> |-<br /> | 17.11.2015 || Xiaohu Li (NAOC) || Indicators of N2 ultraviolet shielding in AGB stars || Tuesday http://doodle.com/poll/qyebmhgd8d683ev3<br /> |-<br /> | 07.12.2015 || TBA || TBA ||<br /> |-<br /> | 21.12.2015 || TBA || TBA ||<br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Seminar_Plan&diff=2186 Seminar Plan 2016-11-17T03:17:33Z <p>Increaselin：​</p> <hr /> <div>{| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title<br /> |-<br /> |2016.11.17 || Shiyin Shen || https://arxiv.org/abs/1611.01753<br /> |-<br /> |2016.11.09 || Jian Fu ?|| <br /> |-<br /> |2016.11.02 || 年會 || <br /> |-<br /> |2016.10.26 || Lin, Chien-Cheng || [[Media:20161026.pdf|Observing Proposals]]<br /> |-<br /> |2016.10.19 || Feng, Shuai || Merging Galaxies?<br /> |-<br /> |2016.10.12 || Students || Thesis opening/progress reports 李林林，张燕琼，居梦婷，李露，杨丽，郑云亮<br /> |-<br /> |2016.08.31 || Ju, Mengting || [[Media:Ju20160831.pdf|光谱简单处理 spectral analysis ]]<br /> |-<br /> |2016.08.17 || Zheng, Yunliang || [[Media:CG_part1.pdf|Compact Groups in Main Galaxy Sample(DR7 data products)]] <br /> |-<br /> |2016.08.10 || Yang, Li || [[Media:20160810.pdf|Data Reduction of Spectroscopy with IRAF]] <br /> |-<br /> |2016.07.27 || Li, Lu || A new method to study the properties of open clusters<br /> |-<br /> |2016.07.20 || Zhang, Chaoli || An introduction to [[MCMC]]<br /> |-<br /> |2016.03.02 || Lin, Chien-Cheng || [[Media:20160302.pdf|Updates on Searching for Be Stars in LAMOST data]]<br /> |-<br /> |2016.01.27 || Liu, Cheng||The nature of stars with common origin: clues from metallicity, elemental abundances, and kinematics<br /> |-<br /> |}<br /> <br /> <br /> ----<br /> <br /> [[Seminar Plan(2014-2015)]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&diff=2185 Lunch talks 2016-11-17T02:32:09Z <p>Increaselin：​</p> <hr /> <div>The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.<br /> <br /> If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:<br /> http://eepurl.com/bomK-9<br /> <br /> == 2016 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 28.11.2016 || Yun Li 李云 (SJTU)|| TBA || mail<br /> |-<br /> |}<br /> <br /> == 2016 Spring ==<br /> 11.04.2016 discussion summarized by Martin: <br /> We decided to keep the discussion series going for a few weeks, but we will try and get PhD students to give talks. Unfortunately not many people turned up today - only around 8 people - so we worry that it may not be enough to sustain it. However, let’s see if the new strategy works. We decided to shift to Wednesday morning, because that works better for some people and it’s my time in 701 so I am happy to “donate” it. We also decided to do this every two weeks. Our current plan is to have 1000-1030 at coffee, then 1030-1130 for the talk, then people can go for lunch. <br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 20.04.2016 || Zhen Yuan (SJTU)|| [[A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv<br /> |-<br /> | 04.05.2016 || TBA || TBA || <br /> |-<br /> | 18.05.2016 || TBA || TBA || <br /> |-<br /> | 08.06.2016 || Zhongli Zhang (SHAO) || TBA || <br /> |-<br /> | 15.06.2016 || Shijie Li (SJTU)|| TBA || <br /> |-<br /> | 29.06.2016 || TBA || TBA || <br /> |-<br /> | 13.07.2016 || TBA || TBA || <br /> |}<br /> <br /> == 2015 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||<br /> |-<br /> | 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||<br /> |-<br /> | 05.10.2015<br /> | colspan=&quot;3&quot;| No talk due to National Day vacation<br /> |-<br /> | 12.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || postponed to 26.10 http://doodle.com/poll/dqupmrgby739nztk<br /> |-<br /> | 26.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || http://doodle.com/poll/dqupmrgby739nztks8pq3x56/admin#table<br /> |-<br /> | 09.11.2015 || Fu-Guo Xie (SHAO) || Radio/X-ray correlation in black hole accreting systems || postpone<br /> |-<br /> | 17.11.2015 || Xiaohu Li (NAOC) || Indicators of N2 ultraviolet shielding in AGB stars || Tuesday http://doodle.com/poll/qyebmhgd8d683ev3<br /> |-<br /> | 07.12.2015 || TBA || TBA ||<br /> |-<br /> | 21.12.2015 || TBA || TBA ||<br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Star_cluster_group&diff=2176 Star cluster group 2016-11-03T03:06:53Z <p>Increaselin：​</p> <hr /> <div>== Discussions ==<br /> === 2016 ===<br /> ==== 2016.11.03 ====<br /> === 2015 ===<br /> ==== 2015.11.25 ====<br /> 觀測<br /> ==== 2015.06.30 ====<br /> &lt;i&gt; Zhang: 討論paper &lt;/i&gt;<br /> * Fitting isochrones to open cluster photometric data. A new global optimization tool [http://adsabs.harvard.edu/abs/2010A%26A...516A...2M]<br /> * Shao : 文章大致翻了一下，还没仔细看，感觉CE方法的重点是如何找到最佳“拟合”，与Bayes方法不完全是一个概念。而且CE方法，或者这篇文章最好是有人精读以后讲一下，是不是可以放在明天中午的组内讨论上讲，然后再讨论。另外，我可以简单介绍一下Bayes方法的概念，这样有一个比较，可以看出各自关心的重点和方法上的特点。另外，这篇文章中值得参考的是likelihood和weighting的取法，这个与参数求解过程无关，是可以借鉴的。<br /> <br /> ==== 2015.06.23 ====<br /> &lt;i&gt; Li: 星團 IMF &lt;/i&gt;<br /> * PADOVA isochrone test<br /> <br /> &lt;i&gt; Zhong: M35 Proper Motion &lt;/i&gt;<br /> * PM+Spatial --&gt; high prob. mem. comp. with LAMOST RV. (need phot info. to support the results)<br /> <br /> ==== 2015.06.18 ====<br /> &lt;i&gt; Lin: 跟中央大學談的合作事項。&lt;/i&gt;<br /> <br /> * PTF 在星團中的變星 -- 饒兆聰，楊庭彰 (造父變星、RR Ly) [[Star_cluster_group#variable_stars]]<br /> * NGC752 科學文章 -- 陳文屏 (蒸發、潮汐的成員，動力自行成員、金屬豐度)<br /> * 星團中的 Brown Dwarfs -- 陳文屏<br /> <br /> ==== 2015.06.08 ====<br /> &lt;i&gt; Lin: 說明用密度找PS1星團，分析距離年齡的方法。 &lt;/i&gt;<br /> * 整理出[[star cluster catalog]]以及[[Be star catalog]]。<br /> <br /> &lt;i&gt; Zhong: LAMOST在星團中的觀測還不足。 &lt;/i&gt;<br /> <br /> &lt;i&gt; Li: 學習Chi-square fitting方法。 &lt;/i&gt;<br /> <br /> == Star Clusters ==<br /> === in LAMOST ===<br /> <br /> === in APGOEE ===<br /> DR12 APOGEE Total Survey Visits [http://www.sdss.org/]<br /> [[ File:APOGEE DR12 sky coverage nvisits galactic color.png|640px]]<br /> ==== [[SouthOpenClusters]]====<br /> ==== [[NorthOpenClusters]]====<br /> ==== NOTE ====<br /> * DR13 path [https://trac.sdss.org/wiki/APOGEE2/DR13Path]<br /> * The current plan for DR13 is to have a public data release of all of APOGEE-1 data with improvements made since DR12 in July 2016. This public release will not have any APOGEE-2 data.<br /> * ASPCAP =&gt; APOGEE Stellar Parameters and Chemical Abundances Pipeline<br /> * CORE TARGETING PLAN FOR APOGEE-2 [https://trac.sdss.org/wiki/APOGEE2/TargetingPlan]<br /> * https://data.sdss.org/sas/apogeework/apogee/spectro/redux/r6/stars/cal/clust.html<br /> <br /> === in Pan-STARRS ===<br /> *[[ps1-flags]]<br /> <br /> === in 2MASS ===<br /> <br /> === in Kepler ===<br /> <br /> == Catalogs ==<br /> === Star clusters ===<br /> ==== collections ====<br /> 1995-mel95-1756.txt Mermilliod, http://www.univie.ac.at/webda/navigation.html WEBDA Navigation<br /> 1997-har97-0157.txt Harris, VII/202 Globular Clusters in the Milky Way (Harris, 1997)<br /> 2002-dia02-2167.txt Dias, B/ocl Optically visible open clusters and Candidates (Dias+ 2002-2014)<br /> 2003-bia03-0276.txt Bica, J/A+A/397/177 IR star clusters and stellar groups catalog (Bica+, 2003)<br /> 2003-bib03-0167.txt Bica, J/A+A/404/223 2MASS IR star clusters in the Galaxy (Bica+, 2003)<br /> 2003-dut03-0179.txt Dutra, J/A+A/400/533 New infrared star clusters in southern Milky Way (Dutra+, 2003) <br /> 2007-fro07-1021.txt Froebrich, J/MNRAS/374/399 Infrared star clusters with |b|&lt;20° (Froebrich+, 2007)<br /> 2009-glu09-0194.txt Glushkova, V/132 SAI Open Clusters Catalog (Glushkova+, 2009)<br /> 2010-fro10-0269.txt Froebrich, J/MNRAS/409/1281/appena Old star clusters in the FSR catalogue (Froebrich+, 2010)<br /> 2011-buk11-0849.txt Bukowiecki, http://www.home.umk.pl/~gmac/OCS/2mass.html Open Clusters in 2MASS Photometry<br /> 2013-kha13-3006.txt Kharchenko, J/A+A/558/A53 Milky Way global survey of star clusters. II. (Kharchenko+, 2013)<br /> 2014-sch14-0139.txt Schmeja, J/A+A/568/A51 Milky Way global survey of star clusters. III. (Schmeja+, 2014)<br /> ===================================================================================================================================================<br /> 2015-lin15-all.txt 4219 Merge all star cluster catalogs<br /> <br /> === variable stars ===<br /> Star cluster sample from (186) Dias et al. 2002[http://vizier.china-vo.org/viz-bin/VizieR-3?-source=B/ocl&amp;-out.max=20&amp;-out.add=_r&amp;-out.add=_RAJ,_DEJ&amp;-sort=_r] and <br /> (320) Kharchenko et al. 2013. [http://vizier.china-vo.org/viz-bin/VizieR?-source=J/A+A/558/A53&amp;-to=3] with age &gt; 10^9 years and 0 &lt; Dec &lt; 80 deg.<br /> <br /> === Be stars ===<br /> ==== collections ====<br /> 1918-hd1catalog.fits III/135A Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989) 272150 rows<br /> 1995-hd2catalog.fits III/182 HDE Charts: positions, proper motions (Nesterov+ 1995) 88883 rows<br /> =============================================================================================================================================<br /> 1982-jas82-1159.txt III/67A Catalogue of Be stars<br /> 1997-koh97-4174.txt III/205 H-alpha Stars in Northern Milky Way<br /> 2001-yud01-0628.txt J/A+A/368/912 Polarization and rotational velocities of Be stars<br /> 2002-men02-1019.txt J/A+A/393/887 SMC Be stars candidates<br /> 2005-sab05-2446.txt J/MNRAS/361/1055 BVI photometry of LMC Be stars<br /> 2005-zha05-1185.txt J/other/NewA/10.325 2MASS observations of Be stars <br /> 2006-wis06-0530.txt J/ApJ/652/458 BVRHα photometry of candidates Be stars<br /> 2007-nei07-2072.txt http://basebe.obspm.fr/basebe/ The BeSS database contains the complete catalog of CBe stars and Herbig Ae/Be stars<br /> 2007-wis07-0368.txt J/ApJ/671/2040 Polarisation of candidates Be stars<br /> 2009-mcs09-0296.txt J/ApJ/700/1216 Spectroscopy of Be stars in open clusters<br /> 2010-sil10-0069.txt J/ApJS/187/228 Hα profiles of Be stars <br /> 2011-mat11-0150.txt J/other/BASI/39.517 Spectroscopy of classical Be stars<br /> 2012-mar12-0104.txt J/AJ/144/158 Properties of B and Be stars in h and χ Persei<br /> 2012-pau12-0102.txt J/MNRAS/421/3622/stars Candidate Be stars in the Magellanic Clouds<br /> 2013-cat13-0049.txt J/A+A/550/A79/stars Hα and Hβ lines of northern Be stars<br /> 2014-sab14-0213.txt J/PASP/126/219 Southern Galactic Be star candidates<br /> 2015-cho15-0261.txt J/AJ/149/7 SDSS-III/APOGEE. I. Be stars<br /> 2015-lin15-0180.txt 2015arXiv150507290L Searching for Classical Be Stars from the LAMOST DR1 <br /> 2015-rad15-0248.txt J/MNRAS/446/274 A deep catalogue of classical Be stars<br /> 2015-yup15-0058.txt 2015AJ....149...43Y Searching for Be Stars in the Open Cluster NGC 663<br /> =============================================================================================================================================<br /> 2015-lin15-all.txt 11266 Merge all Be star catalogs<br /> <br /> ==== APOGEE1&amp;2 ====<br /> https://trac.sdss.org/wiki/APOGEE2/BeStars<br /> <br /> ==== LAMOST DR1&amp;DR2 ====<br /> Searching for Classical Be Stars in LAMOST DR1 [http://adsabs.harvard.edu/abs/2015arXiv150507290L]<br /> We report on searching for Classical B-type emission-line (CBe) stars <br /> in the first data release of the Large Sky Area Multi-Object fiber <br /> Spectroscopic Telescope (LAMOST; also called the Guo Shou Jing Telescope). <br /> A total of 192 objects (including 12 previously known CBes) were identified as <br /> CBes with prominent He~I~$\lambda4387$, He~I~$\lambda4471$ and <br /> Mg~II~$\lambda4481$ absorption lines, as well as H$\beta$~$\lambda4861$ and <br /> H$\alpha$~$\lambda6563$ emission lines. These candidates significantly <br /> increases the currently known sample of CBes by about 8\%. Most of the CBe <br /> candidates are distributed near the Galactic Anti-Center due to the observing <br /> strategy used for LAMOST. Only two of CBes are in star clusters. These two<br /> CBes have ages of 15.8 and 398~Myr, respectively.<br /> <br /> ==== NGC 6830 ====<br /> REPORTING OF NEWLY DISCOVERED BE STARS IN THE OPEN CLUSTER NGC6830 (in prep.)<br /> ABSTRACT<br /> We discovered 2 new Be stars, and re-identified one known Be star in the open <br /> cluster NGC 6830. Eleven Hα emitters were discovered using the Hα imaging <br /> photometry of the Palomar Transient Factory Survey. Stellar membership of the <br /> candidates was verified with photometric and kinematic information using 2MASS <br /> data and proper motions. The spectroscopic confirmation was carried out by using <br /> the Shane 3-m telescope at Lick observatory. Based on their spectral types, three <br /> Hα emitters were confirmed as Be stars with the Hα equivalent widths &gt; −10A. <br /> Two objects were also observed by the new spectrograph SED-Machine on the <br /> Palomar 60 inch Telescope. The SED-Machine results show strong Hα emission <br /> lines, which are consistent with the results of the Lick observations. The high <br /> efficiency of the SED-Machine can provide rapid observations for Be stars in a <br /> comprehensive survey in the future.<br /> <br /> ==== NGC 663 ====<br /> <br /> SEARCHING FOR Be STARS IN THE OPEN CLUSTER NGC 663[http://adsabs.harvard.edu/abs/2015AJ....149...43Y]<br /> ABSTRACT<br /> We present Be star candidates in the open cluster NGC663, identified by Hα imaging <br /> photometry with the Palomar Transient Factory Survey, as a pilot program to investigate <br /> how the Be star phenomena, the emission spectra, extended circumstellar envelopes, <br /> and fast rotation, correlate with massive stellar evolution. Stellar membership of the <br /> candidates was verified by 2MASS magnitudes and colors and by proper motions (PMs). <br /> We discover four new Be stars and exclude one known Be star from being a member due <br /> to its inconsistent PMs. The fraction of Be stars to member stars [N(Be)/N(members)] in <br /> NGC663 is 3.5%. The spectral type of the 34 Be stars in NGC663 shows bimodal peaks <br /> at B0–B2 and B5–B7, which is consistent with the statistics in most star clusters. <br /> Additionally, we also discover 23 emission-line stars of different types, including <br /> non-member Be stars, dwarfs, and giants.<br /> <br /> === Brown dwarfs ===<br /> [[Candidates in the LAMOST by 王有芬]]<br /> <br /> == Bookmarks ==<br /> <br /> Local Group Astrostatistics Conference http://dept.astro.lsa.umich.edu/lgastrostatistics/<br /> <br /> == Members ==<br /> Chen Li &lt;chenli@shao.ac.cn&gt;<br /> Zhengyi Shao &lt;zyshao@shao.ac.cn&gt;<br /> Zhong Jing &lt;jzhong@shao.ac.cn&gt;<br /> Jinliang Hou &lt;houjl@shao.ac.cn&gt;<br /> Li Lu&lt;lilu@shao.ac.cn&gt;<br /> Li Yang&lt;liyang@shao.ac.cn&gt;<br /> Chaolii Zhang&lt;jackzcl@outlook.com&gt;<br /> <br /> [[Category:Internal]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2173 Publications 2016-11-01T12:43:47Z <p>Increaselin：​/* Firs author */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P18 ([[Media:Twj-cclin.pdf|PDF]])<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> #''Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream''<br /> #:'''Li, Jing.'''; '''Smith, Martin C.''' et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])<br /> #:<br /> #''New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars''<br /> #:'''Li, Jing.'''; '''Liu, Chao.''' et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])<br /> <br /> ==Coauthours==<br /> # ''Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST''<br /> #:Lee, Chien-Hsiu and '''Lin, Chien-Cheng''', 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])<br /> #: <br /> # ''Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE''<br /> #:Tang, Baitian; et al. (including '''Lin, Chien-Cheng'''), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2016arXiv161006763T ADS])<br /> #: <br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Twj-cclin.pdf&diff=2172 文件:Twj-cclin.pdf 2016-11-01T12:42:34Z <p>Increaselin：​</p> <hr /> <div></div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2171 Publications 2016-11-01T12:41:00Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P 18<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> #''Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream''<br /> #:'''Li, Jing.'''; '''Smith, Martin C.''' et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])<br /> #:<br /> #''New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars''<br /> #:'''Li, Jing.'''; '''Liu, Chao.''' et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])<br /> <br /> ==Coauthours==<br /> # ''Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST''<br /> #:Lee, Chien-Hsiu and '''Lin, Chien-Cheng''', 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])<br /> #: <br /> # ''Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE''<br /> #:Tang, Baitian; et al. (including '''Lin, Chien-Cheng'''), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2016arXiv161006763T ADS])<br /> #: <br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016RAA....16..138H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2170 Publications 2016-11-01T12:40:18Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P 18<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> #''Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream''<br /> #:'''Li, Jing.'''; '''Smith, Martin C.''' et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])<br /> #:<br /> #''New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars''<br /> #:'''Li, Jing.'''; '''Liu, Chao.''' et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])<br /> <br /> ==Coauthours==<br /> # ''Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST''<br /> #:Lee, Chien-Hsiu and '''Lin, Chien-Cheng''', 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])<br /> #: <br /> # ''Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE''<br /> #:Tang, Baitian; et al. (including '''Lin, Chien-Cheng'''), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2016arXiv161006763T ADS])<br /> #: <br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, 16, 006 ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2169 Publications 2016-11-01T12:38:49Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P 18<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> #''Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream''<br /> #:'''Li, Jing.'''; '''Smith, Martin C.''' et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])<br /> #:<br /> #''New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars''<br /> #:'''Li, Jing.'''; '''Liu, Chao.''' et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])<br /> <br /> ==Coauthours==<br /> # ''Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST''<br /> #:Lee, Chien-Hsiu and '''Lin, Chien-Cheng''', 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])<br /> #: <br /> # ''Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE''<br /> #:Tang, Baitian; et al. (including '''Lin, Chien-Cheng'''), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2016arXiv161006763T ADS])<br /> #: <br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, accepted ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2168 Publications 2016-11-01T12:38:35Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P 18<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> #''Selecting M Giants with Infrared Photometry: Distances, Metallicities, and the Sagittarius Stream''<br /> #:'''Li, Jing.'''; '''Smith, Martin C.''' et al. 2016, ApJ, 823, 59,([http://adsabs.harvard.edu/abs/2016ApJ...823...59L ADS])<br /> #:<br /> #''New tidal debris nearby the Sagittarius leading tail from the LAMOST DR2 M giant stars''<br /> #:'''Li, Jing.'''; '''Liu, Chao.''' et al. 2016, RAA, 16h, 8L,([http://adsabs.harvard.edu/abs/2016RAA....16h...8L ADS])<br /> <br /> ==Coauthours==<br /> # ''Double-lined M-dwarf Eclipsing Binaries from Catalina Sky Survey and LAMOST''<br /> #:Lee, Chien-Hsiu and '''Lin, Chien-Cheng'''), 2016, RAA, accepted ([http://www.raa-journal.org/docs/papers_accepted/0190.pdf PDF])<br /> #: <br /> # ''Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE''<br /> #:Tang, Baitian; et al. (including '''Lin, Chien-Cheng'''), 2016, MNRAS, accepted ([http://adsabs.harvard.edu/abs/2016arXiv161006763T ADS])<br /> #: <br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, accepted ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Photos&diff=2155 Photos 2016-10-26T06:51:11Z <p>Increaselin：​</p> <hr /> <div> 2016.10.26 seminar<br /> [[file:WechatIMG21.JPG|480px]]<br /> <br /> 2014 seminar <br /> [[file:P1160140.JPG|480px]]<br /> <br /> [[SHAO logo]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Photos&diff=2154 Photos 2016-10-26T06:50:55Z <p>Increaselin：​</p> <hr /> <div> 2016.10.26 seminar<br /> [[file:WechatIMG21.JPG|480px]]<br /> <br /> 2014 seminar <br /> [[file:P1160140.JPG|480px]]<br /> <br /> [[SHAO logo]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:WechatIMG21.JPG&diff=2153 文件:WechatIMG21.JPG 2016-10-26T06:50:15Z <p>Increaselin：​</p> <hr /> <div></div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Photos&diff=2152 Photos 2016-10-26T06:49:42Z <p>Increaselin：​</p> <hr /> <div>2016.10.26 seminar<br /> [[file:WechatIMG21.JPG|480px]]<br /> <br /> [[file:P1160140.JPG|480px]]<br /> <br /> [[SHAO logo]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Seminar_Plan&diff=2151 Seminar Plan 2016-10-26T06:03:02Z <p>Increaselin：​</p> <hr /> <div>{| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title<br /> |-<br /> |-<br /> |2016.10.26 || Lin, Chien-Cheng || [[Media:20161026.pdf|Observing Proposals]]<br /> |-<br /> |2016.10.19 || Feng, Shuai || Merging Galaxies?<br /> |-<br /> |2016.10.12 || Students || Thesis opening/progress reports 李林林，张燕琼，居梦婷，李露，杨丽，郑云亮<br /> |-<br /> |2016.08.31 || Ju, Mengting || [[Media:Ju20160831.pdf|光谱简单处理 spectral analysis ]]<br /> |-<br /> |2016.08.17 || Zheng, Yunliang || [[Media:CG_part1.pdf|Compact Groups in Main Galaxy Sample(DR7 data products)]] <br /> |-<br /> |2016.08.10 || Yang, Li || [[Media:20160810.pdf|Data Reduction of Spectroscopy with IRAF]] <br /> |-<br /> |2016.07.27 || Li, Lu || A new method to study the properties of open clusters<br /> |-<br /> |2016.07.20 || Zhang, Chaoli || An introduction to [[MCMC]]<br /> |-<br /> |2016.03.02 || Lin, Chien-Cheng || [[Media:20160302.pdf|Updates on Searching for Be Stars in LAMOST data]]<br /> |-<br /> |2016.01.27 || Liu, Cheng||The nature of stars with common origin: clues from metallicity, elemental abundances, and kinematics<br /> |-<br /> |}<br /> <br /> <br /> ----<br /> <br /> [[Seminar Plan(2014-2015)]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Seminar_Plan&diff=2150 Seminar Plan 2016-10-26T06:02:21Z <p>Increaselin：​</p> <hr /> <div>{| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title<br /> |-<br /> |-<br /> |2016.10.26 || Lin, Chien-Cheng || [[Media:20161026.pdf|Observing Proposals]]<br /> |-<br /> |2016.10.19 || Feng, Shuai || Merging Galaxies?<br /> |-<br /> |2016.10.12 || Students || Thesis opening/progress reports<br /> |-<br /> |2016.08.31 || Ju, Mengting || [[Media:Ju20160831.pdf|光谱简单处理 spectral analysis ]]<br /> |-<br /> |2016.08.17 || Zheng, Yunliang || [[Media:CG_part1.pdf|Compact Groups in Main Galaxy Sample(DR7 data products)]] <br /> |-<br /> |2016.08.10 || Yang, Li || [[Media:20160810.pdf|Data Reduction of Spectroscopy with IRAF]] <br /> |-<br /> |2016.07.27 || Li, Lu || A new method to study the properties of open clusters<br /> |-<br /> |2016.07.20 || Zhang, Chaoli || An introduction to [[MCMC]]<br /> |-<br /> |2016.03.02 || Lin, Chien-Cheng || [[Media:20160302.pdf|Updates on Searching for Be Stars in LAMOST data]]<br /> |-<br /> |2016.01.27 || Liu, Cheng||The nature of stars with common origin: clues from metallicity, elemental abundances, and kinematics<br /> |-<br /> |}<br /> <br /> <br /> ----<br /> <br /> [[Seminar Plan(2014-2015)]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:20160302.pdf&diff=2149 文件:20160302.pdf 2016-10-26T06:02:01Z <p>Increaselin：​</p> <hr /> <div></div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Ju20160831.pdf&diff=2148 文件:Ju20160831.pdf 2016-10-26T05:58:59Z <p>Increaselin：​</p> <hr /> <div></div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:20161026.pdf&diff=2147 文件:20161026.pdf 2016-10-26T05:51:19Z <p>Increaselin：​</p> <hr /> <div></div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Seminar_Plan&diff=2146 Seminar Plan 2016-10-26T05:49:09Z <p>Increaselin：​</p> <hr /> <div>{| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title<br /> |-<br /> |-<br /> |2016.10.26 || Lin, Chien-Cheng || Observing Proposals [2016.10.26.pdf]<br /> |-<br /> |2016.10.19 || Feng, Shuai || Merging Galaxies?<br /> |-<br /> |2016.10.12 || Students || Thesis opening/progress reports<br /> |-<br /> |2016.08.31 || Ju, Mengting || 光谱简单处理 spectral analysis <br /> |-<br /> |2016.08.17 || Zheng, Yunliang || Compact Groups in Main Galaxy Sample(DR7 data products)[http://cluster.shao.ac.cn/wiki/images/f/f7/CG_part1.pdf pdf]<br /> |-<br /> |2016.08.10 || Yang, Li || Data Reduction of Spectroscopy with IRAF [http://cluster.shao.ac.cn/wiki/images/f/ff/20160810.pdf pdf]<br /> |-<br /> |2016.07.27 || Li, Lu || A new method to study the properties of open clusters<br /> |-<br /> |2016.07.20 || Zhang, Chaoli || An introduction to [[MCMC]]<br /> |-<br /> |2016.03.02 || Lin, Chien-Cheng ||Updates on Searching for Be Stars in LAMOST data<br /> |-<br /> |2016.01.27 || Liu, Cheng||The nature of stars with common origin: clues from metallicity, elemental abundances, and kinematics<br /> |-<br /> |}<br /> <br /> <br /> ----<br /> <br /> [[Seminar Plan(2014-2015)]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Seminar_Plan(2014-2015)&diff=2145 Seminar Plan(2014-2015) 2016-10-26T05:43:01Z <p>Increaselin：​</p> <hr /> <div>{| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title<br /> |-<br /> | 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]]<br /> |-<br /> | 2014.09.10 || Lee, Duane || [[Media:duane_talk091014.pdf|A next-generation program for chemical enrichment evolution of dwarf satellite galaxy models]]<br /> |-<br /> | 2014.09.17 || Chen, Li || [[Media:ngc6791_chenli.pdf|WIYN OPEN CLUSTER STUDY. LIX. RADIAL-VELOCITY MEMBERSHIP &lt;br /&gt; OF THE EVOLVED population OF THE OLD OPEN CLUSTER NGC6791 (ref.arXiv:1408.3117)]]<br /> |-<br /> |2014.09.24 || Mamen Argudo|| [[Media:Mamen.pdf|Characterisation of an Isolated Galaxy Sample and the Influence of the Environment]]<br /> |-<br /> |2014.10.01 || National Day || none<br /> |-<br /> |2014.10.08 || National Day || none<br /> |-<br /> |2014.10.15 || Li, Linlin || [[Media:Linlin Li2014.10.15.pdf|Star Count Method to Study Galactic Structure]] <br /> <br /> |-<br /> |2014.10.22 || Molloy, Matthew (KIAA) || Resonant Clumping and Substructure in Galaxy Disks<br /> |-<br /> |2014.10.29 || Annual Meeting of Astronomy || none<br /> |-<br /> |2014.11.05 || No Meeting || none<br /> |-<br /> |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]] <br /> |-<br /> |2014.11.19 || No Meeting || none<br /> |-<br /> |2014.11.26 || Shen, Shiyin || [[Media:The_galaxy_pairs.pdf|The galaxy pairs]]<br /> |-<br /> |2014.12.03 || Conference in Barcelona || The Milky Way Unravelled. The GREAT-ITN Closing Conference<br /> |-<br /> |2014.12.10 || Shao, Zhengyi ||Mixture-model of open clusters and the contemplation of LAMOST <br /> |-<br /> |2014.12.17 || Liu, Chengze ||UCD in the Virgo Cluster<br /> |-<br /> |2014.12.24 || Christmas Day || none<br /> |-<br /> |2014.12.31 || New Year's Day || none<br /> |-<br /> |2015.02.11 || Winter Holiday||<br /> |-<br /> |2015.03.04 || Jing, Zhong/ Xiaoying, Pang|| Discussions on NSFC application<br /> |-<br /> |2015.03.05 || Fu, Jian/ Liu, Chengze|| Discussions on NSFC application<br /> |-<br /> |2015.03.11 || Shiyin, Shen|| Discussions on NSFC application<br /> |-<br /> |2015.03.25 || Meeting in Xiamen|| none<br /> |-<br /> |2015.04.02 || Boeche, Corrado||SP_Ace: a new code to derive stellar parameters and chemical abundances from stellar spectra<br /> |-<br /> |2015.04.08 || Yuan, Fang-Ting||Exploring Star formation properties of mergers using multiwavelength data<br /> |-<br /> |2015.04.15 || Lin, Chien-Cheng||Newly Discovered B-type Emission Stars in the LAMOST DR1<br /> |-<br /> |2015.04.22 || Chang, Rui-Xiang||A simple model of the evolution of local spiral galaxies<br /> |-<br /> |2015.04.29 || Meeting at Jiading||[[LAMOST和SDSS-IV数据讨论会]]<br /> |-<br /> |2015.05.06 || Xie, Xiao-Yi||The redshift and luminosity dependence of the quasar continuum slope<br /> |-<br /> |2015.05.13 || Pang, Xiaoying||GalevNB: conversion from simulations to observations<br /> |-<br /> |2015.05.20 || KIAA-SHAO meeting in Beijing&lt;br /&gt;Young Astronomer Forum in Nanjing||None<br /> |-<br /> |2015.05.27 || Wang, Youfen||L dwarfs discovered in LAMOST low flux spectra<br /> |-<br /> |2015.06.03 || Li, Zhiyuan||Not-so-simple stellar populations in massive star clusters<br /> |-<br /> |2015.06.10 || Meeting in Nanjing || None<br /> |-<br /> |2015.06.17 || John, Vicker||Hypervelocity Stars, Hills Ejecta, and Other Runaways<br /> |-<br /> |2015.06.24 || Carlin, Jeff||What can LAMOST tell us about halo substructure<br /> |-<br /> |2015.07.01 || Fu, Jian||The environment and ram pressure on satellite galaxies in semi-analytic models of galaxy formation<br /> |-<br /> |2015.07.08 || Meeting in Xinglong|| None<br /> |-<br /> |2015.07.16-31 ||Summer Holiday|| None<br /> |-<br /> |2015.08.01-15 ||IAU Meeting in Hawaii|| None<br /> |-<br /> |2015.08.21-28 ||Meetings in Delingha, Qinghai|| None<br /> |-<br /> |2015.09.02||Advanced Telescope and Instrument &lt;br /&gt;Techonlogy Conference in Taiwan|| None<br /> |-<br /> |2015.09.09|| Zhong, Jing|| Open cluster study in the LAMOST DR2<br /> |-<br /> |2015.09.16|| Feng, Shuai|| Isolated galaxy triplet<br /> |-<br /> |2015.09.23|| Yin, Jun|| How could we recover the SFH from the integrated-light and spectrum?<br /> |-<br /> |2015.09.30|| Meeting in Weihai|| None<br /> |-<br /> |2015.10.07|| National Day Holidays|| None<br /> |-<br /> |2015.10.14|| Vicker, John|| Searching for Substructure in the Milky Way Halo<br /> |-<br /> |2015.10.21|| Annual Meeting of Chinese &lt;br /&gt;astronomical society in PKU|| None<br /> |-<br /> |2015.10.28|| None||None<br /> |-<br /> |2015.11.04|| Pang, Xiaoying|| Starburst-like dust found in Galactic star cluster NGC 3603<br /> |-<br /> |2015.11.11|| Argudo-Fernandez, Maria|| Evolution of spiral isolated galaxies with MaNGA<br /> |-<br /> |2015.11.18|| None||None<br /> |-<br /> |2015.11.25|| Smith, Martin||[[Media:20151125-martin.pdf| The life and times of the Milky Way as viewed by LAMOST]]<br /> |-<br /> |2015.12.02 || Virtual Observatory meeting in Tianshui&lt;br /&gt; MANGA meeting in Beijing || None<br /> |-<br /> |2015.12.09 || None || None<br /> |-<br /> |2015.12.16 || None || None<br /> |-<br /> |2015.12.23 || Okamoto, Sakurako|| A Hyper Suprime-Cam view of the interacting galaxies of the M81 group<br /> |-<br /> <br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=2117 Publications 2016-10-19T02:47:10Z <p>Increaselin：​/* Firs author */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 V34, P 18<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, accepted ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Postdocs&diff=1974 Postdocs 2016-08-31T01:21:50Z <p>Increaselin：​/* 林建爭 Roger Chien-Cheng Lin */</p> <hr /> <div><br /> <br /> ==林建爭 Roger Chien-Cheng Lin==<br /> [[File:cclinpic2.png|right|250px|Roger]]<br /> <br /> Office: 1517 <br /> <br /> Tel: 5327 <br /> <br /> Email: cclin<br /> <br /> Research Interests: open clusters, low mass stars, kinematic of star clusters, spiral arms.<br /> <br /> Webpage：http://protostar.no-ip.org<br /> <br /> [[Lunch talks]]<br /> <br /> [[star cluster workshop]]<br /> <br /> ==岡本桜子 Sakurako Okamoto==<br /> [[file:sakurako.jpg|right|130px|Sakurako]]<br /> <br /> Office: 1802<br /> <br /> Tel: ----<br /> <br /> Email: okamoto <br /> <br /> Research Interests: Milky Way satellites, dwarf galaxy, optical photometry<br /> <br /> <br /> ==Emma Small==<br /> [[file:Emma.jpg|right|130px|Emma]]<br /> Office: 1513<br /> <br /> Tel: 5360<br /> <br /> Email: emma <br /> <br /> Research Interests: star formation history of nearby galaxies<br /> <br /> <br /> ==John J Vickers==<br /> [[file:johnjvickers.jpg|right|130px|Emma]]<br /> Office: 1802<br /> <br /> Tel: ----<br /> <br /> Email: johnjvickers <br /> <br /> Research Interests: Galactic Archaeology<br /> <br /> <br /> [[Finished Postdocs]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Postdocs&diff=1973 Postdocs 2016-08-31T01:20:05Z <p>Increaselin：​/* 林建爭 Roger Chien-Cheng Lin */</p> <hr /> <div><br /> <br /> ==林建爭 Roger Chien-Cheng Lin==<br /> [[File:cclinpic2.png|right|130px|Roger]]<br /> <br /> Office: 1517 <br /> <br /> Tel: 5327 <br /> <br /> Email: cclin<br /> <br /> Research Interests: open clusters, low mass stars, kinematic of star clusters, spiral arms.<br /> <br /> Webpage：http://protostar.no-ip.org<br /> <br /> [[Lunch talks]]<br /> <br /> [[star cluster workshop]]<br /> <br /> ==岡本桜子 Sakurako Okamoto==<br /> [[file:sakurako.jpg|right|130px|Sakurako]]<br /> <br /> Office: 1802<br /> <br /> Tel: ----<br /> <br /> Email: okamoto <br /> <br /> Research Interests: Milky Way satellites, dwarf galaxy, optical photometry<br /> <br /> <br /> ==Emma Small==<br /> [[file:Emma.jpg|right|130px|Emma]]<br /> Office: 1513<br /> <br /> Tel: 5360<br /> <br /> Email: emma <br /> <br /> Research Interests: star formation history of nearby galaxies<br /> <br /> <br /> ==John J Vickers==<br /> [[file:johnjvickers.jpg|right|130px|Emma]]<br /> Office: 1802<br /> <br /> Tel: ----<br /> <br /> Email: johnjvickers <br /> <br /> Research Interests: Galactic Archaeology<br /> <br /> <br /> [[Finished Postdocs]]</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=%E6%96%87%E4%BB%B6:Cclinpic2.png&diff=1972 文件:Cclinpic2.png 2016-08-31T01:19:15Z <p>Increaselin：​</p> <hr /> <div></div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1915 Publications 2016-08-10T08:36:21Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 accepted<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng'''), 2016, RAA, accepted ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1914 Publications 2016-08-10T08:36:07Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 accepted<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; et al. (including '''Lin, Chien-Cheng;'''), 2016, RAA, accepted ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1913 Publications 2016-08-10T08:35:05Z <p>Increaselin：​/* Firs author */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''林建争; 陈力; 锺靖''', 2016, 天文学进展 accepted<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; Luo, A-Li; including '''Lin, Chien-Cheng;''' et al., 2016, RAA, accepted ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1912 Publications 2016-08-10T08:32:38Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''Lin, Chien-Cheng'''; '''Chen Li'''; '''Zhong, Jing''', 2016, 天文学进展 accepted<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> # ''Low-resolution spectral analysis of early-type Hα emission stars from the second data release(DR2) of the LAMOST''<br /> #:Hou, Wen; Luo, A-Li; including '''Lin, Chien-Cheng;''' et al., 2016, RAA, accepted ([http://adsabs.harvard.edu/abs/2016arXiv160403704H ADS])<br /> #: <br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1911 Publications 2016-08-10T08:29:12Z <p>Increaselin：​/* Firs author */</p> <hr /> <div>==Firs author==<br /> #''基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''Lin, Chien-Cheng'''; '''Chen Li'''; '''Zhong, Jing''', 2016, 天文学进展 accepted<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1910 Publications 2016-08-10T08:28:35Z <p>Increaselin：​/* Firs author */</p> <hr /> <div>==Firs author==<br /> #'基于LAMOST光谱巡天的Be星搜寻''<br /> #:'''Lin, Chien-Cheng'''; '''Chen Li''', '''Zhong, Jing''', 2016, 天文学进展 accepted<br /> #:<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Lunch_talks&diff=1883 Lunch talks 2016-05-30T16:42:14Z <p>Increaselin：​/* 2016 Spring */</p> <hr /> <div>The SHAO postdocs lunch talks page, contact Martin, Minyi, or Roger to give a talk.<br /> <br /> If any of your colleges are are interested in attending, please encourage them to sign-up to the mailing list here:<br /> http://eepurl.com/bomK-9<br /> <br /> == 2016 Spring ==<br /> 11.04.2016 discussion summarized by Martin: <br /> We decided to keep the discussion series going for a few weeks, but we will try and get PhD students to give talks. Unfortunately not many people turned up today - only around 8 people - so we worry that it may not be enough to sustain it. However, let’s see if the new strategy works. We decided to shift to Wednesday morning, because that works better for some people and it’s my time in 701 so I am happy to “donate” it. We also decided to do this every two weeks. Our current plan is to have 1000-1030 at coffee, then 1030-1130 for the talk, then people can go for lunch. <br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 20.04.2016 || Zhen Yuan (SJTU)|| [[A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv<br /> |-<br /> | 04.05.2016 || TBA || TBA || <br /> |-<br /> | 18.05.2016 || TBA || TBA || <br /> |-<br /> | 08.06.2016 || Zhongli Zhang (SHAO) || TBA || <br /> |-<br /> | 15.06.2016 || Shijie Li (SJTU)|| TBA || <br /> |-<br /> | 29.06.2016 || TBA || TBA || <br /> |-<br /> | 13.07.2016 || TBA || TBA || <br /> |}<br /> <br /> == 2015 Fall ==<br /> {| class=&quot;wikitable&quot;<br /> |-<br /> ! Date !! Speaker !! Title !! Poll<br /> |-<br /> | 07.09.2015 || Baile Li (SHAO) || Supermassive black holes can fully merge in axisymmetric galaxies ||<br /> |-<br /> | 21.09.2015 || Thijs Kouwenhoven (KIAA/PKU) || TBA ||<br /> |-<br /> | 05.10.2015<br /> | colspan=&quot;3&quot;| No talk due to National Day vacation<br /> |-<br /> | 12.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || postponed to 26.10 http://doodle.com/poll/dqupmrgby739nztk<br /> |-<br /> | 26.10.2015 || Prashanth Mohan (SHAO) || Time variability in black hole systems || http://doodle.com/poll/dqupmrgby739nztks8pq3x56/admin#table<br /> |-<br /> | 09.11.2015 || Fu-Guo Xie (SHAO) || Radio/X-ray correlation in black hole accreting systems || postpone<br /> |-<br /> | 17.11.2015 || Xiaohu Li (NAOC) || Indicators of N2 ultraviolet shielding in AGB stars || Tuesday http://doodle.com/poll/qyebmhgd8d683ev3<br /> |-<br /> | 07.12.2015 || TBA || TBA ||<br /> |-<br /> | 21.12.2015 || TBA || TBA ||<br /> |}</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1882 Publications 2016-04-22T04:55:06Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Be Stars in the Open Cluster NGC 6830''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin http://cluster.shao.ac.cn/wiki/index.php?title=Publications&diff=1881 Publications 2016-04-22T04:54:45Z <p>Increaselin：​/* Coauthours */</p> <hr /> <div>==Firs author==<br /> #''An Isolated Compact Galaxy Triplet''<br /> #:'''Feng, Shuai'''; '''Shao Zhengyi''', '''Shen, Shiyin''', '''Fernández, María''' et al., 2016, RAA accepted([http://arxiv.org/abs/1512.02439 arXiv])<br /> #:<br /> #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky Survey''<br /> #:'''Shen, Shiyin''' et al.; 2016, RAA accepted ([http://arxiv.org/abs/1512.02438 arXiv])<br /> #:<br /> #''LAMOST 1: A Disrupted Satellite in the Constellation Draco''<br /> #:'''Vickers, John J.'''; '''Smith, Martin C.''' et al. 2016, ApJL, 816, 2,([http://adsabs.harvard.edu/abs/2016ApJ...816L...2V ADS])<br /> #:<br /> <br /> ==Coauthours==<br /> #''The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant''<br /> #:Raichoor, A. et al., 2016, A&amp;A, 585, 50 ([http://adsabs.harvard.edu/abs/2016A%26A...585A..50R ADS])<br /> #: <br /> # ''Searching for Be Stars in the Open Cluster NGC 663''<br /> #:Yu, Po-Chieh; '''Lin, Chien-Cheng;''' et al., 2016, AJ, 151, 121 ([http://adsabs.harvard.edu/abs/2016arXiv160402276Y ADS])<br /> #: <br /> <br /> <br /> ----<br /> [[2015 publications]]<br /> <br /> [[2014 publications]]<br /> <br /> [[2013 publications]]<br /> <br /> [[2012 publications]]<br /> <br /> [[2011 publications]]<br /> <br /> [[2010 publications]]<br /> <br /> [[2009 publications]]<br /> ----<br /> *ADS custom format，%A,%T,%J,%y,%v,%p</div> Increaselin