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  • Photometry of overlapping galaxy pairs
    ...has become a very important task. More accurate photometry of overlapping galaxy pairs will be more helpful for future research.
    792 bytes (115 words) - 01:52, 22 April 2015
  • Morphology of Alfalfa galaxies
    This project aims to find the galaxy mergers in Alfalfa galaxies. * Are Alfaalfa galaxies biased to merges (galaxy pairs)?
    290 bytes (39 words) - 05:36, 4 March 2021
  • Deep learning on galaxy images: training dataset
    ...is used to collect the training dataset for deep learning applications on galaxy images. ==local galaxy sample==
    1 KB (184 words) - 08:58, 11 November 2021
  • Quanfeng Xu
    Research interests: Deep Learning classification galaxy morphology * [[Deep learning on galaxy morphology profile]]
    304 bytes (36 words) - 05:03, 8 December 2023
  • Intern program for college students
    ==[[Photometry of overlapping galaxy pairs]]== ...has become a very important task. More accurate photometry of overlapping galaxy pairs will be more helpful for future research.
    1 KB (163 words) - 02:39, 5 June 2019
  • Interesting object in LEGAS DR1
    * a beautiful bar galaxy[http://skyserver.sdss3.org/public/en/tools/chart/navi.aspx?ra=133.566710713 * a ring galaxy[http://skyserver.sdss3.org/public/en/tools/explore/summary.aspx?id=0x112d13
    5 KB (737 words) - 12:56, 14 January 2015
  • Galaxy morphology auto classification
    *This page makes collections for galaxy morphology auto classification project of CSST image survey * [[pixel based galaxy morphology classification]] (Renhao Ye)
    3 KB (372 words) - 09:19, 1 October 2022
  • SHAO-KIAA galaxies
    * large scale structure of galaxy distribution ===Galaxy pair and galaxy interaction===
    1 KB (207 words) - 08:39, 24 June 2020
  • CSST projects
    [[Galaxy morphology auto classification]]
    41 bytes (4 words) - 06:47, 4 March 2021
  • Morphology auto classification
    #REDIRECT [[Galaxy morphology auto classification]]
    51 bytes (5 words) - 05:42, 4 March 2021
  • Interesting object in LEGAS DR2
    ==peculiar galaxy== *pair or peanut galaxy[http://skyserver.sdss.org/dr7/en/tools/explore/obj.asp?ra=145.08611&dec=32.
    5 KB (667 words) - 07:56, 9 September 2015
  • Deep learning on galaxy morphology profile
    ...uses on fitting galaxy pictures to their morphological parameters based on galaxy morphology. ...article "Deep learning for galaxy surface brightness profile fitting". The galaxy morphology parameters contain the magnitude of galaxies, the profile Sersic
    2 KB (365 words) - 08:15, 1 October 2022
  • 2013/12/25
    * 尹君 [[Ew(Hα) of one star forming galaxy in LAMOST survey]]
    64 bytes (10 words) - 02:10, 24 December 2013
  • 2013 publications
    *Star formation and metallicity gradients in semi-analytic models of disc galaxy formation[http://adsabs.harvard.edu/abs/2013MNRAS.434.1531F] ...lecular gas on the redshift evolution of star formation and metallicity in galaxy formation models[http://adsabs.harvard.edu/abs/2013IAUS..292..245F]
    1 KB (158 words) - 02:22, 21 October 2014
  • EG sources in LAMOST DR1
    ===main galaxy(r<17,77) without spectra=== **GALAXY , 496
    2 KB (127 words) - 06:56, 11 December 2013
  • Ew(Hα) of one star forming galaxy
    === Exercise: measure the Ew(Hα) of one SFing galaxy in the Lamost survey === ** central wavelength of this galaxy: 6563*(1+z)=6742 A
    1 KB (196 words) - 02:02, 24 December 2013
  • Seminar Plan of the Second Semester of 2014
    ...xt-generation program for chemical enrichment evolution of dwarf satellite galaxy models]] ...09.24 || Mamen Argudo|| [[Media:Mamen.pdf|Characterisation of an Isolated Galaxy Sample and the Influence of the Environment]]
    2 KB (243 words) - 03:18, 13 April 2015
  • Seminar Plan(2016)
    ...ian Fu || The view of HI gas size-mass relation in semi-analytic models of galaxy formation |2016.10.19 || Feng, Shuai || Polar Ring Galaxy in long-slit spectroscopy
    1 KB (168 words) - 07:05, 29 March 2017
  • Seminar Plan(2020)
    |2020.01.15 || Shen Shiyin || How to model the spectrum of a galaxy [[:File:Gal_spectrum.pdf | pdf file]] |2020.03.18 || Shen Mengting || Galaxy Morphology and Gas Content
    1 KB (168 words) - 08:55, 5 March 2021
  • Auto clustering of galaxies after dimensionality reduction
    *The first part is to reduce the dimension of Galaxy data to low dimensional space with VAE. ...first filter out the galaxy data with data shape [3*256*256], and save the galaxy data paths that match this shape into a text file, which constitutes our tr
    3 KB (437 words) - 18:47, 24 November 2023
  • 2017 publications
    ...nction and reddening from the South Galactic Cap U-band Sky Survey: u band galaxy number counts and u−r color distribution'' #''Population gradient in Sextans dSph: Comprehensive mapping of a dwarf galaxy by Suprime-Cam''
    2 KB (319 words) - 00:39, 29 October 2018
  • ArXiv.1601.03039
    *远红外数据很好的trace SFR，特别是对于star forming galaxy
    690 bytes (38 words) - 09:22, 20 January 2016
  • Postdocs Completed
    Research interest: high redshift galaxies, galaxy interaction
    189 bytes (22 words) - 01:10, 14 April 2015
  • Merger identification
    == <big>'''Automatic Galaxy Classification '''</big>== ...an urgent need to employ machine learning approaches to conduct automated galaxy classification tasks. In this work, we are going to find a good enough met
    4 KB (672 words) - 07:07, 3 March 2022
  • Seminar Plan(2023)
    | 2024/4/17 || 陈宓 || Galaxy Decomposition [[:File:Galaxy decomposition 240417组会.pdf|pdf]] | 2023/12/27 || 梁晋宁 (Durham University) || Connection between galaxy morphology and dark-matter halo structure
    2 KB (206 words) - 06:52, 17 April 2024
  • 1/15
    *Ultra compact dwarf galaxy 刘成则
    172 bytes (13 words) - 05:24, 15 January 2014
  • Ew(Hα) of one star forming galaxy in LAMOST survey
    == Exercise: measure the Ew(Hα) of one SFing galaxy in the LAMOST survey == *A blue, compact, normal galaxy
    2 KB (362 words) - 01:48, 25 December 2013
  • LAMOST Science
    *[[Ew(Hα) of one star forming galaxy in LAMOST survey]]
    198 bytes (29 words) - 01:53, 29 October 2018
  • Staff Members
    Research Interest: Galaxy Formation and Evolution, radio astrophysics on neutral gas Research: nearby galaxies, galaxy clusters
    2 KB (294 words) - 01:47, 17 January 2024
  • Close pairs in MaNGA sample
    [[telecon on galaxy pairs in MaNGA 2014/6/17]]
    360 bytes (53 words) - 04:26, 17 June 2014
  • 2012 publications
    * The Growth of the Disk Galaxy UGC8802 [http://adsabs.harvard.edu/abs/2012ApJ...753L..10C] ...lar gas in massive galaxies - III. Comparison with semi-analytic models of galaxy formation [http://adsabs.harvard.edu/abs/2012MNRAS.422..997K]
    2 KB (228 words) - 02:24, 21 October 2014
  • The VIRUS-P Exploration of Nearby Galaxies (VENGA): Radial Gas Inflow and Shock Excitation in NGC 1042
    ...cluster. We present the integral-field-spectroscopy (IFS) studies of this galaxy, based on the data obtained with the Mitchell spectrograph on the 2.7 meter
    1 KB (213 words) - 03:11, 11 March 2016
  • KKC archive
    ==Galaxy==
    10 KB (434 words) - 12:50, 22 August 2022
  • Completed Postdocs
    Research interests: high redshift galaxies, galaxy interaction Research Interests: Milky Way satellites, dwarf galaxy, optical photometry
    1 KB (165 words) - 15:03, 2 February 2021
  • Research Interests
    ...which will provide unique constraints on the shape of the potential of the Galaxy’s dark matter halo. (Jing Zhong, Martin Smith) The present state of our galaxy can tell us a lot about how it has formed and evolved. In particular the st
    6 KB (901 words) - 02:56, 3 November 2020
  • Students
    Research interests: Deep Learning classification galaxy morphology * [[Deep learning on galaxy morphology profile]]
    3 KB (385 words) - 03:47, 4 March 2024
  • Seminar Plan(2014-2015)
    ...xt-generation program for chemical enrichment evolution of dwarf satellite galaxy models]] ...09.24 || Mamen Argudo|| [[Media:Mamen.pdf|Characterisation of an Isolated Galaxy Sample and the Influence of the Environment]]
    5 KB (581 words) - 05:43, 26 October 2016
  • The-10th-c-manga-workshop:agenda
    ...Asymmetries in disk galaxies and its implication for dust attenuation and galaxy orientation * 11:10-11:30 Mengting Ju: Gas accretion of blue compact galaxy?
    3 KB (418 words) - 23:48, 19 December 2019
  • Intern program for high school students
    Detection of a Substantial Molecular Gas Reservoir in a brightest cluster galaxy at z = 1.7 Self-consistent modelling of our Galaxy with Gaia data
    7 KB (253 words) - 07:00, 7 June 2017
  • Telecon on galaxy pairs in MaNGA 2014/6/17
    :*Ryan: pairs in NSA sample, all the interesting objects(include the galaxy with very faint close companions down to r~20).
    563 bytes (84 words) - 04:38, 17 June 2014
  • Close pair
    ;#12 of them with spectra, 7 of them with redshift and classified as GALAXY
    2 KB (250 words) - 11:18, 4 December 2013
  • ALFALFA and MaNGA
    ...PhotoObjID object. It could because that the SDSS catalog has changed the galaxy properties a little bit after DR7, ALFALFA might used the old value (DR7).
    1 KB (168 words) - 09:13, 18 December 2014
  • 2015 publications
    # ''The evolution of interacting spiral galaxy NGC 5194'' # ''Using member galaxy luminosities as halo mass proxies of galaxy groups''
    6 KB (872 words) - 02:18, 18 January 2017
  • 2016 publications
    #''An Isolated Compact Galaxy Triplet'' #''A sample of galaxy pairs identified from the LAMOST spectral survey and the Sloan Digital Sky
    5 KB (694 words) - 01:29, 19 January 2018
  • The-9th-c-manga-workshop:abstracts
    ...examining the maps/profiles of E(B-V) obtained by Niu Li and dependence on galaxy properties. I will summarize the results so far. ...Ha maps of MaNGA galaxies. We will take the advantages of the large MaNGA galaxy sample and explore the statistical properties of these HII regions.
    9 KB (1,355 words) - 06:00, 17 June 2019
  • Seminar Plan(2019)
    |2019.12.04 || Fu Jian || Dust Modelling in the Galaxy Evolution Model and Chemical Evolution Model
    1 KB (169 words) - 04:41, 25 December 2019
  • 2015 KIAA-SHAO workshop
    | Towards a detailed history of the Galaxy via stellar chemical abundance ratio distribution (CARD) analysis |rowspan="10"|4. Large-scale structure, galaxy formation and evolution
    6 KB (795 words) - 11:54, 9 May 2015
  • Astrostat Club
    | Zi hao || DECaLS data(galaxy properties) ||
    1 KB (201 words) - 04:08, 22 March 2022
  • Galaxies Seminar
    | 2016.12.23 || Wang, Tao (CEA, France)|| Star formation in the most distant galaxy cluster, and perspectives with SKA
    1 KB (178 words) - 02:24, 8 April 2017
  • Star cluster catalog
    ...A+A/404/223 2MASS IR star clusters in the Galaxy (Bica+, 2003)
    2 KB (183 words) - 03:56, 11 June 2015
  • The-10th-c-manga-workshop:abstracts
    :Abstract: Galaxy mergers and interactions are expected to play a signicant role leading to o * Title: Host Galaxy Properties of CL-AGNs]{Host Galaxy Properties of Changing-look AGN Revealed in the MaNGA Survey
    11 KB (1,643 words) - 21:48, 19 December 2019
  • MaNGA Tech Group 2018-06-26
    ...axy. Match to find out the SDSS DR7 plate, fiber, mjd information for each galaxy.
    3 KB (581 words) - 15:46, 27 June 2018
  • A Model for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy
    ...this talk, I will briefly summarize my PhD work on Fornax dwarf spheroidal galaxy, the brightest satellite dwarf galaxies of Milky Way. I will focus on the g
    2 KB (266 words) - 16:59, 14 April 2016
  • 2010 publications
    ...omic-to-molecular transition and its relation to the scaling properties of galaxy discs in the local Universe[http://adsabs.harvard.edu/abs/2010MNRAS.409..51
    2 KB (258 words) - 06:48, 18 September 2014
  • Research highlights
    ...J...722..380C]) and also embedded it in the semi-analytic models (SAMs) of galaxy formation and evolution(e.g, Fu et al. 2012, 2013). ...are far enough away, the Milky Way we see will be very similar to Sombrero Galaxy from the edge-on view. (Li et al. 2018 [http://adsabs.harvard.edu/abs/2018A
    12 KB (1,869 words) - 02:27, 29 October 2018
  • Colloquium
    | Astronomy in the big data era: exploring galaxy morphology with citizen science and machine learning - a case study
    2 KB (240 words) - 11:12, 29 April 2024
  • Lunch talks
    ...del for Gas Dynamics and Chemical Evolution of the Fornax Dwarf Spheroidal Galaxy]] || http://doodle.com/poll/9aygarmupsbdw5fv
    3 KB (378 words) - 13:00, 3 January 2017
  • China-Chile Proposal
    ...and separating the effects of interaction-driven evolution in the observed galaxy properties is not trivial. ...m that will advance our understanding of the effects of the environment on galaxy formation and evolution by combining theoretical modelling with MaNGA spect
    26 KB (4,125 words) - 00:43, 26 June 2019
  • Publications
    ...ray luminosity, and baryon budget in the L-Galaxies semi-analytic model of galaxy formation'', #''Mock X-Ray Observations of Hot Gas with L-Galaxies Semi-analytic Models of Galaxy Formation''
    20 KB (2,786 words) - 12:37, 1 January 2024
  • Colloquium Archive
    | Understanding the galaxy formation and metal-enrichment in the view of gas-regulator framework | Dancing together: the spin of large scale filaments and their impact on galaxy spin
    32 KB (4,484 words) - 11:49, 16 February 2024
  • Star cluster group
    ...A+A/404/223 2MASS IR star clusters in the Galaxy (Bica+, 2003)
    11 KB (1,258 words) - 08:09, 2 December 2016
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