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• 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
• 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
• Pixel based galaxy morphology classification
  1 KB (156 words) - 05:41, 6 April 2022
• 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
• 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
• 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
• 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
• 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
• 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

Page text matches

• 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

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