Morphological Number Counts of Galaxies in the Hubble Deep Field South

dc.creatorLee, Myung Gyoon
dc.creatorHwang, Narae
dc.date2000-08-18
dc.date2000-09-14
dc.date.accessioned2026-07-07T01:54:58Z
dc.date.available2026-07-07T01:54:58Z
dc.descriptionWe present a study of photometric properties of the galaxies in the Hubble Deep Field South (HDFS) based on the released WFPC2 images obtained with the Hubble Space Telescope (HST). We have classified about 340 galaxies with $I<26$ mag in the HDFS as well as about 400 galaxies in the Hubble Deep Field North (HDFN) using the visual classification supplemented by inspection of the surface brightness profiles of the galaxies. Galaxy population statistics and morphological number counts for the HDFS are found to be similar to be those for the HDFN. We have also determined photometrically the redshifts of the galaxies with $I<26$ mag in the HDFS and the HDFN using the empirical training set method. Redshift distribution, color-redshift relation, and magnitude-redshift for each type of galaxies are investigated.
dc.description8 pages (LaTex), isasrep.sty, Presented at ISAS workshop, "Mid- and Far-infrared Astronomy and Future Space Missions", 17-18 April 2000, Japan
dc.identifierhttps://arxiv.org/abs/astro-ph/0008286
dc.identifierhttp://arxiv.org/abs/astro-ph/0008286
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1502
dc.subjectAstrophysics
dc.titleMorphological Number Counts of Galaxies in the Hubble Deep Field South
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