Assessing the galaxy population out to z ∼ 2 using the Hubble Deep Field South

Astronomy and Astrophysics

Volumn 426, Issue 2, 2004, Pages 455-462

  Wiegert, T ^a,d   De Mello, D F ^a,b,c   Horellou, C ^a  

^a CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c CATHOLIC UNIVERSITY OF AMERICA   (United States)

^d UNIVERSITY OF MANITOBA   (Canada)

Author keywords

Cosmology: observations; Galaxies: evolution; Galaxies: photometry; Galaxies: statistics

Indexed keywords

COLOR; IMAGE ANALYSIS; MORPHOLOGY; PHOTOMETRY; SPECTROSCOPIC ANALYSIS; TELESCOPES;

COSMOLOGY: OBSERVATIONS; GALAXIES: EVOLUTION; GALAXIES: PHOTOMETRY; GALAXIES: STATISTICS;

GALAXIES;

EID: 8344243775     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041015     Document Type: Article

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