Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-18
Mon.Not.Roy.Astron.Soc.366:609-623,2006
Astronomy and Astrophysics
Astrophysics
Accepted for publication in MNRAS. 16 pages, 15 figures
Scientific paper
10.1111/j.1365-2966.2005.09887.x
We have selected and analysed the properties of a sample of 2905 Ks<21.5 galaxies in ~ 131 sq.arcmin of the Great Observatories Origins Deep Survey (GOODS) Chandra Deep Field South (CDFS), to obtain further constraints on the evolution of Ks-selected galaxies with respect to the results already obtained in previous studies. We made use of the public deep multiwavelength imaging from the optical B through the infrared (IR) 4.5 micron bands, in conjunction with available spectroscopic and COMBO17 data in the CDFS, to construct an optimised redshift catalogue for our galaxy sample. We computed the Ks-band LF and determined that its characteristic magnitude has a substantial brightening and a decreasing total density from z=0 to
Caputi Karina I.
Cirasuolo Michele
Dunlop James S.
McLure Ross J.
Schael A. M.
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