Interpreting the optical data of the Hubble Deep Field South: colors, morphological number counts and photometric redshifts

Details Interpreting the optical data of the Hubble Deep Field South: colors, morphological number counts and photometric redshifts Interpreting the optical data of the Hubble Deep Field South: colors, morphological number counts and photometric redshifts

2000-07-19

arxiv.org/abs/astro-ph/0007283v1

Astronomy and Astrophysics

Astrophysics

15 pages, 21 figures, accepted for publication in A&A

Scientific paper

We present an analysis of the optical data of the Hubble Deep Field South. We derive F300W(AB), F450W(AB), F606W(AB) and F814W(AB) number counts for galaxies in all four bands. The slope is steeper at shortest wavelengths: we estimated gamma(F300W(AB))=0.47, gamma(F450W(AB))=0.35, gamma(F606W(AB))=0.28 and gamma(F814W(AB))=0.28. Morphological number counts are actually dominated by late type galaxies, while early type galaxies show a decreasing slope at faint magnitudes. Combining this information with photometric redshifts, we notice that galaxies contributing with a steep slope to morphological number counts (i.e. spiral and irregular galaxies) have z>1, suggesting a moderate merging. However we emphasize that any cut in apparent magnitude at optical wavelengths results in samples biased against elliptical galaxies, affecting as a consequence the redshift distributions and the implications on the evolution of galaxies along the Hubble sequence.

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