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In this work we use the Hubble Deep Field South (HDF-S) version 2 images toassess the galaxy population out to z ~ 2. We have used two methods oftemplates fitting of the spectral energy distributions to obtain photometricredshifts and classify the objects. The Bayesian photometric redshifts gavebetter results when compared with 54 spectroscopic redshifts available in theliterature. Analysis of the rest-frame colour distribution shows a bimodalityout to z ~ 1.4. We separated our sample in a blue and a red population at B-V =0.29. At low redshifts (0.2<z<0.6), ~ 60% of the galaxies have B-V > 0.29whereas at higher redshifts ~ 60% of the galaxies are bluer than B-V < 0.29.Although in low numbers, a population of early-type galaxies (or heavilyobscured low redshift galaxies) is seen out to z ~ 2.

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