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Fig. 18

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NIR colour–magnitude diagram for J,H, and Ks selected samples obtained from the Ultra-Deep sample (black points). The two oblique dashed lines correspond to the I-band limiting magnitudes of the survey iAB = 23 on the bright end, iAB = 24.75 on the faint end. The VVDS-Deep colour–magnitude distribution is shown as the grey points with the iAB = 17.5 and iAB = 24 limits indicated as long-dashed lines. We are able to extract samples that are nearly complete in spectroscopic redshift measurements, selected down to JAB = 23, HAB = 22.5, and KsAB = 22 (vertical dashed lines). The faint i-band magnitude cut imposes a loss of red objects for fainter magnitudes but it is still 80% complete down to JAB = 24, HAB = 23.5, and KsAB = 23. Typical error bars are shown at the bottom of each panel.

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