Fig. 1


Spectroscopic completeness as a function of observed F775WF160W colour in bins of F775W as indicated on the left. We only include galaxies with CONFID ≥ 2. The bins were chosen to span the distribution in colour and the number of objects per bin varies strongly. This can be inferred from the grey-scale histogram which shows the number of objects as a function of colour, summed over all magnitudes down to F775W = 30. A passive galaxy at z> 1.5 typically has F775WF160W> 2.

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