Fig. 15
Differential number counts of star-forming (top) and passive (bottom) BzK galaxies in the W1 and W4 fields. We compare with deeper observations in CFHTLS deep fields (open squares, Arcila-Osejo & Sawicki 2013) and COSMOS (open triangles, McCracken et al. 2010) and model predictions (dashed lines, Henriques et al. 2013) The inset panels show the photometric redshift distributions with KAB ≤ 22.
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