Fig. 7
Histogram of photometric redshifts computed in the cluster field. We show the photometric redshift distribution of 17 spectroscopic members of WARPJ1415 at z = 1.03 (blue dashed line) and the photometric redshift distribution of 13 candidate members selected from the red sequence of CXO1415 (red solid line). The thinner histogram (solid blue line) marks the spectroscopic redshift distribution of WARPJ1415, while the cyan stripe corresponds to the X-ray redshift zX = 1.46 ± 0.025.
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