Fig. 14
Distribution of B-band luminosities (left) and stellar masses (right) computed for all objects with reliable redshift (flag > 2.0) in the PDR-2 catalogue. These are estimated through SED fitting of all available photometry (from UV to K) as described in Moutard et al. (2016a). Note that an explicit value of H0 = 70 km s-1 Mpc-1 for the Hubble constant is used here.
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