Fig. 3.
Mass–SSFR relation for the [OII] emitters in and around the XMM2215 cluster (green open circles), the six XMM2215 cluster galaxies of the SFvirialized sample (red triangles) and four infalling cluster galaxies (blue symbols). The oblique dashed line shows the MS at z ∼ 1.46 and its dispersion (indicated by the dotted lines) using Eq. (1) in Peng et al. (2010).
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