GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at z∼0.4 - III. The mass–SFR relation and the quenching of cluster galaxies

Open Access

Fig. 14.

Relation of Σ₅ − M_⋆ for (upper panel) active, suppressed, and (lower panel) non-emitter galaxies. Symbols in the upper panel are the same as in Fig. 13. Bins of Σ₅ and M_⋆ are indicated by the horizontal and vertical dashed lines, respectively, and show the separation in low, intermediate and high density or mass subsamples.

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