Fig. 5
Left: histogram of Hα line fluxes for the 174 robust cluster members (after correcting for the strongest component of the [N ii] doublet). Right: histogram of SFR for SF galaxies (i.e. excluding AGN candidates) from the Hα fluxes, when applying a standard 1 mag. extinction correction for the line, and the Kennicutt (1998) luminosity-SFR conversion.
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