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Fig. 9


MSFR relation for A983 and 1731 on the left and right panels, respectively. The histograms on the top and right side of each plot show the stellar mass and SFR distribution of the members. The SFR from only the total IR luminosity is plotted as red diamonds, the SFR from the extinction corrected Hα as open blue triangles, the combined SFR as open green squares. The filled blue triangles show the sources for which the mean extinction correction was used. The light blue shaded area corresponds to the relation with uncertainties found by Noeske et al. (2007). The red dot-dashed and the blue dashed lines indicate the SFR limit evaluated from the detection limit of the IR 24 μm and optical spectral S/N, respectively.

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