Fig. 7
Comparison of our stellar mass and SFR estimates for the XLSSC 116 ICL source (red vertical line for SED estimation and red vertical dotted line for spectroscopic estimation) and BCG (blue vertical line for SED estimation and blue vertical dotted line for spectroscopic estimation) with the Puech et al. (2010) emission line galaxies (continuous histograms) and the Liu et al. (2012) BCGs (dashed histograms). Upper figure: stellar mass, lower figure: SFR.
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