Fig. 13
Left: postage stamp of the third brightest and fourth most massive galaxy in Cl J0227-0421 generated in an identical manner to that of Fig. 11. Right: observed-frame optical/NIR SED of this galaxy plotted against the best-fit galaxy template. Best-fit stellar mass and luminosity-weighted stellar age are shown in the upper left corner of the plot. While this galaxy is also host to a type-1 AGN, the same test was performed on this galaxy as was performed on the galaxy shown in Fig. 12 and negligible differences in the derived stellar mass were found.
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