Fig. 15
The FP of the EDisCS clusters with VLT only photometry. Each cluster is identified by its short name for clarity, see Table 4 for the full name. Colors code the spectroscopic type. The black squares show galaxies with SExtractor flags different from 0 or 2 and therefore unreliable photometric parameters. The dotted magenta line shows the best-fit FP relation for all galaxies. The solid magenta line shows the best-fit FP relation when considering only galaxies with spectroscopy type ≤ 2 and SExtractor flag 0 or 2. The full line shows the Coma cluster at zero redshift. The black dotted and dashed lines show the clusters MS2053-04 at z = 0.58 and MS1054-03 at z = 0.83 from Wuyts et al. (2004), respectively.
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