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This article has an erratum: [https://doi.org/10.1051/0004-6361/201628442e]


Fig. 10

image

Mass-size relation of red-sequence early-type cluster galaxies at z> 1.47 (points color-coded, upper panel) or Coma (z = 0.0232, bottom panel). Coma cluster galaxies occupy the wedge between the two slanted lines, reported in both panels. The horizontal dotted line in the top panel indicates the PSF FWHM. Sizes are not corrected for PSF blurring effects.

This figure is made of several images, please see below:

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