Fig. 12
Mass-size relation of red-sequence early-type cluster galaxies at z> 1. Sizes are corrected for PSF blurring effects. The solid line and shading shows the fitted mass-size relation and its 68% uncertainty (posterior highest density interval). The wedge between the two slanted lines is the locus of Coma galaxies. The horizontal dotted line indicates the PSF FWHM.
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