Comparison of the FWHM from the Gaussian fits with the 50% enclosed light radius from the pysersic procedure of I. Pasha & T. B. Miller (2023). The latter has the PSF deconvolved. The vertical blue line shows our compact galaxy selection using FWHM, and the horizontal blue line shows a similar selection using the pysersic results. We show 68% confidence ranges for the pysersic results and place points that would lie off the top of the figure at nominal values of ﹩0\mathop{.}\limits^{^{\prime\prime} }077﹩. We have not corrected either of these measures for lensing magnification. Published LRDs are shown with red circles.