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Using the very deep Subaru images of the GOODS-N region, from the MOIRCS DeepSurvey and images from the HST/ACS, we have measured the Luminosity Ratio (LR)of the outer to the central regions of massive (M>10^{10.5}M_{Sun}) galaxies atfixed radii in a single rest-frame for z<3.5 as a new approach to the problemof size evolution. We didn't observe any evolution in the median LR. Had asignificant size growth occurred, the outer to central luminosity ratios wouldhave demonstrated a corresponding increase with a decrease in redshift.

Total to central luminosity ratios of quiescent galaxies in MODS as an indicator of size evolution