Morphologies of Galaxies at Uncovered by JWST/NIRCam Imaging: Cosmic Size Evolution and an Identification of an Extremely Compact Bright Galaxy at
arXiv:2208.13582 · doi:10.3847/1538-4357/acd44a
Abstract
We present morphologies of galaxies at resolved by JWST/NIRCam -m imaging. Our sample consists of galaxy candidates identified by stringent dropout and photo- criteria in GLASS, CEERS, SMACS J0723, and Stephan's Quintet flanking fields, one of which has been spectroscopically identified at . We perform surface brightness (SB) profile fitting with GALFIT for bright galaxies with S/N - on an individual basis and for stacked faint galaxies with secure point-spread functions (PSFs) of the NIRCam real data, carefully evaluating systematics by Monte-Carlo simulations. We compare our results with those of previous JWST studies, and confirm that effective radii of our measurements are consistent with those of previous measurements at . We obtain - pc with the exponential-like profiles, Sérsic indexes of -, for galaxies at -, indicating that the relation of for explains cosmic evolution over - for galaxies. One bright ( mag) galaxy at , GL-z12-1, has an extremely compact profile with pc that is surely extended over the PSF. Even in the case that the GL-z12-1 SB is fit by AGNgalaxy composite profiles, the best-fit galaxy component is again compact, pc that is significantly () smaller than the typical value at . Comparing with numerical simulations, we find that such a compact galaxy naturally forms at , and that frequent mergers at the early epoch produce more extended galaxies following the relation.
arXiv comment29 pages, 25 figures, accepted for publication in ApJ
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