A simple idea ID: 175998
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Ly" morphology of LAEs !!Positional differences between UV continuum and Ly" emission !!Ly" luminosity functions from z = 5.7 to 7.7 !!Rest-frame Ly" luminosity and EWs A simple idea ¥! HST and Spitzer imaging of spectroscopically-confirmed galaxies in the Subara Deep Field (SDF) and SXDS. ¥! Three HST programs and two Spitzer programs "! Our imaging data ¥! Optical data from Subaru Suprime-Cam (PSF "! Size-luminosity relation ¥! Brighter galaxies tend to be larger ¥! rhl,in ~ L0.14; very weak at the bright end "! Comparison with previous work ¥ LAEz7p7ENFaint galaxyReference starDeep spectroscopy of a z=7.7 LAE candidate "! !!No diffuse Ly" halos were found around LAEs !!Significant positional differences between Ly" and UV continuum !!