Subaru Super Deep Field with Adaptive Optics. I. Observations and First Implications

Abstract

We present a deep K'-band (2.12 μm) imaging of the 1'×1' Subaru Super Deep Field (SSDF) taken with the Subaru adaptive optics (AO) system. Total integration time of 26.8 hr results in the limiting magnitude of K'~24.7 (5 σ, 0.2" aperture) for point sources and K'~23.5 (5 σ, 0.6" aperture) for galaxies, which is the deepest limit ever achieved in the K' band. The average stellar full width at half-maximum (FWHM) of the co-added image is 0.18". Based on the photometric measurements of detected galaxies, we obtained the differential galaxy number counts, for the first time, down to K'~25, which is more than 0.5 mag deeper than the previous data. We found that the number count slope dlogN/dm is about 0.15 at 22 <25, which is flatter than the previous data. Therefore, detected galaxies in the SSDF have only negligible contribution to the near-infrared extragalactic background light (EBL), and the discrepancy claimed so far between the diffuse EBL measurements and the estimated EBL from galaxy count integration has become more serious. The size distribution of detected galaxies was obtained down to the area size of less than 0.1 arcsec2, which is less than half of that of the previous data in the K' band. We compared the observed size-magnitude relation with a simple pure luminosity evolution model allowing for intrinsic size evolution and found that a model with no size evolution gives the best fit to the data. It implies that the surface brightness of galaxies at high redshift is not much different from that expected from the size-luminosity relation of present-day galaxies. Based on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.