The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field

Abstract

We present deep optical imaging observations of 2 square degree area, covered by the Cosmic Evolution Survey (COSMOS), made by the prime-focus Camera (Supreme-Cam) on the 8.2m Subaru Telescope. Observations were done in six broad-band [B (4459.7 AA), g' (4723.1 AA), V (5483.8 AA), r' (6213.0 AA), i' (7640.8 AA), z' (8855.0 AA)], and one narrow-band (NB816) filters. A total of 10^6 galaxies were detected to i'~26.5 mag. These data, combined with observations at u* and K-band are used to construct the photometric catalogs for the COSMOS and to measure their photometric redshifts, multi-band spectral energy distributions, stellar masses and identification of high redshift candidates. This catalog provides multi-waveband data for scientific analysis of the COSMOS survey.

arXiv comment46 pages, 32 figures, accepted for the COSMOS special issue of ApJS

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• Environmental Effects on the Star Formation Activity at z~0.9 in the COSMOS Field
• On the Origin of the Strong Optical Variability of Emission-line Galaxies
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• Clumpiness of galaxies revealed in the near-infrared with COSMOS-Web
• Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
• The Evolution of the Luminosity Function for Luminous Compact Blue Galaxies to z=1
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• The major merger-active galactic nucleus connection up to the cosmic noon
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• A multiwavelength study of an early galaxy group merger in COSMOS revealed by two tailed radio galaxies at z = 0.35
• Physical properties of distant red galaxies in the COSMOS/UltraVISTA field
• Joint Survey Processing II: Stellar Proper Motions in the COSMOS Field, from Hubble Space Telescope ACS and Subaru Telescope HSC Observations
• Spectral energy distribution similarity of the local galaxies and the 3.6um selected galaxies from the Spitzer Extended Deep Survey