MUSUBI (MegaCam Ultra-deep Survey: -Band Imaging)-Data for the COSMOS and SXDS Fields
arXiv:2205.11546 · doi:10.3847/1538-4365/ac729e
Abstract
The Subaru Hyper Suprime-Cam (HSC) Strategic Survey is the latest-generation multi-band optical imaging survey for galaxy evolution and structure formation. The "Ultra-Deep" component of the HSC survey provides broad-band images over deg to detection limits of -28 AB, along with narrow-band images, in the COSMOS and the SXDS fields. These images provide an unprecedented combination of depths and area coverage, for the studies galaxies up to . However, the lack of coverage at Ang implies incomplete sampling of the rest-frame UV at , which is critically needed for understanding the buildup of stellar mass in the later cosmic time. We conducted a multi-year CFHT -band imaging campaign in the two HSC Ultra-Deep fields with CFHT MegaCam. By including shallower archival data, we reach 5- depths of and 28.4 (AB) at the centers of the COSMOS and SXDS fields, respectively, and and 27.8 in the central 1 deg fields. The image quality is arcsec, fairly good for the band. Both the photometric and astrometric quality of our data are excellent. We show that the combination of our -band and HSC data can lead to high-quality photometric redshifts at -3, and robust measurements of rest-frame UV on galaxies at for distinguishing green-valley galaxies from star-forming and quiescent galaxies. We publicly release our reduced -band images and reference catalogs that can be used readily for scientific studies.
24 pages, 12 figures, accepted for publication on ApJS
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- The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
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