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<ri:Resource created="2021-01-26T12:17:04Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>S2COSMOS: bright SCUBA-2 submm sources in COSMOS</title><shortName>J/ApJ/880/43</shortName><identifier>ivo://CDS.VizieR/J/ApJ/880/43</identifier><altIdentifier>doi:10.26093/cds/vizier.18800043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Simpson J.M.</name></creator><creator><name>Smail I.</name></creator><creator><name>Swinbank A.M.</name></creator><creator><name>Chapman S.C.</name></creator><creator><name>Chen C.-C.</name></creator><creator><name>Geach J.E.,Matsuda Y.</name></creator><creator><name>Wang R.</name></creator><creator><name>Wang W.-H.</name></creator><creator><name>Yang Y.</name></creator><creator><name>Ao Y.</name></creator><creator><name>Asquith R.</name></creator><creator><name>Bourne N.,Coogan R.T.</name></creator><creator><name>Coppin K.</name></creator><creator><name>Gullberg B.</name></creator><creator><name>Hine N.K.</name></creator><creator><name>Ho L.C.</name></creator><creator><name>Hwang H.S.,Ivison R.J.</name></creator><creator><name>Kato Y.</name></creator><creator><name>Lacaille K.</name></creator><creator><name>Lewis A.J.R.</name></creator><creator><name>Liu D.</name></creator><creator><name>Michalowski M.J.,Oteo I.</name></creator><creator><name>Sawicki M.</name></creator><creator><name>Scholtz J.</name></creator><creator><name>Smith D.</name></creator><creator><name>Thomson A.P.</name></creator><creator><name>Wardlow J.L.</name></creator><date role="Updated">2021-07-05T06:51:43Z</date><date role="Created">2021-01-26T12:17:04Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><subject>surveys</subject><description>We present sensitive 850{mu}m imaging of the Cosmological Evolution Survey (COSMOS) field using 640hr of new and archival observations taken with SCUBA-2 at the East Asian Observatory's James Clerk Maxwell Telescope. The SCUBA-2 COSMOS survey (S2COSMOS) achieves a median noise level of {sigma}_850{mu}m_=1.2mJy/beam over an area of 1.6deg^2^ (MAIN; Hubble Space Telescope/Advanced Camera for Surveys footprint), and {sigma}_850{mu}m_=1.7mJy/beam over an additional 1deg^2^ of supplementary (supp) coverage. We present a catalog of 1020 and 127 sources detected at a significance level of &gt;4{sigma} and &gt;4.3{sigma} in the main and supp regions, respectively, corresponding to a uniform 2% false-detection rate. We construct the single-dish 850{mu}m number counts at S_850_&gt;2mJy and show that these S2COSMOS counts are in agreement with previous single-dish surveys, demonstrating that degree-scale fields are sufficient to overcome the effects of cosmic variance in the S_850_=2-10mJy population. To investigate the properties of the galaxies identified by S2COSMOS sources we measure the surface density of near-infrared-selected galaxies around their positions and identify an average excess of 2.0+/-0.2 galaxies within a 13" radius (~100kpc at z~2). The bulk of these galaxies represent near-infrared-selected submillimeter galaxies and/or spatially correlated sources and lie at a median photometric redshift of z=2.0+/-0.1. Finally, we perform a stacking analysis at submillimeter and far-infrared wavelengths of stellar-mass-selected galaxies (M_*_=10^10^-10^12^M_{sun}_) from z=0-4, obtaining high-significance detections at 850{mu}m in all subsets (signal-to-noise ratio, S/N=4-30), and investigate the relation between far-infrared luminosity, stellar mass, and the peak wavelength of the dust spectral energy distribution. The publication of this survey adds a new deep, uniform submillimeter layer to the wavelength coverage of this well-studied COSMOS field.</description><source format="bibcode">2019ApJ...880...43S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/880/43</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/284">II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/95">VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/103">VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/554/803">J/ApJ/554/803 : New VLA Sky Survey (NVSS) Cat of IRAS 2Jy Gal. 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