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<ri:Resource created="2018-08-29T13:04:16Z" status="active" updated="2025-06-13T15:25:00Z" 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>SCUBA-2 EGS deep field</title><shortName>J/MNRAS/464/3369</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/464/3369</identifier><altIdentifier>doi:10.26093/cds/vizier.74643369</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zavala J.A.</name></creator><creator><name>Aretxaga I.</name></creator><creator><name>Geach J.E.</name></creator><creator><name>Hughes D.H.</name></creator><creator><name>Birkinshaw M.,Chapin E.</name></creator><creator><name>Chapman S.</name></creator><creator><name>Chen C.-C.</name></creator><creator><name>Clements D.L.</name></creator><creator><name>Dunlop J.S.</name></creator><creator><name>Farrah D.,Ivison R.J.</name></creator><creator><name>Jenness T.</name></creator><creator><name>Michalowski M.J.</name></creator><creator><name>Robson E.I.</name></creator><creator><name>Scott D.,Simpson J.</name></creator><creator><name>Spaans M.</name></creator><creator><name>Van Der Werf P.</name></creator><date role="Updated">2024-08-16T20:19:32Z</date><date role="Created">2018-08-29T13:04:16Z</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>surveys</subject><subject>galaxies</subject><subject>photometry</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We present deep observations at 450 and 850{mu}m in the Extended Groth Strip field taken with the SCUBA-2 camera mounted on the James Clerk Maxwell Telescope as part of the deep SCUBA-2 Cosmology Legacy Survey (S2CLS), achieving a central instrumental depth of {sigma}_450_=1.2mJy/beam and {sigma}_850_=0.2mJy/beam. We detect 57 sources at 450{mu}m and 90 at 850{mu}m with signal-to-noise ratio &gt;3.5 over ~70arcmin^2^. From these detections, we derive the number counts at flux densities S_450_&gt;4.0mJy and S_850_&gt;0.9mJy, which represent the deepest number counts at these wavelengths derived using directly extracted sources from only blank-field observations with a single-dish telescope. Our measurements smoothly connect the gap between previous shallower blank-field single-dish observations and deep interferometric ALMA results. We estimate the contribution of our SCUBA-2 detected galaxies to the cosmic infrared background (CIB), as well as the contribution of 24{mu}m-selected galaxies through a stacking technique, which add a total of 0.26+/-0.03 and 0.07+/-0.01MJy/sr, at 450 and 850{mu}m, respectively. These surface brightnesses correspond to 60+/-20 and 50+/-20 per cent of the total CIB measurements, where the errors are dominated by those of the total CIB. Using the photometric redshifts of the 24{mu}m-selected sample and the redshift distributions of the submillimetre galaxies, we find that the redshift distribution of the recovered CIB is different at each wavelength, with a peak at z~1 for 450{mu}m and at z~2 for 850{mu}m, consistent with previous observations and theoretical models.</description><source format="bibcode">2017MNRAS.464.3369Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/464/3369</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/J/A+A/526/A72">J/A+A/526/A72 : Early-type galaxies in the EGS (Fernandez Lorenzo+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/2159">J/AJ/132/2159 : IRAC counterparts of 6cm galaxies in EGS (Willner+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/717/1181">J/ApJ/717/1181 : Spitzer power-law galaxies in EGS (Park+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/135">J/ApJ/758/135 : DEEP2 galaxies with UV spectra in the EGS (Kornei+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/177/431">J/ApJS/177/431 : Mid-IR sources in EGS (Barmby+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/13">J/ApJS/193/13 : Spitzer/IRAC sources in the EGS I. SEDs (Barro+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/30">J/ApJS/193/30 : UV-to-FIR analysis of sources in the EGS. II. 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