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<ri:Resource created="2020-04-15T09:51:13Z" 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>SCUBA-2 850um obs. of Herschel gal.</title><shortName>J/MNRAS/477/1099</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/477/1099</identifier><altIdentifier>doi:10.26093/cds/vizier.74771099</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Duivenvoorden S.</name></creator><creator><name>Oliver S.</name></creator><creator><name>Scudder J.M.</name></creator><creator><name>Greenslade J.</name></creator><creator><name>Riechers D.A.,Wilkins S.M.</name></creator><creator><name>Buat V.</name></creator><creator><name>Chapman S.C.</name></creator><creator><name>Clements D.L.</name></creator><creator><name>Cooray A.,Coppin K.E.K.</name></creator><creator><name>Dannerbauer H.</name></creator><creator><name>De Zotti G.</name></creator><creator><name>Dunlop J.S.</name></creator><creator><name>Eales S.A.,Efstathiou A.</name></creator><creator><name>Farrah D.</name></creator><creator><name>Geach J.E.</name></creator><creator><name>Holland W.S.</name></creator><creator><name>Hurley P.D.,Ivison R.J.</name></creator><creator><name>Marchetti L.</name></creator><creator><name>Petitpas G.</name></creator><creator><name>Sargent M.T.</name></creator><creator><name>Scott D.,Symeonidis M.</name></creator><creator><name>Vaccari M.</name></creator><creator><name>Vieira J.D.</name></creator><creator><name>Wang L.</name></creator><creator><name>Wardlow J.</name></creator><creator><name>Zemcov M.</name></creator><date role="Updated">2024-08-18T20:18:54Z</date><date role="Created">2020-04-15T09:51:13Z</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>galaxies</subject><subject>infrared-sources</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><subject>redshifted</subject><description>High-redshift, luminous, dusty star-forming galaxies (DSFGs) constrain the extremity of galaxy formation theories. The most extreme are discovered through follow-up on candidates in large area surveys. Here, we present extensive 850um SCUBA-2 follow-up observations of 188 red DSFG candidates from the Herschel Multitiered Extragalactic Survey (HerMES) Large Mode Survey, covering 274deg^2^. We detected 87% with a signal-to-noise ratio &gt;3 at 850um. We introduce a new method for incorporating the confusion noise in our spectral energy distribution fitting by sampling correlated flux density fluctuations from a confusion limited map. The new 850um data provide a better constraint on the photometric redshifts of the candidates, with photometric redshift errors decreasing from {sigma}_z_/(1+z)~0.21 to 0.15. Comparison spectroscopic redshifts also found little bias (&lt;(z-z_spec_)/(1+z_spec_)&gt;=0.08). The mean photometric redshift is found to be 3.6 with a dispersion of 0.4 and we identify 21 DSFGs with a high probability of lying at z&gt;4. After simulating our selection effects we find number counts are consistent with phenomenological galaxy evolution models. There is a statistically significant excess of WISE-1 and SDSS sources near our red galaxies, giving a strong indication that lensing may explain some of the apparently extreme objects. Nevertheless, our sample includes examples of galaxies with the highest star formation rates in the Universe (&gt;&gt;10^3^M_{sun}_/yr).</description><source format="bibcode">2018MNRAS.477.1099D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/477/1099</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/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/103">VIII/103 : Herschel Multi-tiered Extragalactic Survey (HerMES+, 2012)</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Ahn, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/279">VII/279 : SDSS quasar catalog: twelfth data release (Paris+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/372/1621">J/MNRAS/372/1621 : SCUBA Half-Degree Extragalactic Survey. 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