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<ri:Resource created="2019-10-31T08:36:38Z" 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>Dusty star-forming galaxies with LABOCA 870um obs.</title><shortName>J/ApJ/862/96</shortName><identifier>ivo://CDS.VizieR/J/ApJ/862/96</identifier><altIdentifier>doi:10.26093/cds/vizier.18620096</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lewis A.J.R.</name></creator><creator><name>Ivison R.J.</name></creator><creator><name>Best P.N.</name></creator><creator><name>Simpson J.M.</name></creator><creator><name>Weiss A.</name></creator><creator><name>Oteo I.,Zhang Z.-Y.</name></creator><creator><name>Arumugam V.</name></creator><creator><name>Bremer M.N.</name></creator><creator><name>Chapman S.C.</name></creator><creator><name>Clements D.L.,Dannerbauer H.</name></creator><creator><name>Dunne L.</name></creator><creator><name>Eales S.</name></creator><creator><name>Maddox S.</name></creator><creator><name>Oliver S.J.</name></creator><creator><name>Omont A.,Riechers D.A.</name></creator><creator><name>Serjeant S.</name></creator><creator><name>Valiante E.</name></creator><creator><name>Wardlow J.</name></creator><creator><name>van der Werf P.,De Zotti G.</name></creator><date role="Updated">2021-02-23T11:41:09Z</date><date role="Created">2019-10-31T08:36:38Z</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>submillimeter-astronomy</subject><subject>infrared-photometry</subject><subject>stellar-atmospheric-opacity</subject><subject>redshifted</subject><description>We present images obtained with LABOCA of a sample of 22 galaxies selected via their red Herschel SPIRE colors. We aim to see if these luminous, rare, and distant galaxies are signposting dense regions in the early universe. Our 870{mu}m survey covers an area of ~1deg^2^ down to an average rms of 3.9mJy/beam, with our five deepest maps going 2x deeper still. We catalog 86 dusty star-forming galaxies (DSFGs) around our "signposts," detected above a significance of 3.5{sigma}. This implies a 100+/-30% overdensity of S_870_&gt;8.5mJy (or L_FIR_=6.7x10^12^-2.9x10^13^L_{sun}_) DSFGs, excluding our signposts, when comparing our number counts to those in "blank fields." Thus, we are 99.93% confident that our signposts are pinpointing overdense regions in the universe, and 95% [50%] confident that these regions are overdense by a factor of at least &gt;=1.5x[2x]. Using template spectral energy distributions (SEDs) and SPIRE/LABOCA photometry, we derive a median photometric redshift of z=3.2+/-0.2 for our signposts, with an inter-quartile range of z=2.8-3.6, somewhat higher than expected for 850{mu}m selected galaxies. We constrain the DSFGs that are likely responsible for this overdensity to within |{delta}_z_|&lt;=0.65 of their respective signposts. These "associated" DSFGs are radially distributed within (physical) distances of 1.6+/-0.5Mpc from their signposts, have median star formation rates (SFRs) of ~(1.0+/-0.2)x10^3^M_{sun}_/yr (for a Salpeter stellar initial mass function) and median gas reservoirs of ~1.7x10^11^M_{sun}_. These candidate protoclusters have average total SFRs of at least ~(2.3+/-0.5)x10^3^M_{sun}_/yr and space densities of 9x10^-7^Mpc^-3^, consistent with the idea that their constituents may evolve to become massive early-type galaxies in the centers of the rich galaxy clusters we see today.</description><source format="bibcode">2018ApJ...862...96L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/862/96</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/95">VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/563/629">J/ApJ/563/629 : VIK' photo and redshifts of galaxy clusters (Nelson+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/772">J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/621/673">J/ApJ/621/673 : Line indices for 124 early-type galaxies (Thomas+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1288">J/AJ/131/1288 : Composite spectra of early-type galaxies (Bernardi+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/372/1621">J/MNRAS/372/1621 : SCUBA Half-Degree Extragalactic Survey. 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