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<ri:Resource created="2013-04-19T09:52:48Z" 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>Spectroscopy of galaxy clusters to find LCBGs</title><shortName>J/ApJ/741/98</shortName><identifier>ivo://CDS.VizieR/J/ApJ/741/98</identifier><altIdentifier>doi:10.26093/cds/vizier.17410098</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Crawford S.M.</name></creator><creator><name>Wirth G.D.</name></creator><creator><name>Bershady M.A.</name></creator><creator><name>Hon K.</name></creator><date role="Updated">2017-10-09T13:34:27Z</date><date role="Created">2013-04-19T09:52:48Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>photometry</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>surveys</subject><description>We used the DEIMOS spectrograph on the Keck II Telescope to obtain spectra of galaxies in the fields of five distant, rich galaxy clusters over the redshift range 0.5&lt;z&lt;0.9 in a search for luminous compact blue galaxies (LCBGs). Unlike traditional studies of galaxy clusters, we preferentially targeted blue cluster members identified via multi-band photometric pre-selection based on imaging data from the WIYN telescope. Of the 1288 sources that we targeted, we determined secure spectroscopic redshifts for 848 sources, yielding a total success rate of 66%. Our redshift measurements are in good agreement with those previously reported in the literature, except for 11 targets which we believe were previously in error. Within our sample, we confirm the presence of 53 LCBGs in the five galaxy clusters.</description><source format="bibcode">2011ApJ...741...98C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/741/98</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/ApJS/199/23">J/ApJS/199/23 : IR and UV star formation in ACCEPT BCGs (Hoffer+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/280">J/ApJS/188/280 : Spectroscopic catalog in 24 clusters (Stern+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/724/714">J/ApJ/724/714 : Velocity dispersions of MS1054-03 + Coma gal. 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