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<ri:Resource created="2009-03-04T15:10:51Z" 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 in Shapley supercluster</title><shortName>J/MNRAS/381/1035</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/381/1035</identifier><altIdentifier>doi:10.26093/cds/vizier.73811035</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Smith R.J.</name></creator><creator><name>Lucey J.R.</name></creator><creator><name>Hudson M.J.</name></creator><date role="Updated">2024-07-05T20:15:31Z</date><date role="Created">2009-03-04T15:10:51Z</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>spectroscopy</subject><description>We present new optical spectroscopy for 342 R&lt;18 galaxies in the Shapley supercluster (and 198 supplementary galaxies), obtained from 8-h integrations with the AAOmega facility at the Anglo-Australian Telescope. We describe the observations and measurements of central velocity dispersion {sigma}, emission-line equivalent widths and absorption-line indices. The distinguishing characteristic of the survey is its coverage of a very wide baseline in velocity dispersion (90 per cent range {sigma}=40-230km/s), while achieving high signal-to-noise ratio throughout (median 60{AA}^-1^ at 5000{AA}). The data quality will enable estimates of Balmer-line ages to better than 20 per cent precision even for the faintest galaxies in the sample. Significant emission at H{alpha} was detected in ~30 per cent of the supercluster galaxies, including ~20 per cent of red-sequence members. Using line-ratio diagnostics, we find that the emission is LINER (low ionization nuclear emission region) like at high luminosity, but driven by star formation in low-luminosity galaxies. To characterize the absorption lines, we use the classical Lick indices in the spectral range 4000-5200{AA}. We introduce a new method for applying resolution corrections to the line-strength indices. We define a subset of galaxies with very low emission contamination, based on the H{alpha} line, and fit the index relations for this subset. The final sample analysed in this paper comprises 232 NFPS-selected galaxies meeting both the emission and the redshift criteria, of which 198 have measured velocity dispersions (i.e. are not unresolved).</description><source format="bibcode">2007MNRAS.381.1035S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/381/1035</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/AJ/110/463">J/AJ/110/463 : Kinematics of the Shapley supercluster (Quintana+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/119/329">J/A+AS/119/329 : VR photometry in the Shapley Supercluster (Slezak+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/120/357">J/A+AS/120/357 : R magnitudes in four ESO fields (Infante+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PASA/16.113">J/other/PASA/16.113 : New structure in Shapley supercluster (Drinkwater+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/312/540">J/MNRAS/312/540 : Redshift survey of intercluster galaxies (Bardelli+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/2541">J/AJ/130/2541 : Core of the Shapley supercluster at 1.4GHz (Miller+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/819">J/A+A/445/819 : Systems of galaxies in Shapley supercluster (Ragone+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1558">J/AJ/128/1558 : NOAO Fundamental Plane Survey (Smith+, 2004)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/381/1035</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/381/1035</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/381/1035</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/381/1035</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/381/1035</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/381/1035</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/381/1035/tables (Basic data, principal and supplementary line-strength indices for the sample galaxies (tables 2, 3 and 4 of the paper))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/381/1035/tables?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/381/1035/tables?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/381/1035/tables?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>200.8704167</ra><dec>-31.7116667</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/10959 6/43831 43835</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/381/1035?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/381/1035/tables</name><description>Basic data, principal and supplementary line-strength indices for the sample galaxies (tables 2, 3 and 4 of the paper)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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