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<ri:Resource created="2005-10-22T23:05:02Z" 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>Velocities of spiral galaxies in distant clusters</title><shortName>J/A+A/422/907</shortName><identifier>ivo://CDS.VizieR/J/A+A/422/907</identifier><altIdentifier>doi:10.26093/cds/vizier.34220907</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jaeger K.</name></creator><creator><name>Ziegler B.L.</name></creator><creator><name>Boehm A.</name></creator><creator><name>Heidt J.</name></creator><creator><name>Moellenhoff C.</name></creator><creator><name>Hopp U.,Mendez R.H.</name></creator><creator><name>Wagner S.</name></creator><date role="Updated">2016-06-29T13:08:22Z</date><date role="Created">2005-10-22T23:05:02Z</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><subject>redshifted</subject><description>We have conducted an observing campaign with the FORS instruments at the ESO-Very Large Telescope to explore the kinematical properties of spiral galaxies in distant galaxy clusters. Our main goal is to analyse transformation - and interaction processes of disk galaxies within the special environment of clusters as compared to the hierarchical evolution of galaxies in the field. Spatially resolved multi object spectra have been obtained for seven galaxy clusters at 0.3&lt;z&lt;0.6 to measure rotation velocities of cluster members. For three of the clusters, Cl 0303+17, Cl 0413-65, and MS 1008-12, for which we presented results including a Tully-Fisher-diagram in Ziegler et al. (2003ApJ...598L..87Z), we describe here in detail the sample selection, observations, data reduction, and data analysis. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster designation (G1)</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>PAA</name><description>Value of PA for Setup A</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PAB</name><description>Value of PA for Setup B</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Galaxy</name><description>Galaxy designation, in the cluster (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Galaxy2</name><description>Name of the object in the other setup, for objects observed in both setups</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z</name><description>? 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