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<ri:Resource created="2006-10-11T17:44:27Z" 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>0.06&lt;=z&lt;=1.20 galaxies Tully-Fisher relation</title><shortName>J/MNRAS/366/144</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/366/144</identifier><altIdentifier>doi:10.26093/cds/vizier.73660144</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nakamura O.</name></creator><creator><name>Aragon-Salamanca A.</name></creator><creator><name>Milvang-Jensen B.</name></creator><creator><name>Arimoto N.</name></creator><creator><name>Ikuta C.,Bamford S.P.</name></creator><date role="Updated">2024-07-02T20:16:54Z</date><date role="Created">2006-10-11T17:44:27Z</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>redshifted</subject><subject>galaxy-rotation</subject><description>We have carried out spectroscopic observations in four cluster fields using Subaru's FOCAS multislit spectrograph and obtained spectra for 103 bright disc field and cluster galaxies at 0.06&lt;=z&lt;=1.20. 77 of these show emission lines, and 33 provide reasonably secure determinations of the galaxies' rotation velocity. The rotation velocities, luminosities, colours and emission-line properties of these galaxies are used to study the possible effects of the cluster environment on the star formation history of the galaxies.</description><source format="bibcode">2006MNRAS.366..144N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/366/144</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/113/22">J/AJ/113/22 : Tully-Fisher Relation. I. (Giovanelli+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/420/97">J/A+A/420/97 : Tully-Fisher relation at 0.1&lt;z&lt;1.0 (Boehm+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/361/109">J/MNRAS/361/109 : Distant cluster gal. 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