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<ri:Resource created="1997-12-09T20:40:27Z" 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>Tully-Fisher Relation. I.</title><shortName>J/AJ/113/22</shortName><identifier>ivo://CDS.VizieR/J/AJ/113/22</identifier><altIdentifier>doi:10.26093/cds/vizier.51130022</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Giovanelli R.</name></creator><creator><name>Haynes M.P.</name></creator><creator><name>Herter T.</name></creator><creator><name>Vogt N.P.</name></creator><creator><name>Wegner G.,Salzer J.J.</name></creator><creator><name>Da Costa L.N.</name></creator><creator><name>Freudling W.</name></creator><date role="Updated">2023-04-06T16:50:25Z</date><date role="Created">1997-12-09T20:40:27Z</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>photometry</subject><subject>galaxy-classification-systems</subject><subject>radial-velocity</subject><description>Observational parameters which can be used for redshift-independent distance determination using the Tully-Fisher (TF) technique are given for 782 spiral galaxies in the fields of 24 clusters or groups. I band photometry for the full sample was either obtained by us or compiled from published literature. Rotational velocities are derived either from 21 cm spectra or optical emission line long-slit spectra, and converted to a homogeneous scale. 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