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<ri:Resource created="2007-10-24T16:02:49Z" status="active" updated="2025-06-13T15:25:00Z" 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>Redshifts in equatorial strip</title><shortName>J/AJ/105/1637</shortName><identifier>ivo://CDS.VizieR/J/AJ/105/1637</identifier><altIdentifier>doi:10.26093/cds/vizier.51051637</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Huchra J.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Nicolaci da Costa L.</name></creator><creator><name>Pellegrini P.S.,Willmer C.N.A.</name></creator><date role="Updated">2023-04-06T16:49:26Z</date><date role="Created">2007-10-24T16:02:49Z</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>galaxies</subject><subject>visible-astronomy</subject><subject>radial-velocity</subject><subject>redshifted</subject><description>We present 865 redshifts of galaxies located in the equatorial strip -17.5 deg &lt;= Dec. &lt;= -2.5 deg in the right ascension range 20 h &lt;= R.A. &lt;= 5 h. Redshifts have been obtained for the complete sample of all 833 galaxies in the Morphological Catalog of Galaxies with magnitudes brighter than m = 14.5 (corresponding approximately to m(Zwicky) = 15.0). This sample also includes three galaxies from other sources with more reliable magnitudes, satisfying this limit, and 29 fainter galaxies, usually companions of the galaxies in the magnitude limited sample. 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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>Name</name><description>Name of the galaxy adopting the order NGC, IC, or coordinates as suggested by the IAU</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>RA1950</name><description>Right ascension 1950.0 (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE1950</name><description>Declination 1950.0 (1)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>m(B)</name><description>? 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