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<ri:Resource created="2009-04-15T08:18:19Z" 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>Magnitudes and spectral types in 5 galactic fields</title><shortName>III/230</shortName><identifier>ivo://CDS.VizieR/III/230</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Voroshilov V.I.</name></creator><creator><name>Guseva N.G.</name></creator><creator><name>Kalandadze N.B.</name></creator><creator><name>Kolesnik L.N.,Kuznetsov V.I.</name></creator><creator><name>Metreveli M.D.</name></creator><creator><name>Shapovalov A.N.</name></creator><date role="Updated">2018-02-12T08:45:34Z</date><date role="Created">2009-04-15T08:18:19Z</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>visible-astronomy</subject><subject>photographic-photometry</subject><subject>morgan-keenan-classification</subject><description>This catalog was initially compiled at the Abastumani Observatory, containing photographic BV magnitudes and spectral classes for about 6000 stars up to V(lim)=13.0mag in five circular areas of 18{deg}^2^ located near the galactic-equator plane; the observations were made with the Abastumani 70cm Maksutov plus 4{deg} and 8{deg} prisms, yielding dispersions of 166 and 666 {AA}/mm at H-{gamma}. 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