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<ri:Resource created="1997-12-09T18:18:55Z" 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>IRAS galaxies behind the Milky Way</title><shortName>J/A+AS/104/529</shortName><identifier>ivo://CDS.VizieR/J/A+AS/104/529</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Takata T.</name></creator><creator><name>Yamada T.</name></creator><creator><name>Saito M.</name></creator><creator><name>Chamaraux P.</name></creator><creator><name>Kazes I.</name></creator><date role="Updated">2018-01-02T13:42:58Z</date><date role="Created">1997-12-09T18:18:55Z</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>infrared-sources</subject><subject>redshifted</subject><description>We made a search for IRAS galaxies behind the Northern Milky Way by infrared selection using IRAS Point Source Catalog and visual inspection on POSS (Palomar Observatory Sky Survey) paper prints, and carried out a redshift survey of the identified objects. This paper presents a catalog of 649 IRAS galaxies with f_60_&gt;=0.6Jy between l=150deg and 240deg at |b|&lt;=15deg, which contains 254 newly identified galaxies and 188 newly measured radial velocities. Due to galactic extinction, our sample is a lower limit sample of the flux limited sample of IRAS galaxies, but it can give some information on the distribution of galaxies in the region perpendicular to the Supergalactic Plane. We confirm two regions with enhanced density at l~160deg, cz~5000km/s and l~190deg, cz~5000km/s and at least two possible voids.</description><source format="bibcode">1994A&amp;AS..104..529T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/104/529</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/II/174">II/174 : IRAS 2Jy Redshift Survey Data File</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/140">VII/140 : Catalog of Galaxies behind the Milky Way (Saito et al., 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