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<ri:Resource created="2009-06-15T11:34:13Z" status="active" updated="2026-03-17T20:04:50Z" 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>Water maser in galactic IRAS sources</title><shortName>J/PASJ/59/1185</shortName><identifier>ivo://CDS.VizieR/J/PASJ/59/1185</identifier><altIdentifier>doi:10.26093/cds/vizier/bj-1v-151</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sunada K.</name></creator><creator><name>Nakazato T.</name></creator><creator><name>Ikeda N.</name></creator><creator><name>Hongo S.</name></creator><creator><name>Kitamura Y.</name></creator><creator><name>Yang J.</name></creator><date role="Updated">2026-03-17T20:04:50Z</date><date role="Created">2009-06-15T11:34:13Z</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>surveys</subject><subject>infrared-sources</subject><subject>astrophysical-masers</subject><subject>radio-astronomy</subject><description>We present H_2_O maser data from a survey toward IRAS sources in the Galaxy with the Nobeyama 45m telescope. This survey had a 1{sigma} noise level as small as 0.24Jy, resulting in one of the most sensitive water-maser surveys. The maximum distance of the masers to be detected by our survey is estimated to be 3kpc for sources with F_nu,1kpc_&lt;10Jy and 10kpc for those with 10Jy&lt;=F_nu,1kpc_&lt;100Jy, where F_nu,1kpc_ is the maser flux density converted at a distance of 1kpc. For strong masers with F_nu,1kpc_&gt;=100Jy, our survey could detect all sources in the Galaxy. We carried out a total of 2229 observations toward 1563 sources and detected water-maser emission toward 222 sources. Our survey newly found masers from 75 of the 222 sources.</description><source format="bibcode">2007PASJ...59.1185S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/59/1185</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/MNRAS/276/57">J/MNRAS/276/57 : IRAS Galactic star-forming regions. II. (Codella+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/115/283">J/A+AS/115/283 : A catalogue of high velocity molecular outflows (Wu+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/53/517">J/PASJ/53/517 : Water maser survey of late-type stars (Takaba+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/426/503">J/A+A/426/503 : Catalogue of high velocity molecular outflows (Wu+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/651/L125">J/ApJ/651/L125 : Water masers associated with IR dark cloud cores (Wang+, 2006)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASJ/59/1185</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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