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<ri:Resource created="2006-07-08T05:20:42Z" 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>Class I and class II methanol masers</title><shortName>J/MNRAS/359/1498</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/359/1498</identifier><altIdentifier>doi:10.26093/cds/vizier.73591498</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ellingsen S.P.</name></creator><date role="Updated">2024-07-01T20:14:40Z</date><date role="Created">2006-07-08T05:20:42Z</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>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>radio-sources</subject><description>The Australia Telescope National Facility Mopra millimetre telescope has been used to search for 95.1-GHz class I methanol masers towards 62 6.6-GHz class II methanol masers. A total of 26 95.1-GHz masers were detected, 18 of these being new discoveries. Combining the results of this search with observations reported in the literature, a near complete sample of 66 6.6-GHz class II methanol masers has been searched in the 95.1-GHz transition, with detections towards 38 per cent (25 detections; not all of the sources studied in this paper qualify for the complete sample, and some of the sources in the sample were not observed in the present observations).</description><source format="bibcode">2005MNRAS.359.1498E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/359/1498</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/A+A/432/737">J/A+A/432/737 : General Catalogue of 6.7GHz Methanol Masers (Pestalozzi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/72/22">J/AZh/72/22 : A 95 GHz Survey of Methanol Masers (Valtts+, 1995)</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/MNRAS/359/1498</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/359/1498</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/359/1498</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/359/1498</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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sources)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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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>Source name, based on galactic position</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>n_Name</name><description>[ab] Note on Name (G1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Vell</name><description>Lower value of velocity range</description><unit>km/s</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Velu</name><description>Upper value of Velocity range</description><unit>km/s</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>3sigma</name><description>3{sigma} rms noise level as measured in the Hanning smoothed spectra</description><unit>Jy</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/359/1498/table3</name><description>Comparison of peak flux density and velocity range of 6.6-GHz class II and 95.1-GHz class I methanol masers</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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