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<ri:Resource created="2020-07-29T10:16:58Z" 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>44 and 95GHz observations of class I methanol masers</title><shortName>J/ApJS/248/18</shortName><identifier>ivo://CDS.VizieR/J/ApJS/248/18</identifier><altIdentifier>doi:10.26093/cds/vizier.22480018</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yang W.</name></creator><creator><name>Xu Ye</name></creator><creator><name>Choi Y.K.</name></creator><creator><name>Ellingsen S.P.</name></creator><creator><name>Sobolev A.M.</name></creator><creator><name>Chen Xi</name></creator><creator><name>Li J.,Lu D.</name></creator><date role="Updated">2020-10-09T09:48:01Z</date><date role="Created">2020-07-29T10:16:58Z</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><subject>infrared-sources</subject><subject>interferometry</subject><subject>h-ii-regions</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We report a simultaneous 44 and 95GHz class I methanol maser survey toward 144 sources from the 95GHz class I methanol maser catalog. The observations were made with the three telescopes of the Korean very long baseline interferometry network operating in single-dish mode. The detection rates are 89% at 44GHz and 77% at 95GHz. There are 106 new discoveries at 44GHz. Comparing the previous 95GHz detections with new observations of the same transitions made using the Purple Mountain Observatory 13.7m radio telescope shows no clear evidence of variability on a timescale of six years. Emission from the 44 and 95GHz transitions shows strong correlations in peak velocity, peak flux density, and integrated flux density, indicating that they are likely cospatial. We found that the peak flux density ratio S_pk,95_/S_pk,44_ decreases as the 44GHz peak flux density increases. We found that some class I methanol masers in our sample might be associated with infrared dark clouds, while others are associated with HII regions, indicating that some sources occur at an early stage of high-mass star formation, while others are located toward more evolved sources.</description><source format="bibcode">2020ApJS..248...18Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/248/18</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/125">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/96">VIII/96 : 6-GHz methanol multibeam maser catalogue (Caswell+, 2010-12)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/91/659">J/ApJS/91/659 : Ultracompact HII regions radio images (Kurtz+ 1994)</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><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/314/615">J/A+A/314/615 : Maps of the 36 GHz methanol emission (Liechti+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/308/573">J/A+A/308/573 : Ammonia on YSOs IRAS sources (Molinari+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/336/339">J/A+A/336/339 : VLA obs. of ultracompact HII regions (Molinari+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/301/640">J/MNRAS/301/640 : Ultracompact H II regions studies. 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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 identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>m_Name</name><description>The 44GHz component identifier</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Vpk44</name><description>[-57.7/114.4] The 44GHz peak velocity</description><unit>km/s</unit><ucd>phys.veloc;em.mm.30-50GHz;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vpk44</name><description>[0/0.4] Uncertainty in Vpk44 (1)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DelV44</name><description>[0.2/5.5] The 44GHz line width</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_DelV44</name><description>[0/1.5] Uncertainty in DelV44 (1)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Spk44</name><description>[0.5/335] Peak 44GHz flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.mm.30-50GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Spk44</name><description>[0.2/2.6] Uncertainty in Spk44 (1)</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S44</name><description>[0.3/185] Integrated 44GHz flux density</description><unit>J.km**-1.s**-1</unit><ucd>phot.flux.density;em.mm.30-50GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S44</name><description>[0.1/6.8] Uncertainty in S44 (1)</description><unit>J.km**-1.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>intS44</name><description>[0.4/221.1]? 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Total integrated 95GHz flux density (2)</description><unit>J.km**-1.s**-1</unit><ucd>phot.flux.density;em.mm.50-100GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/248/18/table6</name><description>The IRAS counterparts for 44-GHz class I methanol masers</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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 identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>ASep</name><description>[0/59] Angular separation between Source and IRAS positions</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>IRAS</name><description>IRAS identifier (HHMm+DDMM; B1950)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>F12</name><description>[0.2/78.5] IRAS 12um band flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F25</name><description>[1.6/478.2] IRAS 25um band flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F60</name><description>[13.5/12790] IRAS 60um band flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F100</name><description>[43.8/26780] IRAS 100um band flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>q_F12</name><description>[1/3] Flux quality in F12</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>q_F25</name><description>[1/3] Flux quality in F25</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>q_F60</name><description>[1/3] Flux quality in F60</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>q_F100</name><description>[1/3] Flux quality in F100</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dist</name><description>[0.3/11.7] Distance (1)</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LBol</name><description>[0.1/665.6] Bolometric luminosity of IRAS source (2)</description><unit>1000solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJS/248/18/table8</name><description>Masers that may be associated with HII regions</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Maser identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>ASep</name><description>[2/48] Angular separation of KVN targeted center and WISE HII regions</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>WISE</name><description>WISE HII region identifier</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Rad</name><description>[19/608] WISE radius of HII region</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vel0</name><description>Lower velocity range of class I methanol maser</description><unit>km/s</unit><ucd>phys.veloc;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vel1</name><description>Upper velocity range of class I methanol maser</description><unit>km/s</unit><ucd>phys.veloc;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vrrl</name><description>[-28.2/108.1] RRL velocity of HII regions</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Spkr</name><description>[0.4/0.9]? Peak flux density ratio between 95 and 44GHz methanol masers (S_pk,95_/S_pk,44_)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>