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<ri:Resource created="2012-04-18T15:04:16Z" 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>1.2-mm dust clumps with luminous water masers</title><shortName>J/MNRAS/416/178</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/416/178</identifier><altIdentifier>doi:10.26093/cds/vizier.74160178</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Breen S.L.</name></creator><creator><name>Ellingsen S.P.</name></creator><date role="Updated">2024-07-15T20:16:30Z</date><date role="Created">2012-04-18T15:04:16Z</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>molecular-clouds</subject><subject>radio-astronomy</subject><subject>astrophysical-masers</subject><description>We have conducted a sensitive water maser search with the Australia Telescope Compact Array towards 267 1.2-mm dust clumps presented in the literature. We combine our new observations with previous water maser observations to extend our sample to 294 1.2-mm dust clumps, towards which we detect 165 distinct water maser sites towards 128 1.2-mm dust clumps. Within the fields of our observations, we additionally find four water masers with no apparent associated 1.2-mm dust continuum emission. Our overall detection rate of 44 per cent appears to vary as a function of Galactic longitude. We find that there is an excellent correspondence between the locations of the detected water masers with the peak of the target 1.2-mm dust clump sources. As expected from previous similar studies, the water masers are chiefly detected towards the bigger, brighter and more massive 1.2-mm dust clumps.</description><source format="bibcode">2011MNRAS.416..178B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/416/178</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/363/405">J/MNRAS/363/405 : SIMBA observations of cold cores (Hill+, 2005)</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/416/178</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/416/178</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/416/178</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/416/178</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/416/178</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/416/178</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/416/178/table2 (Target 1.2-mm dust clumps, probability of water maser association, followed by a description of the water maser observations including any detections)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/416/178/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/416/178/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/416/178/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>91.949583</ra><dec>-6.3825</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/21458 28829-28831 28890 28896 28912-28913 28918-28919 29070 29090-29092 29094 29096-29097 29100-29101 29103 29114-29116 29118 29461 29505 29510 29529 29532-29533 29535 30218-30219 30241 30256 30259 30262 30319 30330 30405 30420 37244 37343 37839 37846 37850 37897 37900 37923-37924 37938 38020 41653 41655 41677 41696 41777 41804 42159 42169 43013 43015 43019 43024 43041</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/416/178?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/416/178/table2</name><description>Target 1.2-mm dust clumps, probability of water maser association, followed by a description of the water maser observations including any detections</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>Clump</name><description>1.2mm dust clump name (l, b) [HBM2005] (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RAJ2000</name><description>1.2mm dust clump right ascension (J2000) (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>1.2mm dust clump declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Prob</name><description>Calculated probability of water maser presence (2)</description><ucd>stat.probability;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Inst</name><description>Array and epoch (3)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Maser</name><description>Water maser name (l, b), [HBM2005]</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RA1</name><description>? 1.2mm dust clump right ascension (J2000)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DE1</name><description>? 1.2mm dust clump declination (J2000)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>Sep</name><description>? Separation between water maser and 1.2-mm dust clump peak</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>n_Sep</name><description>[*] * no dust clump reported at this position</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_Sp</name><description>Limit flag for 5{sigma} limit on Sp</description><ucd>meta.code.error;src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Sp</name><description>Water maser peak flux density or 5{sigma} detection limit</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vp</name><description>? Velocity of the water maser peak emission</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vr1</name><description>? Velocity range of either the detected emission or the observed velocity range if no detection</description><unit>km/s</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Vr2</name><description>? Velocity range of either the detected emission or the observed velocity range if no detection</description><unit>km/s</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Int</name><description>? 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