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<ri:Resource created="2017-01-04T13:01:16Z" 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>WISE census of YSOs in Canis Major</title><shortName>J/ApJ/827/96</shortName><identifier>ivo://CDS.VizieR/J/ApJ/827/96</identifier><altIdentifier>doi:10.26093/cds/vizier.18270096</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fischer W.J.</name></creator><creator><name>Padgett D.L.</name></creator><creator><name>Stapelfeldt K.L.</name></creator><creator><name>Sewilo M.</name></creator><date role="Updated">2018-10-08T11:57:16Z</date><date role="Created">2017-01-04T13:01:16Z</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>young-stellar-objects</subject><subject>infrared-photometry</subject><description>With the Wide-field Infrared Survey Explorer (WISE), we searched for young stellar objects (YSOs) in a 100deg^2^ region centered on the lightly studied Canis Major star-forming region. Applying stringent magnitude cuts to exclude the majority of extragalactic contaminants, we find 144 Class I candidates and 335 Class II candidates. The sensitivity to Class II candidates is limited by their faintness at the distance to Canis Major (assumed as 1000pc). More than half the candidates (53%) are found in 16 groups of more than four members, including four groups with more than 25 members each. The ratio of Class II to Class I objects, N_II_/N_I_, varies from 0.4 to 8.3 in just the largest four groups. We compare our results to those obtainable with combined Two Micron All Sky Survey and post-cryogenic Spitzer Space Telescope data; the latter approach recovers missing Class II sources. Via a comparison to protostars characterized with the Herschel Space Observatory, we propose new WISE color criteria for flat-spectrum and Class 0 protostars, finding 80 and 7 of these, respectively. The distribution of YSOs in CMa OB1 is consistent with supernova-induced star formation, although the diverse N_II_/N_I_ ratios are unexpected if this parameter traces age and the YSOs are due to the same supernova. Less massive clouds feature larger N_II_/N_I_ ratios, suggesting that initial conditions play a role in determining this quantity.</description><source format="bibcode">2016ApJ...827...96F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/827/96</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/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/5">J/ApJS/224/5 : Herschel Orion Protostar Survey (HOPS): SEDs (Furlan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/100">J/AJ/150/100 : WISE YSO cand. near {sigma} and {lambda} Ori (Koenig+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/787/107">J/ApJ/787/107 : Spatial structure of young stellar clusters. I. (Kuhn+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/45">J/ApJ/772/45 : Hi-GAL obs.: star formation in the 3rd quadrant (Elia+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/36">J/ApJ/767/36 : APEX observations of HOPS protostars (Stutz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/94">J/AJ/145/94 : Protostar luminosities from 2 Spitzer surveys (Dunham+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/547/A49">J/A+A/547/A49 : Herschel EPoS: high-mass overview (Ragan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/18">J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/321">J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/693/L81">J/ApJ/693/L81 : Extinction in star-forming regions (McClure, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/56/313">J/PASJ/56/313 : 13CO survey of Mon + CMa molecular clouds (Kim+, 2004)</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/ApJ/827/96</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/827/96</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/827/96</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/827/96</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/827/96</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/827/96</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/ApJ/827/96/table1 (WISE YSO candidates)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/827/96/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/827/96/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/827/96/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>101.75103</ra><dec>-9.99581</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/5409 5411 5417 5418 5419 5422 6/20948 20952 20977 20981 20983 21515 21518 21537 21539 21540 21542 21548 21550 21551 21560 21562 21633 21634 21635 21641 21642 21643 21648 21649 21651 21653 21657 21658 21659 21660 21662 21665 21666 21667 21680 21681 21683 21684 21685 22020 22021 22023 22032</spatial><spectral>8.157980699529898e-21 1.7003137259100215e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/827/96?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/827/96/table1</name><description>WISE YSO candidates</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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