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<ri:Resource created="2020-02-20T08:33:02Z" 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>Gaia DR2 x AllWISE catalogue</title><shortName>II/360</shortName><identifier>ivo://CDS.VizieR/II/360</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Marton G.</name></creator><creator><name>Abraham P.</name></creator><creator><name>Szegedi-Elek E.</name></creator><creator><name>Varga J.</name></creator><creator><name>Kun M.</name></creator><creator><name>Kospal A.,Varga-Verebelyi E.</name></creator><creator><name>Hodgkin S.</name></creator><creator><name>Szabados L.</name></creator><creator><name>Beck R.</name></creator><creator><name>Kiss Cs.</name></creator><date role="Updated">2024-01-08T13:57:31Z</date><date role="Created">2020-02-20T08:33:02Z</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>visible-astronomy</subject><subject>narrow-band-photometry</subject><subject>infrared-photometry</subject><subject>astronomical-object-identification</subject><description>The second Gaia Data Release (DR2) contains astrometric and photometric data for more than 1.6 billion objects with mean Gaia G magnitude &lt;20.7, including many Young Stellar Objects (YSOs) in different evolutionary stages. In order to explore the YSO population of the Milky Way, we combined the Gaia DR2 database with WISE and Planck measurements and made an all-sky probabilistic catalogue of YSOs using machine learning techniques, such as Support Vector Machines, Random Forests, or Neural Networks. Our input catalogue contains 103 million objects from the DR2xAllWISE cross-match table. We classified each object into four main classes: YSOs, extragalactic objects, main-sequence stars and evolved stars. At a 90% prob- ability threshold we identified 1 129 295 YSO candidates. To demonstrate the quality and potential of our YSO catalogue, here we present two applications of it. (1) We explore the 3D structure of the Orion A star forming complex and show that the spatial distribution of the YSOs classified by our procedure is in agreement with recent results from the literature. (2) We use our catalogue to classify published Gaia Science Alerts. As Gaia measures the sources at multiple epochs, it can efficiently discover transient events, including sudden brightness changes of YSOs caused by dynamic processes of their circumstellar disk. However, in many cases the physical nature of the published alert sources are not known. A cross-check with our new catalogue shows that about 30% more of the published Gaia alerts can most likely be attributed to YSO activity. The catalogue can be also useful to identify YSOs among future Gaia alerts.</description><source format="bibcode">2019MNRAS.487.2522M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/II/360</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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(LMS)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_LMS</name><description>Error of the LMS probability (LMSerr)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Source</name><description>Gaia DR2 source ID (gid)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RA_ICRS</name><description>Barycentric right ascension (ICRS) at Ep=2015.5 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Barycentric declination (ICRS) at Ep=2015.5 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>LE</name><description>Probability of the source being an evolved star using all WISE bands (LE)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_LE</name><description>Error of the LE probability (LEerr)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LY</name><description>Probability of the source being a YSO using all WISE bands (LY)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_LY</name><description>Error of the LY probability (LYerr)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Gmag</name><description>G-band mean magnitude (Vega) (gmean)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>tau</name><description>353GHz R2.01 Planck dust opacity value (tau)</description><ucd>phys.absorption.coeff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>AllWISE</name><description>AllWISE designation (wid)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType><flag>indexed</flag></column><column><name>RAAdeg</name><description>AllWISE Right ascension (J2000) (raw)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEAdeg</name><description>AllWISE Declination (J2000) (decw)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>W1mag</name><description>AllWISE W1 magnitude (W1mag)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W2mag</name><description>AllWISE W2 magnitude (W2mag)</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W3mag</name><description>AllWISE W3 magnitude (W3mag)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W4mag</name><description>AllWISE W4 magnitude (W4mag)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag</name><description>2MASS J magnitude (Jmag)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>2MASS H magnitude (Hmag)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>2MASS K magnitude (Kmag)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_W1mag</name><description>? AllWISE W1 Magnitude error (e_W1mag)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W2mag</name><description>? AllWISE W2 Magnitude error (e_W2mag)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W3mag</name><description>? AllWISE W3 Magnitude error (e_W3mag)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W4mag</name><description>? AllWISE W4 Magnitude error (e_W4mag)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Jmag</name><description>? 2MASS J magnitude error (e_Jmag)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Hmag</name><description>? 2MASS H magnitude error (e_Hmag)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Kmag</name><description>? 2MASS K magnitude error (e_Kmag)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R</name><description>Probability that WISE W3 and W4 detections are real (R)</description><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SE</name><description>Probability of the source being an evolved star without W3 and W4 WISE bands (SE)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SE</name><description>Error of the SE probability (SEerr)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SEG</name><description>Probability of the source being an extragalactic object without W3 and W4 WISE bands (SEG)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SEG</name><description>Error of the SEG probability (SEGerr)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SMS</name><description>Probability of the source being a main-sequence star without W3 and W4 WISE bands (SMS)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SMS</name><description>Error of the SMS probability (SMSerr)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SY</name><description>Probability of the source being a YSO without W3 and W4 WISE bands (SY)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SY</name><description>Error of the SY probability (SYerr)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>