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<ri:Resource created="2014-04-28T08:26:16Z" 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>Classification of sources from the 2XMMi-DR3 cat.</title><shortName>J/ApJ/756/27</shortName><identifier>ivo://CDS.VizieR/J/ApJ/756/27</identifier><altIdentifier>doi:10.26093/cds/vizier.17560027</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lin D.</name></creator><creator><name>Webb N.A.</name></creator><creator><name>Barret D.</name></creator><date role="Updated">2017-11-29T11:48:48Z</date><date role="Created">2014-04-28T08:26:16Z</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>x-ray-sources</subject><subject>surveys</subject><subject>astronomical-object-identification</subject><description>We carry out classification of 4330 X-ray sources in the 2XMMi-DR3 catalog. They are selected under the requirement of being a point source with multiple XMM-Newton observations and at least one detection with the signal-to-noise ratio larger than 20. For about one-third of them we are able to obtain reliable source types from the literature. They mostly correspond to various types of stars (611), active galactic nuclei (AGNs, 753), and compact object systems (138) containing white dwarfs, neutron stars, and stellar-mass black holes. We find that about 99% of stars can be separated from other source types based on their low X-ray-to-IR flux ratios and frequent X-ray flares. AGNs have remarkably similar X-ray spectra, with the power-law photon index centered around 1.91+/-0.31, and their 0.2-4.5keV flux long-term variation factors have a median of 1.48, with 98.5% being less than 10. In contrast, 70% of compact object systems can be very soft or hard, highly variable in X-rays, and/or have very large X-ray-to-IR flux ratios, separating them from AGNs. Using these results, we derive a source type classification scheme to classify the other sources and find 644 candidate stars, 1376 candidate AGNs, and 202 candidate compact object systems, whose false identification probabilities are estimated to be about 1%, 3%, and 18%, respectively. There are still 320 sources associated with nearby galaxies and 151 in the Galactic plane, which we expect to be mostly compact object systems or background AGNs. We also have 100 candidate ultraluminous X-ray sources. They are found to be much less variable than other accreting compact objects.</description><source format="bibcode">2012ApJ...756...27L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/756/27</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/B/cb">B/cb : Cataclysmic Binaries, LMXBs, and related objects (Ritter+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/xmm">B/xmm : XMM-Newton Obs. 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F14min</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Significance of flux variation</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_USNOB1</name><description>? 1 if the optical match is bad</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>USNOB1</name><description>? USNO B1.0 Source designation (I/284)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Dxo</name><description>[0/59]? Angular separation between the X-ray position and USNOB1 source</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B1mag</name><description>[-0.2/24.8]? USNOB1 B1 magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R1mag</name><description>[0/25.5]? USNOB1 R1 magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B2mag</name><description>[0/25.2]? USNOB1 B2 magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R2mag</name><description>[0/50]? USNOB1 R2 magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Imag</name><description>[0/19.6]? USNOB1 I magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_2MASS</name><description>? 1 if the IR match is bad</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>2MASS</name><description>? 2MASS PSC Source designation (II/246)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>Dxir</name><description>[0/29]? Angular separation between the X-ray position and 2MASS PSC source</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Jmag</name><description>[-1.5/18.8]? 2MASS J magnitude; 1.2um</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Jmag</name><description>[0/10]? Mean error on J magnitude</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>Hmag</name><description>[-1.9/17.8]? 2MASS H magnitude; 1.6um</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Hmag</name><description>[0/0.7]? Mean error on H magnitude</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Kmag</name><description>[-2.1/17]? 2MASS Ks magnitude; 2.2um</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Kmag</name><description>[0/0.4]? Mean error on Ks magnitude</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>RC3Name</name><description>? RC3 Galaxy name</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RA3deg</name><description>? Right ascension (J2000), from RC3 or NED</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DE3deg</name><description>? Declination (J2000), from RC3 or NED</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>D3</name><description>[0.1/36585]? Angular separation from the RC3 match</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rD3</name><description>? Ratio of angular separation to D25 isophote elliptical radius</description><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>[0.05/232.2]? Distance to the galaxy</description><unit>Mpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lmax</name><description>? Maximum 0.2-12.0 keV luminosity (erg/s)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/756/27/table3</name><description>Source detections and simple fits with an absorbed power law</description><column><name>dof</name><description>? Degrees of freedom</description><ucd>stat.fit.dof</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><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>Source</name><description>[837/262284] Unique source identifier (SRCID)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>Obsno</name><description>Observation identifier</description><ucd>meta.id;obs.param;obs</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>detID</name><description>? Unique detection ID (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>R1</name><description>[0/67.2] R1 MOS1-medium-filter equivalent count rate in 0.2-0.5 keV</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R1</name><description>Error in R1</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R2</name><description>R2 MOS1-medium-filter equivalent count rate in 0.5-1.0 keV</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R2</name><description>Error in R2</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R3</name><description>R3 MOS1-medium-filter equivalent count rate in 1.0-2.0 keV</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R3</name><description>Error in R3</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R4</name><description>R4 MOS1-medium-filter equivalent count rate in 2.0-4.5 keV</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R4</name><description>Error in R4</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R5</name><description>R5 MOS1-medium-filter equivalent count rate in 4.5-12 keV</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R5</name><description>Error in R5</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>chi2</name><description>[0/92]? Reduced {chi}^2^ of fit with absorbed power law (PL)</description><ucd>phys.luminosity;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NH</name><description>[0/20]? Best-fitting column density</description><unit>1e+22cm**-2</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_NH</name><description>? Lower 90% confidence bound of NH</description><unit>1e+22cm**-2</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_NH</name><description>? Upper 90% confidence bound of NH</description><unit>1e+22cm**-2</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gamma</name><description>[-2/10]? Best-fitting PL photon index {Gamma}</description><ucd>meta.code;spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Gamma</name><description>[-2/10]? Lower 90% confidence bound of Gamma</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Gamma</name><description>[-2/10]? Upper 90% confidence bound of Gamma</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Flux</name><description>? Power law fit 0.2-12 keV flux</description><unit>mW.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Flux</name><description>? Lower 90% confidence bound of Flux</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Flux</name><description>? Upper 90% confidence bound of Flux</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>