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<ri:Resource created="2015-06-26T15:17:30Z" status="active" updated="2025-06-13T15:25:00Z" 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 IRS sources in the SMC</title><shortName>J/MNRAS/451/3504</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/451/3504</identifier><altIdentifier>doi:10.26093/cds/vizier.74513504</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ruffle P.M.E.</name></creator><creator><name>Kemper F.</name></creator><creator><name>Jones O.C.</name></creator><creator><name>Sloan G.C.</name></creator><creator><name>Kraemer K.E.</name></creator><creator><name>Woods P.M.,Boyer M.L.</name></creator><creator><name>Srinivasan S.</name></creator><creator><name>Antoniou V.</name></creator><creator><name>Lagadec E.</name></creator><creator><name>Matsuura M.,McDonald I.</name></creator><creator><name>Oliveira J.M.</name></creator><creator><name>Sargent B.A.</name></creator><creator><name>Sewilo M.</name></creator><creator><name>Szczerba R.,van Loon J.T.</name></creator><creator><name>Volk K.</name></creator><creator><name>Zijlstra A.A.</name></creator><date role="Updated">2024-08-15T20:13:54Z</date><date role="Created">2015-06-26T15:17:30Z</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>magellanic-clouds</subject><subject>infrared-sources</subject><subject>young-stellar-objects</subject><subject>h-ii-regions</subject><subject>carbon-stars</subject><subject>supergiant-stars</subject><subject>planetary-nebulae</subject><description>The Magellanic clouds are uniquely placed to study the stellar contribution to dust emission. Individual stars can be resolved in these systems even in the mid-infrared, and they are close enough to allow detection of infrared excess caused by dust. We have searched the Spitzer Space Telescope data archive for all Infrared Spectrograph (IRS) staring-mode observations of the Small Magellanic Cloud (SMC) and found that 209 Infrared Array Camera (IRAC) point sources within the footprint of the Surveying the Agents of Galaxy Evolution in the Small Magellanic Cloud (SAGE-SMC) Spitzer Legacy programme were targeted, within a total of 311 staring mode observations. We classify these point sources using a decision tree method of object classification, based on infrared spectral features, continuum and spectral energy distribution shape, bolometric luminosity, cluster membership and variability information. We find 58 asymptotic giant branch (AGB) stars, 51 young stellar objects (YSOs), 4 post-AGB objects, 22 Red Supergiants (RSGs), 27 stars (of which 23 are dusty OB stars), 24 planetary nebulae (PNe), 10 Wolf-Rayet (WR) stars, 3 HII regions, 3 R Coronae Borealis (R CrB) stars, 1 Blue Supergiant and 6 other objects, including 2 foreground AGB stars. We use these classifications to evaluate the success of photometric classification methods reported in the literature.</description><source format="bibcode">2015MNRAS.451.3504R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/451/3504</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/denis">B/denis : The DENIS database (DENIS Consortium, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/236">II/236 : UBVR CCD survey of the Magellanic clouds (Massey+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/288">II/288 : IRSF Magellanic Clouds Point Source Catalog (Kato+ 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/281">II/281 : 2MASS 6X Point Source Working Database / Catalog (Cutri+ 2006)</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/AJ/123/855">J/AJ/123/855 : Magellanic Clouds Photometric Survey: the SMC (Zaritsky+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/669/327">J/ApJ/669/327 : S3MC: YSOs in N66, in SMC (Simon+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/61/217">J/AcA/61/217 : VI light curves of SMC long-period variables (Soszynski+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/778/15">J/ApJ/778/15 : SAGE-SMC III. 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magnitude in WISE band 4 (22 um)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N3mag</name><description>? magnitude in AKARI band N3 (3.2 um)</description><unit>mag</unit><ucd>phot.mag;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N4mag</name><description>? magnitude in AKARI band N4 (4.1 um)</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S7mag</name><description>? magnitude in AKARI band S7 (7 um)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S11mag</name><description>? magnitude in AKARI band S11 (11 um)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>L15mag</name><description>? magnitude in AKARI band L15 (15 um)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>L24mag</name><description>? magnitude in AKARI band L24 (24 um)</description><unit>mag</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MIPS24</name><description>MIPS-24 counterpart (eHHMMSS.ss+DDMMSS.s, where the epoch 'e' is 1 or 2, 0 for merged)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>[24]</name><description>? magnitude in the MIPS 24-um band</description><unit>mag</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MIPS70</name><description>MIPS-70 counterpart (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>[70]</name><description>? magnitude in the MIPS 70-um band</description><unit>mag</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MIPS160</name><description>MIPS-160 counterpart (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>[160]</name><description>? magnitude in the MIPS 160-um band</description><unit>mag</unit><ucd>phot.flux.density;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M1</name><description>[-8/-1] Absolute bolometric magnitude by interpolation of JHKs, IRAC, MIPS24 photometry</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M2</name><description>[-8/-1]? Absolute bolometric magnitude as M1 but with WISE photometry added</description><unit>mag</unit><ucd>phys.magAbs.bol</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M1s</name><description>[-8/-1] Absolute bolometric magnitude as M1 but with IRS spectrum added</description><unit>mag</unit><ucd>phys.magAbs.bol</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M2s</name><description>[-8/-1]? Absolute bolometric magnitude as M2 with IRS spectrum added</description><unit>mag</unit><ucd>phys.magAbs.bol</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mmcd</name><description>[-7.2/-3.4]? Absolute bolometric magnitude from code of McDonald et al. (2)</description><unit>mag</unit><ucd>phys.magAbs.bol</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lmcd</name><description>[1846/60004]? Luminosity from Mmcd</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Tmcd</name><description>[2025/22125]? Effective temperature determined as Mmcd</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>G09</name><description>Counterpart from Groenewegen et al. 2009 (J/A+A/506/1277)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>P1</name><description>[183/1749]? Pulsation period from Groenewegen et al. 2009 (J/A+A/506/1277)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>LPV</name><description>[1141/17525]? OGLE III variable counterpart (J/AcA/61/217)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>&lt;Imag&gt;</name><description>? Mean I magnitude in OGLE III</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>&lt;Vmag&gt;</name><description>? Mean V magnitude in OGLE III</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Iamp</name><description>[0.02/3.9]? I-band amplitude in OGLE III</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>P2</name><description>[23/1859]? pulsation period from OGLE III</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Cl1</name><description>Colour classification from Boyer et al. (5)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Cl2</name><description>Colour classification from Matsuura et al. (6)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Cl3</name><description>Colour classification from Sewilo et al. (7)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table></schema></tableset></ri:Resource>