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<ri:Resource created="2014-01-23T12:40:37Z" 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>The MYStIX IR-Excess Source catalog (MIRES)</title><shortName>J/ApJS/209/31</shortName><identifier>ivo://CDS.VizieR/J/ApJS/209/31</identifier><altIdentifier>doi:10.26093/cds/vizier.22090031</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Povich M.S.</name></creator><creator><name>Kuhn M.A.</name></creator><creator><name>Getman K.V.</name></creator><creator><name>Busk H.A.</name></creator><creator><name>Feigelson E.D.</name></creator><creator><name>Broos P.S.,Townsley L.K.</name></creator><creator><name>King R.R.</name></creator><creator><name>Naylor T.</name></creator><date role="Updated">2014-02-10T15:41:18Z</date><date role="Created">2014-01-23T12:40:37Z</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>infrared-photometry</subject><subject>pre-main-sequence-stars</subject><subject>young-stellar-objects</subject><subject>h-ii-regions</subject><subject>open-star-clusters</subject><description>The Massive Young Star-Forming Complex Study in Infrared and X-rays (MYStIX) project provides a comparative study of 20 Galactic massive star-forming complexes (d=0.4-3.6kpc). Probable stellar members in each target complex are identified using X-ray and/or infrared data via two pathways: X-ray detections of young/massive stars with coronal activity/strong winds or (2) infrared excess (IRE) selection of young stellar objects (YSOs) with circumstellar disks and/or protostellar envelopes. We present the methodology for the second pathway using Spitzer/IRAC, 2MASS, and UKIRT imaging and photometry. Although IRE selection of YSOs is well-trodden territory, MYStIX presents unique challenges. The target complexes range from relatively nearby clouds in uncrowded fields located toward the outer Galaxy (e.g., NGC 2264, the Flame Nebula) to more distant, massive complexes situated along complicated, inner Galaxy sightlines (e.g., NGC 6357, M17). We combine IR spectral energy distribution (SED) fitting with IR color cuts and spatial clustering analysis to identify IRE sources and isolate probable YSO members in each MYStIX target field from the myriad types of contaminating sources that can resemble YSOs: extragalactic sources, evolved stars, nebular knots, and even unassociated foreground/background YSOs. Applying our methodology consistently across 18 of the target complexes, we produce the MYStIX IRE Source (MIRES) Catalog comprising 20719 sources, including 8686 probable stellar members of the MYStIX target complexes. We also classify the SEDs of 9365 IR counterparts to MYStIX X-ray sources to assist the first pathway, the identification of X-ray-detected stellar members.</description><source format="bibcode">2013ApJS..209...31P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/209/31</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/293">II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/27">J/ApJS/209/27 : MYStIX: the Chandra X-ray sources (Kuhn+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/28">J/ApJS/209/28 : MYStIX Wide-Field NIR data: crowded fields (King+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/29">J/ApJS/209/29 : MYStIX: MIR observations and catalogs (Kuhn+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/30">J/ApJS/209/30 : MYStIX: Bayesian matching (Naylor+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/32">J/ApJS/209/32 : MYStIX probable young stars (MPCM) (Broos+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/553/A48">J/A+A/553/A48 : Near-infrared variability in RCW 38 (Doerr+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/10">J/ApJS/194/10 : NIR properties of YSO in the CCCP (Preibisch+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/35">J/ApJ/741/35 : NIR photometry and polarization in NGC 2264 (Kwon+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/714/L285">J/ApJ/714/L285 : YSO candidates in M17 SWex (Povich+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/407/1170">J/MNRAS/407/1170 : IRAC photometry of M8 (Kumar+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/392/1034">J/MNRAS/392/1034 : IZJHKL' photometry of NGC 6611 (Oliveira+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1116">J/AJ/138/1116 : A Spitzer view of NGC 2264 (Sung+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/698/1">J/ApJ/698/1 : Spitzer observations of NGC 2362 (Currie+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/696/1278">J/ApJ/696/1278 : The extended star-forming environment of M17 (Povich+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/488/211">J/A+A/488/211 : Infrared photometry of NGC 1893 (Caramazza+, 2008)</relatedResource><relatedResource 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