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<ri:Resource created="2018-05-14T09:42:49Z" 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>Spectroscopy of the foreground population in Orion A</title><shortName>J/AJ/153/188</shortName><identifier>ivo://CDS.VizieR/J/AJ/153/188</identifier><altIdentifier>doi:10.26093/cds/vizier.51530188</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fang M.</name></creator><creator><name>Kim J.S.</name></creator><creator><name>Pascucci I.</name></creator><creator><name>Apai D.</name></creator><creator><name>Zhang L.</name></creator><creator><name>Sicilia-Aguilar A.,Alonso-Martinez M.</name></creator><creator><name>Eiroa C.</name></creator><creator><name>Wang H.</name></creator><date role="Updated">2019-08-20T06:51:16Z</date><date role="Created">2018-05-14T09:42:49Z</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>stellar-associations</subject><subject>young-stellar-objects</subject><subject>accretion</subject><subject>spectroscopy</subject><subject>stellar-spectral-types</subject><subject>line-intensities</subject><subject>extinction</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><description>We perform a spectroscopic survey of the foreground population in Orion A with MMT/Hectospec. We use these data, along with archival spectroscopic data and photometric data, to derive spectral types, extinction values, and masses for 691 stars. Using the Spitzer Space Telescope data, we characterize the disk properties of these sources. We identify 37 new transition disk (TD) objects, 1 globally depleted disk candidate, and 7 probable young debris disks. We discover an object with a mass of less than 0.018-0.030 M_{sun}_, which harbors a flaring disk. Using the H{alpha} emission line, we characterize the accretion activity of the sources with disks, and confirm that the fraction of accreting TDs is lower than that of optically thick disks (46%+/-7% versus 73%+/-9%, respectively). Using kinematic data from the Sloan Digital Sky Survey and APOGEE INfrared Spectroscopy of the Young Nebulous Clusters program (IN-SYNC), we confirm that the foreground population shows similar kinematics to their local molecular clouds and other young stars in the same regions. Using the isochronal ages, we find that the foreground population has a median age of around 1-2 Myr, which is similar to that of other young stars in Orion A. Therefore, our results argue against the presence of a large and old foreground cluster in front of Orion A.</description><source format="bibcode">2017AJ....153..188F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/153/188</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/J/A+AS/123/329">J/A+AS/123/329 : New weak-line T Tauri stars in Lupus (Krautter+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/602/816">J/ApJ/602/816 : Chamaeleon I star-forming region census (Luhman, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1733">J/AJ/130/1733 : Optical spectroscopy of {rho} Oph stars (Wilking+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/460/695">J/A+A/460/695 : Search for Associations Containing Young stars (Torres+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/866">J/AJ/132/866 : New M dwarfs in solar neighborhood (Riaz+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2524">J/AJ/133/2524 : Spectra of young nearby stars (White+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/667/308">J/ApJ/667/308 : Weak-line T Tauri in Spitzer c2d Survey. 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