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<ri:Resource created="2016-10-20T12:28:12Z" 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>ALMA and GeMS observations of the OMC1 region</title><shortName>J/ApJ/826/16</shortName><identifier>ivo://CDS.VizieR/J/ApJ/826/16</identifier><altIdentifier>doi:10.26093/cds/vizier.18260016</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Eisner J.A.</name></creator><creator><name>Bally J.M.</name></creator><creator><name>Ginsburg A.</name></creator><creator><name>Sheehan P.D.</name></creator><date role="Updated">2019-04-01T15:24:46Z</date><date role="Created">2016-10-20T12:28:12Z</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>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>infrared-photometry</subject><subject>stellar-masses</subject><subject>young-stellar-objects</subject><description>We present ALMA observations of the Orion Nebula that cover the OMC1 outflow region. Our focus in this paper is on compact emission from protoplanetary disks. We mosaicked a field containing ~600 near-IR-identified young stars, around which we can search for sub-millimeter emission tracing dusty disks. Approximately 100 sources are known proplyds identified with the Hubble Space Telescope. We detect continuum emission at 1mm wavelengths toward ~20% of the proplyd sample, and ~8% of the larger sample of near-IR objects. The noise in our maps allows 4{sigma} detection of objects brighter than ~1.5mJy, corresponding to protoplanetary disk masses larger than 1.5M_J_ (using standard assumptions about dust opacities and gas-to-dust ratios). None of these disks are detected in contemporaneous CO(2-1) or C^18^O(2-1) observations, suggesting that the gas-to-dust ratios may be substantially smaller than the canonical value of 100. Furthermore, since dust grains may already be sequestered in large bodies in Orion Nebula cluster (ONC) disks, the inferred masses of disk solids may be underestimated. Our results suggest that the distribution of disk masses in this region is compatible with the detection rate of massive planets around M dwarfs, which are the dominant stellar constituent in the ONC.</description><source format="bibcode">2016ApJ...826...16E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/826/16</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/ApJ/814/130">J/ApJ/814/130 : Planet occurrence rates calculated for KOIs (Mulders+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/579/A130">J/A+A/579/A130 : Near-IR BN/KL outflow images (Bally+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/802/77">J/ApJ/802/77 : Protoplanetary disk masses in NGC 2024 cluster (Mann+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/782/8">J/ApJ/782/8 : Spectroscopy of 104 objects in the ONC (Ingraham+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/435/1671">J/MNRAS/435/1671 : SCUBA-2 850um survey in {sigma}Ori cluster (Williams+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/85">J/AJ/146/85 : Spectral types of optical stars in ONC (Hillenbrand+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/771/129">J/ApJ/771/129 : Submillimetric Class II sources of Taurus (Andrews+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/123/412">J/PASP/123/412 : Exoplanet Orbit Database (Wright+, 2011)</relatedResource><relatedResource 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1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/1733">J/AJ/113/1733 : Orion Nebula Cluster population (Hillenbrand 1997)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/826/16</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/826/16</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/826/16</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/826/16</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/826/16</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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