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<ri:Resource created="2010-03-26T06:12:32Z" 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>Optical photometry of the ONC</title><shortName>J/ApJS/183/261</shortName><identifier>ivo://CDS.VizieR/J/ApJS/183/261</identifier><altIdentifier>doi:10.26093/cds/vizier.21830261</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Da Rio N.</name></creator><creator><name>Robberto M.</name></creator><creator><name>Soderblom D.R.</name></creator><creator><name>Panagia N.</name></creator><creator><name>Hillenbrand L.A.,Palla F.</name></creator><creator><name>Stassun K.</name></creator><date role="Updated">2017-09-19T14:21:47Z</date><date role="Created">2010-03-26T06:12:32Z</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>visible-astronomy</subject><subject>h-alpha-photometry</subject><subject>infrared-photometry</subject><subject>broad-band-photometry</subject><subject>line-intensities</subject><subject>m-stars</subject><subject>surveys</subject><subject>stellar-spectral-types</subject><description>We present U, B, V, I broadband, 6200{AA} TiO medium band, and H{alpha} narrow band photometry of the Orion Nebula Cluster (ONC) obtained with the WFI imager at the ESO/MPI 2.2 telescope at La Silla Observatory. The nearly simultaneous observations cover the entire ONC in a field of about 34x34arcmin^2^. They enable us to determine stellar colors avoiding the additional scatter in the photometry induced by stellar variability typical of pre-main-sequence stars. We identify 2612 point-like sources in the I band; 58%, 43%, and 17% of them are also detected in V, B, and U, respectively. 1040 sources are identified in the H{alpha} band. In this paper we present the observations, the calibration techniques adopted, and the resulting catalog. We show the derived color-magnitude diagram of the population and discuss the completeness of our photometry. We define a spectrophotometric TiO index that takes into account the fluxes in the V, I, and TiO bands. Comparing it with spectral types of ONC members in the literature, we find a correlation between the index and the spectral type valid for M-type stars, which is accurate to better than 1 spectral subclass for M3-M6 types and better than 2 spectral subclasses for M0-M2 types. This allows us to newly classify 217 stars.</description><source format="bibcode">2009ApJS..183..261D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/183/261</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/AJ/113/1733">J/AJ/113/1733 : Orion Nebula Cluster population (Hillenbrand 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/1676">J/AJ/121/1676 : ONC low-mass stars photometry (Rebull+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/574/258">J/ApJ/574/258 : Orion nebula X-ray-emitting young stars (Feigelson+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/160/353">J/ApJS/160/353 : Membership of the Orion nebula population (Getman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/660/704">J/ApJ/660/704 : Optical and X-ray variability of ONC PMS (Stassun+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/660/1462">J/ApJ/660/1462 : Abundances of ONC X-ray PMS stars (Maggio+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/502/883">J/A+A/502/883 : I phot. of very low mass ONC stars (Rodriguez-Ledesma+, 2009)</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/ApJS/183/261</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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