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<ri:Resource created="2013-06-13T12:46:05Z" 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>Deep infrared photometry of {sigma} Ori cluster</title><shortName>J/ApJ/743/64</shortName><identifier>ivo://CDS.VizieR/J/ApJ/743/64</identifier><altIdentifier>doi:10.26093/cds/vizier.17430064</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bejar V.J.S.</name></creator><creator><name>Zapatero Osorio M.R.</name></creator><creator><name>Rebolo R.</name></creator><creator><name>Caballero J.A.</name></creator><creator><name>Barrado D.,Martin E.L.</name></creator><creator><name>Mundt R.</name></creator><creator><name>Bailer-Jones C.A.L.</name></creator><date role="Updated">2017-07-06T06:26:17Z</date><date role="Created">2013-06-13T12:46:05Z</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>infrared-photometry</subject><subject>surveys</subject><description>We present a deep I, Z photometric survey covering a total area of 1.12deg^2^ of the {sigma} Orionis cluster and reaching completeness magnitudes of I=22 and Z=21.5mag. From I, I-Z color-magnitude diagrams we have selected 153 candidates that fit the previously known sequence of the cluster. They have magnitudes in the range I=16-23mag, which corresponds to a mass interval from 0.1 down to 0.008M_{sun}_ at the most probable age of {sigma} Orionis (2-4Myr). Using J-band photometry, we find that 124 of the 151 candidates within the completeness of the optical survey (82%) follow the previously known infrared photometric sequence of the cluster and are probably members. We have studied the spatial distribution of the very low mass stars and brown dwarf population of the cluster and found that there are objects located at distances greater than 30 arcmin to the north and west of {sigma} Orionis that probably belong to different populations of the Orion's Belt. For the 102 bona fide {sigma} Orionis cluster member candidates, we find that the radial surface density can be represented by a decreasing exponential function ({sigma}={sigma}_0_e^-r/r_0_^) with a central density of {sigma}_0_=0.23+/-0.03 objects arcmin^-2^ and a characteristic radius of r_0_=9.5+/-0.7 arcmin. Using near-infrared JHK-band data from Two Micron All Sky Survey and UKIRT Deep Infrared Sky Survey and mid-infrared data from Infrared Array Camera/Spitzer, we find that about 5%-9% of the brown dwarf candidates in the {sigma} Orionis cluster have K-band excesses and 30%+/-7% of them show mid-infrared excesses at wavelengths longer than 5.8um. These are probably related to the presence of disks, most of which are "transition disks".</description><source format="bibcode">2011ApJ...743...64B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/743/64</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/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/191/389">J/ApJS/191/389 : Photometric monitoring in {sigma} Ori cluster (Cody+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/931">J/A+A/493/931 : MAD observations of {sigma} Ori (Bouy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/478/667">J/A+A/478/667 : The Mayrit catalogue (Caballero, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/488/167">J/A+A/488/167 : Low-mass stars in {sigma} Ori and {lambda} Ori (Sacco+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/688/362">J/ApJ/688/362 : Disks around brown dwarfs in sigma Ori cluster (Luhman+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/485/931">J/A+A/485/931 : Young stars and brown dwarfs in Ori OB1b (Caballero+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/466/917">J/A+A/466/917 : Brightest stars of sigma Orionis cluster (Caballero+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/356/1583">J/MNRAS/356/1583 : Sigma Ori low-mass candidate members (Burningham+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/356/89">J/MNRAS/356/89 : sigma Ori low-mass stars (Kenyon+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/2316">J/AJ/128/2316 : BVRIJHKs photometry in sigma Ori cluster (Sherry+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/419/249">J/A+A/419/249 : RJHKs photometry of sigma Ori low-mass stars (Scholz+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/325/705">J/AN/325/705 : RIJHKs of low-mass stars in sigma Ori (Bejar+, 2004)</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/743/64</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Field</name><description>Field name (SO1 to SO4)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Det</name><description>Detector number (D1 to D4)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Name</name><description>Position-based name (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>OName</name><description>Previous name (S Ori NN or MNNNNNNN; &lt;[BZR99] S Ori NN&gt; or &lt;Mayrit NNNNNNN&gt; in Simbad)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Ref</name><description>? 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