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<ri:Resource created="2023-07-20T15:30:20Z" status="active" updated="2025-06-13T15:25:00Z" 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>GTC/CanariCam deep MIR survey of stars within 5pc</title><shortName>J/ApJ/923/119</shortName><identifier>ivo://CDS.VizieR/J/ApJ/923/119</identifier><altIdentifier>doi:10.26093/cds/vizier.19230119</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gauza B.</name></creator><creator><name>Bejar V.J.S.</name></creator><creator><name>Rebolo R.</name></creator><creator><name>Alvarez C.</name></creator><creator><name>Zapatero Osorio M.R.,Bihain G.</name></creator><creator><name>Caballero J.A.</name></creator><creator><name>Pinfield D.J.</name></creator><creator><name>Telesco C.M.</name></creator><creator><name>Packham C.</name></creator><date role="Updated">2023-11-03T13:21:31Z</date><date role="Created">2023-07-20T15:30:20Z</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>variable-stars</subject><subject>infrared-sources</subject><subject>visible-astronomy</subject><subject>proper-motions</subject><subject>trigonometric-parallax</subject><subject>surveys</subject><subject>stellar-spectral-types</subject><description>In this work we present the results of a direct imaging survey for brown dwarf companions around the nearest stars at the mid-infrared 10um range ({lambda}_c_=8.7{mu}m, {Delta}{lambda}=1.1{mu}m) using the CanariCam instrument on the 10.4m Gran Telescopio Canarias (GTC). We imaged the 25 nearest stellar systems within 5pc of the Sun at declinations {delta}{&gt;}-25{deg} (at least half have planets from radial-velocity studies), reaching a mean detection limit of 11.3+/-0.2mag (1.5mJy) in the Si-2 8.7{mu}m band over a range of angular separations from 1" to 10". This would have allowed us to uncover substellar companions at projected orbital separations between ~2 and 50au, with effective temperatures down to 600K and masses greater than 30M_Jup_ assuming an average age of 5Gyr and masses down to the deuterium-burning mass limit for objects with ages &lt;1Gyr. From the nondetection of such companions, we determined upper limits on their occurrence rate at depths and orbital separations yet unexplored by deep imaging programs. For the M dwarfs, the main component of our sample, we found with a 90% confidence level that fewer than 20% of these low-mass stars have L- and T-type brown dwarf companions with m&gt;~30M_Jup_ and T_eff_&gt;~600K at ~3.5-35au projected orbital separations.</description><source format="bibcode">2021ApJ...923..119G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/923/119</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/2189">J/AJ/121/2189 : Stars within 8 pc of the Sun (Oppenheimer+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/670/1367">J/ApJ/670/1367 : Gemini Deep Planet Survey (Lafreniere+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/1264">J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/A21">J/A+A/511/A21 : Radial velocities of GJ876 planetary system (Correia+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/719/890">J/ApJ/719/890 : Keck radial velocities of GJ 876 (Rivera+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/141">J/ApJ/743/141 : T dwarf companions around M, L, T dwarfs in IR (Carson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/64">J/AJ/144/64 : Solar neighborhood. 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