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<ri:Resource created="2020-01-14T11:42:23Z" 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>Confirmed members of nearby young moving groups</title><shortName>J/AJ/158/187</shortName><identifier>ivo://CDS.VizieR/J/AJ/158/187</identifier><altIdentifier>doi:10.26093/cds/vizier.51580187</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Baron F.</name></creator><creator><name>Lafreniere D.</name></creator><creator><name>Artigau E.</name></creator><creator><name>Gagne J.</name></creator><creator><name>Rameau J.</name></creator><creator><name>Delorme P.,Naud M.-E.</name></creator><date role="Updated">2020-01-14T10:50:16Z</date><date role="Created">2020-01-14T11:42:23Z</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>stellar-spectral-types</subject><subject>proper-motions</subject><subject>stellar-distance</subject><subject>stellar-masses</subject><subject>exoplanets</subject><description>We present the first statistical analysis of exoplanet direct imaging surveys combining adaptive optics (AO) imaging at small separations with deep seeing-limited observations at large separations allowing us to study the entire orbital separation domain from 5 to 5000 au simultaneously. Our sample of 344 stars includes only confirmed members of nearby young associations and is based on all AO direct-imaging detection limits readily available online, with addition of our own previous seeing-limited surveys. Assuming that the companion distribution in mass and a semimajor axis follows a power-law distribution and adding a dependence on the mass of the host star, such as d^2^{prop.to}fM^{alpha}^a^{beta}^(M_*_/M_{sun}_)^{gamma}^dMda, we constrain the parameters to obtain {alpha}=-0.18_-0.65_^+0.77^, {beta}=-1.43_-0.24_^+0.23^, and {gamma}=0.62_-0.50_^+0.56^ at a 68% confidence level, and we obtain f=0.11_-0.05_^+0.11^ for the overall planet occurrence rate for companions with masses between 1 and 20 M_Jup_ in the range of 5-5000 au. Thus, we find that occurrence of companions is negatively correlated with a semimajor axis and companion mass (marginally) but is positively correlated with the stellar host mass. Our inferred mass distribution is in good agreement with other distributions found previously from direct imaging surveys for planets and brown dwarfs, but is shallower as a function of mass than the distributions inferred by radial velocity surveys of gas giants in the 1-3 au range. This may suggest that planets at these wide and very wide separations represent the low-mass tail of the brown dwarfs and stellar companion distribution rather than an extension of the distribution of the inner planets.</description><source format="bibcode">2019AJ....158..187B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/158/187</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/ApJ/670/1367">J/ApJ/670/1367 : Gemini Deep Planet Survey (Lafreniere+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A52">J/A+A/509/A52 : Search for companions with VLT/NACO (Chauvin+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A9">J/A+A/544/A9 : The International Deep Planet Survey. I. (Vigan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/785/47">J/ApJ/785/47 : Sources around target stars in Upper Scorpius</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/593">J/MNRAS/454/593 : Young moving groups in solar neighbourhood (Bell+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/129">J/AJ/154/129 : PSYM-WIDE: planetary-mass companions to YMG members</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/137">J/AJ/156/137 : Wide-orbit Exoplanet search with IR Direct imaging</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/856/23">J/ApJ/856/23 : BANYAN. XI. 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