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<ri:Resource created="2026-07-10T08:19:59Z" status="active" updated="2026-08-03T00:00:00Z" 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>SPHERE infrared survey for exoplanets. V.</title><shortName>J/A+A/711/A136</shortName><identifier>ivo://CDS.VizieR/J/A+A/711/A136</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Squicciarini V.</name></creator><creator><name>Desidera S.</name></creator><creator><name>Chauvin G.</name></creator><creator><name>Kiefer F.</name></creator><creator><name>D'Orazi V.,Fontanive C.</name></creator><creator><name>Vigan A.</name></creator><creator><name>Nardiello D.</name></creator><creator><name>Messina S.</name></creator><creator><name>Albert D.</name></creator><creator><name>Bergeon S.,Beuzit J.-L.</name></creator><creator><name>Biller B.</name></creator><creator><name>Boccaletti A.</name></creator><creator><name>Bonavita M.</name></creator><creator><name>Bonnefoy M.,Brandner W.</name></creator><creator><name>Cantalloube F.</name></creator><creator><name>Cheetham A.</name></creator><creator><name>Delorme P.</name></creator><creator><name>Dominik C.</name></creator><creator><name>Feldt M.,Galicher R.</name></creator><creator><name>Gratton R.</name></creator><creator><name>Hagelberg J.</name></creator><creator><name>Henning T.</name></creator><creator><name>Janson M.</name></creator><creator><name>Lagadec E.,Lagrange A.-M.</name></creator><creator><name>Langlois M.</name></creator><creator><name>Lazzoni C.</name></creator><creator><name>Le Coroller H.</name></creator><creator><name>Ligi R.,Maire A.-L.</name></creator><creator><name>Marleau G.-D.</name></creator><creator><name>Menard F.</name></creator><creator><name>Mesa D.</name></creator><creator><name>Meunier N.</name></creator><creator><name>Meyer M.,Mordasini C.</name></creator><creator><name>Moutou C.</name></creator><creator><name>Mueller A.</name></creator><creator><name>Perrot C.</name></creator><creator><name>Samland M.</name></creator><creator><name>Schmid H.M.,Schmidt T.</name></creator><creator><name>Sissa E.</name></creator><creator><name>Turatto M.</name></creator><creator><name>Udry S.</name></creator><creator><name>Zurlo A.</name></creator><creator><name>Abe L.</name></creator><creator><name>Antichi J.,Baruffolo A.</name></creator><creator><name>Baudoz P.</name></creator><creator><name>Baudrand J.</name></creator><creator><name>Bazzon A.</name></creator><creator><name>Blanchard P.</name></creator><creator><name>Bohn A.J.,Carbillet M.</name></creator><creator><name>Carle M.</name></creator><creator><name>Cascone E.</name></creator><creator><name>Charton J.</name></creator><creator><name>Claudi R.</name></creator><creator><name>Costille A.,De Caprio V.</name></creator><creator><name>Delboulbe A.</name></creator><creator><name>Dohlen K.</name></creator><creator><name>Engler N.</name></creator><creator><name>Fantinel D.</name></creator><creator><name>Feautrier P.,Fusco T.</name></creator><creator><name>Gigan P.</name></creator><creator><name>Girard J.H.</name></creator><creator><name>Giro E.</name></creator><creator><name>Gisler D.</name></creator><creator><name>Glueck L.</name></creator><creator><name>Gry C.,Hubin N.</name></creator><creator><name>Hugot E.</name></creator><creator><name>Jaquet M.</name></creator><creator><name>Kasper M.</name></creator><creator><name>Le Mignant D.</name></creator><creator><name>Llored M.,Madec F.</name></creator><creator><name>Magnard Y.</name></creator><creator><name>Martinez P.</name></creator><creator><name>Maurel D.</name></creator><creator><name>Moeller-Nilsson O.,Mouillet D.</name></creator><creator><name>Moulin T.</name></creator><creator><name>Origne A.</name></creator><creator><name>Pavlov A.</name></creator><creator><name>Perret D.</name></creator><creator><name>Petit C.</name></creator><creator><name>Pragt J.,Puget P.</name></creator><creator><name>Rabou P.</name></creator><creator><name>Ramos J.</name></creator><creator><name>Rigal F.</name></creator><creator><name>Rochat S.</name></creator><creator><name>Roelfsema R.</name></creator><creator><name>Rousset G.,Roux A.</name></creator><creator><name>Salasnich B.</name></creator><creator><name>Sauvage J.-F.</name></creator><creator><name>Sevin A.</name></creator><creator><name>Soenke C.</name></creator><creator><name>Stadler E.,Suarez M.</name></creator><creator><name>Wahhaj Z.</name></creator><creator><name>Weber L.</name></creator><creator><name>Wildi F.</name></creator><date role="Updated">2026-07-10T07:21:53Z</date><date role="Created">2026-07-10T08:19:59Z</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>multiple-stars</subject><subject>exoplanets</subject><subject>infrared-astronomy</subject><subject>x-ray-sources</subject><subject>visible-astronomy</subject><subject>proper-motions</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><description>Unbiased surveys of large stellar samples are the prime means through which the prevalence of exoplanets can be derived, and crucial constraints to planet formation models can be set.Direct imaging (DI) is ideally positioned to probe the outer regions (5-300au) of planetary systems, providing complementary information to techniques such as transits and radial velocities. We present the full sample of the SpHere INfrared survey for Exoplanets (SHINE), the second largest DI campaign to date. SHINE observed 460 stars between 2015 and 2023 thanks to the guaranteed time observations (GTO) allocated by ESO to the SPHERE consortium at VLT. The goal of this paper is to homogeneously derive the stellar properties of the targets and to define a subsample of young single hosts to be used as a starting point for the final statistical analysis of the survey. Stellar ages were determined based on kinematic indicators (such as the membership to young moving groups), age diagnostics (lithium abundance, rotation, and activity), and isochrone fitting. A thorough vetting for binarity was undertaken combining astrometric, spectroscopic, and imaging data. A subsample of 333 stars, covering a large extent of stellar ages and masses, was constructed. Selection criteria, global features, as well as the properties of individual stars are reported and discussed.</description><source format="bibcode">2026A&amp;A...711A.136S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/711/A136</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/A+A/651/A70">J/A+A/651/A70 : SHINE sample definition (Desidera+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/651/A71">J/A+A/651/A71 : SHINE II (Langlois+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/697/A99">J/A+A/697/A99 : SHINE IV. 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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>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Age</name><description>[1/6000] Age</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_Age</name><description>[0.5/5000] Lower age</description><unit>Myr</unit><ucd>time.age;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_Age</name><description>[1.8/7000] Upper age</description><unit>Myr</unit><ucd>time.age;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>method</name><description>Method for age determination (1)</description><ucd>stat.fit</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Mass</name><description>[0.18/4.1] Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_Mass</name><description>[0.17/4.04] Lower mass</description><unit>solMass</unit><ucd>phys.mass;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_Mass</name><description>[0.19/4.17] Upper mass</description><unit>solMass</unit><ucd>phys.mass;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Stat</name><description>is the star in the statistical subsample?</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Remarks</name><description>Reason for rejection of the star from the statistical sample (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="43*">char</dataType></column></table><table><name>J/A+A/711/A136/tabled5</name><description>Stellar companions</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>plx</name><description>Parallax</description><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ruweSNR</name><description>? SNR of RUWE from GaiaPMEX</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>pmaSNR</name><description>? SNR of proper motion anomaly from GaiaPMEX</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PMEXbin</name><description>Binarity status according to GaiaPMEX</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>MultType</name><description>[1/3] Multiplicity type: (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>DetMethod</name><description>Detection method (2)</description><ucd>meta.code;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>binn</name><description>Notes on binarity (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Ref</name><description>References (4)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Name2</name><description>Companion name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>Mass2</name><description>? Companion mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Sep2</name><description>? Companion separation</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Sep2au</name><description>Companion separation in au</description><unit>au</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sep2UL</name><description>? Companion separation</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Sep2ULau</name><description>? Companion separation in au</description><unit>au</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Comment2</name><description>Comment on the companion (5)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table></schema></tableset></ri:Resource>