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<ri:Resource created="2021-06-30T08:14:49Z" 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>10 parsec sample in the Gaia era first update</title><shortName>J/A+A/650/A201</shortName><identifier>ivo://CDS.VizieR/J/A+A/650/A201</identifier><altIdentifier>doi:10.26093/cds/vizier.36500201</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Reyle C.</name></creator><creator><name>Jardine K.</name></creator><creator><name>Fouque P.</name></creator><creator><name>Caballero J.A.</name></creator><creator><name>Smart R.L.</name></creator><creator><name>Sozzetti A.</name></creator><date role="Updated">2023-08-25T14:44:53Z</date><date role="Created">2021-06-30T08:14:49Z</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>trigonometric-parallax</subject><subject>proper-motions</subject><subject>infrared-photometry</subject><subject>exoplanets</subject><description>The nearest stars provide a fundamental constraint for our understanding of stellar physics and the Galaxy. The nearby sample serves as an anchor where all objects can be seen and understood with precise data. This work is triggered by the most recent data release of the astrometric space mission Gaia and uses its unprecedented high precision parallax measurements to review the census of objects within 10pc. The first aim of this work was to compile all stars and brown dwarfs within 10pc observable by Gaia and compare it with the Gaia Catalogue of Nearby Stars as a quality assurance test. We complement the list to get a full 10 pc census, including bright stars, brown dwarfs, and exoplanets. We started our compilation from a query on all objects with a parallax larger than 100 mas using the Set of Identifications, Measurements, and Bibliography for Astronomical Data database (SIMBAD). We completed the census by adding companions, brown dwarfs with recent parallax measurements not in SIMBAD yet, and vetted exoplanets. The compilation combines astrometry and photometry from the recent Gaia Early Data Release 3 with literature magnitudes, spectral types, and line-of-sight velocities. We give a description of the astrophysical content of the 10pc sample. We find a multiplicity frequency of around 27%. Among the stars and brown dwarfs, we estimate that around 61% are M stars and more than half of the M stars are within the range from M3.0 V to M5.0 V. We give an overview of the brown dwarfs and exoplanets that should be detected in the next Gaia data releases along with future developments. We provide a catalogue of 541 stars, brown dwarfs, and exoplanets in 339 systems, within 10pc from the Sun. This list is as volume-complete as possible from current knowledge and it provides benchmark stars that can be used, for instance, to define calibration samples and to test the quality of the forthcoming Gaia releases. It also has a strong outreach potential.</description><source format="bibcode">2021A&amp;A...650A.201R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/650/A201</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>https://gruze.org/10pc : This catalog</relatedResource><relatedResource>https://gucds.inaf.it : GUCDS Home Page</relatedResource><relatedResource>https://zenodo.org/record/7576096 : Update description</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/650/A201/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>217.392321472</ra><dec>-62.676075117</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/10 22 131 137 250 309 527 546 684 725 811 1307 1938 2737 2923 3005 3020 3345 3406 3715 3751 3791 3946 4158 4444 4462 4693 4867 4948 5000 5024-5025 5333 5377 5420 5534 5590 5669 5853 6039 6133 6261 6552 6672 6726 6783 6894 6974 7103 7264 7395 7512 8023 8123 8281 8440 8519 8719 8790 9009 9339 9585 9629 9696 10027 10037 10142 10149 10375 10448 10899 11034 11292 11435 11496 11636 11645 11834 11940 12045 12262 12427 12454 12519 12679 12865 13301 13446 13451 13688 13743 13875 13885 14127 14266 14278 14351 14515 14638 14772 14858 14906 15311 15346 15355 15548 15602 15651 15960 16041 16069 16105 16391 16502 16697 16754 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Gaia G band magnitude measured, given only if GCode is 2 or 3</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Gest</name><description>? Gaia G band magnitude estimated, given only if GCode is 10 or 20</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GBPmag</name><description>? Gaia BP band magnitude measured, given only if GCode is 2 or 3</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><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>Seq</name><description>Running number for object</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sys</name><description>Running number for system</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name of the system</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><column><name>ObjType</name><description>Type of the object (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>ObjName</name><description>Name of the object</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><column><name>RAICRS</name><description>Right ascension in ICRS at Epoch</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEICRS</name><description>Declination in ICRS at Epoch</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Epoch</name><description>Epoch for position</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>Parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_plx</name><description>? Parallax uncertainty</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_plx</name><description>Reference for the parallax</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="31*">char</dataType></column><column><name>pmRA</name><description>? Proper motion in right ascension, pmRA*cosDE</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_pmRA</name><description>? Proper motion uncertainty in right ascension</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>pmDE</name><description>? 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Line-of-sight velocity uncertainty</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_RV</name><description>Reference for line-of-sight velocity</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>SpType</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>r_SpType</name><description>Reference for spectral type</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>SpMethod</name><description>Method used to derive the spectral type</description><ucd>meta.code;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>GCode</name><description>[2/20]? Code for Gmag origin (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GRPmag</name><description>? Gaia RP band magnitude measured, given only if GCode is 2 or 3</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Umag</name><description>? U band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Bmag</name><description>? B band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vmag</name><description>? V band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rmag</name><description>? R band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Imag</name><description>? I band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Jmag</name><description>? J band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Hmag</name><description>? H band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ksmag</name><description>? 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