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<ri:Resource created="2024-05-13T12:17:00Z" 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>Correspondence TOIs &amp; TESS control stars</title><shortName>J/AJ/167/74</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/74</identifier><altIdentifier>doi:10.26093/cds/vizier.51670074</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Littlefield C.</name></creator><creator><name>Howell S.B.</name></creator><creator><name>Ciardi D.R.</name></creator><creator><name>Lester K.V.</name></creator><creator><name>Everett M.E.,Furlan E.</name></creator><creator><name>Matson R.A.</name></creator><creator><name>Fajardo-Acosta S.B.</name></creator><creator><name>Gnilka C.L.</name></creator><date role="Updated">2024-11-06T20:20:45Z</date><date role="Created">2024-05-13T12:17:00Z</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>exoplanets</subject><subject>interferometry</subject><subject>astrometry</subject><description>The large number of exoplanets discovered with the Transiting Exoplanet Survey Satellite (TESS) means that any observational biases from TESS could influence the derived stellar multiplicity statistics of exoplanet host stars. To investigate this problem, we obtained speckle interferometry of 207 control stars whose properties in the TESS Input Catalog (TIC) closely match those of an exoplanetary host star in the TESS Object of Interest (TOI) catalog, with the objective of measuring the fraction of these stars that have companions within ~1.2". Our main result is the identification of a bias in the creation of the control sample that prevents the selection of binaries with 0.1"&lt;~{rho}&lt;~1.2" and {Delta}mag&lt;~3. This bias is the result of large astrometric residuals that cause binaries with these parameters to fail the quality checks used to create the TIC, which in turn causes them to have incomplete stellar parameters (and uncertainties) in the TIC. Any stellar multiplicity study that relies exclusively upon TIC stellar parameters to identify its targets will struggle to select unresolved binaries in this parameter space. Left uncorrected, this selection bias disproportionately excludes high-mass-ratio binaries, causing the mass-ratio distribution of the companions to deviate significantly from the uniform distribution expected of FGK-type field binaries. After accounting for this bias, the companion rate of the FGK control stars is consistent with the canonical 46%{+/-}2% rate from Raghavan et al., and the mass-ratio distribution agrees with that of binary TOI host stars. There is marginal evidence that the control-star companions have smaller projected orbital separations than TOI host stars from previous studies.</description><source format="bibcode">2024AJ....167...74L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/74</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/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/1">J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/45">J/AJ/141/45 : Speckle observations of HIP stars (Horch+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/19">J/AJ/142/19 : Speckle observations of KOI (Howell+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/745/19">J/ApJ/745/19 : Binary systems in Taurus-Auriga (Kraus+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/8">J/AJ/152/8 : Impact of star multipl on planetary systems I. (Kraus+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/117">J/AJ/153/117 : KOIs companions from high-resolution imaging (Hirsch+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/102">J/AJ/156/102 : TESS Input Catalog and Candidate Target List (Stassun+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/211">J/AJ/157/211 : Unresolved binarie in TESS with speckle imaging (Matson+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/216">J/AJ/157/216 : Star multiplicity rate of Mdwarfs within 25 pc (Winters+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/19">J/AJ/159/19 : SOAR TESS survey. I. (Ziegler+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/254/39">J/ApJS/254/39 : Exoplanet candidates from TESS first 2yr obs (Guerrero+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/134">J/AJ/161/134 : Survey of stellar &amp; planetary comp. within 25pc (Hirsch+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/164">J/AJ/161/164 : Observation of 186 TESS stars with NESSI (WYIN) (Howell+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/162/75">J/AJ/162/75 : Speckle obs TESS exoplanet host stars. II. 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