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<ri:Resource created="2021-12-07T07:23:53Z" 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>Speckle observations TESS exoplanet host stars. II.</title><shortName>J/AJ/162/75</shortName><identifier>ivo://CDS.VizieR/J/AJ/162/75</identifier><altIdentifier>doi:10.26093/cds/vizier.51620075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lester K.V.</name></creator><creator><name>Matson R.A.</name></creator><creator><name>Howell S.B.</name></creator><creator><name>Furlan E.</name></creator><creator><name>Gnilka C.L.</name></creator><creator><name>Scott N.J.,Ciardi D.R.</name></creator><creator><name>Everett M.E.</name></creator><creator><name>Hartman Z.D.</name></creator><creator><name>Hirsch L.A.</name></creator><date role="Updated">2023-06-07T09:19:13Z</date><date role="Created">2021-12-07T07:23:53Z</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>multiple-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>interferometry</subject><subject>effective-temperature</subject><description>We present high-angular-resolution imaging observations of 517 host stars of TESS exoplanet candidates using the 'Alopeke and Zorro speckle cameras at Gemini North and South. The sample consists mainly of bright F, G, K stars at distances of less than 500pc. Our speckle observations span angular resolutions of ~20mas out to 1.2", yielding spatial resolutions of &lt;10-500au for most stars, and our contrast limits can detect companion stars 5-9mag fainter than the primary at optical wavelengths. We detect 102 close stellar companions and determine the separation, magnitude difference, mass ratio, and estimated orbital period for each system. Our observations of exoplanet host star binaries reveal that they have wider separations than field binaries, with a mean orbital semimajor axis near 100 au. Other imaging studies have suggested this dearth of very closely separated binaries in systems which host exoplanets, but incompleteness at small separations makes it difficult to disentangle unobserved companions from a true lack of companions. With our improved angular resolution and sensitivity, we confirm that this lack of close exoplanet host binaries is indeed real. We also search for a correlation between planetary orbital radii versus binary star separation; but, given the very short orbital periods of the TESS planets, we do not find any clear trend. We do note that in exoplanet systems containing binary host stars, there is an observational bias against detecting Earth-size planet transits due to transit depth dilution caused by the companion star.</description><source format="bibcode">2021AJ....162...75L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/162/75</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/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><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 stellar multip. on planetary systems I. 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