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<ri:Resource created="2024-05-28T12:54:18Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Giant Outer Transiting Exoplanet Mass Survey. III.</title><shortName>J/AJ/166/239</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/239</identifier><altIdentifier>doi:10.26093/cds/vizier.51660239</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mann C.R.</name></creator><creator><name>Dalba P.A.</name></creator><creator><name>Lafreniere D.</name></creator><creator><name>Fulton B.J.</name></creator><creator><name>Hebrard G.</name></creator><creator><name>Boisse I.,Dalal S.</name></creator><creator><name>Deleuil M.</name></creator><creator><name>Delfosse X.</name></creator><creator><name>Demangeon O.</name></creator><creator><name>Forveille T.</name></creator><creator><name>Heidari N.,Kiefer F.</name></creator><creator><name>Martioli E.</name></creator><creator><name>Moutou C.</name></creator><creator><name>Endl M.</name></creator><creator><name>Cochran W.D.</name></creator><creator><name>MacQueen P.,Marchis F.</name></creator><creator><name>Dragomir D.</name></creator><creator><name>Gupta A.F.</name></creator><creator><name>Feliz D.L.</name></creator><creator><name>Nicholson B.A.,Ziegler C.</name></creator><creator><name>Villanueva S.J.</name></creator><creator><name>Rowe J.</name></creator><creator><name>Talens G.J.</name></creator><creator><name>Thorngren D.,LaCourse D.</name></creator><creator><name>Jacobs T.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Bieryla A.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Rabus M.,Fetherolf T.</name></creator><creator><name>Hellier C.</name></creator><creator><name>Howell S.B.</name></creator><creator><name>Plavchan P.</name></creator><creator><name>Reefe M.</name></creator><creator><name>Combs D.,Bowen M.</name></creator><creator><name>Wittrock J.</name></creator><creator><name>Ricker G.R.</name></creator><creator><name>Seager S.</name></creator><creator><name>Winn J.N.</name></creator><creator><name>Jenkins J.M.,Barclay T.</name></creator><creator><name>Watanabe D.</name></creator><creator><name>Collins K.A.</name></creator><creator><name>Eastman J.D.</name></creator><creator><name>Ting E.B.</name></creator><date role="Updated">2024-11-06T20:18:21Z</date><date role="Created">2024-05-28T12:54:18Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>Large-scale exoplanet surveys like the Transiting Exoplanet Survey Satellite (TESS) mission are powerful tools for discovering large numbers of exoplanet candidates. Single-transit events are commonplace within the resulting candidate list due to the unavoidable limitation of the observing baseline. These single-transit planets often remain unverified due to their unknown orbital periods and consequent difficulty in scheduling follow-up observations. In some cases, radial velocity (RV) follow up can constrain the period enough to enable a future targeted transit detection. We present the confirmation of one such planet: TOI-2010b. Nearly three years of RV coverage determined the period to a level where a broad window search could be undertaken with the Near-Earth Object Surveillance Satellite, detecting an additional transit. An additional detection in a much later TESS sector solidified our final parameter estimation. We find TOI-2010 b to be a Jovian planet (MP=1.29MJup, RP=1.05RJup) on a mildly eccentric orbit (e=0.21) with a period of P=141.83403 days. Assuming a simple model with no albedo and perfect heat redistribution, the equilibrium temperature ranges from about 360 to 450 K from apastron to periastron. Its wide orbit and bright host star (V=9.85) make TOI-2010b a valuable test bed for future low-insolation atmospheric analysis.</description><source format="bibcode">2023AJ....166..239M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/239</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/312">II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/322">I/322 : UCAC4 Catalogue (Zacharias+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/39">VI/39 : Model Atmospheres (Kurucz, 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/853">J/A+A/505/853 : HD16760 radial velocity curve (Bouchy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/1118">J/ApJ/720/1118 : i-band photometry of HAT-P-16 (Buchhave+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/A+ARV/18.67">J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A75">J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 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/other/Nat/486.375">J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/24">J/AJ/144/24 : The Kepler-INT survey (Greiss+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/805/175">J/ApJ/805/175 : Keck and APF radial velocities of HD7924 (Fulton+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/580/A23">J/A+A/580/A23 : Stroemgren-Crawford uvbybeta photometry cat (Paunzen, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/89">J/ApJ/821/89 : 12yrs radial velocity obs. of exoplanet systems (Bryan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/831/64">J/ApJ/831/64 : Mass-metallicity relation for giant planets (Thorngren+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/222/14">J/ApJS/222/14 : Planetary candidates from 1st yr K2mission (Vanderburg+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/17">J/ApJ/834/17 : Mass &amp; radius of planets, moons, low mass stars (Chen+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/600/A30">J/A+A/600/A30 : Limb-darkening for TESS satellite (Claret, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/107">J/AJ/154/107 : California-Kepler Survey. 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