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<ri:Resource created="2024-08-09T09:06:16Z" 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>BD-14 3065b (TOI-4987b) 2D spectra</title><shortName>J/A+A/688/A120</shortName><identifier>ivo://CDS.VizieR/J/A+A/688/A120</identifier><altIdentifier>doi:10.26093/cds/vizier.36880120</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Subjak J.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Quinn S.N.</name></creator><creator><name>Berlind P.</name></creator><creator><name>Calkins M.L.</name></creator><creator><name>Esquerdo G.A.,Brahm R.</name></creator><creator><name>Caballero J.A.</name></creator><creator><name>Collins K.A.</name></creator><creator><name>Guenther E.</name></creator><creator><name>Janik J.</name></creator><creator><name>Kabath P.,Schwarz R.P.</name></creator><creator><name>Tan T.-G.</name></creator><creator><name>Vanzi L.</name></creator><creator><name>Zambelli R.</name></creator><creator><name>Ziegler C.</name></creator><creator><name>Jenkins J.M.,Mireles I.</name></creator><creator><name>Seager S.</name></creator><creator><name>Shporer A.</name></creator><creator><name>Striegel S.</name></creator><creator><name>Winn J.N.</name></creator><date role="Updated">2024-11-29T20:04:36Z</date><date role="Created">2024-08-09T09:06:16Z</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>spectroscopy</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><description>The present study confirms BD-14 3065b as a transiting planet-brown dwarf in a triple-star system, with a mass near the deuterium-burning boundary. BD-14 3065b has the largest radius observed within the sample of giant planets and brown dwarfs around post-main sequence stars. Its orbital period is 4.3 days and it transits a subgiant F-type star with a mass of M*=1.41+/-0.05M_{sun}_, a radius of R*=2.35+/-0.08R_{sun}_, an effective temperature of Teff=6935+/-90K, and a metallicity of -0.34+/-0.05dex. By combining TESS photometry with high-resolution spectra acquired with the TRES and Pucheros+ spectrographs, we measured a mass of Mp = 12.37+/-0.92M_Jup_ and a radius of Rp = 1.926+/-0.094R_Jup_. Our discussion of potential processes that could be responsible for the inflated radius led us to conclude that deuterium burning is a plausible explanation for the heating taking place in BD-14 3065b's interior. Detections of the secondary eclipse with TESS photometry enabled a precise determination of the eccentricity, ep=0.066+/-0.011, and reveal that BD-14 3065b has a brightness temperature of 3520+/-130K. With its unique characteristics, BD-14 3065b presents an excellent opportunity to study its atmosphere via thermal emission spectroscopy.</description><source format="bibcode">2024A&amp;A...688A.120S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/688/A120</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/688/A120</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/688/A120</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/688/A120</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/688/A120</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/688/A120</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/688/A120</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability><description>Associated data</description><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/688/A120</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/688/A120/list</name><description>List of fits 2D spectra</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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