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<ri:Resource created="2023-07-05T08:33:42Z" 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>g and i'-band light curve of TOI-5205 with SDSS</title><shortName>J/AJ/165/120</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/120</identifier><altIdentifier>doi:10.26093/cds/vizier.51650120</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kanodia S.</name></creator><creator><name>Mahadevan S.</name></creator><creator><name>Libby-Roberts J.</name></creator><creator><name>Stefansson G.</name></creator><creator><name>Canas C.I.,Piette A.A.A.</name></creator><creator><name>Boss A.</name></creator><creator><name>Teske J.</name></creator><creator><name>Chambers J.</name></creator><creator><name>Zeimann G.</name></creator><creator><name>Monson A.,Robertson P.</name></creator><creator><name>Ninan J.P.</name></creator><creator><name>Lin A.S.J.</name></creator><creator><name>Bender C.F.</name></creator><creator><name>Cochran W.D.,Diddams S.A.</name></creator><creator><name>Gupta A.F.</name></creator><creator><name>Halverson S.</name></creator><creator><name>Hawley S.</name></creator><creator><name>Kobulnicky H.A.,Metcalf A.J.</name></creator><creator><name>Parker B.A.</name></creator><creator><name>Powers L.</name></creator><creator><name>Ramsey L.W.</name></creator><creator><name>Roy A.</name></creator><creator><name>Schwab C.,Swaby T.N.</name></creator><creator><name>Terrien R.C.</name></creator><creator><name>Wisniewski J.</name></creator><date role="Updated">2023-09-27T10:10:46Z</date><date role="Created">2023-07-05T08:33:42Z</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>m-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>We present the discovery of TOI-5205b, a transiting Jovian planet orbiting a solar metallicity M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometry and then confirmed using a combination of precise radial velocities, ground-based photometry, spectra, and speckle imaging. TOI-5205b has one of the highest mass ratios for M-dwarf planets, with a mass ratio of almost 0.3%, as it orbits a host star that is just 0.392{+/-}0.015 M{sun}. Its planetary radius is 1.03{+/-}0.03R_Jup_, while the mass is 1.08{+/-}0.06M_Jup_. Additionally, the large size of the planet orbiting a small star results in a transit depth of ~7%, making it one of the deepest transits of a confirmed exoplanet orbiting a main-sequence star. The large transit depth makes TOI-5205b a compelling target to probe its atmospheric properties, as a means of tracing the potential formation pathways. While there have been radial-velocity-only discoveries of giant planets around mid-M dwarfs, this is the first transiting Jupiter with a mass measurement discovered around such a low-mass host star. The high mass of TOI-5205b stretches conventional theories of planet formation and disk scaling relations that cannot easily recreate the conditions required to form such planets.</description><source format="bibcode">2023AJ....165..120K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/120</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/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/121">VI/121 : Linelist of HCN and HNC (Harris+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/133">VI/133 : A variationally computed hot NH3 line list - BYTe (Yurchenko+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/773">J/AJ/106/773 : Mass-luminosity relation (Henry+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/337/403">J/A+A/337/403 : Low-mass stars evolutionary models (Baraffe+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. 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