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<ri:Resource created="2022-05-09T08:04:41Z" 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>THYME. VI. TOI-1227 radial velocity</title><shortName>J/AJ/163/156</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/156</identifier><altIdentifier>doi:10.26093/cds/vizier.51630156</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mann A.W.</name></creator><creator><name>Wood M.L.</name></creator><creator><name>Schmidt S.P.</name></creator><creator><name>Barber M.G.</name></creator><creator><name>Owen J.E.,Tofflemire B.M.</name></creator><creator><name>Newton E.R.</name></creator><creator><name>Mamajek E.E.</name></creator><creator><name>Bush J.L.</name></creator><creator><name>Mace G.N.,Kraus A.L.</name></creator><creator><name>Thao P.C.</name></creator><creator><name>Vanderburg A.</name></creator><creator><name>Llama J.</name></creator><creator><name>Johns-krull C.M.</name></creator><creator><name>Prato L.,Stahl A.G.</name></creator><creator><name>Tang S.-Y.</name></creator><creator><name>Fields M.J.</name></creator><creator><name>Collins K.A.</name></creator><creator><name>Collins K.I.</name></creator><creator><name>Gan T.,Jensen E.L.N.</name></creator><creator><name>Kamler J.</name></creator><creator><name>Schwarz R.P.</name></creator><creator><name>Furlan E.</name></creator><creator><name>Gnilka C.L.,Howell S.B.</name></creator><creator><name>Lester K.V.</name></creator><creator><name>Owens D.A.</name></creator><creator><name>Suarez O.</name></creator><creator><name>Mekarnia D.</name></creator><creator><name>Guillot T.,Abe L.</name></creator><creator><name>Triaud A.H.M.J.</name></creator><creator><name>Johnson M.C.</name></creator><creator><name>Milburn R.P.</name></creator><creator><name>Rizzuto A.C.,Quinn S.N.</name></creator><creator><name>Kerr R.</name></creator><creator><name>Ricker G.R.</name></creator><creator><name>Vanderspek R.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Seager S.,Winn J.N.</name></creator><creator><name>Jenkins J.M.</name></creator><creator><name>Guerrero N.M.</name></creator><creator><name>Shporer A.</name></creator><creator><name>Schlieder J.E.,Mclean B.</name></creator><creator><name>Wohler B.</name></creator><date role="Updated">2024-10-11T20:10:11Z</date><date role="Created">2022-05-09T08:04:41Z</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>pre-main-sequence-stars</subject><subject>exoplanets</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><subject>radial-velocity</subject><description>Mature super-Earths and sub-Neptunes are predicted to be ~Jovian radius when younger than 10Myr. Thus, we expect to find 5-15 R{Earth} planets around young stars even if their older counterparts harbor none. We report the discovery and validation of TOI1227b, a 0.85{+/-}0.05R _J_ (9.5R{Earth}) planet transiting a very-low-mass star (0.170{+/-}0.015M{sun}) every 27.4days. TOI 1227's kinematics and strong lithium absorption confirm that it is a member of a previously discovered subgroup in the Lower Centaurus Crux OB association, which we designate the Musca group. We derive an age of 11{+/-}2Myr for Musca, based on lithium, rotation, and the color-magnitude diagram of Musca members. The TESS data and ground-based follow-up show a deep (2.5%) transit. We use multiwavelength transit observations and radial velocities from the IGRINS spectrograph to validate the signal as planetary in nature, and we obtain an upper limit on the planet mass of ~0.5M _J_. Because such large planets are exceptionally rare around mature low-mass stars, we suggest that TOI1227b is still contracting and will eventually turn into one of the more common &lt;5R{Earth} planets.</description><source format="bibcode">2022AJ....163..156M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/156</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/A+A/551/A46">J/A+A/551/A46 : Compiled photometry Cham I &amp; II members (Lopez Marti+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/435/1325">J/MNRAS/435/1325 : Membership of the {eta} Cha association (Murphy+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/81">J/ApJ/788/81 : BANYAN III. RVel and rotation of low-mass stars (Malo+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/573/A126">J/A+A/573/A126 : VLT/NaCo Large program I. Sample (Desidera+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/234">J/AJ/157/234 : ACRONYM. III. Candidate low-mass stars (Schneider+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/65">J/AJ/161/65 : THYME. IV. 3 Exoplanets around TOI-451 B (Newton+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/171">J/AJ/161/171 : THYME. V. 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