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<ri:Resource created="2024-10-11T12:23:15Z" status="active" updated="2025-11-12T20:03:55Z" 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. X. MELANGE-5 association cand. members</title><shortName>J/AJ/168/41</shortName><identifier>ivo://CDS.VizieR/J/AJ/168/41</identifier><altIdentifier>doi:10.26093/cds/vizier.51680041</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Thao Pa C.</name></creator><creator><name>Mann A.W.</name></creator><creator><name>Barber M.G.</name></creator><creator><name>Kraus A.L.</name></creator><creator><name>Tofflemire B.M.,Bush J.L.</name></creator><creator><name>Wood M.L.</name></creator><creator><name>Collins K.A.</name></creator><creator><name>Vanderburg A.</name></creator><creator><name>Quinn S.N.</name></creator><creator><name>Zhou G.,Newton E.R.</name></creator><creator><name>Ziegler C.</name></creator><creator><name>Law N.</name></creator><creator><name>Barkaoui K.</name></creator><creator><name>Pozuelos F.J.,Timmermans M.</name></creator><creator><name>Gillon M.</name></creator><creator><name>Jehin E.</name></creator><creator><name>Schwarz R.P.</name></creator><creator><name>Gan T.</name></creator><creator><name>Shporer A.,Horne K.</name></creator><creator><name>Sefako R.</name></creator><creator><name>Suarez O.</name></creator><creator><name>Mekarnia D.</name></creator><creator><name>Guillot T.</name></creator><creator><name>Abe L.,Triaud A.H.M.J.</name></creator><creator><name>Radford D.J.</name></creator><creator><name>Lopez Murillo A.I.</name></creator><creator><name>Ricker G.R.</name></creator><creator><name>Winn J.N.,Jenkins J.M.</name></creator><creator><name>Bouma L.G.</name></creator><creator><name>Fausnaugh M.</name></creator><creator><name>Guerrero N.M.</name></creator><creator><name>Kunimoto M.</name></creator><date role="Updated">2025-11-12T20:03:55Z</date><date role="Created">2024-10-11T12:23:15Z</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>stellar-associations</subject><subject>radial-velocity</subject><subject>line-intensities</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>photometry</subject><description>Young (&lt;500Myr) planets are critical to studying how planets form and evolve. Among these young planetary systems, multiplanet configurations are particularly useful, as they provide a means to control for variables within a system. Here, we report the discovery and characterization of a young planetary system, TOI-1224. We show that the planet host resides within a young population we denote as MELANGE-5. By employing a range of age-dating methods-isochrone fitting, lithium abundance analysis, gyrochronology, and Gaia excess variability-we estimate the age of MELANGE-5 to be 210+/-27Myr. MELANGE-5 is situated in close proximity to previously identified younger (80-110Myr) associations, Crius 221 and Theia 424/Volans-Carina, motivating further work to map out the group boundaries. In addition to a planet candidate detected by the TESS pipeline and alerted as a TESS object of interest, TOI-1224 b, we identify a second planet, TOI-1224 c, using custom search tools optimized for young stars (Notch and LOCoR). We find that the planets are 2.10+/-0.09R_{Earth}_ and 2.88+/-0.10R_{Earth}_ and orbit their host star every 4.18 and 17.95 days, respectively. With their bright (K=9.1mag), small (R*=0.44R_{sun}_), and cool (Teff=3326K) host star, these planets represent excellent candidates for atmospheric characterization with JWST.</description><source format="bibcode">2024AJ....168...41T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/41</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/VII/233">VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)</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/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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