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<ri:Resource created="2024-06-25T08:15:00Z" 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>TOI-421 light and velocity curves</title><shortName>J/A+A/686/A301</shortName><identifier>ivo://CDS.VizieR/J/A+A/686/A301</identifier><altIdentifier>doi:10.26093/cds/vizier.36860301</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Krenn A.F.</name></creator><creator><name>Kubyshkina D.</name></creator><creator><name>Fossati L.</name></creator><creator><name>Egger J.A.</name></creator><creator><name>Bonfanti A.</name></creator><creator><name>Deline A.,Ehrenreich D.</name></creator><creator><name>Beck M.</name></creator><creator><name>Benz W.</name></creator><creator><name>Cabrera J.</name></creator><creator><name>Wilson T.G.</name></creator><creator><name>Leleu A.,Sousa S.G.</name></creator><creator><name>Adibekyan V.</name></creator><creator><name>Correia A.C.M.</name></creator><creator><name>Alibert Y.</name></creator><creator><name>Delrez L.</name></creator><creator><name>Lendl M.,Patel J.A.</name></creator><creator><name>Venturini J.</name></creator><creator><name>Alonso R.</name></creator><creator><name>Anglada G.</name></creator><creator><name>Asquier J.</name></creator><creator><name>Barczy T.,Barrado Navascues D.</name></creator><creator><name>Barros S.C.C.</name></creator><creator><name>Baumjohann W.</name></creator><creator><name>Beck T.</name></creator><creator><name>Billot N.,Bonfils X.</name></creator><creator><name>Borsato L.</name></creator><creator><name>Brandeker A.</name></creator><creator><name>Broeg C.</name></creator><creator><name>Charnoz S.,Collier Cameron A.</name></creator><creator><name>Csizmadia Sz.</name></creator><creator><name>Cubillos P.E.</name></creator><creator><name>Davies M.B.</name></creator><creator><name>Deleuil M.,Demangeon O.D.S.</name></creator><creator><name>Demory B.-O.</name></creator><creator><name>Erikson A.</name></creator><creator><name>Fortier A.</name></creator><creator><name>Fridlund M.,Gandolfi D.</name></creator><creator><name>Gillon M.</name></creator><creator><name>Guedel M.</name></creator><creator><name>Guenther M.N.</name></creator><creator><name>Hasiba J.</name></creator><creator><name>Heitzmann A.,Helling C.</name></creator><creator><name>Hoyer S.</name></creator><creator><name>Isaak K.G.</name></creator><creator><name>Kiss L.L.</name></creator><creator><name>Lam K.W.F.</name></creator><creator><name>Laskar J.,Lecavelier des Etangs A.</name></creator><creator><name>Lovis C.</name></creator><creator><name>Magrin D.</name></creator><creator><name>Maxted P.F.L.</name></creator><creator><name>Mordasini C.,Nascimbeni V.</name></creator><creator><name>Olofsson G.</name></creator><creator><name>Ottensamer R.</name></creator><creator><name>Pagano I.</name></creator><creator><name>Palle E.</name></creator><creator><name>Peter G.,Piotto G.</name></creator><creator><name>Pollacco D.</name></creator><creator><name>Queloz D.</name></creator><creator><name>Ragazzoni R.</name></creator><creator><name>Rando N.</name></creator><creator><name>Rauer H.,Ribas I.</name></creator><creator><name>Rieder M.</name></creator><creator><name>Santos N.C.</name></creator><creator><name>Scandariato G.</name></creator><creator><name>Segransan D.</name></creator><creator><name>Simon A.E.,Smith A.M.S.</name></creator><creator><name>Stalport M.</name></creator><creator><name>Steller M.</name></creator><creator><name>Szabo Gy.M.</name></creator><creator><name>Thomas N.</name></creator><creator><name>Udry S.,Ulmer B.</name></creator><creator><name>Van Grootel V.</name></creator><creator><name>Villaver E.</name></creator><creator><name>Viotto V.</name></creator><creator><name>Walton N.A.</name></creator><creator><name>Zingales T.</name></creator><date role="Updated">2024-11-21T20:01:15Z</date><date role="Created">2024-06-25T08:15:00Z</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>photometry</subject><subject>visible-astronomy</subject><subject>radial-velocity</subject><description>The TOI-421 planetary system contains two sub-Neptune-type planets (Pb~5.2-days, T_eq,b_~900K, and Pc~16.1-days, T_eq,c_~650K) and is a prime target to study the formation and evolution of planets and their atmospheres. The inner planet is especially interesting as the existence of a hydrogen-dominated atmosphere at its orbital separation cannot be explained by current formation models without previous orbital migration. We aim to improve the system parameters to further use them to model the interior structure and simulate the atmospheric evolution of both planets, to finally gain insights into their formation and evolution. We also investigate the possibility of detecting transit timing variations (TTVs). We jointly analysed photometric data of three TESS sectors and six CHEOPS visits as well as 156 radial velocity data points to retrieve improved planetary parameters. We also searched for TTVs and modelled the interior structure of the planets. Finally, we simulated the evolution of the primordial H-He atmospheres of the planets using two different modelling frameworks. We determine the planetary radii and masses of TOI-421 b and c to be R_b_=2.64+/-0.08R_{Earth}_, M_b_=6.7+/-0.6M_{Earth}_, R_c_=5.09+/-0.07R_{Earth}_, and M_c_=14.1+/-1.4M_{Earth}_. Using these results we retrieved average planetary densities of rho_b_=0.37+/-0.05rho_{Earth}_ and rho_c_=0.107+/-0.012rho_{Earth}_. We do not detect any statistically significant TTV signals. Assuming the presence of a hydrogen-dominated atmosphere, the interior structure modelling results in both planets having extensive envelopes. While the modelling of the atmospheric evolution predicts for TOI-421 b to have lost any primordial atmosphere that it could have accreted at its current orbital position, TOI-421 c could have started out with an initial atmospheric mass fraction somewhere between 10 and 35%. We conclude that the low observed mean density of TOI-421b can only be explained by either a bias in the measured planetary parameters (e.g. driven by high-altitude clouds) and/or in the context of orbital migration. We also find that the results of atmospheric evolution models are strongly dependent on the employed planetary structure model.</description><source format="bibcode">2024A&amp;A...686A.301K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/686/A301</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/J/AJ/160/114">J/AJ/160/114 : Radial velocity monitoring of TOI-421 (Carleo+, 2020)</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/686/A301</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/686/A301</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/686/A301</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/686/A301</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/686/A301</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/686/A301</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/686/A301/cheops1</name><description>Raw CHEOPS photometric time series with auxiliary detrending vectors</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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