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dc.contributor.authorThao, Pa Chia
dc.contributor.authorMann, Andrew W.
dc.contributor.authorBarber, Madyson G.
dc.contributor.authorKraus, Adam L.
dc.contributor.authorTofflemire, Benjamin M.
dc.contributor.authorBush, Jonathan L.
dc.contributor.authorWood, Mackenna L.
dc.contributor.authorCollins, Karen A.
dc.contributor.authorVanderburg, Andrew
dc.contributor.authorQuinn, Samuel N.
dc.contributor.authorZhou, George
dc.contributor.authorNewton, Elisabeth R.
dc.contributor.authorZiegler, Carl
dc.contributor.authorLaw, Nicholas
dc.contributor.authorBarkaoui, Khalid
dc.contributor.authorPozuelos, Francisco J.
dc.contributor.authorTimmermans, Mathilde
dc.contributor.authorGillon, Michaël
dc.contributor.authorJehin, Emmanuël
dc.contributor.authorSchwarz, Richard P.
dc.contributor.authorGan, Tianjun
dc.contributor.authorShporer, Avi
dc.contributor.authorHorne, Keith
dc.contributor.authorSefako, Ramotholo
dc.contributor.authorSuarez, Olga
dc.contributor.authorMekarnia, Djamel
dc.contributor.authorGuillot, Tristan
dc.contributor.authorAbe, Lyu
dc.contributor.authorTriaud, Amaury H. M. J.
dc.contributor.authorRadford, Don J.
dc.contributor.authorLopez Murillo, Ana Isabel
dc.contributor.authorRicker, George R.
dc.contributor.authorWinn, Joshua N.
dc.contributor.authorJenkins, Jon M.
dc.contributor.authorBouma, Luke G.
dc.contributor.authorFausnaugh, Michael
dc.contributor.authorGuerrero, Natalia M.
dc.contributor.authorKunimoto, Michelle
dc.date.accessioned2024-07-19T14:30:10Z
dc.date.available2024-07-19T14:30:10Z
dc.date.issued2024-07-01
dc.identifier305543784
dc.identifier10246d2c-f1b4-4c9a-af1b-46af7347a742
dc.identifier85197061480
dc.identifier.citationThao , P C , Mann , A W , Barber , M G , Kraus , A L , Tofflemire , B M , Bush , J L , Wood , M L , Collins , K A , Vanderburg , A , Quinn , S N , Zhou , G , Newton , E R , Ziegler , C , Law , N , Barkaoui , K , Pozuelos , F J , Timmermans , M , Gillon , M , Jehin , E , Schwarz , R P , Gan , T , Shporer , A , Horne , K , Sefako , R , Suarez , O , Mekarnia , D , Guillot , T , Abe , L , Triaud , A H M J , Radford , D J , Lopez Murillo , A I , Ricker , G R , Winn , J N , Jenkins , J M , Bouma , L G , Fausnaugh , M , Guerrero , N M & Kunimoto , M 2024 , ' TESS hunt for young and maturing exoplanets (THYME). X. A two-planet system in the 210 Myr MELANGE-5 association ' , Astronomical Journal , vol. 168 , no. 1 , 41 . https://doi.org/10.3847/1538-3881/ad4993en
dc.identifier.issn0004-6256
dc.identifier.otherJisc: 2077038
dc.identifier.otherpublisher-id: ajad4993
dc.identifier.othermanuscript: ad4993
dc.identifier.otherother: aas52898
dc.identifier.urihttps://hdl.handle.net/10023/30241
dc.descriptionFunding: P.C.T. was supported by an NSF Graduate Research Fellowship (DGE-1650116), the NC Space Grant Graduate Research Fellowship, the Zonta International Amelia Earhart Fellowship, and the Jack Kent Cooke Foundation Graduate Scholarship. A.W.M. was supported by grants from the NSF CAREER program (AST-2143763) and NASA’s exoplanet research program (XRP 80NSSC21K0393). M.G.B. was supported by an NSF Graduate Research Fellowship (DGE2040435) and the NC Space Grant Graduate Research Fellowship. F.J.P. acknowledges financial support from the grant CEX2021-001131-S funded by MCIN/AEI/ 10.13039/ 501100011033 and through projects PID2019-109522GB-C52 and PID2022-137241NB-C43. This research also received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No. 803193/BEBOP) and from the Science and Technology Facilities Council (STFC; grant No. ST/S00193X/1). The postdoctoral fellowship of K.B. is funded by F.R.S.-FNRS grant T.0109.20 and by the Francqui Foundation. K.A.C. acknowledges support from the TESS mission via subaward s3449 from MIT. M.K. acknowledges support from the MIT Kavli Institute as a Juan Carlos Torres Fellow. This publication benefits from the support of the French Community of Belgium in the context of the FRIA Doctoral Grant awarded to M.T.en
dc.description.abstractYoung (<500 Myr) 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 ± 27 Myr. MELANGE-5 is situated in close proximity to previously identified younger (80–110 Myr) 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 ± 0.09 R⊕ and 2.88 ± 0.10 R⊕ and orbit their host star every 4.18 and 17.95 days, respectively. With their bright (K = 9.1 mag), small (R* = 0.44 R⊙), and cool (Teff = 3326 K) host star, these planets represent excellent candidates for atmospheric characterization with JWST.
dc.format.extent24
dc.format.extent20873025
dc.language.isoeng
dc.relation.ispartofAstronomical Journalen
dc.subjectStellar activityen
dc.subjectTransit timing variation methoden
dc.subjectExoplanet astronomyen
dc.subjectStellar agesen
dc.subjectYoung star clustersen
dc.subjectTransit photometryen
dc.subjectQB Astronomyen
dc.subjectDASen
dc.subject.lccQBen
dc.titleTESS hunt for young and maturing exoplanets (THYME). X. A two-planet system in the 210 Myr MELANGE-5 associationen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.3847/1538-3881/ad4993
dc.description.statusPeer revieweden


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