TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars
Bryant, E. et al.-- Full list of authors: Bryant, Edward M.; Bayliss, Daniel; Hartman, Joel D.; Sedaghati, Elyar; Hobson, Melissa J.; Jordán, Andrés; Brahm, Rafael; Bakos, Gaspar Á.; Almenara, Jose Manuel; Barkaoui, Khalid; Bonfils, Xavier; Cointepas, Marion; Collins, Karen A.; Dransfield, Georgina;...
| Autores: | , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/372623 |
| Acceso en línea: | http://hdl.handle.net/10261/372623 |
| Access Level: | acceso abierto |
| Palabra clave: | Planets and satellites: formation Planets and satellites: gaseous planets Planets and satellites: individual: TOI2379 b Planets and satellites: individual: TOI-2384 b Stars: low-mass. |
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TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars |
| title |
TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars |
| spellingShingle |
TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars Bryant, E. Planets and satellites: formation Planets and satellites: gaseous planets Planets and satellites: individual: TOI2379 b Planets and satellites: individual: TOI-2384 b Stars: low-mass. |
| title_short |
TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars |
| title_full |
TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars |
| title_fullStr |
TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars |
| title_full_unstemmed |
TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars |
| title_sort |
TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host stars |
| dc.creator.none.fl_str_mv |
Bryant, E. Pozuelos, Francisco José |
| author |
Bryant, E. |
| author_facet |
Bryant, E. Pozuelos, Francisco José |
| author_role |
author |
| author2 |
Pozuelos, Francisco José |
| author2_role |
author |
| dc.contributor.none.fl_str_mv |
Agencia Estatal de Investigación (España) Ministerio de Ciencia e Innovación (España) Fédération Wallonie-Bruxelles NASA European Research Council Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Planets and satellites: formation Planets and satellites: gaseous planets Planets and satellites: individual: TOI2379 b Planets and satellites: individual: TOI-2384 b Stars: low-mass. |
| topic |
Planets and satellites: formation Planets and satellites: gaseous planets Planets and satellites: individual: TOI2379 b Planets and satellites: individual: TOI-2384 b Stars: low-mass. |
| description |
Bryant, E. et al.-- Full list of authors: Bryant, Edward M.; Bayliss, Daniel; Hartman, Joel D.; Sedaghati, Elyar; Hobson, Melissa J.; Jordán, Andrés; Brahm, Rafael; Bakos, Gaspar Á.; Almenara, Jose Manuel; Barkaoui, Khalid; Bonfils, Xavier; Cointepas, Marion; Collins, Karen A.; Dransfield, Georgina; Evans, Phil; Gillon, Michaël; Jehin, Emmanuël; Murgas, Felipe; Pozuelos, Francisco J.; Schwarz, Richard P.; Timmermans, Mathilde; Watkins, Cristilyn N.; Wünsche, Anaël; Butler, R. Paul; Crane, Jeffrey D.; Shectman, Steve; Teske, Johanna K.; Charbonneau, David; Essack, Zahra; Jenkins, Jon M.; Lewis, Hannah M.; Seager, Sara; Ting, Eric B.; Winn, Joshua N.-- This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. |
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2024 |
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2024 2024 2024 2024 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
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http://hdl.handle.net/10261/372623 |
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http://hdl.handle.net/10261/372623 |
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Inglés |
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Inglés |
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info:eu-repo/semantics/openAccess |
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openAccess |
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Oxford University Press |
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Oxford University Press |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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TOI-2379 b and TOI-2384 b: Two super-Jupiter mass planets transiting low-mass host starsBryant, E.Pozuelos, Francisco JoséPlanets and satellites: formationPlanets and satellites: gaseous planetsPlanets and satellites: individual: TOI2379 bPlanets and satellites: individual: TOI-2384 bStars: low-mass.Bryant, E. et al.-- Full list of authors: Bryant, Edward M.; Bayliss, Daniel; Hartman, Joel D.; Sedaghati, Elyar; Hobson, Melissa J.; Jordán, Andrés; Brahm, Rafael; Bakos, Gaspar Á.; Almenara, Jose Manuel; Barkaoui, Khalid; Bonfils, Xavier; Cointepas, Marion; Collins, Karen A.; Dransfield, Georgina; Evans, Phil; Gillon, Michaël; Jehin, Emmanuël; Murgas, Felipe; Pozuelos, Francisco J.; Schwarz, Richard P.; Timmermans, Mathilde; Watkins, Cristilyn N.; Wünsche, Anaël; Butler, R. Paul; Crane, Jeffrey D.; Shectman, Steve; Teske, Johanna K.; Charbonneau, David; Essack, Zahra; Jenkins, Jon M.; Lewis, Hannah M.; Seager, Sara; Ting, Eric B.; Winn, Joshua N.-- This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.Short-period gas giant planets have been shown to be significantly rarer for host stars less massive than the Sun. We report the discovery of two transiting giant planets - TOI-2379 b and TOI-2384 b - with low-mass (early M) host stars. Both planets were detected using Transiting Exoplanet Survey Satellite photometry and for both the transit signal was validated using ground-based photometric facilities. We confirm the planetary nature of these companions and measure their masses using radial velocity observations. We find that TOI-2379 b has an orbital period of 5.469 d and a mass and radius of 5.76 ±0.20 M and 1.046 ±0.023 R and TOI-2384 b has an orbital period of 2.136 d and a mass and radius of 1.966 ±0.059 M and 1.025 ±0.021 R. TOI-2379 b and TOI-2384 b have the highest and third highest planet-to-star mass ratios, respectively, out of all transiting exoplanets with a low-mass host star, placing them uniquely among the population of known exoplanets and making them highly important pieces of the puzzle for understanding the extremes of giant planet formation. © 2024 The Author(s).The contributions at the Mullard Space Science Laboratory by EMB have been supported by STFC through the consolidated grant ST/W001136/1. The post-doctoral fellowship of KB is funded by F.R.S.-FNRS grant T.0109.20 and by the Francqui Foundation. FJP 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. JDH and GAB acknowledge funding from NASA XRP grant 80NSSC22K0315. This publication benefits from the support of the French Community of Belgium in the context of the FRIA Doctoral Grant awarded to MT. The research leading to these results has received funding from the ARC grant for Concerted Research Actions, financed by the Wallonia-Brussels Federation. TRAPPIST is funded by the Belgian Fund for Scientific Research (Fond National de la Recherche Scientifique, FNRS) under the grant PDR T.0120.21. MG is F.R.S.-FNRS Research Director and EJis F.R.S.-FNRS Senior Research Associate. Observations were carried out from ESO La Silla Observatory. Funding for the TESS mission is provided by NASA’s Science Mission Directorate. KAC and CNW acknowledge support from the TESS mission via subaward s3449 from MIT. This paper used data collected by the TESS mission, obtained from the Mikulski Archive for Space Telescopes MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. We acknowledge the use of public TESS data from pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. We acknowledge funding from the European Research Council under the ERC grant agreement no. 337591-ExTrA. This work uses observationsfromthe LCOGT network. Part ofthe LCOGT telescope time was granted by NOIRLab through the Mid-Scale Innovations Program (MSIP). MSIP is funded by NSF. This research has used the Exoplanet Follow-up Observation Program (ExoFOP; DOI: 10.26134/ExoFOP5) website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).Peer reviewedOxford University PressAgencia Estatal de Investigación (España)Ministerio de Ciencia e Innovación (España)Fédération Wallonie-BruxellesNASAEuropean Research CouncilConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2024202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/372623reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-109522GB-C52info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2022-137241NB-C43info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2021- 515001131-SSíinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3726232026-05-22T06:33:51Z |
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15,81155 |