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Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era
dc.contributor.author | Garai, Z. | |
dc.contributor.author | Claret, A. | |
dc.date.accessioned | 2022-06-02T11:51:10Z | |
dc.date.available | 2022-06-02T11:51:10Z | |
dc.date.issued | 2022-04-25 | |
dc.identifier.citation | Z Garai... [et al.]. Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era, Monthly Notices of the Royal Astronomical Society, Volume 513, Issue 2, June 2022, Pages 2822–2840, [https://doi.org/10.1093/mnras/stac1095] | es_ES |
dc.identifier.uri | http://hdl.handle.net/10481/75203 | |
dc.description | We thank the anonymous reviewer for the helpful comments and suggestions. We also thank Dr. K. G. Isaak, the ESA CHEOPS Project Scientist, responsible for the ESA CHEOPS Guest Observers Programme, for the helpful discussions and support. This work was supported by the Hungarian National Research, Development and Innovation Office (NKFIH) grant K-125015, the PRODEX Experiment Agreement No. 4000137122 between the ELTE University and the European Space Agency (ESA-D/SCI-LE-2021-0025), the City of Szombathely under agreement No. 67.177-21/2016, and by the VEGA grant of the Slovak Academy of Sciences No. 2/0031/22. TP acknowledges support from the Slovak Research and Development Agency -contract No. APVV-20-0148. AC acknowledges financial support from the State Agency for Research of the Spanish MCIU through the `Center of Excellence Severo Ochoa' award for the Instituto de Astrophysics of Andalusia (SEV-2017-0709). CHEOPS is an ESA mission in partnership with Switzerland with important contributions to the payload and the ground segment from Austria, Belgium, France, Germany, Hungary, Italy, Portugal, Spain, Sweden, and the UK. The authors acknowledge the observing time awarded within the CHEOPS Guest Observers Programme No. 1 (AO-1) and the support from the Science Operations Centre. This paper includes data collected with the TESS mission, obtained from the 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 526555. This work has used data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium).Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. | es_ES |
dc.description.abstract | Rapidly rotating early-type main-sequence stars with transiting planets are interesting in many aspects. Unfortunately, several astrophysical effects in such systems are not well understood yet. Therefore, we performed a photometric mini-surv e y of three rapidly rotating stars with transiting planets, namely KEL T -17b, KEL T -19Ab, and KEL T -21b, using the Characterising Exoplanets Satellite ( CHEOPS ), complemented with Transiting Exoplanet Survey Satellite ( TESS ) data, and spectroscopic data. We aimed at investigating the spin-orbit misalignment and its photometrical signs, therefore the high-quality light curves of the selected objects were tested for transit asymmetry, transit duration variations, and orbital precession. In addition, we performed transit time variation analyses, obtained new stellar parameters, and refined the system parameters. For KEL T -17b and KEL T - 19Ab, we obtained significantly smaller planet radius as found before. The gravity-darkening effect is very small compared to the precision of CHEOPS data. We can report only on a tentative detection of the stellar inclination of KEL T -21, which is about 60 deg. In KEL T -17b and KEL T -19Ab, we were able to exclude long-term transit duration variations causing orbital precession. The shorter transit duration of KEL T -19Ab compared to the disco v ery paper is probably a consequence of a smaller planet radius. KEL T -21b is promising from this viewpoint, but further precise observations are needed. We did not find any convincing evidence for additional objects in the systems. | es_ES |
dc.description.sponsorship | National Research, Development & Innovation Office (NRDIO) - Hungary K-125015 | es_ES |
dc.description.sponsorship | ELTE University 4000137122 | es_ES |
dc.description.sponsorship | European Space Agency European Commission 4000137122 ESA-D/SCI-LE-2021-0025 | es_ES |
dc.description.sponsorship | City of Szombathely 67.177-21/2016 | es_ES |
dc.description.sponsorship | Slovak Academy of Sciences 2/0031/22 Slovak Research and Development Agency APVV-20-0148 | es_ES |
dc.description.sponsorship | Spanish Government SEV-2017-0709 | es_ES |
dc.description.sponsorship | CHEOPS Guest Observers Programme 1 (AO-1) | es_ES |
dc.description.sponsorship | Science Operations Centre | es_ES |
dc.description.sponsorship | National Aeronautics & Space Administration (NASA) NAS 526555 | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Oxford University Press | es_ES |
dc.rights | Atribución-NoComercial-SinDerivadas 3.0 España | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.subject | Methods: observational | es_ES |
dc.subject | Techniques: photometric | es_ES |
dc.subject | Techniques: spectroscopic | es_ES |
dc.subject | Planets and satellites: individual: KELT-17b, KELT-19Ab, KELT-21b | es_ES |
dc.title | Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era | es_ES |
dc.type | journal article | es_ES |
dc.rights.accessRights | open access | es_ES |
dc.identifier.doi | 10.1093/mnras/stac1095 | |
dc.type.hasVersion | VoR | es_ES |