| dc.date.accessioned | 2022-01-20T14:32:49Z | |
| dc.date.available | 2021-10-27T19:57:59Z | |
| dc.date.available | 2022-01-20T14:32:49Z | |
| dc.date.issued | 2020-05 | |
| dc.date.submitted | 2020-03 | |
| dc.identifier.issn | 1538-3881 | |
| dc.identifier.uri | https://hdl.handle.net/1721.1/134078.2 | |
| dc.description.abstract | © 2020. The American Astronomical Society. All rights reserved. We report the discovery of HATS-71b, a transiting gas giant planet on a day orbit around a mag M3 dwarf star. HATS-71 is the coolest M dwarf star known to host a hot Jupiter. The loss of light during transits is 4.7%, more than in any other confirmed transiting planet system. The planet was identified as a candidate by the ground-based HATSouth transit survey. It was confirmed using ground-based photometry, spectroscopy, and imaging, as well as space-based photometry from the NASA Transiting Exoplanet Survey Satellite mission (TIC 234523599). Combining all of these data, and utilizing Gaia DR2, we find that the planet has a radius of 1.024± 0.018 R J and mass of 0.37,± 0.24 M J (95% confidence upper limit of < 0.80 M J), while the star has a mass of 0.4861 pm 0.0060 M⊙ and a radius of 0.4783± 0.0060 R⊙. | en_US |
| dc.language.iso | en | |
| dc.publisher | American Astronomical Society | en_US |
| dc.relation.isversionof | http://dx.doi.org/10.3847/1538-3881/AB8AD1 | en_US |
| dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
| dc.source | The American Astronomical Society | en_US |
| dc.title | HATS-71b: A Giant Planet Transiting an M3 Dwarf Star in TESS Sector 1 | en_US |
| dc.type | Article | en_US |
| dc.contributor.department | MIT Kavli Institute for Astrophysics and Space Research | |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences | |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Aeronautics and Astronautics | |
| dc.relation.journal | Astronomical Journal | en_US |
| dc.eprint.version | Final published version | en_US |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
| eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
| dc.date.updated | 2021-09-29T18:07:54Z | |
| dspace.orderedauthors | Bakos, GÁ; Bayliss, D; Bento, J; Bhatti, W; Brahm, R; Csubry, Z; Espinoza, N; Hartman, JD; Henning, T; Jordán, A; Mancini, L; Penev, K; Rabus, M; Sarkis, P; Suc, V; de Val-Borro, M; Zhou, G; Butler, RP; Crane, J; Durkan, S; Shectman, S; Kim, J; Lázár, J; Papp, I; Sári, P; Ricker, G; Vanderspek, R; Latham, DW; Seager, S; Winn, JN; Jenkins, J; Chacon, AD; Fűrész, G; Goeke, B; Li, J; Quinn, S; Quintana, EV; Tenenbaum, P; Teske, J; Vezie, M; Yu, L; Stockdale, C; Evans, P; Relles, HM | en_US |
| dspace.date.submission | 2021-09-29T18:07:55Z | |
| mit.journal.volume | 159 | en_US |
| mit.journal.issue | 6 | en_US |
| mit.license | PUBLISHER_POLICY | |
| mit.metadata.status | Authority Work Needed | en_US |
