dc.contributor.author | Soto, MG | |
dc.contributor.author | Díaz, MR | |
dc.contributor.author | Jenkins, JS | |
dc.contributor.author | Rojas, F | |
dc.contributor.author | Espinoza, N | |
dc.contributor.author | Brahm, R | |
dc.contributor.author | Drass, H | |
dc.contributor.author | Jones, MI | |
dc.contributor.author | Rabus, M | |
dc.contributor.author | Hartman, J | |
dc.contributor.author | Sarkis, P | |
dc.contributor.author | Jordán, A | |
dc.contributor.author | Lachaume, R | |
dc.contributor.author | Pantoja, B | |
dc.contributor.author | Vučković, M | |
dc.contributor.author | Ciardi, DR | |
dc.contributor.author | Crossfield, Ian Jm | |
dc.contributor.author | Dressing, C | |
dc.contributor.author | Gonzales, E | |
dc.contributor.author | Hirsch, L | |
dc.date.accessioned | 2022-07-15T14:35:05Z | |
dc.date.available | 2021-10-27T20:10:45Z | |
dc.date.available | 2022-07-15T14:35:05Z | |
dc.date.issued | 2018 | |
dc.identifier.uri | https://hdl.handle.net/1721.1/135102.2 | |
dc.description.abstract | © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We report the discovery of two hot Jupiters orbiting the stars K2-237 and K2-238. We used photometric data from Campaigns 11 and 12 of the Kepler K2 mission and radial velocity data obtained using the HARPS, FEROS, and CORALIE spectrographs. K2-237 b and K2-238 b have masses of 1.60-0.11+0.11 and 0.86+-0.120.13MJup, radii of 1.65-0.08+0.07 and 1.30-0.14+0.15 RJup, and are orbiting their host stars in 2.18-and 3.20-d orbits, respectively. The large radius of K2-237 b leads us to conclude that this candidate corresponds to a highly inflated hot Jupiter. K2-238 b has a radius consistent with theoretical models, considering the high incident flux falling on the planet. We consider K2-237 b to be an excellent system for follow-up studies, since not only is it very inflated, but it also orbits a relatively bright star (V = 11.6). | en_US |
dc.language.iso | en | |
dc.publisher | Oxford University Press (OUP) | en_US |
dc.relation.isversionof | 10.1093/MNRAS/STY1334 | en_US |
dc.rights | Creative Commons Attribution-Noncommercial-Share Alike | en_US |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | en_US |
dc.source | Prof. Crossfield | en_US |
dc.title | K2-237 b and K2-238 b: discovery and characterization of two new transiting hot Jupiters from K2 | en_US |
dc.title.alternative | K2-237 b and K2-238 b: discovery and characterization of two new transiting hot Jupiters from K2 | en_US |
dc.type | Article | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | en_US |
dc.relation.journal | Monthly Notices of the Royal Astronomical Society | en_US |
dc.eprint.version | Author's final manuscript | 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 | 2019-06-10T13:40:43Z | |
dspace.orderedauthors | Soto, MG; Díaz, MR; Jenkins, JS; Rojas, F; Espinoza, N; Brahm, R; Drass, H; Jones, MI; Rabus, M; Hartman, J; Sarkis, P; Jordán, A; Lachaume, R; Pantoja, B; Vučković, M; Ciardi, DR; Crossfield, I; Dressing, C; Gonzales, E; Hirsch, L | en_US |
dspace.date.submission | 2019-06-10T13:40:45Z | |
mit.journal.volume | 478 | en_US |
mit.journal.issue | 4 | en_US |
mit.metadata.status | Publication Information Needed | en_US |