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dc.contributor.authorSoto, MG
dc.contributor.authorDíaz, MR
dc.contributor.authorJenkins, JS
dc.contributor.authorRojas, F
dc.contributor.authorEspinoza, N
dc.contributor.authorBrahm, R
dc.contributor.authorDrass, H
dc.contributor.authorJones, MI
dc.contributor.authorRabus, M
dc.contributor.authorHartman, J
dc.contributor.authorSarkis, P
dc.contributor.authorJordán, A
dc.contributor.authorLachaume, R
dc.contributor.authorPantoja, B
dc.contributor.authorVučković, M
dc.contributor.authorCiardi, DR
dc.contributor.authorCrossfield, Ian Jm
dc.contributor.authorDressing, C
dc.contributor.authorGonzales, E
dc.contributor.authorHirsch, L
dc.date.accessioned2022-07-15T14:35:05Z
dc.date.available2021-10-27T20:10:45Z
dc.date.available2022-07-15T14:35:05Z
dc.date.issued2018
dc.identifier.urihttps://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.isoen
dc.publisherOxford University Press (OUP)en_US
dc.relation.isversionof10.1093/MNRAS/STY1334en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourceProf. Crossfielden_US
dc.titleK2-237 b and K2-238 b: discovery and characterization of two new transiting hot Jupiters from K2en_US
dc.title.alternativeK2-237 b and K2-238 b: discovery and characterization of two new transiting hot Jupiters from K2en_US
dc.typeArticleen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.relation.journalMonthly Notices of the Royal Astronomical Societyen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-06-10T13:40:43Z
dspace.orderedauthorsSoto, 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, Len_US
dspace.date.submission2019-06-10T13:40:45Z
mit.journal.volume478en_US
mit.journal.issue4en_US
mit.metadata.statusPublication Information Neededen_US


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