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HATS-31b through HATS-35b: Five Transiting Hot Jupiters Discovered By the HATSouth Survey

Author(s): de Val-Borro, Miguel; Bakos, Gaspar Aron; Brahm, R; Hartman, Joel D.; Espinoza, N; et al

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dc.contributor.authorde Val-Borro, Miguel-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorBrahm, R-
dc.contributor.authorHartman, Joel D.-
dc.contributor.authorEspinoza, N-
dc.contributor.authorPenev, K-
dc.contributor.authorCiceri, S-
dc.contributor.authorJordán, A.-
dc.contributor.authorBhatti, W-
dc.contributor.authorCsubry, Zoltan-
dc.contributor.authorBayliss, D-
dc.contributor.authorBento, J-
dc.contributor.authorZhou, G-
dc.contributor.authorRabus, M-
dc.contributor.authorMancini, L-
dc.contributor.authorHenning, T-
dc.contributor.authorSchmidt, B-
dc.contributor.authorTan, TG-
dc.contributor.authorTinney, CG-
dc.contributor.authorWright, DJ-
dc.contributor.authorKedziora-Chudczer, L-
dc.contributor.authorBailey, J-
dc.contributor.authorSuc, V-
dc.contributor.authorDurkan, S-
dc.contributor.authorLázár, J.-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.date.accessioned2019-04-10T19:30:40Z-
dc.date.available2019-04-10T19:30:40Z-
dc.date.issued2016-12en_US
dc.identifier.citationde Val-Borro, M, Bakos, GÁ, Brahm, R, Hartman, JD, Espinoza, N, Penev, K, Ciceri, S, Jordán, A, Bhatti, W, Csubry, Z, Bayliss, D, Bento, J, Zhou, G, Rabus, M, Mancini, L, Henning, T, Schmidt, B, Tan, TG, Tinney, CG, Wright, DJ, Kedziora-Chudczer, L, Bailey, J, Suc, V, Durkan, S, Lázár, J, Papp, I, Sári, P. (2016). HATS-31b through HATS-35b: Five Transiting Hot Jupiters Discovered By the HATSouth Survey. \aj, 152 (161 - 161. doi:10.3847/0004-6256/152/6/161en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1pq62-
dc.description.abstractWe report the discovery of five new transiting hot-Jupiter planets discovered by the HATSouth survey, HATS-31b through HATS-35b. These planets orbit moderately bright stars with V magnitudes within the range of 11.9–14.4 mag while the planets span a range of masses of 0.88–1.22 MJ and have somewhat inflated radii between 1.23 and 1.64 RJ. These planets can be classified as typical hot Jupiters, with HATS-31b and HATS-35b being moderately inflated gas giant planets with radii of 1.64 0.2  2 RJ and - + 1.464 0.044 0.069 RJ, respectively, that can be used to constrain inflation mechanisms. All five systems present a higher Bayesian evidence for a fixed-circular-orbit model than for an eccentric orbit. The orbital periods range from 1.8209993 0.0000016  day for HATS-35b) to 3.377960 0.00001  2 day for HATS-31b. Additionally, HATS-35b orbits a relatively young F star with an age of 2.13 0.51  Gyr. We discuss the analysis to derive the properties of these systems and compare them in the context of the sample of well-characterized transiting hot Jupiters known to date.en_US
dc.language.isoen_USen_US
dc.relation.ispartofAstronomical Journalen_US
dc.rightsAuthor's manuscripten_US
dc.titleHATS-31b through HATS-35b: Five Transiting Hot Jupiters Discovered By the HATSouth Surveyen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.3847/0004-6256/152/6/161-
dc.date.eissued2016-11-11en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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