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HATS-3b: An Inflated Hot Jupiter Transiting an F-type Star

Author(s): Bayliss, D; Zhou, G; Penev, K; Bakos, Gaspar Aron; Hartman, Joel D.; et al

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dc.contributor.authorBayliss, D-
dc.contributor.authorZhou, G-
dc.contributor.authorPenev, K-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorHartman, Joel D.-
dc.contributor.authorJordán, A.-
dc.contributor.authorMancini, L-
dc.contributor.authorMohler-Fischer, M-
dc.contributor.authorSuc, V-
dc.contributor.authorRabus, M-
dc.contributor.authorBéky, B-
dc.contributor.authorCsubry, Zoltan-
dc.contributor.authorBuchhave, Lars A.-
dc.contributor.authorHenning, T-
dc.contributor.authorNikolov, N-
dc.contributor.authorCsák, B-
dc.contributor.authorBrahm, R-
dc.contributor.authorEspinoza, N-
dc.contributor.authorNoyes, Robert W.-
dc.contributor.authorSchmidt, B-
dc.contributor.authorConroy, P-
dc.contributor.authorWright, DJ-
dc.contributor.authorTinney, CG-
dc.contributor.authorAddison, BC-
dc.contributor.authorSackett, PD-
dc.contributor.authorSasselov, DD-
dc.contributor.authorLázár, J.-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.date.accessioned2019-04-10T19:31:39Z-
dc.date.available2019-04-10T19:31:39Z-
dc.date.issued2013-11en_US
dc.identifier.citationBayliss, D, Zhou, G, Penev, K, Bakos, GÁ, Hartman, JD, Jordán, A, Mancini, L, Mohler-Fischer, M, Suc, V, Rabus, M, Béky, B, Csubry, Z, Buchhave, L, Henning, T, Nikolov, N, Csák, B, Brahm, R, Espinoza, N, Noyes, RW, Schmidt, B, Conroy, P, Wright, DJ, Tinney, CG, Addison, BC, Sackett, PD, Sasselov, DD, Lázár, J, Papp, I, Sári, P. (2013). HATS-3b: An Inflated Hot Jupiter Transiting an F-type Star. \aj, 146 (113 - 113. doi:10.1088/0004-6256/146/5/113en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr10h5g-
dc.description.abstractWe report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V = 12 . 4F dwarf star. HATS-3b has a period of P = 3 . 5479 days, mass of M p = 1 . 07 M J , and radius of R p = 1 . 38 R J .Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity ( v sin i = 9 . 0kms − 1 ), this system will make an interesting target for future observations to measure the Rossiter–McLaughlin effect and determine its spin–orbit alignment. We detail the low- / medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transiting planet candidates produced by the HATSouth survey. We show that this important step in discovering planets produces log g and T eff parameters at a precision suitable for efficient candidate vetting, as well as efficiently identifying stellar mass eclipsing binaries with radial velocity semi-amplitudes as low as 1 km s − 1 .en_US
dc.language.isoen_USen_US
dc.relation.ispartofAstronomical Journalen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleHATS-3b: An Inflated Hot Jupiter Transiting an F-type Staren_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-6256/146/5/113-
dc.date.eissued2013-09-27en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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