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HATS-5b: A Transiting Hot Saturn from the HATSouth Survey

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

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dc.contributor.authorZhou, G-
dc.contributor.authorBayliss, D-
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, M-
dc.contributor.authorCsubry, Zoltan-
dc.contributor.authorCiceri, S-
dc.contributor.authorBrahm, R-
dc.contributor.authorRabus, M-
dc.contributor.authorBuchhave, Lars A.-
dc.contributor.authorHenning, T-
dc.contributor.authorSuc, V-
dc.contributor.authorEspinoza, N-
dc.contributor.authorBéky, B-
dc.contributor.authorNoyes, Robert W.-
dc.contributor.authorSchmidt, B-
dc.contributor.authorButler, RP-
dc.contributor.authorShectman, S-
dc.contributor.authorThompson, I-
dc.contributor.authorCrane, J-
dc.contributor.authorSato, B-
dc.contributor.authorCsák, B-
dc.contributor.authorLázár, J.-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.contributor.authorNikolov, N-
dc.date.accessioned2019-04-10T19:32:08Z-
dc.date.available2019-04-10T19:32:08Z-
dc.date.issued2014-06en_US
dc.identifier.citationZhou, G, Bayliss, D, Penev, K, Bakos, GÁ, Hartman, JD, Jordán, A, Mancini, L, Mohler, M, Csubry, Z, Ciceri, S, Brahm, R, Rabus, M, Buchhave, L, Henning, T, Suc, V, Espinoza, N, Béky, B, Noyes, RW, Schmidt, B, Butler, RP, Shectman, S, Thompson, I, Crane, J, Sato, B, Csák, B, Lázár, J, Papp, I, Sári, P, Nikolov, N. (2014). HATS-5b: A Transiting Hot Saturn from the HATSouth Survey. \aj, 147 (144 - 144. doi:10.1088/0004-6256/147/6/144en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1wh78-
dc.description.abstractWe report the discovery of HATS-5b, a transiting hot Saturn orbiting a G-type star, by the HATSouth survey. HATS-5b has a mass of M p ≈ 0 . 24 M J , radius of R p ≈ 0 . 91 R J , and transits its host star with a period of P ≈ 4 . 7634 days. The radius of HATS-5b is consistent with both theoretical and empirical models. The host star has a V -band magnitude of 12.6, mass of 0 . 94 M , and radius of 0 . 87 R . The relatively high scale height of HATS-5b and the bright, photometrically quiet host star make this planet a favorable target for future transmission spectroscopy follow-up observations. We reexamine the correlations in radius, equilibrium temperature, and metallicity of the close-in gas giants and find hot Jupiter-mass planets to exhibit the strongest dependence between radius and equilibrium temperature. We find no significant dependence in radius and metallicity for the close-in gas giant population.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-5b: A Transiting Hot Saturn from the HATSouth Surveyen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-6256/147/6/144-
dc.date.eissued2014-05-06en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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