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HATS-17b: A Transiting Compact Warm Jupiter in a 16.3 Day Circular Orbit

Author(s): Brahm, R; Jordán, A.; Bakos, Gaspar Aron; Penev, K; Espinoza, N; et al

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dc.contributor.authorBrahm, R-
dc.contributor.authorJordán, A.-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorPenev, K-
dc.contributor.authorEspinoza, N-
dc.contributor.authorRabus, M-
dc.contributor.authorHartman, Joel D.-
dc.contributor.authorBayliss, D-
dc.contributor.authorCiceri, S-
dc.contributor.authorZhou, G-
dc.contributor.authorMancini, L-
dc.contributor.authorTan, TG-
dc.contributor.authorde Val-Borro, Miguel-
dc.contributor.authorBhatti, W-
dc.contributor.authorCsubry, Zoltan-
dc.contributor.authorBento, J-
dc.contributor.authorHenning, T-
dc.contributor.authorSchmidt, B-
dc.contributor.authorRojas, F-
dc.contributor.authorSuc, V-
dc.contributor.authorLázár, J.-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.identifier.citationBrahm, R, Jordán, A, Bakos, GÁ, Penev, K, Espinoza, N, Rabus, M, Hartman, JD, Bayliss, D, Ciceri, S, Zhou, G, Mancini, L, Tan, TG, de Val-Borro, M, Bhatti, W, Csubry, Z, Bento, J, Henning, T, Schmidt, B, Rojas, F, Suc, V, Lázár, J, Papp, I, Sári, P. (2016). HATS-17b: A Transiting Compact Warm Jupiter in a 16.3 Day Circular Orbit. \aj, 151 (89 - 89. doi:10.3847/0004-6256/151/4/89en_US
dc.description.abstractWe report the discovery of HATS-17b, the first transiting warm Jupiter of the HATSouth network. HATS-17b transits its bright (V = 12.4) G-type (M =1.131 0.030  M, R = - + 1.091 0.046 0.070 R) metal-rich ([Fe/ H] = +0.3 dex) host star in a circular orbit with a period of P =16.2546 days. HATS-17b has a very compact radius of 0.777 0.056  RJ given its Jupiter-like mass of 1.338 0.065  MJ. Up to 50% of the mass of HATS-17b may be composed of heavy elements in order to explain its high density with current models of planetary structure. HATS-17b is the longest period transiting planet discovered to date by a ground-based photometric survey, and is one of the brightest transiting warm Jupiter systems known. The brightness of HATS-17 will allow detailed followup observations to characterize the orbital geometry of the system and the atmosphere of the planet.en_US
dc.relation.ispartofAstronomical Journalen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleHATS-17b: A Transiting Compact Warm Jupiter in a 16.3 Day Circular Orbiten_US
dc.typeJournal Articleen_US

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