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HATS-1b: The First Transiting Planet Discovered by the HATSouth Survey

Author(s): Penev, K; Bakos, Gaspar Aron; Bayliss, D; Jordán, A; Mohler, M; et al

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dc.contributor.authorPenev, K-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorBayliss, D-
dc.contributor.authorJordán, A-
dc.contributor.authorMohler, M-
dc.contributor.authorZhou, G-
dc.contributor.authorSuc, V-
dc.contributor.authorRabus, M-
dc.contributor.authorHartman, JD-
dc.contributor.authorMancini, L-
dc.contributor.authorBéky, B-
dc.contributor.authorCsubry, Z-
dc.contributor.authorBuchhave, L-
dc.contributor.authorHenning, T-
dc.contributor.authorNikolov, N-
dc.contributor.authorCsák, B-
dc.contributor.authorBrahm, R-
dc.contributor.authorEspinoza, N-
dc.contributor.authorConroy, P-
dc.contributor.authorNoyes, RW-
dc.contributor.authorSasselov, DD-
dc.contributor.authorSchmidt, B-
dc.contributor.authorWright, DJ-
dc.contributor.authorTinney, CG-
dc.contributor.authorAddison, BC-
dc.contributor.authorLázár, J-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.date.accessioned2019-04-10T19:32:20Z-
dc.date.available2019-04-10T19:32:20Z-
dc.date.issued2013-01en_US
dc.identifier.citationPenev, K, Bakos, GÁ, Bayliss, D, Jordán, A, Mohler, M, Zhou, G, Suc, V, Rabus, M, Hartman, JD, Mancini, L, Béky, B, Csubry, Z, Buchhave, L, Henning, T, Nikolov, N, Csák, B, Brahm, R, Espinoza, N, Conroy, P, Noyes, RW, Sasselov, DD, Schmidt, B, Wright, DJ, Tinney, CG, Addison, BC, Lázár, J, Papp, I, Sári, P. (2013). HATS-1b: The First Transiting Planet Discovered by the HATSouth Survey. \aj, 145 (5 - 5. doi:10.1088/0004-6256/145/1/5en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1x995-
dc.description.abstractWe report the discovery of HATS-1b, a transiting extrasolar planet orbiting the moderately bright V = 12 . 05 G dwarf star GSC 6652-00186, and the first planet discovered by HATSouth, a global network of autonomous wide-field telescopes. HATS-1b has a period of P ≈ 3 . 4465 days, mass of M p ≈ 1 . 86 M J , and radius of R p ≈ 1 . 30 R J .The host star has a mass of 0 . 99 M and radius of 1 . 04 R . The discovery light curve of HATS-1b has near-continuous coverage over several multi-day timespans, demonstrating the power of using a global network of telescopes to discover transiting planets.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-1b: The First Transiting Planet Discovered by the HATSouth Surveyen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-6256/145/1/5-
dc.date.eissued2012-11-21en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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