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HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey

Author(s): Hartman, JD; Bhatti, W; Bakos, Gaspar Aron; Bieryla, A; Kovács, G; et al

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dc.contributor.authorHartman, JD-
dc.contributor.authorBhatti, W-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorBieryla, A-
dc.contributor.authorKovács, G-
dc.contributor.authorLatham, DW-
dc.contributor.authorCsubry, Z-
dc.contributor.authorde Val-Borro, M-
dc.contributor.authorPenev, K-
dc.contributor.authorBuchhave, LA-
dc.contributor.authorTorres, G-
dc.contributor.authorHoward, AW-
dc.contributor.authorMarcy, GW-
dc.contributor.authorJohnson, JA-
dc.contributor.authorIsaacson, H-
dc.contributor.authorSato, B-
dc.contributor.authorBoisse, I-
dc.contributor.authorFalco, E-
dc.contributor.authorEverett, ME-
dc.contributor.authorSzklenar, T-
dc.contributor.authorFulton, BJ-
dc.contributor.authorShporer, A-
dc.contributor.authorKovács, T-
dc.contributor.authorHansen, T-
dc.contributor.authorBéky, B-
dc.contributor.authorNoyes, RW-
dc.contributor.authorLázár, J-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.date.accessioned2019-04-10T19:31:22Z-
dc.date.available2019-04-10T19:31:22Z-
dc.date.issued2015-12en_US
dc.identifier.citationHartman, JD, Bhatti, W, Bakos, GÁ, Bieryla, A, Kovács, G, Latham, DW, Csubry, Z, de Val-Borro, M, Penev, K, Buchhave, LA, Torres, G, Howard, AW, Marcy, GW, Johnson, JA, Isaacson, H, Sato, B, Boisse, I, Falco, E, Everett, ME, Szklenar, T, Fulton, BJ, Shporer, A, Kovács, T, Hansen, T, Béky, B, Noyes, RW, Lázár, J, Papp, I, Sári, P. (2015). HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey. \aj, 150 (168 - 168. doi:10.1088/0004-6256/150/6/168en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr10q5r-
dc.description.abstractWe report the discovery and characterization of four transiting exoplanets by the HATNet survey. The planet HATP-50b has a mass of 1.35 MJ and radius of 1.29 RJ, and orbits a bright (V = 11.8 mag) M = 1.27 M, R = 1.70 R star every P = 3.1220 days. The planet HAT-P-51b has a mass of 0.31 MJ and radius of 1.29 RJ, and orbits a V = 13.4 mag, M = 0.98 M, R = 1.04 R star with a period of P = 4.2180 days. The planet HAT-P-52b has a mass of 0.82MJ and radius of 1.01 RJ, and orbits a V = 14.1mag, M = 0.89 M, R = 0.89 R star with a period of P = 2.7536 days. The planet HAT-P-53b has a mass of 1.48 MJ and radius of 1.32 RJ, and orbits a V = 13.7 mag, M = 1.09 M, R = 1.21R star with a period of P = 1.9616 days. All four planets are consistent with having circular orbits and have masses and radii measured to better than 10% precision. The low stellar jitter and favorable Rp/R ratio for HAT-P-51 make it a promising target for measuring the Rossiter–McLaughlin effect for a Saturnmass planet.en_US
dc.language.isoen_USen_US
dc.relation.ispartofAstronomical Journalen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleHAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Surveyen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-6256/150/6/168-
dc.date.eissued2015-11-04en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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