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|Abstract:||We 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.|
|Electronic Publication Date:||4-Nov-2015|
|Citation:||Hartman, 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:10.1088/0004-6256/150/6/168|
|Type of Material:||Journal Article|
|Journal/Proceeding Title:||Astronomical Journal|
|Version:||Final published version. Article is made available in OAR by the publisher's permission or policy.|
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