Quinn, S. N. and Bakos, G. Á. and Hartmann, J. and Torres, G. and Kovács, G. and Latham, D. W. and Noyes, R. W. and Fischer, D. A. and Johnson, J. A. and Marcy, G. W. and Howard, A. W. and Szentgyorgyi, A. and Fűrész, G. and Buchhave, L. A. and Béky, B. and Sasselov, D. D. and Stefanik, R. P. and Perumpilly, G. and Everett, M. and Lázár, J. and Papp, I. and Sári, P. (2012) Hat-P-25b: A Hot-Jupiter Transiting a Moderately Faint G Star. Astrophysical Journal, 745 (1). Art. No. 80. ISSN 0004-637X http://resolver.caltech.edu/CaltechAUTHORS:20120404-072516851
- Published Version
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20120404-072516851
We report the discovery of HAT-P-25b, a transiting extrasolar planet orbiting the V = 13.19 G5 dwarf star GSC 1788-01237, with a period P = 3.652836 ± 0.000019 days, transit epoch T_c = 2455176.85173 ± 0.00047 (BJD—barycentric Julian dates throughout the paper are calculated from Coordinated Universal Time, UTC), and transit duration 0.1174 ± 0.0017 days. The host star has a mass of 1.01 ± 0.03 M_☉, radius of 0.96^(+0.05)_(– 0.04) R_☉, effective temperature 5500 ± 80 K, and metallicity [Fe/H] = +0.31 ± 0.08. The planetary companion has a mass of 0.567 ± 0.022 M_J and radius of 1.190^(+0.081)_(–0.056) R_J yielding a mean density of 0.42 ± 0.07 g cm^(–3).
|Additional Information:||© 2012 American Astronomical Society. Received 2010 August 20; accepted 2011 November 4; published 2011 December 29. Based in part on observations obtained at the W. M. Keck Observatory, which is operated by the University of California and the California Institute of Technology. Keck time has been granted by NOAO (A201Hr), NASA (N018Hr and N167Hr), and the NASA Gemini-Keck time-exchange program (G329Hr). Based in part on observations made with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. HATNet operations have been funded by NASA grants NNG04GN74G, NNX08AF23G, and SAO IR&D grants. Work of G.Á.B. and J. Johnson were supported by the Postdoctoral Fellowship of the NSF Astronomy and Astrophysics Program (AST-0702843 and AST-0702821, respectively). G.T. acknowledges partial support from NASA grant NNX09AF59G. We acknowledge partial support also from the Kepler Mission under NASA Cooperative Agreement NCC2-1390 (PI: D.W. Latham). G.K. thanks the Hungarian Scientific Research Foundation (OTKA) for support through grant K-81373. This research has made use of Keck telescope time granted through NOAO (A201Hr), NASA (N018Hr and N167Hr), and the NASA Gemini-Keck time-exchange program (G329Hr). This research has also made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.|
|Subject Keywords:||planetary systems; stars: individual (HAT-P-25, GSC 1788-01237); techniques: photometric; techniques: spectroscopic|
|Official Citation:||HAT-P-25b: A Hot-Jupiter Transiting a Moderately Faint G Star S. N. Quinn et al. 2012 ApJ 745 80|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||04 Apr 2012 15:48|
|Last Modified:||26 Dec 2012 15:01|
Repository Staff Only: item control page