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HAT-P-58b -- HAT-P-64b: Seven Planets Transiting Bright Stars

Bakos, G. Á. and Hartman, J. D. and Bhatti, W. and Csubry, Z. and Penev, K. and Bieryla, A. and Latham, D. W. and Quinn, S. and Buchhave, L. A. and Kovács, G. and Torres, G. and Noyes, R. W. and Falco, E. and Béky, B. and Szklenár, T. and Esquerdo, G. A. and Howard, A. W. and Isaacson, H. and Marcy, G. and Sato, B. and Boisse, I. and Santerne, A. and Hébrard, G. and Rabus, M. and Harbeck, D. and McCully, C. and Everett, M. E. and Horch, E. P. and Hirsch, L. and Howell, S. B. and Huang, C. X. and Lázár, J. and Papp, I. and Sári, P. (2020) HAT-P-58b -- HAT-P-64b: Seven Planets Transiting Bright Stars. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20200817-104917526

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Abstract

We report the discovery and characterization of 7 transiting exoplanets from the HATNet survey. The planets, which are hot Jupiters and Saturns transiting bright sun-like stars, include: HAT-P-58b (with mass M_p = 0.37 M_J, radius R_p = 1.33 R_J, and orbital period P = 4.0138 days), HAT-P-59b (M_p = 1.54 M_J, R_p = 1.12 R_J, P = 4.1420 days), HAT-P-60b (M_p = 0.57 M_J, R_p = 1.63 R_J, P = 4.7948 days), HAT-P-61b (M_p = 1.06 M_J, R_p = 0.90 R_J, P = 1.9023 days), HAT-P-62b (M_p = 0.76 M_J, R_p = 1.07 R_J, P = 2.6453 days), HAT-P-63b (M_p = 0.61 M_J, R_p = 1.12 R_J, P = 3.3777 days), and HAT-P-64b (M_p = 0.58 M_J, R_p = 1.70 R_J, P = 4.0072 days). The typical errors on these quantities are 0.06 M_J, 0.03 R_J, and 0.2 seconds, respectively. We also provide accurate stellar parameters for each of the hosts stars. With V = 9.710±0.050mag, HAT-P-60 is an especially bright transiting planet host, and an excellent target for additional follow-up observations. With Rp = 1.703±0.070 R_J, HAT-P-64b is a highly inflated hot Jupiter around a star nearing the end of its main-sequence lifetime, and is among the largest known planets. Five of the seven systems have long-cadence observations by TESS which are included in the analysis. Of particular note is HAT-P-59 (TOI-1826.01) which is within the Northern continuous viewing zone of the TESS mission, and HAT-P-60, which is the TESS candidate TOI-1580.01.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
https://arxiv.org/abs/2007.05528v1arXivDiscussion Paper
ORCID:
AuthorORCID
Bakos, G. Á.0000-0001-7204-6727
Hartman, J. D.0000-0001-8732-6166
Bhatti, W.0000-0002-0628-0088
Penev, K.0000-0003-4464-1371
Bieryla, A.0000-0001-6637-5401
Latham, D. W.0000-0001-9911-7388
Quinn, S.0000-0002-8964-8377
Buchhave, L. A.0000-0003-1605-5666
Torres, G.0000-0002-5286-0251
Esquerdo, G. A.0000-0002-9789-5474
Howard, A. W.0000-0001-8638-0320
Santerne, A.0000-0002-3586-1316
Rabus, M.0000-0003-2935-7196
McCully, C.0000-0001-5807-7893
Everett, M. E.0000-0002-0885-7215
Horch, E. P.0000-0003-2159-1463
Hirsch, L.0000-0001-8058-7443
Howell, S. B.0000-0002-2532-2853
Huang, C. X.0000-0003-0918-7484
Additional Information:Based on observations of the Hungarian-made Automated Telescope Network and observations obtained at the following observatories: W. M. Keck Observatory, the 1.5m and the 1.2m telescopes at the Fred Lawrence Whipple Observatory of the Smithsonian Astrophysical Observatory, the Kitt Peak National Observatory, the 1.93m telescope at Observatoire de Haute-Provence, the Subaru Telescope of the National Astronomical Observatory of Japan, the Nordic Optical Telescope in the Spanish Observatorio del Roque de los Muchachos of the Intituto de Astrofisica de Canarias, and the Apache Point Observatory 3.5m telescope. HATNet operations have been funded by NASA grants NNG04GN74G, NNX08AF23G, and NNX13AJ15G. Follow-up of HATNet targets has been partially supported through NSF grant AST-1108686. G._A.B, J.H., Z.C. and K.P. acknowledge partial support from NASA grant NNX17AB61G. G.B. acknowledges support from the Hungarian Academy of Sciences, and thanks for the warm hospitality of Konkoly Observatory in carrying out some of his research. J.H. acknowledges support from NASA grant NNX14AF87G. K.P. acknowledges support from NASA grant 80NSSC18K1009. G.K. thanks the support from the National Research, Development and Innovation Office (grant K 129249). We acknowledge partial support also from the Kepler Mission under NASA Cooperative Agreement NNX13AB58A (D.W.L., PI). Data presented in this paper are based on observations obtained at the HAT station at the Submillimeter Array of SAO, and the HAT station at the Fred Lawrence Whipple Observatory of SAO. We acknowledge J.A. Johnson in supporting the Keck HIRES observations. The authors wish to acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. This research has made use of Keck telescope time granted through NOAO (programs: A245Hr, A202Hr; PI: G.B) and NASA (programs: N154Hr, N133Hr, N136Hr, N143Hr, N169Hr, N186Hr; PI: G.B). Based on observations at Kitt Peak National Observatory, National Optical Astronomy Observatory (NOAO Prop. ID: 2015B-0156; PI: J.H.), which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. Based on radial velocities obtained with the SOPHIE spectrograph mounted on the 1.93m telescope at Observatoire de Haute-Provence. Based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. Based on observations made with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Norway, Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Intituto de Astrofisica de Canarias. Based on observations obtained with the Apache Point Observatory 3.5m telescope, which is owned and operated by the Astrophysical Research Consortium. This research was made possible through the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program.
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
David and Lucile Packard FoundationUNSPECIFIED
NASANNG04GN74G
NASANNX08AF23G
NASANNX13AJ15G
NSFAST-1108686
NASANNX17AB61G
Hungarian Academy of SciencesUNSPECIFIED
NASANNX14AF87G
NASA80NSSC18K1009
National Research, Development and Innovation Office (Hungary)K 129249
NASANNX13AB58A
Subject Keywords:planetary systems - stars: individual (HAT-P-58, GSC 3740-01482, HAT-P-59, GSC 4234-02195 HAT-P-60, GSC 3292-01330 HAT-P-61, GSC 3352-00595 HAT-P-62, GSC 3348-01101 HAT-P-63, GSC 0429-01697 HAT-P-64, GSC 0086-00341) techniques: spectroscopic, photometric
Record Number:CaltechAUTHORS:20200817-104917526
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200817-104917526
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104978
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:17 Aug 2020 18:32
Last Modified:17 Aug 2020 18:32

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