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

Bakos, G. A. 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 Kovacs, G. and Torres, Guillermo and Noyes, R. W. and Falco, E. and Beky, Bence and Szklenar, 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 Hebrard, 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. ORCID: https://orcid.org/0000-0003-0918-7484 and Lazar, J. and Papp, I. and Sari, P. (2021) HAT-P-58b–HAT-P-64b: Seven Planets Transiting Bright Stars. The Astronomical Journal, 162 (1):7. pp. 1-31. ISSN 0004-6256

Text (Published Version)

Download (5MB) | Preview


We report the discovery and characterization of seven 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 s, respectively. We also provide accurate stellar parameters for each of the host stars. With V = 9.710 0.050 mag, HAT-P-60 is an especially bright transiting planet host, and an excellent target for additional follow-up observations. With R p = 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.

Statistics for USQ ePrint 47437
Statistics for this ePrint Item
Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Additional Information: Published version deposited in accordance with the copyright policy of the publisher.
Faculty/School / Institute/Centre: No Faculty
Faculty/School / Institute/Centre: No Faculty
Date Deposited: 04 Apr 2022 00:59
Last Modified: 13 Apr 2022 00:07
Uncontrolled Keywords: Exoplanets (498); Hot Jupiters (753); Exoplanet astronomy (486); Astronomical instrumentation (799); Astrophysics - Earth and Planetary Astrophysics; Astrophysics - Instrumentation and Methods for Astrophysics
Fields of Research (2020): 51 PHYSICAL SCIENCES > 5101 Astronomical sciences > 510109 Stellar astronomy and planetary systems
Identification Number or DOI: https://doi.org/10.3847/1538-3881/abf637
URI: http://eprints.usq.edu.au/id/eprint/47437

Actions (login required)

View Item Archive Repository Staff Only