HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey

Mancini, L. and Hartman, J. D. and Penev, K. and Bakos, G. A. and Brahm, R. and Ciceri, S. and Henning, Th. and Csubry, Z. and Bayliss, D. and Zhou, G. and Rabus, M. and de Val-Borro, M. and Espinoza, N. and Jordan, A. and Suc, V. and Bhatti, W. and Schmidt, B. and Sato, B. and Tan, T. G. and Wright, D. J. and Tinney, C. G. and Addison, B. C. and Noyes, R. W. and Lazar, J. and Papp, I. and Sari, P. (2015) HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey. Astronomy and Astrophysics, 580 :A63. pp. 1-13. ISSN 0004-6361


We report the discovery of HATS-13b and HATS-14b, which are two hot-Jupiter transiting planets discovered by the HATSouth survey. The host stars are quite similar to each other (HATS-13: V = 13.9 mag, M-star = 0.96 M-circle dot, R-star = 0.89 R-circle dot, T-eff approximate to 5500 K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, M-star = 0.97 M-circle dot, R-star = 0.93 R-circle dot, T-eff approximate to 5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of similar to 3 days and a separation of similar to 0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. HATS-13b, with a mass of M-p = 0.543 +/- 0.072 M-J and a radius of R-p = 1.212 +/- 0.035 R-J, appears as an inflated planet, while HATS-14b, having a mass of M-p = 1.071 +/- 0.070 M-J and a radius of R-p = 1.039 +/- 0.032 R-J, is only slightly larger in radius than Jupiter.

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Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Faculty/School / Institute/Centre: No Faculty
Faculty/School / Institute/Centre: No Faculty
Date Deposited: 09 Sep 2019 02:37
Last Modified: 08 Jun 2021 04:39
Uncontrolled Keywords: planetary systems, stars, fundamental parameters, radial velocities, photometric, HATS-13 (aka GSC6928-00497), HATS-14 (aka GSC6926-00259)
Fields of Research (2008): 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Fields of Research (2020): 51 PHYSICAL SCIENCES > 5101 Astronomical sciences > 510109 Stellar astronomy and planetary systems
Identification Number or DOI: https://doi.org/10.1051/0004-6361/201526069
URI: http://eprints.usq.edu.au/id/eprint/36380

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