HATS-31b through HATS-35b: five transiting hot Jupiters discovered by the HATSouth survey

de Val-Borro, M. and Bakos, G. A.. and Brahm, R. and Hartman, J. D. and Espinoza, N. and Penev, K. and Ciceri, S. and Jordan, A. and Bhatti, W. and Csubry, Z. and Bayliss, D. and Bento, J. and Zhou, G. ORCID: https://orcid.org/0000-0002-4891-3517 and Rabus, M. and Mancini, L. and Henning, T. and Schmidt, B. and Tan, T. G. and Tinney, C. G. and Wright, D. J. and Kedziora-Chudczer, L. and Bailey, J. and Suc, V. and Durkan, S. and Lazar, J. and Papp, I. and Sari, P. (2016) HATS-31b through HATS-35b: five transiting hot Jupiters discovered by the HATSouth survey. The Astronomical Journal, 152 (6):161. pp. 1-16. ISSN 0004-6256


We report the discovery of five new transiting hot-Jupiter planets discovered by the HATSouth survey, HATS-31b through HATS-35b. These planets orbit moderately bright stars with V magnitudes within the range of 11.9-14.4 mag while the planets span a range of masses of. 0.88-1.22 M-J. and have somewhat inflated radii between 1.23 and 1.64 R-J. These planets can be classified as typical hot Jupiters, with HATS-31b and HATS-35b being moderately inflated gas giant planets with radii of 1.64 +/- 0.22 R-J and 1.464(-0.044)(+0.069) R-J, respectively, that can be used to constrain inflation mechanisms. All five systems present a higher Bayesian evidence for a fixed-circular-orbit model than for an eccentric orbit. The orbital periods range from 1.8209993 +/- 0.0000016 day for HATS-35b) to 3.377960 +/- 0.000012 day for HATS-31b. Additionally, HATS-35b orbits a relatively young F star with an age of 2.13 +/- 0.51 Gyr. We discuss the analysis to derive the properties of these systems and compare them in the context of the sample of well-characterized transiting hot Jupiters known to date.

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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 01:47
Last Modified: 31 May 2021 01:30
Uncontrolled Keywords: planetary systems, stars individual, techniques photometric, techniques spectroscopic
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/10.3847/0004-637X/823/1/29
URI: http://eprints.usq.edu.au/id/eprint/36375

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