HATS-3b: An Inflated Hot Jupiter Transiting an F-type Star

Bayliss, D. and Zhou, G. ORCID: https://orcid.org/0000-0002-4891-3517 and Penev, K. and Bakos, G. A. and Hartman, J. D. and Jordan, A. and Mancini, L. and Mohler-Fischer, M. and Suc, V. and Rabus, M. and Beky, B. and Csubry, Z. and Buchhave, L. and Henning, T. and Nikolov, N. and Csak, B. and Brahm, R. and Espinoza, N. and Noyes, R. W. and Schmidt, B. and Conroy, P. and Wright, D. J. and Tinney, C. G. and Addison, B. C. and Sackett, P. D. and Sasselov, D. D. and Lazar, J. and Papp, I. and Sari, P. (2013) HATS-3b: An Inflated Hot Jupiter Transiting an F-type Star. The Astronomical Journal, 146 (5):113. pp. 1-11. ISSN 0004-6256

[img]
Preview
Text (Accepted Version)
1306.0624.pdf

Download (1MB) | Preview

Abstract

We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V = 12.4 F dwarf star. HATS-3b has a period of P = 3.5479 days, mass of Mp = 1.07 M J, and radius of R p = 1.38 R J. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsin i = 9.0 km s-1), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low-/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transiting planet candidates produced by the HATSouth survey. We show that this important step in discovering planets produces log g and T eff parameters at a precision suitable for efficient candidate vetting, as well as efficiently identifying stellar mass eclipsing binaries with radial velocity semi-amplitudes as low as 1 km s-1.


Statistics for USQ ePrint 44967
Statistics for this ePrint Item
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: 28 Jan 2022 01:43
Last Modified: 28 Jan 2022 01:43
Uncontrolled Keywords: planetary systems; stars: individual: HATS-3 GSC 6926–00454; techniques: photometric; techniques: spectroscopic; Astrophysics - Earth; and Planetary Astrophysics
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
Socio-Economic Objectives (2008): E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Socio-Economic Objectives (2020): 28 EXPANDING KNOWLEDGE > 2801 Expanding knowledge > 280120 Expanding knowledge in the physical sciences
Identification Number or DOI: https://doi.org/10.1088/0004-6256/146/5/113
URI: http://eprints.usq.edu.au/id/eprint/44967

Actions (login required)

View Item Archive Repository Staff Only