HAT-P-39b--HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters
J. D. Hartman, G.\'A. Bakos, B. B\'eky, G. Torres, D. W. Latham, Z., Csubry, K. Penev, A. Shporer, B. J. Fulton, L. A. Buchhave, J. A. Johnson, A., W. Howard, G. W. Marcy, D. A. Fischer, G. Kov\'acs, R. W. Noyes, G. A., Esquerdo, M. Everett, T. Szklen\'ar, S. N. Quinn
TL;DR
This paper reports the discovery of three highly inflated hot Jupiters orbiting moderately bright F stars, expanding understanding of the properties and diversity of such exoplanets.
Contribution
It presents the discovery and characterization of three new inflated hot Jupiters, adding valuable data to the population of known exoplanets with large radii.
Findings
The planets have periods between 2.6940 and 4.4572 days.
Their radii range from 1.57 to 1.73 R_J.
They are part of an emerging population of highly inflated Jupiters.
Abstract
We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V=11.1 to 12.4) F stars. The planets have periods of P = 2.6940 d to 4.4572 d, masses of 0.60 M_J to 0.80 M_J, and radii of 1.57 R_J to 1.73 R_J. They orbit stars with masses between 1.40 M_sun and 1.51 M_sun. The three planets are members of an emerging population of highly inflated Jupiters with 0.4 M_J < M < 1.5 M_J and R > 1.5 R_J.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.