Turner, OD, Anderson, DR ORCID: https://orcid.org/0000-0001-7416-7522, Collier Cameron, A, Delrez, L, Evans, DF, Gillon, M, Hellier, C ORCID: https://orcid.org/0000-0002-3439-1439, Jehin, E, Lendl, M and Maxted, PFL ORCID: https://orcid.org/0000-0003-3794-1317 (2016) WASP-120b, WASP-122b, and WASP-123b: Three Newly Discovered Planets from the WASP-South Survey. Publications of the Astronomical Society of the Pacific, 128.

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We present the discovery by the WASP-South survey of three planets transiting moderately bright stars (V ≈ 11). WASP-120 b is a massive (4.85 M Jup ) planet in a 3.6-day orbit that we find likely to be eccentric around an F5 star. WASP-122 b is a hot Jupiter (1.28 M Jup , 1.74 R Jup ) in a 1.7-day orbit about a G4 star. Our predicted transit depth variation caused by the atmosphere of WASP-122 b suggests it is well suited to characterization. WASP-123 b is a hot Jupiter (0.90 M Jup , 1.32 R Jup ) in a 3.0-day orbit around an old (∼7 Gyr) G5 star.

Item Type: Article
Uncontrolled Keywords: astrophysics, stars, astronomy
Subjects: Q Science > QB Astronomy > QB460 Astrophysics
Divisions: Faculty of Natural Sciences > School of Chemical and Physical Sciences
Depositing User: Symplectic
Date Deposited: 27 Mar 2018 14:40
Last Modified: 10 Jan 2020 13:45
URI: https://eprints.keele.ac.uk/id/eprint/4649

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