WASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South survey
Abstract
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 (e={0.059}-0.018+0.025) 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 (0.90M Jup, 1.32 R Jup) in a 3.0-day orbit around an old (∼7 Gyr) G5 star.
Citation
Turner , O D , Anderson , D R , Cameron , A C , Delrez , L , Evans , D F , Gillon , M , Hellier , C , Jehin , E , Lendl , M , Maxted , P F L , Pepe , F , Pollacco , D , Queloz , D , Ségransan , D , Smalley , B , Smith , A M S , Triaud , A H M J , Udry , S & West , R G 2016 , ' WASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South survey ' Publications of the Astronomical Society of the Pacific , vol 128 , no. 964 , 64401 . DOI: 10.1088/1538-3873/128/964/064401
Version
Postprint
Publication
Publications of the Astronomical Society of the Pacific
Status
Peer reviewed
ISSN
0004-6280Type
Journal article
Rights
© 2016, Astronomical Society of the Pacific. This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at iopscience.iop.org / https://dx.doi.org/10.1088/1538-3873/128/964/064401
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