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The highly inflated giant planet WASP-174b

Mancini, L; Sarkis, P; Henning, T; Bakos, G A; Bayliss, D; Bento, Joao; Bhatti, Waqas; Brahm, R; Csubry, Z; Espinoza, N; Hartman, J D


Context. The transiting exoplanetary system WASP-174 was reported to be composed by a main-sequence F star (V = 11.8 mag) and a giant planet, WASP-174b (orbital period Porb = 4.23 days). However only an upper limit was placed on the planet mass (<1.3 MJup), and a highly uncertain planetary radius (0.7−1.7 RJup) was determined. Aims. We aim to better characterise both the star and the planet and precisely measure their orbital and physical parameters. Methods. In order to constrain the mass of...[Show more]

CollectionsANU Research Publications
Date published: 2020
Type: Journal article
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201936532
Access Rights: Open Access


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