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27 April 2024
 
  » arxiv » 2004.6622

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Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b
Benjamin F. Cooke ; Don Pollacco ; Y. Almleaky ; K. Barkaoui ; Z. Benkhaldoun ; James A. Blake ; François Bouchy ; Panos Boumis ; D. J. A. Brown ; Ivan Bruni ; A. Burdanov ; Andrew Collier Cameron ; Paul Chote ; A. Daassou ; Giuseppe D'ago ; Shweta Dalal ; Mario Damasso ; L. Delrez ; A. P. Doyle ; E. Ducrot ; M. Gillon ; G. Hébrard ; C. Hellier ; Thomas Henning ; E. Jehin ; Flavien Kiefer ; George W. King ; Alexios Liakos ; Théo Lopez ; Luigi Mancini ; Rosemary Mardling ; P. F. L. Maxted ; James McCormac ; C. Murray ; Louise D. Nielsen ; Hugh Osborn ; E. Palle ; Francesco Pepe ; F. J. Pozuelos ; J. Prieto-Arranz ; D. Queloz ; Nicole Schanche ; Damien Ségransan ; Barry Smalley ; John Southworth ; S. Thompson ; Oliver Turner ; Stéphane Udry ; S. Velasco ; Richard West ; Pete Wheatley ;
Date 14 Apr 2020
AbstractWe report the discovery of two transiting exoplanets from the WASP survey, WASP-150b and WASP-176b. WASP-150b is an eccentric ($e$ = 0.38) hot Jupiter on a 5.6 day orbit around a $V$ = 12.03, F8 main-sequence host. The host star has a mass and radius of 1.4 $ m M_{odot}$ and 1.7 $ m R_{odot}$ respectively. WASP-150b has a mass and radius of 8.5 $ m M_J$ and 1.1 $ m R_J$, leading to a large planetary bulk density of 6.4 $ m ho_J$. WASP-150b is found to be $sim3$ Gyr old, well below its circularisation timescale, supporting the eccentric nature of the planet. WASP-176b is a hot Jupiter planet on a 3.9 day orbit around a $V$ = 12.01, F9 sub-giant host. The host star has a mass and radius of 1.3 $ m M_{odot}$ and 1.9 $ m R_{odot}$. WASP-176b has a mass and radius of 0.86 $ m M_J$ and 1.5 $ m R_J$ respectively, leading to a planetary bulk density of 0.23 $ m ho_J$.
Source arXiv, 2004.6622
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