The highly inflated giant planet WASP-174b

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 P orb = 4.23 days). However only an upper limit was placed on the planet mass (

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Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 2020-01, Vol.633, p.A30
Main Authors: Mancini, L., Sarkis, P., Henning, Th, Bakos, G. Á., Bayliss, D., Bento, J., Bhatti, W., Brahm, R., Csubry, Z., Espinoza, N., Hartman, J., Jordán, A., Penev, K., Rabus, M., Suc, V., de Val-Borro, M., Zhou, G., Chen, G., Damasso, M., Southworth, J., Tan, T. G.
Format: Article
Language:English
Subjects:
Confidence intervals
Darkening
Density
Empirical analysis
Extrasolar planets
F stars
Orbits
Parameters
Photometry
Physical properties
Planetary systems
Radial velocity
Space telescopes
Stellar systems
Transit
Transits
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Summary: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 P orb = 4.23 days). However only an upper limit was placed on the planet mass (
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/201936532