2012A&A...542A...4G

We present twenty-three transit light curves and seven occultation light curves for the ultra-short period planet WASP-43b, in addition to eight new measurements of the radial velocity of the star. Thanks to this extensive data set, we improve significantly the parameters of the system. Notably, the largely improved precision on the stellar density (2.41±0.08ρ_☉) combined with constraining the age to be younger than a Hubble time allows us to break the degeneracy of the stellar solution mentioned in the discovery paper. The resulting stellar mass and size are 0.717±0.025M_☉ and 0.667±0.011R_☉. Our deduced physical parameters for the planet are 2.034±0.052M_Jup and 1.036±0.019R_Jup. Taking into account its level of irradiation, the high density of the planet favors an old age and a massive core. Our deduced orbital eccentricity, 0.0035_–0.0025^+0.0060, is consistent with a fully circularized orbit. We detect the emission of the planet at 2.09µm at better than 11-σ, the deduced occultation depth being 1560±140ppm. Our detection of the occultation at 1.19µm is marginal (790±320ppm) and more observations are needed to confirm it. We place a 3-σ upper limit of 850ppm on the depth of the occultation at ∼0.9µm. Together, these results strongly favor a poor redistribution of the heat to the night-side of the planet, and marginally favor a model with no day-side temperature inversion.