Nicolas Iro

TL;DR: In this paper, a chemical network was developed for the temperature and pressure range relevant to hot Jupiters atmospheres, and the authors compared the predictions obtained from this scheme with equilibrium calculations, with different schemes available in the literature that contain N-bearing species and with previously published photochemical models.

TL;DR: The Transiting Exoplanet Survey Satellite (TESS) as discussed by the authors will discover transiting planets orbiting the brightest stars, enabling, in principle, an atmospheric survey of 102-103 bright hot Jupiters and warm sub-Neptunes.

TL;DR: In this paper, the authors measured the amplitude, shape and phase of the thermal phase effect for the massive hot Jupiter system WASP-18b with the Spitzer spacecraft covering the entire orbit at 3.6 micron and 4.5 micron.

TL;DR: In this paper, the authors measured the amplitude, shape and phase of the thermal phase effect for the massive hot Jupiter system WASP-18 b with the Spitzer spacecraft covering the entire orbit at 3.6 and 4.5 μm.

TL;DR: Gautier et al. as discussed by the authors proposed an interpretation of the composition of volatiles observed in comets based on their trapping in the form of clathrate hydrates in the solar nebula.