There are no planets intermediate in size between Earth and Neptune in our Solar System,
yet these objects are found around a substantial fraction of other stars. Population statistics …

We provide a database of transit times and updated ephemerides for 382 planets based on
data from the NASA Transiting Exoplanet Survey Satellite (TESS) and previously reported …

We present the dayside thermal emission spectrum of WASP-77Ab from 2.8 to 5.2 μm as
observed with the NIRSpec instrument on the James Webb Space Telescope (JWST) …

Transit surveys indicate that there is a deficit of Neptune-sized planets on close-in orbits. If
this" Neptune desert" is entirely cleared out by atmospheric mass loss, then planets at its …

The metastable helium triplet in the near-infrared (10 833 Å) is among the most important
probes of exoplanet atmospheres. It can trace their extended outer layers and constrain …

Exoplanet atmospheres are inherently three-dimensional systems in which thermal/chemical
variation and winds can strongly influence spectra. Recently, the ultra-hot Jupiter WASP-76 …

The Ariel Target List: The Impact of TESS and the Potential for Characterizing Multiple
Planets within a System - IOPscience Skip to content IOP Science home Accessibility Help …

The number of exoplanets discovered already exceeds 5000 and continues to increase
daily. The characterization of exoplanets will be the main goal of future space missions. The …

We present an atmospheric analysis of LTT 9779 b, a rare planet situated in the hot-Neptune
desert, that has been observed with Hubble Space Telescope (HST)/WFC3 with G102 and …

Context. Tidal orbital decay is suspected to occur for hot Jupiters in particular, with the only
observationally confirmed case of this being WASP-12b. By examining this effect …