Transmission spectroscopy is one of the premier methods used to probe the temperature,
composition, and cloud properties of exoplanet atmospheres. Recent studies have …

We report the discovery, mass, and radius determination of TOI-1801 b, a temperate mini-
Neptune around a young M dwarf. TOI-1801 b was observed in TESS sectors 22 and 49 …

HD 191939 (TOI-1339) is a nearby (d= 54 pc), bright (V= 9 mag), and inactive Sun-like star
(G9 V) known to host a multi-planet transiting system. Ground-based spectroscopic …

Context. The NASA mission TESS is currently doing an all-sky survey from space to detect
transiting planets around bright stars. As part of the validation process, the most promising …

We report the discovery and characterization of TOI-1759 b, a temperate (400 K) sub-
Neptune-sized exoplanet orbiting the M dwarf TOI-1759 (TIC 408636441). TOI-1759 b was …

We report the discovery and characterization of two small transiting planets orbiting the
bright M3. 0V star TOI-1468 (LSPM J0106+ 1913), whose transit signals were detected in …

We report the discovery of a multiplanetary system transiting the M0 V dwarf HD 260655 (GJ
239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655 b …

We present a comprehensive analysis of the Hubble Space Telescope observations of the
atmosphere of WASP-121 b, an ultra-hot Jupiter. After reducing the transit, eclipse, and …

Context. The current architecture of a given multi-planetary system is a key fingerprint of its
past formation and dynamical evolution history. Long-term follow-up observations are key to …

The chromatic contamination that arises from photospheric heterogeneities, eg, spots and
faculae on the host star presents a significant noise source for exoplanet transmission …