Abstract Study Analysis Group 21 (SAG21) of NASA's Exoplanet Exploration Program
Analysis Group was organized to study the effect of stellar contamination on space-based …

Ultracool dwarf stars are abundant, long-lived and uniquely suited to enable the
atmospheric study of transiting terrestrial companions with the JWST. Among them, the most …

Molecular oxygen is a strong indicator of life on Earth and may indicate biological processes
on exoplanets too. Recent studies proposed that Earth-like O2 levels might be detectable on …

Context. Several planetary formation models have been proposed to explain the observed
abundance and variety of compositions of super-Earths and mini-Neptunes. In this context …

We present the discovery of an Earth-mass planet (M b sin i= 1.26±0.21 M⊕) on a 15.6 d
orbit of a relatively nearby (d~ 9.6 pc) and low-mass (0.167±0.011 M⊙) M5. 0 V star, Wolf …

We present the discovery and validation of two TESS exoplanets orbiting nearby M dwarfs:
TOI-2084 b, and TOI-4184b. We characterized the host stars by combining spectra from …

Humanity is close to characterizing the atmospheres of rocky exoplanets due to the advent
of JWST. These astronomical observations motivate us to understand exoplanetary …

We report the discovery of two exoplanets around the M dwarfs GJ 724 and GJ 3988 using
the radial velocity (RV) method. We obtained a total of 153 3.5 m Calar Alto/CARMENES …

The main scientific goal of TESS is to find planets smaller than Neptune around stars that
are bright enough to allow for further characterization studies. Given our current …

In the last decade, a dozen close-in giant planets have been discovered orbiting stars with
spectral types ranging from M0 to M4, a mystery since known formation pathways do not …