We report the discovery of a Neptune-like planet (LP 714-47 b, P= 4.05204 d, mb=
30.8±1.5M⊕, R b= 4.7±0.3 R⊕) located in the “hot Neptune desert”. Confirmation of the …

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 …

Despite their activity, low-mass stars are of particular importance for the search of
exoplanets by the means of Doppler spectroscopy, as planets with lower masses become …

We report on the first star discovered to host a planet detected by radial velocity (RV)
observations obtained within the CARMENES survey for exoplanets around M dwarfs. HD …

We report the discovery of two planetary systems, namely G 264–012, an M 4.0 dwarf with
two terrestrial planets (M⊕ and M⊕), and Gl 393, a bright M 2.0 dwarf with one terrestrial …

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 a temperate sub-Neptune around the nearby mid-
M dwarf TIC 470381900 (TOI-1696), with a radius of 3.09±0.11 R⊕ and an orbital period of …

Context. The nearby ultra-compact multiplanetary system YZ Ceti consists of at least three
planets, and a fourth tentative signal. The orbital period of each planet is the subject of …

We present the discovery and characterisation of two transiting planets observed by the
Transiting Exoplanet Survey Satellite (TESS) orbiting the nearby (d⋆≈ 22 pc), bright (J≈ 9 …

Context. Teegarden's Star is the brightest and one of the nearest ultra-cool dwarfs in the
solar neighbourhood. For its late spectral type (M7. 0 V), the star shows relatively little …