The CARMENES radial velocity (RV) survey is observing 324 M dwarfs to search for any
orbiting planets. In this paper, we present the survey sample by publishing one CARMENES …

Aims. The main goal of this work is to measure rotation periods of the M-type dwarf stars
being observed by the CARMENES exoplanet survey to help distinguish radial-velocity …

During the first billion years of their life, exoplanet atmospheres are modified by different
atmospheric escape phenomena that can strongly affect the shape and morphology of the …

Present and future high-precision radial-velocity spectrometers dedicated to the discovery of
low-mass planets orbiting low-mass dwarfs need to focus on the best selected stars to make …

Since 2012, thanks to the installation of the high-resolution echelle spectrograph in the
optical range HARPS-N, the Italian telescope TNG (La Palma) became one of the key …

Aims. HD 142527 is one of the most frequently studied Herbig Ae/Be stars with a transitional
disk that hosts a large cavity that is up to about 100 au in radius. For this reason, it has been …

Context. Transiting ultra-hot Jupiters are ideal candidates for studying the exoplanet
atmospheres and their dynamics, particularly by means of high-resolution spectra with high …

Context. The distribution of exoplanets around low-mass stars is still not well understood.
Such stars, however, present an excellent opportunity for reaching down to the rocky and …

A wave of precision radial velocity (RV) instruments will open the door to exploring the
populations of companions of low-mass stars. The Palomar Radial Velocity Instrument …

Context. An inner companion has recently been discovered orbiting the prototype of
classical Cepheids, δ Cep, whose orbital parameters are still not fully constrained. Aims. We …