Abstract The Second Workshop on Extreme Precision Radial Velocities defined circa 2015
the state of the art Doppler precision and identified the critical path challenges for reaching …

Exoplanets can be detected with various observational techniques. Among them, radial
velocity (RV) has the key advantages of revealing the architecture of planetary systems and …

Context. The solar telescope connected to HARPS-N has been observing the Sun since the
summer of 2015. Such a high-cadence, long-baseline data set is crucial for understanding …

Stellar magnetic activity produces time-varying distortions in the photospheric line profiles of
solar-type stars. These lead to systematic errors in high-precision radial-velocity …

We present a spectroscopic analysis of a 1-yr intensive monitoring campaign of the 22-Myr
old planet-hosting M dwarf AU Mic using the HARPS spectrograph. In a companion paper …

Context. Although the new generation of radial-velocity (RV) instruments such as
ESPRESSO are expected to reach the long-term precision required to find other earths, the …

Aims. Even the most precise radial-velocity instruments gather high-resolution spectra that
present systematic errors that a data reduction pipeline cannot identify and correct for …

The detection of Earth-like planets with the radial-velocity (RV) method is currently limited by
the presence of stellar activity signatures. On rotational time-scales, spots and plages (or …

A new regime of precision radial-velocity measurements in the search for Earth-like
exoplanets is being facilitated by high-resolution spectrographs calibrated by laser …

Context. Radial-velocity (RV) signals arising from stellar photospheric phenomena are the
main limitation for precise RV measurements. Those signals induce RV variations an order …