Multiplicity of M dwarfs from close spectroscopic binaries to ultra-wide systems
Complete multiplicity study ranging from close spectroscopic binaries to ultra-wide companions.
These publications provide the scientific foundation for the code projects featured here.
All my publications are listed on ADS . For more details about my scientific output, see my CV .
Keywords: cool stars · binaries · exoplanets · radial velocity
Complete multiplicity study ranging from close spectroscopic binaries to ultra-wide companions.
Gaia EDR3 study of known and newly identified multiple systems containing cool dwarfs.
Benchmark study of colours and stellar parameters in the CARMENES input catalogue.
Follow-up of TESS candidates with radial velocities and photometry.
Two super-Earth- or sub-Neptune-mass planets orbiting a quiet K7 star.
Kinematic analysis of 2187 M dwarfs, identifying 191 young star candidates.
Study of 212 exoplanet host stars in multiple systems.
Characterisation of the nearby warm rocky planet Gl 486 b.
Spectral-synthesis study of stellar parameters for 343 M dwarfs.
Analysis of the potential for stable exomoons around M-dwarf planets.
Comparison of methods for radii and masses of nearby M dwarfs.