The fates of planetary systems provide unassailable insights into their formation and
represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main …

Context. The main goal of the CARMENES survey is to find Earth-mass planets around
nearby M-dwarf stars. Seven M dwarfs included in the CARMENES sample had been …

Context. We have obtained precise radial velocities for a sample of 373 G and K type giants
at Lick Observatory regularly over more than 12 years. Planets have been identified around …

Context. Radial velocity surveys of evolved stars allow us to probe a higher stellar mass
range, on average, compared to main-sequence samples. Hence, differences between the …

Observations of the population of cold Jupiter planets (r> 1 AU) show that nearly all of these
planets orbit their host star on eccentric orbits. For planets up to a few Jupiter masses …

Context. Exoplanet searches have revealed interesting correlations between the stellar
properties and the occurrence rate of planets. In particular, different independent surveys …

Most of our knowledge of planets orbiting nearby stars comes from Doppler surveys. For
spaced-based, high-contrast imaging missions, nearby stars with Doppler-discovered …

TOI-2202 b is a transiting warm Jovian-mass planet with an orbital period of P= 11.91 days
identified from the Full Frame Images data of five different sectors of the TESS mission. Ten …

I consider the dynamics of mean-motion resonances (MMRs) between pairs of coplanar
planets and derive a new integrable Hamiltonian model for the planets' resonant motion …

Abstract In about 6 Gyr our Sun will evolve into a red giant and finally end its life as a white
dwarf. This stellar metamorphosis will occur to virtually all known host stars of exoplanetary …