Context. Following the first discovery of a planet orbiting a giant star in 2002, we started the CORALIE radial-velocity search for companions around evolved stars. We present the observations of three stars conducted at the 1.2 m Leonard Euler Swiss telescope at La Silla Observatory, Chile, using the CORALIE spectrograph. Aims. We aim to detect planetary companions to intermediate-mass G- and K- type evolved stars and perform a statistical analysis of this population. We searched for new planetary systems around the stars HD 22532 (TIC 200851704), HD 64121 (TIC 264770836), and HD 69123 (TIC 146264536). Methods. We have followed a volume-limited sample of 641 red giants since 2006 to obtain high-precision radial-velocity measurements. We us...
Context. Precision radial velocities are required to discover and characterize exoplanets. Optical s...
Context. Since 1998, a planet-search program around main sequence stars within 50 pc in th...
Artículo de publicación ISIContext. More than 40 planets have been found around giant stars, reveali...
Context. Following the first discovery of a planet orbiting a giant star in 2002, we started the COR...
International audienceContext. Following the first discovery of a planet orbiting a giant star in 20...
Context. Increasing the number of detected exoplanets is far from anecdotal, especially for long-per...
International audienceContext. Since 1998, a planet-search around main sequence stars within 50 pc i...
Context. Since 1998, a planet-search around main sequence stars within 50 pc in the southern hemisph...
Very little is known about giant planets and brown dwarfs at an orbital separation greater than 5 AU...
Aims. The aim of our paper is to investigate the low-amplitude and long-period variations in evolved...
Context. The advent of asteroseismology as the golden path to precisely characterize single stars na...
The radial velocity (RV), or Doppler, technique is one of the most successful methods in the search ...
Artículo de publicación ISIContext. Precision radial velocities are required to discover and charact...
Context. Precision radial velocities are required to discover and characterize exoplanets. Optical s...
Context. Since 1998, a planet-search program around main sequence stars within 50 pc in th...
Artículo de publicación ISIContext. More than 40 planets have been found around giant stars, reveali...
Context. Following the first discovery of a planet orbiting a giant star in 2002, we started the COR...
International audienceContext. Following the first discovery of a planet orbiting a giant star in 20...
Context. Increasing the number of detected exoplanets is far from anecdotal, especially for long-per...
International audienceContext. Since 1998, a planet-search around main sequence stars within 50 pc i...
Context. Since 1998, a planet-search around main sequence stars within 50 pc in the southern hemisph...
Very little is known about giant planets and brown dwarfs at an orbital separation greater than 5 AU...
Aims. The aim of our paper is to investigate the low-amplitude and long-period variations in evolved...
Context. The advent of asteroseismology as the golden path to precisely characterize single stars na...
The radial velocity (RV), or Doppler, technique is one of the most successful methods in the search ...
Artículo de publicación ISIContext. Precision radial velocities are required to discover and charact...
Context. Precision radial velocities are required to discover and characterize exoplanets. Optical s...
Context. Since 1998, a planet-search program around main sequence stars within 50 pc in th...
Artículo de publicación ISIContext. More than 40 planets have been found around giant stars, reveali...