We describe a high-precision Doppler search for giant planets orbiting a well-defined sample of metal-poor dwarfs in the field. This experiment constitutes a fundamental test of theoretical predictions which will help discriminate between proposed giant planet formation and migration models. We present here details on the survey as well as an overall assessment of the quality of our measurements, making use of the results for the stars that show no significant velocity variation
Comparisons between the planet populations around solar-type stars and those orbiting M dwarfs shed ...
We report precise Doppler measurements of the nearby (d = 10.34 pc) M dwarf Gl 649 that reveal the p...
We review the observed properties of exoplanets found by the Doppler technique that has revealed 152...
We describe a high-precision Doppler search for giant planets orbiting a well-defined sample of meta...
We describe a high-precision Doppler search for giant planets orbiting a well-defined sample of meta...
We present an analysis of three years of precision radial velocity (RV) measurements of 160 metal-po...
One of the most promising methods of discovering nearby, low-mass planets in the habitable zones of ...
Analyses of exoplanet statistics suggest a trend of giant planet occurrence with host star mass, a c...
The 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018We p...
Transiting extrasolar planets are now discovered jointly by photometric surveys and by radial veloci...
Context. Radial velocity surveys of evolved stars allow us to probe a higher stellar mass range, on ...
The radial velocity (RV), or Doppler, technique is one of the most successful methods in the search ...
Searching for extrasolar planets around stars of different metallicity may provide strong constraint...
We constrain the densities of Earth- to Neptune-size planets around very cool (Te = 3660-4660K) Kepl...
Analyses of exoplanet statistics suggest a trend of giant planet occurrence with host star mass, a c...
Comparisons between the planet populations around solar-type stars and those orbiting M dwarfs shed ...
We report precise Doppler measurements of the nearby (d = 10.34 pc) M dwarf Gl 649 that reveal the p...
We review the observed properties of exoplanets found by the Doppler technique that has revealed 152...
We describe a high-precision Doppler search for giant planets orbiting a well-defined sample of meta...
We describe a high-precision Doppler search for giant planets orbiting a well-defined sample of meta...
We present an analysis of three years of precision radial velocity (RV) measurements of 160 metal-po...
One of the most promising methods of discovering nearby, low-mass planets in the habitable zones of ...
Analyses of exoplanet statistics suggest a trend of giant planet occurrence with host star mass, a c...
The 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018We p...
Transiting extrasolar planets are now discovered jointly by photometric surveys and by radial veloci...
Context. Radial velocity surveys of evolved stars allow us to probe a higher stellar mass range, on ...
The radial velocity (RV), or Doppler, technique is one of the most successful methods in the search ...
Searching for extrasolar planets around stars of different metallicity may provide strong constraint...
We constrain the densities of Earth- to Neptune-size planets around very cool (Te = 3660-4660K) Kepl...
Analyses of exoplanet statistics suggest a trend of giant planet occurrence with host star mass, a c...
Comparisons between the planet populations around solar-type stars and those orbiting M dwarfs shed ...
We report precise Doppler measurements of the nearby (d = 10.34 pc) M dwarf Gl 649 that reveal the p...
We review the observed properties of exoplanets found by the Doppler technique that has revealed 152...