International audienceThe star GJ 676A is an M0 dwarf hosting both gas-giant and super-Earth-type planets that were discovered with radial-velocity measurements. Using FORS2/VLT, we obtained position measurements of the star in the plane of the sky that tightly constrain its astrometric reflex motion caused by the super-Jupiter planet "b" in a 1052-day orbit. This allows us to determine the mass of this planet to be , which is 40% higher than the minimum mass inferred from the radial-velocity orbit. Using new HARPS radial-velocity measurements, we improve upon the orbital parameters of the inner low-mass planets "d" and "e" and we determine the orbital period of the outer giant planet "c" to be Pc = 7340 days under the assumption of a circu...
Context. Several M dwarfs are targets of systematical monitoring in searches for Doppler signals cau...
International audienceThe source GJ1132 is a nearby red dwarf known to host a transiting Earth-size ...
International audienceContext. We present the results of a seven-year-long radial velocity survey of...
International audienceThe star GJ 676A is an M0 dwarf hosting both gas-giant and super-Earth-type pl...
The star GJ 676A is an M0 dwarf hosting both gas-giant and super-Earth-type planets that were discov...
International audiencePrecise radial-velocity measurements for data acquired with the HARPS spectrog...
International audiencePrecise radial-velocity measurements for data acquired with the HARPS spectrog...
Precise radial-velocity measurements for data acquired with the HARPS spectrograph infer that three...
Fewer giants planets are found around M dwarfs than around more massive stars, and this dependence o...
VizieR On-line Data Catalog: J/A+A/511/A21Precise radial-velocity measurements for data acquired wit...
International audienceContext. The β Pictoris system with its debris disk and a massive giant planet...
Context. Several M dwarfs are targets of systematical monitoring in searches for Doppler signals cau...
International audienceThe source GJ1132 is a nearby red dwarf known to host a transiting Earth-size ...
International audienceContext. We present the results of a seven-year-long radial velocity survey of...
International audienceThe star GJ 676A is an M0 dwarf hosting both gas-giant and super-Earth-type pl...
The star GJ 676A is an M0 dwarf hosting both gas-giant and super-Earth-type planets that were discov...
International audiencePrecise radial-velocity measurements for data acquired with the HARPS spectrog...
International audiencePrecise radial-velocity measurements for data acquired with the HARPS spectrog...
Precise radial-velocity measurements for data acquired with the HARPS spectrograph infer that three...
Fewer giants planets are found around M dwarfs than around more massive stars, and this dependence o...
VizieR On-line Data Catalog: J/A+A/511/A21Precise radial-velocity measurements for data acquired wit...
International audienceContext. The β Pictoris system with its debris disk and a massive giant planet...
Context. Several M dwarfs are targets of systematical monitoring in searches for Doppler signals cau...
International audienceThe source GJ1132 is a nearby red dwarf known to host a transiting Earth-size ...
International audienceContext. We present the results of a seven-year-long radial velocity survey of...