SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) is a second generation instrument for the VLT optimized for the very high-contrast imaging around bright stars [J.-L. Beuzit, M. Feldt, K. Dohlen et al. in Messenger 125, 29 (2006)]. The primary goal is the detection and characterization of new giant planets around a variety of nearby stars. Together with the observation of early planetary systems and disks, and in association with the results of other planet search techniques, SPHERE will be a primary contributor to get a complete picture of the variety of planetary systems and to better understand their mechanisms of formation and evolution. Such results will be obtained before even more ambitious projects for the direct imagi...
Direct detection and spectral characterization of extra-solar planets is one of the most exciting bu...
International audience<p>SPHERE, the high contrast imaging facility at the VLT has contributed...
International audienceDirect imaging and spectral characterisation of exoplanets is one of the most ...
SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) is a second generation instrument for...
Direct detection and spectral characterization of extra-solar planets is one of the most exciting bu...
The Planet Finder instrument for ESO's VLT telescope, scheduled for first light in 2010, aims to det...
SPHERE (Beuzit et al,. 2019) has now been in operation at the VLT for more than 5 years, demonstrati...
Direct detection and spectral characterization of extra-solar planets is one of the most exciting bu...
Direct detection and spectral characterization of extra-solar planets is one of the most exciting bu...
International audience<p>SPHERE, the high contrast imaging facility at the VLT has contributed...
International audienceDirect imaging and spectral characterisation of exoplanets is one of the most ...
SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) is a second generation instrument for...
Direct detection and spectral characterization of extra-solar planets is one of the most exciting bu...
The Planet Finder instrument for ESO's VLT telescope, scheduled for first light in 2010, aims to det...
SPHERE (Beuzit et al,. 2019) has now been in operation at the VLT for more than 5 years, demonstrati...
Direct detection and spectral characterization of extra-solar planets is one of the most exciting bu...
Direct detection and spectral characterization of extra-solar planets is one of the most exciting bu...
International audience<p>SPHERE, the high contrast imaging facility at the VLT has contributed...
International audienceDirect imaging and spectral characterisation of exoplanets is one of the most ...