International audienceDirect detection and spectral characterisation of extrasolar planets is one of the most exciting but also one of the most challenging areas in modern astronomy. For its second-generation instrumentation on the VLT, ESO has supported two phase A studies for a so-called ‘Planet Finder' dedicated instrument. Based on the results of these two studies, a unique instrument, SPHERE, is now considered for first light in 2010, including a powerful extreme adaptive optics system (SAXO), various coronagraphs, an infrared differential imaging camera (IRDIS), an infrared integral field spectrograph (IFS) and a visible differential polarimeter (ZIMPOL)
The Planet Finder instrument for ESO's VLT telescope, scheduled for first light in 2010, aims to det...
SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) is a second generation instrument for...
International audienceObservations of circumstellar environments that look for the direct signal of ...
International audienceDirect detection and spectral characterisation of extrasolar planets is one of...
The Planet Finder instrument for ESO's VLT telescope, scheduled for first light in 2010, aims to det...
SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) is a second generation instrument for...
International audienceObservations of circumstellar environments that look for the direct signal of ...
International audienceDirect detection and spectral characterisation of extrasolar planets is one of...
The Planet Finder instrument for ESO's VLT telescope, scheduled for first light in 2010, aims to det...
SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) is a second generation instrument for...
International audienceObservations of circumstellar environments that look for the direct signal of ...