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The SPHERE exoplanet imager: status report at PDR
2007
Astronomical Adaptive Optics Systems and Applications III
The SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric observations. It is a complete system with a core made of an extreme-Adaptive Optics (AO) turbulence correction, pupil tracker and interferential coronagraphs. At its back end, an Infra-Red Dual-beam Imaging and Spectroscopy science module and an integral field spectrograph work in the Near Infrared (NIR) Y, J,
doi:10.1117/12.734785
fatcat:wzl3lcitmbc3lge4cwvomspxw4