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The Spectro-Polarimetric High-contrast Exoplanet REsearch - SPHERE - is the extreme adaptive optics system and coronagraphic facility at the VLT. Its primary science goal is imaging, low-resolution spectroscopic, and polarimetric characterization of extra-solar planetary systems at optical and near-infrared wavelengths.

SPHERE consists for four arms: the common path infrastructure (CPI) with the AO system and the coronograph, the infrared integral field spectrograph (IFS), the infrared dual-band imager and spectrograph (IRDIS) and the Zurich imaging polarimeter (ZIMPOL) operating in the optical.

These pages contain information about SPHERE Quality Control, pipeline processing, and data flow operations.

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