ZIMPOL/CHEOPS is a polarimetric imager being developed for the Very Large Telescope for the direct detection of extra-solar planets. The imager is operated by the European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile.
The Zurich Imaging Polarimeter (ZIMPOL) provides diffraction limited classical imaging and differential polarimetric imaging (DPI) at 15 mas resolution in the visible spectrum and is one of three scientific subsystem integrated into the VLT-SPHERE instrument used at VLT's Unit Telescope 3, Melipal.
- Schmid, H. M.; Gisler, D.; Joos, F.; Povel, H. P.; Stenflo, J. O.; Feldt, M.; et al. (2005-12-01) [15–19 March 2004]. A. Adamson; C. Aspin; C. J. Davis; T. Fujiyoshi, eds. "ZIMPOL/CHEOPS: a Polarimetric Imager for the Direct Detection of Extra-solar Planets". Astronomical Polarimetry: Current Status and Future Directions ASP Conference Series, Conference Proceedings. Waikoloa, Hawai'i, USA. 343: 89. Bibcode:2005ASPC..343...89S. Retrieved 2012-01-22.
- "ZIMPOL - The Zurich IMaging POLarimeter". Retrieved 2012-01-21.[dead link]
- "SPHERE Exposure Time Calculator – Instrument description". 26 February 2015. Retrieved 3 July 2015.
- "CHaracterizing Extrasolar planets by Opto-infrared Polarimetry and Spectroscopy". Archived from the original on 2012-01-23. Retrieved 2012-01-21.
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