Paper
10 July 2008 The infra-red dual imaging and spectrograph for SPHERE: design and performance
Kjetil Dohlen, Maud Langlois, Michel Saisse, Lucien Hill, Alain Origne, Marc Jacquet, Christophe Fabron, Jean-Claude Blanc, Marc Llored, Michael Carle, Claire Moutou, Arthur Vigan, Anthony Boccaletti, Marcel Carbillet, David Mouillet, Jean-Luc Beuzit
Author Affiliations +
Abstract
The SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) planet finder instrument for ESO's VLT telescope, scheduled for first light in 2011, aims to detect giant extra-solar planets in the vicinity of bright stars by the aid of an extreme-AO turbulence compensation system and to characterize the objects found through spectroscopic and polarimetric observations. Dual imaging observations within the Y, J, H and Ks atmospheric windows (~0.95 - 2.32μm) will be done by the aid of the IRDIS cryogenic camera. We describe briefly the science goals of IRDIS and present its system architecture. Current status of the instrument design is presented, and expected performance is described in terms of end-to-end simulations.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kjetil Dohlen, Maud Langlois, Michel Saisse, Lucien Hill, Alain Origne, Marc Jacquet, Christophe Fabron, Jean-Claude Blanc, Marc Llored, Michael Carle, Claire Moutou, Arthur Vigan, Anthony Boccaletti, Marcel Carbillet, David Mouillet, and Jean-Luc Beuzit "The infra-red dual imaging and spectrograph for SPHERE: design and performance", Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 70143L (10 July 2008); https://doi.org/10.1117/12.789786
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Cited by 122 scholarly publications.
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KEYWORDS
Stars

Optical spheres

Coronagraphy

Optical filters

Imaging spectroscopy

Planets

Adaptive optics

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