9 August 2016 DESI-GFA testbench facilities for CCDs characterization
Author Affiliations +
The DESI-GFA subsystem, used for Guiding, Focusing and Alignment, is one of the key parts for the DESI instrument (The Dark Energy Spectroscopic Instrument), planned for the Mayall 4-meter telescope at Kitt Peak National Observatory, Arizona, U.S. On this paper are presented the test bench facilities developed for the characterization of an e2v CCD230-42 CCD which is expected to be used at room temperature on each one of the ten small cameras composing the DESI-GFA system.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jorge Jiménez , Jorge Jiménez , José M. Illa, José M. Illa, Juan de Vicente, Juan de Vicente, Ricard Casas, Ricard Casas, } "DESI-GFA testbench facilities for CCDs characterization", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99088A (9 August 2016); doi: 10.1117/12.2232430; https://doi.org/10.1117/12.2232430


CCD emulator design for LSST camera
Proceedings of SPIE (July 26 2016)
An overview of AONGC and the ESO adaptive optics wave...
Proceedings of SPIE (September 12 2012)
CCD detector upgrade for NOAO's 8192x8192 Mosaic
Proceedings of SPIE (July 08 1998)
Software configurable CCD camera for SOHO mission
Proceedings of SPIE (November 24 1996)

Back to Top