7 March 2003 CCD imaging systems for DEIMOS
Author Affiliations +
The DEep Imaging Multi-Object Spectrograph (DEIMOS) images with an 8K x 8K science mosaic composed of eight 2K x 4K MIT/Lincoln Lab (MIT/LL) CCDs. It also incorporates two 1200 x 600 Orbit Semiconductor CCDs for active, close-loop flexure compensation. The science mosaic CCD controller system reads out all eight science CCDs in 40 seconds while maintaining the low noise floor of the MIT/Lincoln Lab CCDs. The flexure compensation (FC) CCD controller reads out the FC CCDs several times per minute during science mosaic exposures. The science mosaic CCD controller and the FC CCD controller are located on the electronics ring of DEIMOS. Both the MIT/Lincoln Lab CCDs and the Orbit flexure compensation CCDs and their associated cabling and printed circuit boards are housed together in the same detector vessel that is approximately 10 feet away from the electronics ring. Each CCD controller has a modular hardware design and is based on the San Diego State University (SDSU) Generation 2 (SDSU-2) CCD controller. Provisions have been made to the SDSU-2 video board to accommodate external CCD preamplifiers that are located at the detector vessel. Additional circuitry has been incorporated in the CCD controllers to allow the readback of all clocks and bias voltages for up to eight CCDs, to allow up to 10 temperature monitor and control points of the mosaic, and to allow full-time monitoring of power supplies and proper power supply sequencing. Software control features of the CCD controllers are: software selection between multiple mosaic readout modes, readout speeds, selectable gains, ramped parallel clocks to eliminate spurious charge on the CCDs, constant temperature monitoring and control of each CCD within the mosaic, proper sequencing of the bias voltages of the CCD output MOSFETs, and anti-blooming operation of the science mosaic. We cover both the hardware and software highlights of both of these CCD controller systems as well as their respective performance.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christopher A.F. Wright, Christopher A.F. Wright, Robert I. Kibrick, Robert I. Kibrick, Barry Alcott, Barry Alcott, David Kirk Gilmore, David Kirk Gilmore, Terry Pfister, Terry Pfister, David J. Cowley, David J. Cowley, "CCD imaging systems for DEIMOS", Proc. SPIE 4841, Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, (7 March 2003); doi: 10.1117/12.461881; https://doi.org/10.1117/12.461881


IDSAC-IUCAA digital sampler array controller
Proceedings of SPIE (July 26 2016)
SEDHI a new generation of detection electronics for earth...
Proceedings of SPIE (November 20 2017)
Optimization of CCD performances at high frequencies
Proceedings of SPIE (May 15 2003)
Astros: A Sub-Arcsec CCD Star Tracker
Proceedings of SPIE (November 07 1984)
AAO2: a general purpose CCD controller for the AAT
Proceedings of SPIE (September 28 2004)

Back to Top