9 July 2008 The Dark Energy Survey CCD imager design
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The Dark Energy Survey is planning to use a 3 sq. deg. camera that houses a ~ 0.5m diameter focal plane of 62 2k×4k CCDs. The camera vessel including the optical window cell, focal plate, focal plate mounts, cooling system and thermal controls is described. As part of the development of the mechanical and cooling design, a full scale prototype camera vessel has been constructed and is now being used for multi-CCD readout tests. Results from this prototype camera are described.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
H. Cease, H. Cease, D. DePoy, D. DePoy, G. Derylo, G. Derylo, H. T. Diehl, H. T. Diehl, J. Estrada, J. Estrada, B. Flaugher, B. Flaugher, V. Guarino, V. Guarino, K. Kuk, K. Kuk, S. Kuhlmann, S. Kuhlmann, K. Schultz, K. Schultz, R. L. Schmitt, R. L. Schmitt, A. Stefanik, A. Stefanik, A. Zhao, A. Zhao, } "The Dark Energy Survey CCD imager design", Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 70146N (9 July 2008); doi: 10.1117/12.788200; https://doi.org/10.1117/12.788200


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