25 September 2012 Architecture of PAU survey camera readout electronics
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PAUCam is a new camera for studying the physics of the accelerating universe. The camera will consist of eighteen 2Kx4K HPK CCDs: sixteen for science and two for guiding. The camera will be installed at the prime focus of the WHT (William Herschel Telescope). In this contribution, the architecture of the readout electronics system is presented. Back- End and Front-End electronics are described. Back-End consists of clock, bias and video processing boards, mounted on Monsoon crates. The Front-End is based on patch panel boards. These boards are plugged outside the camera feed-through panel for signal distribution. Inside the camera, individual preamplifier boards plus kapton cable completes the path to connect to each CCD. The overall signal distribution and grounding scheme is shown in this paper.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Javier Castilla, Javier Castilla, Laia Cardiel-Sas, Laia Cardiel-Sas, Juan De Vicente, Juan De Vicente, Joseph Illa, Joseph Illa, Jorge Jimenez, Jorge Jimenez, Marino Maiorino, Marino Maiorino, Gustavo Martinez, Gustavo Martinez, } "Architecture of PAU survey camera readout electronics", Proc. SPIE 8453, High Energy, Optical, and Infrared Detectors for Astronomy V, 84532P (25 September 2012); doi: 10.1117/12.924890; https://doi.org/10.1117/12.924890


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