9 August 2016 Integration and verification testing of the Large Synoptic Survey Telescope camera
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We present an overview of the Integration and Verification Testing activities of the Large Synoptic Survey Telescope (LSST) Camera at the SLAC National Accelerator Lab (SLAC). The LSST Camera, the sole instrument for LSST and under construction now, is comprised of a 3.2 Giga-pixel imager and a three element corrector with a 3.5 degree diameter field of view. LSST Camera Integration and Test will be taking place over the next four years, with final delivery to the LSST observatory anticipated in early 2020. We outline the planning for Integration and Test, describe some of the key verification hardware systems being developed, and identify some of the more complicated assembly/integration activities. Specific details of integration and verification hardware systems will be discussed, highlighting some of the technical challenges anticipated.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Travis Lange, Travis Lange, Tim Bond, Tim Bond, James Chiang, James Chiang, Kirk Gilmore, Kirk Gilmore, Seth Digel, Seth Digel, Richard Dubois, Richard Dubois, Tom Glanzman, Tom Glanzman, Tony Johnson, Tony Johnson, Margaux Lopez, Margaux Lopez, Scott P. Newbry, Scott P. Newbry, Martin E. Nordby, Martin E. Nordby, Andrew P. Rasmussen, Andrew P. Rasmussen, Kevin A. Reil, Kevin A. Reil, Aaron J. Roodman, Aaron J. Roodman, } "Integration and verification testing of the Large Synoptic Survey Telescope camera", Proc. SPIE 9911, Modeling, Systems Engineering, and Project Management for Astronomy VI, 991108 (9 August 2016); doi: 10.1117/12.2234506; https://doi.org/10.1117/12.2234506


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