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Integrated system tests of the LSST raft tower modules

Lead Author: 
O'Connor, Paul
Other Authors/Credits: 
Antilogus, P.; Doherty, P.; Haupt, J.; Herrmann, S.; Huffer, M.; Juramy-Giles, C.; Kuczewski, J.; Russo, S.; Stubbs, C.; Van Berg, R.
Publication Date: 
Wednesday, July 27, 2016
Conference Papers
P. O'Connor ; P. Antilogus ; P. Doherty ; J. Haupt ; S. Herrmann, et al. " Integrated system tests of the LSST raft tower modules ", Proc. SPIE 9915, High Energy, Optical, and Infrared Detectors for Astronomy VII, 99150X (July 27, 2016); doi:10.1117/12.2232729;
Journal or Publication name: 
SPIE Proceedings
The science focal plane of the LSST camera is made up of 21 fully autonomous 144 Mpixel imager units designated raft tower modules (RTM). These imagers incorporate nine 4K x 4K fully-depleted CCDs and 144 channels of readout electronics, including a dedicated CMOS video processing ASIC and...

Financial support for LSST comes from the National Science Foundation (NSF) through Cooperative Agreement No. 1258333, the Department of Energy (DOE) Office of Science under Contract No. DE-AC02-76SF00515, and private funding raised by the LSST Corporation. The NSF-funded LSST Project Office for construction was established as an operating center under management of the Association of Universities for Research in Astronomy (AURA).  The DOE-funded effort to build the LSST camera is managed by the SLAC National Accelerator Laboratory (SLAC).
The National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.
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