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CCD emulator design for LSST camera

Lead Author: 
Lu, W.
Other Authors/Credits: 
O’Connor, P; Fried, J.; Kuczewski, J.
Publication Date: 
Wednesday, July 27, 2016
Conference Papers
SPIE
Publication-111
W. Lu ; P. O'Connor ; J. Fried and J. Kuczewski " CCD emulator design for LSST camera ", Proc. SPIE 9915, High Energy, Optical, and Infrared Detectors for Astronomy VII, 99152O (July 27, 2016); doi:10.1117/12.2234033; http://dx.doi.org/10.1117/12.2234033
Journal or Publication name: 
SPIE Proceedings
Citable: 
no
Abstract: 
As part of the LSST project, a comprehensive CCD emulator that operates three CCDs simultaneously has been developed for testing multichannel readout electronics. Based on an Altera Cyclone V FPGA for timing and control, the emulator generates 48 channels of simulated video waveform in response to...

Financial support for Rubin Observatory 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 Rubin Observatory 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 Rubin Observatory LSST Camera (LSSTCam) 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.
NSF and DOE will continue to support Rubin Observatory in its Operations phase. They will also provide support for scientific research with LSST data.   




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