Publication: The guider and wavefront curvature sensor subsystem for the Large Synoptic Survey Telescope
Open/View Files
Date
2014
Published Version
Journal Title
Journal ISSN
Volume Title
Publisher
Society of Photo-Optical Instrumentation Engineers (SPIE)
The Harvard community has made this article openly available. Please share how this access benefits you.
Citation
Riot, Vincent J., Kirk Arndt, Chuck Claver, Peter E. Doherty, D. K. Gilmore, et al. 2014. "The guider and wavefront curvature sensor subsystem for the Large Synoptic Survey Telescope", Proceedings of Society of Photo-Optical Instrumentation Engineers (SPIE) 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914774, Montreal, Canada, July 8, 2014.
Research Data
Abstract
The Large Synoptic Survey Telescope instrument include four guiding and wavefront sensing subsystems called corner raft subsystems, in addition to the main science array of 189 4K x 4K CCDs. These four subsystems are placed at the four corners of the instrumented field of view. Each wavefront/guiding subsystem comprises a pair of 4K x 4K guide sensors, capable of producing 9 frames/second, and a pair of offset 2K x 4K wavefront curvature sensors from which the images are read out at the cadence of the main camera system, providing 15 sec integrations. These four guider/wavefront corner rafts are mechanically and electrically isolated from the science sensor rafts and can be installed or removed independently from any other focal plane subsystem. We present the implementation of this LSST subsystem detailing both hardware and software development and status.
Description
Other Available Sources
Keywords
Large Synoptic Survey Telescope, guide sensors, Wavefront sensors, ground-based telescope
Terms of Use
This article is made available under the terms and conditions applicable to Open Access Policy Articles (OAP), as set forth at Terms of Service