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dc.contributor.authorRiot, Vincent J.
dc.contributor.authorArndt, Kirk
dc.contributor.authorClaver, Chuck
dc.contributor.authorDoherty, Peter E.
dc.contributor.authorGilmore, D. K.
dc.contributor.authorHascall, Patrick A.
dc.contributor.authorHerrmann, Sven
dc.contributor.authorKotov, Ivan
dc.contributor.authorO, Paul
dc.contributor.authorSebag, Jacques
dc.contributor.authorStubbs, Christopher William
dc.contributor.authorWarner, Michael
dc.date.accessioned2015-07-20T15:09:31Z
dc.date.issued2014
dc.identifier.citationRiot, 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.en_US
dc.identifier.isbn9780819496157en_US
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:17491780
dc.description.abstractThe 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.en_US
dc.description.sponsorshipAstronomyen_US
dc.language.isoen_USen_US
dc.publisherSociety of Photo-Optical Instrumentation Engineers (SPIE)en_US
dc.relation.isversionofdoi:10.1117/12.2056605en_US
dash.licenseOAP
dc.subjectLarge Synoptic Survey Telescopeen_US
dc.subjectguide sensorsen_US
dc.subjectWavefront sensorsen_US
dc.subjectground-based telescopeen_US
dc.titleThe guider and wavefront curvature sensor subsystem for the Large Synoptic Survey Telescopeen_US
dc.typeConference Paperen_US
dc.description.versionAccepted Manuscripten_US
dash.depositing.authorStubbs, Christopher William
dc.date.available2015-07-20T15:09:31Z
dc.relation.bookGround-based and Airborne Instrumentation for Astronomy V: Proceedings of Society of Photo-Optical Instrumentation Engineers (SPIE) 9147en_US
dash.funder.nameNSF Scientific Program Order No. 9en_US
dash.funder.nameNSF Scientific Program Order No. 1en_US
dash.funder.nameU.S. Department of Energyen_US
dash.funder.nameU.S. Department of Energyen_US
dash.funder.nameU.S. Department of Energy Office of High Energy Physicsen_US
dash.funder.awardAST-0551161en_US
dash.funder.awardAST-0244680en_US
dash.funder.awardDE-AC02-76SF00515en_US
dash.funder.awardDEAC52-07NA27344en_US
dash.funder.awardDE-FG02-91ER40681A29en_US
dc.identifier.doi10.1117/12.2056605*
dash.authorsorderedfalse
dash.contributor.affiliatedStubbs, Christopher


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