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dc.contributor.authorDoherty, Peter Edward
dc.contributor.authorAntilogus, Pierre
dc.contributor.authorAstier, Pierre
dc.contributor.authorChiang, James
dc.contributor.authorGilmore, D. Kirk
dc.contributor.authorGuyonnet, Augustin
dc.contributor.authorHuang, Dajun
dc.contributor.authorKelly, Heather
dc.contributor.authorKotov, Ivan
dc.contributor.authorKubanek, Petr
dc.contributor.authorNomerotski, Andrei
dc.contributor.authorO’Connor, Paul
dc.contributor.authorRasmussen, Andrew
dc.contributor.authorRiot, Vincent J.
dc.contributor.authorStubbs, Christopher William
dc.contributor.authorTakacs, Peter
dc.contributor.authorTyson, J. Anthony
dc.contributor.authorVetter, Kurt
dc.date.accessioned2015-08-26T19:42:58Z
dc.date.issued2014
dc.identifier.citationDoherty, Peter E., et al. 2014. Electro-optical testing of fully depleted CCD image sensors for the Large Synoptic Survey Telescope camera. In the Proceedings of High Energy, Optical, and Infrared Detectors for Astronomy VI (SPIE 9154), June 22, 2014, Montreal, Quebec, Canada: August 12, 2014. doi:10.1117/12.2056733en_US
dc.identifier.issn0277-786Xen_US
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:20562432
dc.description.abstractThe LSST Camera science sensor array will incorporate 189 large format Charge Coupled Device (CCD) image sensors. Each CCD will include over 16 million pixels and will be divided into 16 equally sized segments and each segment will be read through a separate output amplifier. The science goals of the project require CCD sensors with state of the art performance in many aspects. The broad survey wavelength coverage requires fully depleted, 100 micrometer thick, high resistivity, bulk silicon as the imager substrate. Image quality requirements place strict limits on the image degradation that may be caused by sensor effects: optical, electronic, and mechanical. In this paper we discuss the design of the prototype sensors, the hardware and software that has been used to perform electro-optic testing of the sensors, and a selection of the results of the testing to date. The architectural features that lead to internal electrostatic fields, the various effects on charge collection and transport that are caused by them, including charge diffusion and redistribution, effects on delivered PSF, and potential impacts on delivered science data quality are addressed.en_US
dc.description.sponsorshipPhysicsen_US
dc.language.isoen_USen_US
dc.publisherSociety of Photo-optical Instrumentation Engineersen_US
dc.relation.isversionofdoi:10.1117/12.2056733en_US
dash.licenseLAA
dc.titleElectro-optical testing of fully depleted CCD image sensors for the Large Synoptic Survey Telescope cameraen_US
dc.typeConference Paperen_US
dc.description.versionVersion of Recorden_US
dc.relation.journalHigh Energy, Optical, and Infrared Detectors for Astronomy VIen_US
dash.depositing.authorStubbs, Christopher William
dc.date.available2015-08-26T19:42:58Z
dc.identifier.doi10.1117/12.2056733*
dash.authorsorderedfalse
dash.contributor.affiliatedStubbs, Christopher
dash.contributor.affiliatedDoherty, Peter


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