Show simple item record

dc.contributor.authorPrigozhin, Gregory
dc.contributor.authorGendreau, Keith
dc.contributor.authorDoty, John P.
dc.contributor.authorArzoumanian, Zaven
dc.contributor.authorBaumgartner, Wayne
dc.contributor.authorScholze, Frank
dc.contributor.authorLaubis, Christian
dc.contributor.authorKrumrey, Michael
dc.contributor.authorHuber, Alan
dc.contributor.authorRemillard, Ronald A
dc.contributor.authorMalonis, Andrew C.
dc.contributor.authorVezie, Michael L.
dc.contributor.authorEgan, Mark
dc.contributor.authorVillasenor, Jesus Noel Samonte
dc.contributor.authorFoster, Richard F.
dc.contributor.authorLa Marr, Beverly J.
dc.date.accessioned2018-07-20T14:27:15Z
dc.date.available2018-07-20T14:27:15Z
dc.date.issued2016-07
dc.identifier.urihttp://hdl.handle.net/1721.1/117024
dc.description.abstractAn instrument called Neutron Star Interior Composition ExploreR (NICER) will be placed on-board the International Space Station in 2017. It is designed to detect soft X-ray emission from compact sources and to provide both spectral and high resolution timing information about the incoming ux. The focal plane is populated with 56 customized Silicon Drift Detectors. The paper describes the detector system architecture, the electronics and presents the results of the laboratory testing of both ight and engineering units, as well as some of the calibration results obtained with synchrotron radiation in the laboratory of PTB at BESSY II.en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Contract NNG14PJ13C)en_US
dc.publisherSPIEen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.2231718en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceSPIEen_US
dc.titleNICER instrument detector subsystem: description and performanceen_US
dc.typeArticleen_US
dc.identifier.citationPrigozhin, Gregory, et al. "NICER Instrument Detector Subsystem: Description and Performance." Proceedings Volume 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 26 June - 1 July, 2016, Edinburgh, United Kingdom, edited by Jan-Willem A. den Herder et al., SPIE, 2016, p. 99051I. © 2016 SPIE.en_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorFoster, Richard F
dc.contributor.mitauthorRemillard, Ronald A
dc.contributor.mitauthorMalonis, Andrew C.
dc.contributor.mitauthorLa Marr, Beverly J
dc.contributor.mitauthorVezie, Michael L.
dc.contributor.mitauthorEgan, Mark
dc.contributor.mitauthorVillasenor, Jesus Noel Samonte
dc.relation.journalProceedings Volume 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Rayen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2018-03-16T16:08:30Z
dspace.orderedauthorsPrigozhin, Gregory; Gendreau, Keith; Doty, John P.; Foster, Richard; Remillard, Ronald; Malonis, Andrew; LaMarr, Beverly; Vezie, Michael; Egan, Mark; Villasenor, Jesus; Arzoumanian, Zaven; Baumgartner, Wayne; Scholze, Frank; Laubis, Christian; Krumrey, Michael; Huber, Alanen_US
dspace.embargo.termsNen_US
mit.licensePUBLISHER_POLICYen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record