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dc.contributor.authorGendreau, Keith C.
dc.contributor.authorArzoumanian, Zaven
dc.contributor.authorMarkwardt, Craig B.
dc.contributor.authorBaumgartner, Wayne H.
dc.contributor.authorPrigozhin, Gregory
dc.contributor.authorRemillard, Ronald A
dc.contributor.authorMalonis, Andrew C.
dc.contributor.authorLa Marr, Beverly J.
dc.date.accessioned2018-04-30T13:36:39Z
dc.date.available2018-04-30T13:36:39Z
dc.date.issued2016-07
dc.date.submitted2016-06
dc.identifier.issn0277-786X
dc.identifier.issn1996-756X
dc.identifier.urihttp://hdl.handle.net/1721.1/115079
dc.description.abstractThe Neutron star Interior Composition ExploreR (NICER) is set to be deployed on the International Space Station (ISS) in early 2017. It will use an array of 56 Silicon Drift Detectors (SDDs) to detect soft X-rays (0.2 - 12 keV) with 100 nanosecond timing resolution. Here we describe the effort to calibrate the detectors in the lab primarily using a Modulated X-ray Source (MXS). The MXS that was customized for NICER provides more than a dozen emission lines spread over the instrument bandwidth, providing calibration measurements for detector gain and spectral resolution. In addition, the fluorescence source in the MXS was pulsed at high frequency to enable measurement of the delay due to charge collection in the silicon and signal processing in the detector electronics. A second chamber, designed to illuminate detectors with either 55 Fe, an optical LED, or neither, provided additional calibration of detector response, optical blocking, and effectiveness of background rejection techniques. The overall ground calibration achieved total operating time that was generally in the range of 500-1500 hours for each of the 56 detectors. Keywords: Silicon Drift Detectors; X-rays; timing spectroscopy; calibrationen_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Contract NNG14PJ13C)en_US
dc.publisherSPIEen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.2232784en_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.titleGround calibration of the Silicon Drift Detectors for NICERen_US
dc.typeArticleen_US
dc.identifier.citationLaMarr, B. et al. “Ground Calibration of the Silicon Drift Detectors for NICER.” Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, June - July 2016, Edinburgh, United Kingdom, SPIE, July 2016 © 2016 SPIEen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorLa Marr, Beverly J
dc.contributor.mitauthorPrigozhin, Gregory
dc.contributor.mitauthorRemillard, Ronald A
dc.contributor.mitauthorMalonis, Andrew C.
dc.relation.journalSpace 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.updated2018-03-16T15:34:49Z
dspace.orderedauthorsLaMarr, B.; Prigozhin, G.; Remillard, R.; Malonis, A.; Gendreau, K. C.; Arzoumanian, Z.; Markwardt, C. B.; Baumgartner, W. H.en_US
dspace.embargo.termsNen_US
mit.licensePUBLISHER_POLICYen_US


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