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dc.contributor.authorRamsey, Brian .
dc.contributor.authorGuenther, Hans Moritz
dc.contributor.authorWindt, David L.
dc.contributor.authorGullikson, Eric M.
dc.contributor.authorPareschi, Giovanni
dc.contributor.authorTagliaferri, Gianpiero
dc.contributor.authorJorstad, Svetlana
dc.contributor.authorMarscher, Alan
dc.contributor.authorWeisskopf, Martin
dc.contributor.authorMarshall, Herman
dc.contributor.authorSchulz, Norbert S
dc.contributor.authorHeilmann, Ralf K
dc.contributor.authorHeine, Sarah N.T.
dc.contributor.authorGuenther, Hans Moritz
dc.contributor.authorEgan, Mark
dc.contributor.authorHellickson, Timothy H
dc.contributor.authorSchattenburg, Mark L
dc.contributor.authorChakrabarty, Deepto
dc.date.accessioned2018-05-02T13:48:38Z
dc.date.available2018-05-02T13:48:38Z
dc.date.issued2017-08
dc.identifier.isbn9781510612518
dc.identifier.isbn9781510612525
dc.identifier.urihttp://hdl.handle.net/1721.1/115151
dc.description.abstractThe Rocket Experiment Demonstration of a Soft X-ray Polarimeter (REDSoX Polarimeter) is a sounding rocket instrument that can make the first measurement of the linear X-ray p olarization of an extragalactic source in the 0.2-0.8 keV band as low as 10%. We employ multilayer-coated mirrors as Bragg reflectors at the Brewster angle. By matching the dispersion of a spectrometer using replicated optics from MSFC and critical angle transmission gratings from MIT to three laterally graded multilayer mirrors (LGMLs), we achieve polarization modulation factors over 90%. We present a novel arrangement of gratings, designed optimally for the purpose of polarimetry with a converging beam. The entrance aperture is divided into six equal sectors; pairs of blazed gratings from opposite sectors are oriented to disperse to the same LGML. The LGML position angles are 120 degrees to each other. CCD detectors then measure the intensities of the dispersed spectra after reflection and polarizing by the LGMLs, giving the three Stokes parameters needed to determine a source's linear polarization fraction and orientation. A current grant is funding further development to improve the LGMLs. Sample gratings for the project have been fabricated at MIT and the development team continues to improve them under separate funding. Our technological approach is the basis for a possible orbital mission. Keywords: X-ray, polarimeter, astronomy, multilayer, mirror, gratingen_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Grant NNX17AE11G)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Grant NNX12AH12G)en_US
dc.description.sponsorshipKavli Institute for Astrophysics and Space Research (Research Investment Grant)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Grant NNX17AG43G)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Grant NNX15AC43G)en_US
dc.publisherSPIEen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.2274107en_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.titleThe rocket experiment demonstration of a soft x-ray polarimeter (REDSoX Polarimeter)en_US
dc.typeArticleen_US
dc.identifier.citationMarshall, Herman, et al. "The Rocket Experiment Demonstration of a Soft X-Ray Polarimeter (REDSoX Polarimeter)." 6-10 August, 2017, San Diego, California, edited by Oswald H. Siegmund, SPIE, 2017, p. 21. © COPYRIGHT SPIEen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorMarshall, Herman
dc.contributor.mitauthorSchulz, Norbert S
dc.contributor.mitauthorHeilmann, Ralf K
dc.contributor.mitauthorHeine, Sarah N.T.
dc.contributor.mitauthorGuenther, Hans Moritz
dc.contributor.mitauthorEgan, Mark
dc.contributor.mitauthorHellickson, Timothy H
dc.contributor.mitauthorSchattenburg, Mark L
dc.contributor.mitauthorChakrabarty, Deepto
dc.relation.journalProceedings Volume 10397, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2018-04-24T16:42:15Z
dspace.orderedauthorsMarshall, Herman .; Schulz, Norbert .; Heilmann, Ralf K.; Ramsey, Brian .; Heine, Sarah; Egan, Mark D.; Hellickson, Timothy; Guenther, Moritz; Windt, David L.; Gullikson, Eric M.; Pareschi, Giovanni; Tagliaferri, Gianpiero; Jorstad, Svetlana; Marscher, Alan; Weisskopf, Martin; Chakrabarty, Deepto; Schattenburg, Marken_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-6492-1293
dc.identifier.orcidhttps://orcid.org/0000-0001-9980-5295
dc.identifier.orcidhttps://orcid.org/0000-0003-4081-6322
dc.identifier.orcidhttps://orcid.org/0000-0003-4243-2840
dc.identifier.orcidhttps://orcid.org/0000-0001-6932-2612
dc.identifier.orcidhttps://orcid.org/0000-0001-8804-8946
dspace.mitauthor.errortrue
mit.licensePUBLISHER_POLICYen_US


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