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dc.contributor.authorMarshall, Herman L
dc.contributor.authorHeine, Sarah
dc.contributor.authorGarner, Alan
dc.contributor.authorGullikson, Eric
dc.contributor.authorGuenther, Moritz
dc.contributor.authorLeitz, Christopher
dc.contributor.authorMasterson, Rebecca
dc.contributor.authorMiller, Eric
dc.contributor.authorZhang, William
dc.contributor.authorBoissay Malaquin, Rozenn
dc.contributor.authorCaiazzo, Ilaria
dc.contributor.authorChakrabarty, Deepto
dc.contributor.authorDavidson, Rosemary
dc.contributor.authorGallo, Luigi
dc.contributor.authorHeilmann, Ralf K
dc.contributor.authorHeyl, Jeremy
dc.contributor.authorKara, Erin
dc.contributor.authorMarscher, Alan
dc.contributor.authorSchulz, Norbert
dc.date.accessioned2022-03-31T13:34:15Z
dc.date.available2022-03-31T13:34:15Z
dc.date.issued2020
dc.identifier.urihttps://hdl.handle.net/1721.1/141433
dc.description.abstract© 2020 SPIE We describe a new implementation of a broad-band soft X-ray polarimeter, substantially based on a previous design. This implementation, the Pioneer Soft X-ray Polarimeter (PiSoX) is a SmallSat, designed for NASA's call for Astrophysics Pioneers, small missions that could be CubeSats, balloon experiments, or SmallSats. As in REDSoX, the grating arrangement is designed optimally for the purpose of polarimetry with broad-band focussing optics by matching the dispersion of the spectrometer channels to laterally graded multilayers (LGMLs). The system can achieve polarization modulation factors over 90%. For PiSoX, the optics are lightweight Si mirrors in a one-bounce parabolic configuration. High efficiency, blazed gratings from opposite sectors are oriented to disperse to a LGML forming a channel covering the wavelength range from 35 Å to 75 Å (165 - 350 eV). Upon satellite rotation, the intensities of the dispersed spectra, after reflection and polarizing by the LGMLs, give the three Stokes parameters needed to determine a source's linear polarization fraction and orientation. The design can be extended to higher energies as LGMLs are developed further. We describe examples of the potential scientific return from instruments based on this design.en_US
dc.language.isoen
dc.publisherSPIE-Intl Soc Optical Engen_US
dc.relation.isversionof10.1117/12.2562811en_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.titleA small satellite version of a soft x-ray polarimeteren_US
dc.typeArticleen_US
dc.identifier.citationMarshall, Herman L, Heine, Sarah, Garner, Alan, Gullikson, Eric, Guenther, Moritz et al. 2020. "A small satellite version of a soft x-ray polarimeter." Proceedings of SPIE - The International Society for Optical Engineering, 11444.
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Research
dc.relation.journalProceedings of SPIE - The International Society for Optical Engineeringen_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.updated2022-03-31T13:14:03Z
dspace.orderedauthorsMarshall, HL; Heine, S; Garner, A; Gullikson, E; Guenther, M; Leitz, C; Masterson, R; Miller, E; Zhang, W; Boissay Malaquin, R; Caiazzo, I; Chakrabarty, D; Davidson, R; Gallo, L; Heilmann, RK; Heyl, J; Kara, E; Marscher, A; Schulz, Nen_US
dspace.date.submission2022-03-31T13:14:06Z
mit.journal.volume11444en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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