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Multilayer mirror-based soft x-ray polarimeter for astronomical observations

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dc.contributor.author Panini, S. S
dc.contributor.author Sreekumar, P
dc.contributor.author Marshall, H. L
dc.contributor.author Narendranath, S
dc.contributor.author Nayak, M
dc.contributor.author Athiray, P. S
dc.date.accessioned 2020-11-10T02:30:24Z
dc.date.available 2020-11-10T02:30:24Z
dc.date.issued 2018-01
dc.identifier.citation Journal of Astronomical Telescopes, Instruments, and Systems, Vol. 3, No. 4, pp. 011002-1 - 011002-9 en_US
dc.identifier.issn 2329-4221
dc.identifier.uri http://prints.iiap.res.in/handle/2248/6731
dc.description Restricted Access © SPIE--The International Society for Optical Engineering; https://doi.org/10.1117/1.JATIS.4.1.011002 en_US
dc.description.abstract A simple design of a soft x-ray polarimeter using multilayer mirrors is presented. A multilayer mirror acts as a linear polarization analyzer for x-rays at incidence angles close to the Brewster angle. The instrument consists of an x-ray concentrator, a set of multilayer mirrors placed at 45 deg from the optical axis, and a detector at Nasmyth focus. The instrument rotating about its optical axis during observations can measure the linear polarization of 0.2- to 0.7-keV x-rays from astronomical sources. The use of a soft x-ray concentrator with geometrical area ∼630  cm2 provides sufficient sensitivity to address key scientific questions. Five different multilayer mirrors placed on a rotating wheel provide the option to measure polarization in any of the five narrow bands spanning the 0.2- to 0.7-keV range. Design and estimated performance of the design are discussed. en_US
dc.language.iso en en_US
dc.publisher SPIE-The International Society for Optical Engineering en_US
dc.subject Multilayer mirrors en_US
dc.subject Soft x-rays en_US
dc.subject Polarimeter en_US
dc.title Multilayer mirror-based soft x-ray polarimeter for astronomical observations en_US
dc.type Article en_US


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