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- W2021017411 abstract "Recent development of cryogenic detectors enabled high resolutiondiagnostics of emission line and absorption line/edgestructures. These studies are quite important to investigate physicsof interstellar/intergalactic plasma and dynamics of matters aroundblack holes, for example.Soft X-ray telescopes for such purpose, sensitive up to 10 keV, areusually designed using Au, Pt, or Ir for their large electron densityand large critical angle. However in fact, these materials are notvery suitable in a few to 8 keV region, because they have wide anddeep M-shell absorption edge structures in 2--4 keV region.Considering absorption edges and also thin-film characteristics, C orNi can be alternatives. However, these materials alone cannot be agood mirror, again from absorption edges in the energy region ofinterest (0.1-10 keV). We designed composite structure consisting ofC, Ni and Pt with thickness of 30 to 300 A, to get smooth and highreflectivity all across the energy region. Test fabrication showedinterfacial roughness is as low as expected, indicating match ofmaterials is also good.We applied this result to the baseline design of NeXT/Soft X-rayTelescope, by substituting current material (Au) with C-Ni-Ptcomposite, and obtained 20% larger effective area in 2-8 keV region." @default.
- W2021017411 created "2016-06-24" @default.
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- W2021017411 date "2004-10-11" @default.
- W2021017411 modified "2023-09-23" @default.
- W2021017411 title "Application of composite-layer mirror to soft x-ray telescopes" @default.
- W2021017411 doi "https://doi.org/10.1117/12.552461" @default.
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