• 首頁> 外文會議>UV and Gamma-Ray Space Telescope Systems pt.1 >Upgraded Hard X-ray Telescope with Multilayer Supermirror for the InFOCμS balloon Experiment
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    Upgraded Hard X-ray Telescope with Multilayer Supermirror for the InFOCμS balloon Experiment

    機譯:用于InFOCμS氣球實驗的具有多層超鏡的升級版硬X射線望遠鏡

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    Hard X-ray focusing observation is important to reveal non-thermal emission mechanism and origin in active galaxies and clusters of galaxies. We have carried out the hard X-ray observation throughout the InFOCμS program, which is an international balloon-borne experiment in collaboration with NASA/GSFC and Nagoya University. The telescope is conical approximation of Wolter-Ⅰ optics with 8 m focal length and 40 cm diameter. It consists of 255 nested thin (0.17 mm thickness) reflectors with incidence angles of 0.10° to 0.36°. Reflectors are coated with depth-graded platinum-carbon (Pt/C) multilayers, so-called supermirrors, with periodic length of 2.6 to 13 nm and bi-layer number of 28 to 79, depending on incidence angles. We are now continuously fabricating advanced next hard X-ray telescope for the second InFOCμS flight in 2004. Compared with the first telescope, the following improvements have been made on the second one. Supermirror reflectors have wider sensitivity in energy band of 20 — 60 keV adopting optimum supermirror design for balloon observation, and smaller interfacial roughness owing to complete replication technique. For upgrading of the image quality, we then adopted stiffer reflector substrate, selected replication mandrel with better shape, and the modified telescope housing with higher alignment accuracy for reflectors. The performance of the new hard X-ray telescope was measured in X-ray beamline facility in ISAS/JAXA and synchrotron radiation facility SPring-8. The effective area and image quality are obtained to be 45 cm~2 at 30 keV and 23 cm~2 at 40 keV, and 2.5 arcmin in half power diameter, respectively. In this paper we report our development of the upgraded hard X-ray telescope for the second balloon flight experiment.
    機譯:硬X射線聚焦觀察對于揭示活躍星系和星系團中的非熱輻射機理和起源很重要。我們在整個InFOCμS計劃中進行了硬X射線觀察,這是與NASA / GSFC和名古屋大學合作開展的一項國際氣球載實驗。望遠鏡是焦距為8 m,直徑為40 cm的Wolter-Ⅰ光學系統的圓錐近似。它由255個嵌套的薄反射器(厚度為0.17 mm)組成,入射角為0.10°至0.36°。反射器涂有深度漸變的鉑碳(Pt / C)多層膜,即所謂的超級鏡,其周期長度為2.6至13 nm,雙層數為28至79,具體取決于入射角?,F在,我們正在為2004年的第二次InFOCμS飛行連續制造先進的下一代硬X射線望遠鏡。與第一架望遠鏡相比,第二架進行了以下改進。超級反射鏡反射器在20-60 keV的能帶中具有更寬的靈敏度,采用最佳的超級反射鏡設計進行氣球觀察,由于采用了完整的復制技術,因此界面粗糙度較小。為了提高圖像質量,我們隨后采用了更硬的反射鏡基板,選定的具有更好形狀的復制芯軸以及改進的望遠鏡殼體,以提高反射鏡的對準精度。新型硬X射線望遠鏡的性能在ISAS / JAXA的X射線束線設施和同步加速器輻射設施SPring-8中進行了測量。有效面積和圖像質量在30 keV時為45 cm?2,在40 keV時為23 cm?2,半功率直徑分別為2.5 arcmin。在本文中,我們報告了用于第二次氣球飛行實驗的升級版硬X射線望遠鏡的開發情況。

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