Translator Disclaimer
27 September 2012 Measurement of reflectivity of x-ray mirror for soft x-ray telescope onboard ASTRO-H
Author Affiliations +
X-ray reflection mirror of the Soft X-ray Telescope onboard ASTRO-H was coated by gold thin layer. Gold have M-shell X-ray absorption edge around 2 keV which is included in the energy band covered with the focal plane detector such as Soft X-ray Imager and Soft X-ray Spectrometer. It is important to make response function taken int account the Au M-dege structure especially for the Soft X-ray Spectrometer because It has unprecedented high energy resolution of 5 eV from 0.3 to 12 keV. We performed the detailed measurements of of reflectivity of the mirror using reflectometer in the synchrotron radiation facility KEK PF BL-11B from Nov. 29, 2011 to Dec. 5. X-ray beam of BL–11B was monochromatized to E/deltaE of 5000 by Double crystal monochromator using Si(111). We obtained the reflectivity at the grazing incident angles of 1.0, 1.2, and 1.4 degrees. While the energy pitch was set to be 2 eV in the 2.1–4.1 keV band, the reflectivity in the 2.2–2.35 keV band was also measured in detail with the energy pitch of 0.25 eV. We report the results and optical parameters of the SXT mirror such as reflectivity, and roughness calculated from the measurements.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Satoshi Sugita, Akihiro Furuzawa, Kazunori Ishibashi, Keisuke Tamura, Takashi Okajima, Yoshitomo Maeda, Takuro Sato, Kou Ichihara, Kazuki Tomikawa, Ryo Iizuka, Takashi Awaya, and Kohta Okada "Measurement of reflectivity of x-ray mirror for soft x-ray telescope onboard ASTRO-H", Proc. SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, 844358 (27 September 2012);


Back to Top