TY - GEN
T1 - Development and performance of the advanced hard x-ray telescope for the balloon experiment
AU - Miyazawa, Takuya
AU - Shibata, Ryo
AU - Ogasaka, Yasushi
AU - Fukaya, Yoshihiro
AU - Naitou, Masataka
AU - Iwahara, Tomonaga
AU - Shimoda, Kenta
AU - Tamura, Keisuke
AU - Furuzawa, Akihiro
AU - Kunieda, Hideyo
AU - Yamashita, Koujun
AU - Yokoi, Shin
AU - Yoshii, Takuma
AU - Watanabe, Naoya
AU - Namba, Yoshiharu
PY - 2006
Y1 - 2006
N2 - Imaging observation in the hard X-ray band of 10 - 100 keV is one of the important subjects in X-ray astronomy. Though SUMIT balloon-borne experiment, we have developed thin-foil-nested hard X-ray telescope employing depth-graded Pt/C multilayer (multilayer-supermirror). We have improved production process of the replica reflector and telescope optics compared with InFOCμS-2004 telescope. The new telescope was measured at synchrotron radiation facility, SPring-8. The image quality and throughtput were estimated to be 2.06 arcmin (half power diameter) and 85 % at 30 keV, respectively. These values were about 24 % and 30 % improvement compared to InFOC/μS-2004, respectively. Limiting factors of its performance are also investigated. Based on such an investigation we are now continuously developing hard X-ray telescope for SUMIT 2006 flight.
AB - Imaging observation in the hard X-ray band of 10 - 100 keV is one of the important subjects in X-ray astronomy. Though SUMIT balloon-borne experiment, we have developed thin-foil-nested hard X-ray telescope employing depth-graded Pt/C multilayer (multilayer-supermirror). We have improved production process of the replica reflector and telescope optics compared with InFOCμS-2004 telescope. The new telescope was measured at synchrotron radiation facility, SPring-8. The image quality and throughtput were estimated to be 2.06 arcmin (half power diameter) and 85 % at 30 keV, respectively. These values were about 24 % and 30 % improvement compared to InFOC/μS-2004, respectively. Limiting factors of its performance are also investigated. Based on such an investigation we are now continuously developing hard X-ray telescope for SUMIT 2006 flight.
UR - https://www.scopus.com/pages/publications/33749028993
UR - https://www.scopus.com/pages/publications/33749028993#tab=citedBy
U2 - 10.1117/12.671346
DO - 10.1117/12.671346
M3 - Conference contribution
AN - SCOPUS:33749028993
SN - 0819463310
SN - 9780819463319
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation II
T2 - Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray
Y2 - 24 May 2006 through 31 May 2006
ER -