Current Status Of The X-Ray Mirror For The Xl-Calibur Experiment

K. Hattori,H. Matsumoto,Q. Abarr, H. Awaki,M. G. Baring,R. Bose, D. Braun,G. De Geronimoe, P. Dowkontt, J. Elliot,T. Enoto,M. Errando, Y. Fukazawa, A. Furuzawa, T. Gadson, E. Gau, V Guarino,S. Gunji, K. Hall, K. Harmon, K. Hayashida, S. Heatwole, A. Hossen, F. Imazato,K. Ishibashi,M. Ishida,N. K. Iyer,F. Kislat, M. Kiss, T. Kitaguchiu, D. Kotsifakis,H. Krawczynski, J. Lanzi,L. Lisalda,Y. Maeda, H. Matake,T. Mineta,T. Miyazawa,T. Mizuno, N. Nakaniwa, T. Okajima, I Pastrani,M. Pearce, Z. Peterson, C. Purdy,B. Rauch, F. Ryde, Y. Saito, C. Shreeves, G. Simburger, C. Snow,S. Spooner, T. A. Stana, D. Stuchlik, H. Takahashi, T. Takeda,M. Takeo, T. Tamagawa,K. Tamura, H. Tsunemi,N. Uchida,Y. Uchida, K. Uchiyama, B. Vincent,A. T. West, E. A. Wulf, R. Yamamoto, Y. Yoshida

SPACE TELESCOPES AND INSTRUMENTATION 2020: ULTRAVIOLET TO GAMMA RAY(2021)

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摘要
XL-Calibur is a balloon-borne hard X-ray polarimetry mission, the first flight of which is currently foreseen for 2022. XL-Calibur carries an X-ray telescope consists of 213 Wolter I grazing-incidence mirrors which are nested in a coaxial and cofocal configuration. The optics design is nearly identical to the Hard X-ray Telescope (HXT) on board the ASTRO-H satellite. The telescope was originally fabricated for the Formation Flying Astronomical Survey Telescope (FFAST) project. However, the telescope can be used for XL-Calibur, since the FFAST project was terminated before completion. The mirror surfaces are coated with Pt/C depth-graded multilayers to reflect hard X-rays above 10 keV by Bragg reflection. The effective area of the telescope is larger than 300 cm(2) at 20 keV. This paper reports the current status of the telescope for XL-Calibur.
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关键词
XL-Calibur, polarimetry, X-ray telescope
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