Abstract
Mass production of replicated thin aluminum x-ray reflecting foils for the InFOCμS (International Focusing Optics Collaboration for Micro-Crab Sensitivity) balloon payload is complete, and the full mirror has been assembled. InFOCμS is an 8-meter focal length hard x-ray telescope scheduled for first launch in July 2001 and will be the first instrument to focus and image x-rays at high energies (20-40 keV) using multilayer-based reflectors. The individual reflecting elements are replicated thin aluminum foils, in a conical approximation Wolter-I system similar to those built for ASCA and ASTRO-E. These previous imaging systems achieved half-power-diameters of 3.5 and 1.7-2.1 arcminutes respectively. The InFOCμS mirror is expected to have angular resolution similar to the ASTRO-E mirror. The reflecting foils for InFOCμS, however, utilize a vertically graded Pt/C multilayer to provide broad-band high-energy focusing. We present the results of our pre-flight characterization of the full mirror, including imaging and sensitivity evaluations. If possible, we will include imaging results from the first flight of a multilayer-based high-energy focusing telescope.
| Original language | English |
|---|---|
| Pages (from-to) | 115-126 |
| Number of pages | 12 |
| Journal | Proceedings of SPIE - The International Society for Optical Engineering |
| Volume | 4496 |
| DOIs | |
| Publication status | Published - 01-01-2002 |
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All Science Journal Classification (ASJC) codes
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering
Cite this
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Characterization and performance of the InFOCμS 20-40 keV x-ray focusing mirror. / Owens, S. M.; Berendse, F.; Okajima, T.; Misaki, K.; Ogasaka, Y.; Tamura, K.; Tawara, Y.; Kunieda, H.; Chan, K. W.; Soong, Y.; Baumgartner, W. H.; Krimm, H.; Tueller, J.; Serlemitsos, P. J.; Yamashita, K.; Haga, K.; Ichimaru, S.; Takahashi, S.; Gotou, A.; Kitou, H.; Fukuda, S.; Kamata, Y.; Furuzawa, A.; Akimoto, F.; Yoshioka, T.; Kondou, K.; Haba, Y.; Tanaka, T.
In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 4496, 01.01.2002, p. 115-126.Research output: Contribution to journal › Article
TY - JOUR
T1 - Characterization and performance of the InFOCμS 20-40 keV x-ray focusing mirror
AU - Owens, S. M.
AU - Berendse, F.
AU - Okajima, T.
AU - Misaki, K.
AU - Ogasaka, Y.
AU - Tamura, K.
AU - Tawara, Y.
AU - Kunieda, H.
AU - Chan, K. W.
AU - Soong, Y.
AU - Baumgartner, W. H.
AU - Krimm, H.
AU - Tueller, J.
AU - Serlemitsos, P. J.
AU - Yamashita, K.
AU - Haga, K.
AU - Ichimaru, S.
AU - Takahashi, S.
AU - Gotou, A.
AU - Kitou, H.
AU - Fukuda, S.
AU - Kamata, Y.
AU - Furuzawa, A.
AU - Akimoto, F.
AU - Yoshioka, T.
AU - Kondou, K.
AU - Haba, Y.
AU - Tanaka, T.
PY - 2002/1/1
Y1 - 2002/1/1
N2 - Mass production of replicated thin aluminum x-ray reflecting foils for the InFOCμS (International Focusing Optics Collaboration for Micro-Crab Sensitivity) balloon payload is complete, and the full mirror has been assembled. InFOCμS is an 8-meter focal length hard x-ray telescope scheduled for first launch in July 2001 and will be the first instrument to focus and image x-rays at high energies (20-40 keV) using multilayer-based reflectors. The individual reflecting elements are replicated thin aluminum foils, in a conical approximation Wolter-I system similar to those built for ASCA and ASTRO-E. These previous imaging systems achieved half-power-diameters of 3.5 and 1.7-2.1 arcminutes respectively. The InFOCμS mirror is expected to have angular resolution similar to the ASTRO-E mirror. The reflecting foils for InFOCμS, however, utilize a vertically graded Pt/C multilayer to provide broad-band high-energy focusing. We present the results of our pre-flight characterization of the full mirror, including imaging and sensitivity evaluations. If possible, we will include imaging results from the first flight of a multilayer-based high-energy focusing telescope.
AB - Mass production of replicated thin aluminum x-ray reflecting foils for the InFOCμS (International Focusing Optics Collaboration for Micro-Crab Sensitivity) balloon payload is complete, and the full mirror has been assembled. InFOCμS is an 8-meter focal length hard x-ray telescope scheduled for first launch in July 2001 and will be the first instrument to focus and image x-rays at high energies (20-40 keV) using multilayer-based reflectors. The individual reflecting elements are replicated thin aluminum foils, in a conical approximation Wolter-I system similar to those built for ASCA and ASTRO-E. These previous imaging systems achieved half-power-diameters of 3.5 and 1.7-2.1 arcminutes respectively. The InFOCμS mirror is expected to have angular resolution similar to the ASTRO-E mirror. The reflecting foils for InFOCμS, however, utilize a vertically graded Pt/C multilayer to provide broad-band high-energy focusing. We present the results of our pre-flight characterization of the full mirror, including imaging and sensitivity evaluations. If possible, we will include imaging results from the first flight of a multilayer-based high-energy focusing telescope.
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U2 - 10.1117/12.454364
DO - 10.1117/12.454364
M3 - Article
AN - SCOPUS:0038368128
VL - 4496
SP - 115
EP - 126
JO - Proceedings of SPIE - The International Society for Optical Engineering
JF - Proceedings of SPIE - The International Society for Optical Engineering
SN - 0277-786X
ER -