TY - CHAP
T1 - InFOCμS hard X-ray imaging telescope
AU - Tueller, J.
AU - Krimm, H. A.
AU - Okajima, T.
AU - Barthelmy, S. D.
AU - Owens, S. M.
AU - Serlemitsos, P. J.
AU - Soong, Y.
AU - Chan, K. W.
AU - Ogasaka, Y.
AU - Shibata, R.
AU - Tamura, K.
AU - Furuzawa, A.
AU - Tawara, Y.
AU - Kunieda, H.
AU - Yamashita, K.
PY - 2006
Y1 - 2006
N2 - InFOCμS is a new generation balloon-borne hard X-ray telescope with focusing optics and spectroscopy. We had a successful 22.5-hour flight from Fort Sumner, NM on September 16,17, 2004. In this paper, we present the performance of the hard X-ray telescope, which consists of a depth-graded platinum/carbon multilayer mirror and a CdZnTe detector. The telescope has an effective area of 49 cm2 at 30 keV, an angular resolution of 2.4 arcmin (HPD), and a field of view of 11 arcmin (FWHM) depending on energies. The CdZnTe detector is configured with a 12 × 12 segmented array of detector pixels. The pixels are 2mmsquare, and are placed on 2.1mm centers. An averaged energy resolution is 4.4 keV at 60 keV and its standard deviation is 0.36 keV over 128 pixels. The detector is surrounded by a 3-cm thick CsI anti coincidence shield to reduce background from particles and photons not incident along the mirror focal direction. The inflight background is 2.9 × 10-4 cts cm -2 sec-1 keV-1 in the 20-50 keV band.
AB - InFOCμS is a new generation balloon-borne hard X-ray telescope with focusing optics and spectroscopy. We had a successful 22.5-hour flight from Fort Sumner, NM on September 16,17, 2004. In this paper, we present the performance of the hard X-ray telescope, which consists of a depth-graded platinum/carbon multilayer mirror and a CdZnTe detector. The telescope has an effective area of 49 cm2 at 30 keV, an angular resolution of 2.4 arcmin (HPD), and a field of view of 11 arcmin (FWHM) depending on energies. The CdZnTe detector is configured with a 12 × 12 segmented array of detector pixels. The pixels are 2mmsquare, and are placed on 2.1mm centers. An averaged energy resolution is 4.4 keV at 60 keV and its standard deviation is 0.36 keV over 128 pixels. The detector is surrounded by a 3-cm thick CsI anti coincidence shield to reduce background from particles and photons not incident along the mirror focal direction. The inflight background is 2.9 × 10-4 cts cm -2 sec-1 keV-1 in the 20-50 keV band.
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U2 - 10.1007/978-1-4020-5304-7_14
DO - 10.1007/978-1-4020-5304-7_14
M3 - Chapter
AN - SCOPUS:84890006724
SN - 1402053037
SN - 9781402053030
SP - 121
EP - 129
BT - Focusing Telescopes in Nuclear Astrophysics
PB - Springer Netherlands
ER -