InFOCμS hard X-ray imaging telescope

J. Tueller, H. A. Krimm, T. Okajima, S. D. Barthelmy, S. M. Owens, P. J. Serlemitsos, Y. Soong, K. W. Chan, Y. Ogasaka, R. Shibata, K. Tamura, A. Furuzawa, Y. Tawara, H. Kunieda, K. Yamashita

研究成果: Chapter

抄録

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.

元の言語English
ホスト出版物のタイトルFocusing Telescopes in Nuclear Astrophysics
出版者Springer Netherlands
ページ121-129
ページ数9
ISBN(印刷物)1402053037, 9781402053030
DOI
出版物ステータスPublished - 01-12-2006
外部発表Yes

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telescopes
pixels
detectors
x rays
mirrors
balloons
angular resolution
field of view
standard deviation
platinum
flight
optics
energy
carbon
photons
spectroscopy

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

これを引用

Tueller, J., Krimm, H. A., Okajima, T., Barthelmy, S. D., Owens, S. M., Serlemitsos, P. J., ... Yamashita, K. (2006). InFOCμS hard X-ray imaging telescope. : Focusing Telescopes in Nuclear Astrophysics (pp. 121-129). Springer Netherlands. https://doi.org/10.1007/978-1-4020-5304-7_14
Tueller, J. ; Krimm, H. A. ; Okajima, T. ; Barthelmy, S. D. ; Owens, S. M. ; Serlemitsos, P. J. ; Soong, Y. ; Chan, K. W. ; Ogasaka, Y. ; Shibata, R. ; Tamura, K. ; Furuzawa, A. ; Tawara, Y. ; Kunieda, H. ; Yamashita, K. / InFOCμS hard X-ray imaging telescope. Focusing Telescopes in Nuclear Astrophysics. Springer Netherlands, 2006. pp. 121-129
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Tueller, J, Krimm, HA, Okajima, T, Barthelmy, SD, Owens, SM, Serlemitsos, PJ, Soong, Y, Chan, KW, Ogasaka, Y, Shibata, R, Tamura, K, Furuzawa, A, Tawara, Y, Kunieda, H & Yamashita, K 2006, InFOCμS hard X-ray imaging telescope. : Focusing Telescopes in Nuclear Astrophysics. Springer Netherlands, pp. 121-129. https://doi.org/10.1007/978-1-4020-5304-7_14

InFOCμS hard X-ray imaging telescope. / Tueller, J.; Krimm, H. A.; Okajima, T.; Barthelmy, S. D.; Owens, S. M.; Serlemitsos, P. J.; Soong, Y.; Chan, K. W.; Ogasaka, Y.; Shibata, R.; Tamura, K.; Furuzawa, A.; Tawara, Y.; Kunieda, H.; Yamashita, K.

Focusing Telescopes in Nuclear Astrophysics. Springer Netherlands, 2006. p. 121-129.

研究成果: Chapter

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 - 2006/12/1

Y1 - 2006/12/1

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 -

Tueller J, Krimm HA, Okajima T, Barthelmy SD, Owens SM, Serlemitsos PJ その他. InFOCμS hard X-ray imaging telescope. : Focusing Telescopes in Nuclear Astrophysics. Springer Netherlands. 2006. p. 121-129 https://doi.org/10.1007/978-1-4020-5304-7_14