Modeling of proton-induced radioactivation background in hard X-ray telescopes: Geant4-based simulation and its demonstration by Hitomi’s measurement in a low Earth orbit
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Yasushi Fukazawa | Motohide Kokubun | Kazutaka Yamaoka | Olivier Limousin | Teruaki Enoto | Hirofumi Noda | Daniel Maier | Katsuhiro Hayashi | Hirokazu Odaka | Goro Sato | Yasuyuki Tanaka | Hideki Uchiyama | Shin Watanabe | Yoichi Yatsu | Philippe Laurent | Kunishiro Mori | Shin'ichiro Takeda | Andreas Zoglauer | Toshio Nakano | Junichiro Katsuta | Taketo Mimura | Katsuma Miyake | Masanori Ohno | Rie Sato | Madoka Kawaharada | Makoto Asai | Tsunefumi Mizuno | Tatsumi Koi | Masanobu Ozaki | Yukikatsu Terada | Takayuki Yuasa | Shogo B. Kobayashi | Yasuyuki T. Tanaka | Jun Kataoka | Dennis H. Wright | Francois Lebrun | Hiroyasu Tajima | Kazuo Makishima | Takeshi Nakamori | Kazuhiro Nakazawa | Hiromitsu Takahashi | Kouichi Hagino | Masayuki Ohta | Tadayuki Takahashi | Yasunobu Uchiyama | M. Asai | D. Wright | T. Koi | R. Sato | K. Makishima | M. Kawaharada | K. Hayashi | K. Yamaoka | Y. Yatsu | Y. Fukazawa | T. Mizuno | Shin Watanabe | K. Nakazawa | J. Kataoka | T. Enoto | K. Hagino | J. Katsuta | M. Kokubun | P. Laurent | F. Lebrun | O. Limousin | D. Maier | T. Nakamori | T. Nakano | H. Noda | H. Odaka | M. Ohno | M. Ozaki | S. Saito | G. Sato | H. Tajima | Hiromitsu Takahashi | Tadayuki Takahashi | S. Takeda | Takaaki Tanaka | Y. Terada | H. Uchiyama | Y. Uchiyama | G. Madejski | A. Zoglauer | T. Mimura | Katsuma Miyake | Hiroaki Murakami | Tamotsu Satō | T. Yuasa | Greg Madejski | Hiroaki Murakami | Shinya Saito | Takaaki Tanaka | K. Mori | Tamotsu Sato | M. Ohta | T. Yasuda | Tetsuya Yasuda | S. Watanabe | Y. Tanaka | S. Kobayashi | H. Takahashi | Tamotsu Sato | H. Murakami
[1] A. Dell'Acqua,et al. Geant4 - A simulation toolkit , 2003 .
[2] T. Koi,et al. Geant 4 Developments and Applications , 2013 .
[3] J. Chiang,et al. The Bayesian Block Algorithm , 2013, 1304.2818.
[4] T. Takahashi,et al. Monte Carlo simulation study of in-orbit background for the soft gamma-ray detector on-board ASTRO-H , 2010, Astronomical Telescopes + Instrumentation.
[5] Motohide Kokubun,et al. The hard x-ray imager (HXI) onboard ASTRO-H , 2016, Astronomical Telescopes + Instrumentation.
[6] Kristin K. Madsen,et al. NuSTAR OBSERVATIONS OF THE BULLET CLUSTER: CONSTRAINTS ON INVERSE COMPTON EMISSION , 2014, 1403.2722.
[7] D. Caruge,et al. Recent Developments in Geant4 , 2014, ICS 2014.
[8] Shogo B. Kobayashi,et al. The Si/CdTe semiconductor camera of the ASTRO-H Hard X-ray Imager (HXI) , 2016 .
[9] B. L. Colborn,et al. Trapped Radiation Model Uncertainties: Model-Data and Model-Model Comparisons , 2000 .
[10] T. Tanaka,et al. In-Orbit Performance of the Hard X-Ray Detector on Board Suzaku , 2006, astro-ph/0611233.
[11] Yoshiharu Namba,et al. The ASTRO-H (Hitomi) x-ray astronomy satellite , 2016, Astronomical Telescopes + Instrumentation.
[12] Tadayuki Takahashi,et al. In-orbit performance and calibration of the Hard X-ray Imager onboard Hitomi (ASTRO-H) , 2018, 1805.08344.
[13] M. Casolino,et al. Geomagnetically trapped, albedo and solar energetic particles: Trajectory analysis and flux reconstruction with PAMELA , 2016, 1607.02870.
[14] Logan J. Harr. Precise Calculation of Complex Radioactive Decay Chains , 2007 .
[15] S. Incerti,et al. Geant4 developments and applications , 2006, IEEE Transactions on Nuclear Science.
[16] G. Sato,et al. Activation properties of Schottky CdTe diodes irradiated by 150 MeV protons , 2002, 2002 IEEE Nuclear Science Symposium Conference Record.
[17] G. Weidenspointner,et al. MGGPOD: a Monte Carlo Suite for Modeling Instrumental Line and Continuum Backgrounds in Gamma-Ray Astronomy , 2004, astro-ph/0408399.
[18] Robert Andritschke,et al. MEGAlib – The Medium Energy Gamma-ray Astronomy Library , 2006 .
[19] J. Scargle. Studies in Astronomical Time-series Analysis. VII. An Enquiry Concerning Nonlinearity, the rms–Mean Flux Relation, and Lognormal Flux Distributions , 2020, The Astrophysical Journal.
[20] Kentaro Uesugi,et al. Imaging and spectral performance of CdTe double-sided strip detectors for the hard x-ray imager onboard ASTRO-H , 2012, Other Conferences.
[21] Dieter Bilitza,et al. NASA/National Space Science Data Center trapped radiation models , 1994 .
[22] Tadayuki Takahashi,et al. Design and performance of Soft Gamma-ray Detector onboard the Hitomi (ASTRO-H) satellite , 2018 .
[23] Yasushi Fukazawa,et al. Development of an integrated response generator for Si/CdTe semiconductor Compton cameras , 2010 .
[24] Tadayuki Takahashi,et al. The soft gamma-ray detector (SGD) onboard ASTRO-H , 2016, Astronomical Telescopes + Instrumentation.
[25] Tuneyoshi Kamae,et al. Hard X-Ray Detector (HXD) on Board Suzaku , 2006, astro-ph/0611232.
[26] Akihiro Furuzawa,et al. A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit , 2012, Other Conferences.
[27] A. V. Karelin,et al. TRAPPED PROTON FLUXES AT LOW EARTH ORBITS MEASURED BY THE PAMELA EXPERIMENT , 2014, 1412.1258.
[28] J. Chiang,et al. STUDIES IN ASTRONOMICAL TIME SERIES ANALYSIS. VI. BAYESIAN BLOCK REPRESENTATIONS , 2012, 1207.5578.