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Simulations and measurements of the background encountered by a high-altitude balloon-borne experiment for hard X-ray astronomy

1997/09/01 by Kenneth S. K. Lum, K. S. K. Lum, J. J. Mohr +7 · 1 citation
Medicine · Physics and Astronomy · #Astrophysical Phenomena and Observations #Nuclear Physics and Applications #Radiation Therapy and Dosimetry #astro-ph

paper · pdf · doi:10.1016/s0168-9002(97)00785-7

published as Nucl.Instrum.Meth. A396 (1997) 350-359 · 17 pages Latex (uses aaspp4.sty) plus 7 postscript figures: available in file figs.tar.gz

openalex publication_date 1997/09/01 · arxiv created 1997/12/31 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We have modelled the hard X-ray background expected for a high-altitude balloon flight of the Energetic X-ray Telescope Experiment (EXITE2), an imaging phoswich detector/telescope for the 20--600 keV energy range. Photon and neutron-induced contributions to the background are considered. We describe the code and the results of a series of simulations with different shielding configurations. The simulated hard X-ray background for the actual flight configuration agrees reasonably well (within a factor of ∼ 2) with the results measured on the first flight of EXITE2 from Palestine, Texas. The measured background flux at 100 keV is ∼ 4 × 10-4 counts cm-2 s-1 keV-1.

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