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6 December 2022 NuSTAR non-x-ray background
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Abstract

We present an overview of the NuSTAR non x-ray background. This is dominated by proton scattering in the detector and surrounding material as well as activation lines from of material in the detector and its housing. We also discuss contributions from the solar component (when the Sun is active), and the impact of short-lived radiation belts on the NuSTAR background and activation in the detectors.

CC BY: © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 International License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.
Brian W. Grefenstette, Kristin K. Madsen, Hiromasa Miyasaka, and Andreas Zoglauer "NuSTAR non-x-ray background," Journal of Astronomical Telescopes, Instruments, and Systems 8(4), 047001 (6 December 2022). https://doi.org/10.1117/1.JATIS.8.4.047001
Received: 28 June 2022; Accepted: 14 November 2022; Published: 6 December 2022
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Cited by 1 scholarly publication.
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KEYWORDS
X-rays

Solar processes

Sun

Equipment

Particles

Solar radiation

Satellites

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