Open Access
27 October 2017 Observational artifacts of Nuclear Spectroscopic Telescope Array: ghost rays and stray light
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Abstract
The Nuclear Spectroscopic Telescope Array (NuSTAR) launched in June 2012, flies two conical approximation Wolter-I mirrors at the end of a 10.15-m mast. The optics are coated with multilayers of Pt/C and W/Si that operate from 3 to 80 keV. Since the optical path is not shrouded, aperture stops are used to limit the field of view (FoV) from background and sources outside the FoV. However, there is still a sliver of sky ( ∼1.0  deg to 4.0 deg) where photons may bypass the optics altogether and fall directly on the detector array. We term these photons stray light. Additionally, there are also photons that do not undergo the focused double reflections in the optics, and we term these ghost rays. We present detailed analysis and characterization of these two components and discuss how they impact observations. Finally, we discuss how they could have been prevented and should be in future observatories.
CC BY: © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.
Kristin K. Madsen, Finn E. Christensen, William W. Craig, Karl W. Forster, Brian W. Grefenstette, Fiona A. Harrison, Hiromasa Miyasaka, and Vikram Rana "Observational artifacts of Nuclear Spectroscopic Telescope Array: ghost rays and stray light," Journal of Astronomical Telescopes, Instruments, and Systems 3(4), 044003 (27 October 2017). https://doi.org/10.1117/1.JATIS.3.4.044003
Received: 27 June 2017; Accepted: 3 October 2017; Published: 27 October 2017
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CITATIONS
Cited by 35 scholarly publications.
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KEYWORDS
Photons

Sensors

Mirrors

Telescopes

Space telescopes

Reflection

Spectroscopes

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