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Application of an EMCCD camera for calibration of hard x-ray telescopes

Vogel, Julia K. and Pivovaroff, Michael J. and Nagarkar, Vivek V. and Kudrolli, Haris and Kruse Madsen, Kristin and Koglin, Jason E. and Christensen, Finn E. and Brejnholt, Nicolai F. (2011) Application of an EMCCD camera for calibration of hard x-ray telescopes. In: 2011 IEEE Nuclear Science Symposium Conference Record. IEEE , Piscataway, NJ, pp. 1204-1212. ISBN 978-1-4673-0120-6 . https://resolver.caltech.edu/CaltechAUTHORS:20170228-164605693

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Abstract

Recent technological innovations now make it feasible to construct hard x-ray telescopes for space-based astronomical missions. Focusing optics are capable of improving the sensitivity in the energy range above 10 keV by orders of magnitude compared to previously used instruments. The last decade has seen focusing optics developed for balloon experiments [1] and they will soon be implemented in approved space missions such as the Nuclear Spectroscopic Telescope Array (NuSTAR) [2] and ASTRO-H [3]. The full characterization of x-ray optics for astrophysical and solar imaging missions, including measurement of the point spread function (PSF) as well as scattering and reflectivity properties of substrate coatings, requires a very high spatial resolution, high sensitivity, photon counting and energy discriminating, large area detector. Novel back-thinned Electron Multiplying Charge-Coupled Devices (EMCCDs) [4] are highly suitable detectors for ground-based calibrations. Their chip can be optically coupled to a microcolumnar CsI(Tl) scintillator [5] via a fiberoptic taper. Not only does this device exhibit low noise and high spatial resolution inherent to CCDs, but the EMCCD is also able to handle high frame rates due to its controllable internal gain. Additionally, thick CsI(Tl) yields high detection efficiency for x-rays [6]. This type of detector has already proven to be a unique device very suitable for calibrations in astrophysics: such a camera was used to support the characterization of the performance for all NuSTAR optics [7]-[9]. Further optimization will enable similar cameras to be improved and used to calibrate x-ray telescopes for future space missions. In this paper, we discuss the advantages of using an EMCCD to calibrate hard x-ray optics. We will illustrate the promising features of this detector solution using examples of data obtained during the ground calibration of the NuSTAR telescopes performed at Columbia University during 2010/2011. Finally, we give an outlook on ongoing development and optimizations, such as the use of single photon counting mode to enhance spectral resolution.


Item Type:Book Section
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https://doi.org/10.1109/NSSMIC.2011.6154603DOIArticle
http://ieeexplore.ieee.org/document/6154603/PublisherArticle
Additional Information:© 2011 IEEE. Manuscript received November 18, 2011. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. The support of the Laboratory Directed Research and Development Pro­gram is gratefully acknowledged. We thank our colleagues at NuSTAR for their support and cooperation and Columbia University for hospitality. We also thank NASA for funding this research under grant number NNXIICH32P.
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-AC52-07NA27344
NASANNXIICH32P
Subject Keywords:MCCD, NuSTAR, hard x-ray mission, hard x-ray detectors, calibration, scintillator, x-ray detectors
Record Number:CaltechAUTHORS:20170228-164605693
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170228-164605693
Official Citation:J. K. Vogel et al., "Application of an EMCCD camera for calibration of hard x-ray telescopes," 2011 IEEE Nuclear Science Symposium Conference Record, Valencia, 2011, pp. 1204-1212. doi: 10.1109/NSSMIC.2011.6154603
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74617
Collection:CaltechAUTHORS
Deposited By: Kristin Buxton
Deposited On:01 Mar 2017 00:57
Last Modified:03 Oct 2019 16:40

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