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Astrophysics > Instrumentation and Methods for Astrophysics

arXiv:2010.10608 (astro-ph)
[Submitted on 20 Oct 2020]

Title:XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission

Authors:Q. Abarr, H. Awaki, M.G. Baring, R. Bose, G. De Geronimo, P. Dowkontt, M. Errando, V. Guarino, K. Hattori, K. Hayashida, F. Imazato, M. Ishida, N.K. Iyer, F. Kislat, M. Kiss, T. Kitaguchi, H. Krawczynski, L. Lisalda, H. Matake, Y. Maeda, H. Matsumoto, T. Mineta, T. Miyazawa, T. Mizuno, T. Okajima, M. Pearce, B.F. Rauch, F. Ryde, C. Shreves, S. Spooner, T.-A. Stana, H. Takahashi, M. Takeo, T. Tamagawa, K. Tamura, H. Tsunemi, N. Uchida, Y. Uchida, A.T. West, E.A. Wulf, R. Yamamoto
View a PDF of the paper titled XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission, by Q. Abarr and 40 other authors
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Abstract:XL-Calibur is a hard X-ray (15-80 keV) polarimetry mission operating from a stabilised balloon-borne platform in the stratosphere. It builds on heritage from the X-Calibur mission, which observed the accreting neutron star GX 301-2 from Antarctica, between December 29th 2018 and January 1st 2019. The XL-Calibur design incorporates an X-ray mirror, which focusses X-rays onto a polarimeter comprising a beryllium rod surrounded by Cadmium Zinc Telluride (CZT) detectors. The polarimeter is housed in an anticoincidence shield to mitigate background from particles present in the stratosphere. The mirror and polarimeter-shield assembly are mounted at opposite ends of a 12 m long lightweight truss, which is pointed with arcsecond precision by WASP - the Wallops Arc Second Pointer. The XL-Calibur mission will achieve a substantially improved sensitivity over X-Calibur by using a larger effective area X-ray mirror, reducing background through thinner CZT detectors, and improved anticoincidence shielding. When observing a 1 Crab source for $t_{\rm day}$ days, the Minimum Detectable Polarisation (at 99% confidence level) is $\sim$2$\%\cdot t_{\rm day}^{-1/2}$. The energy resolution at 40 keV is $\sim$5.9 keV. The aim of this paper is to describe the design and performance of the XL-Calibur mission, as well as the foreseen science programme.
Comments: 19 pages, 17 figures. Accepted for publication in Astroparticle Physics
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); High Energy Astrophysical Phenomena (astro-ph.HE)
Cite as: arXiv:2010.10608 [astro-ph.IM]
  (or arXiv:2010.10608v1 [astro-ph.IM] for this version)
  https://doi.org/10.48550/arXiv.2010.10608
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1016/j.astropartphys.2020.102529
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From: Mark Pearce [view email]
[v1] Tue, 20 Oct 2020 20:37:57 UTC (3,371 KB)
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