XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission
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. Th...
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ftdatacite:10.48550/arxiv.2010.10608 2023-05-15T14:06:41+02:00 XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission Abarr, Q. Awaki, H. Baring, M. G. Bose, R. De Geronimo, G. Dowkontt, P. Errando, M. Guarino, V. Hattori, K. Hayashida, K. Imazato, F. Ishida, M. Iyer, N. K. Kislat, F. Kiss, M. Kitaguchi, T. Krawczynski, H. Lisalda, L. Matake, H. Maeda, Y. Matsumoto, H. Mineta, T. Miyazawa, T. Mizuno, T. Okajima, T. Pearce, M. Rauch, B. F. Ryde, F. Shreves, C. Spooner, S. Stana, T. -A. Takahashi, H. Takeo, M. Tamagawa, T. Tamura, K. Tsunemi, H. Uchida, N. Uchida, Y. West, A. T. Wulf, E. A. Yamamoto, R. 2020 https://dx.doi.org/10.48550/arxiv.2010.10608 https://arxiv.org/abs/2010.10608 unknown arXiv https://dx.doi.org/10.1016/j.astropartphys.2020.102529 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2020 ftdatacite https://doi.org/10.48550/arxiv.2010.10608 https://doi.org/10.1016/j.astropartphys.2020.102529 2022-03-10T15:09:59Z 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. : 19 pages, 17 figures. Accepted for publication in Astroparticle Physics Article in Journal/Newspaper Antarc* Antarctica DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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unknown |
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Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
spellingShingle |
Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Abarr, Q. Awaki, H. Baring, M. G. Bose, R. De Geronimo, G. Dowkontt, P. Errando, M. Guarino, V. Hattori, K. Hayashida, K. Imazato, F. Ishida, M. Iyer, N. K. Kislat, F. Kiss, M. Kitaguchi, T. Krawczynski, H. Lisalda, L. Matake, H. Maeda, Y. Matsumoto, H. Mineta, T. Miyazawa, T. Mizuno, T. Okajima, T. Pearce, M. Rauch, B. F. Ryde, F. Shreves, C. Spooner, S. Stana, T. -A. Takahashi, H. Takeo, M. Tamagawa, T. Tamura, K. Tsunemi, H. Uchida, N. Uchida, Y. West, A. T. Wulf, E. A. Yamamoto, R. XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission |
topic_facet |
Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
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. : 19 pages, 17 figures. Accepted for publication in Astroparticle Physics |
format |
Article in Journal/Newspaper |
author |
Abarr, Q. Awaki, H. Baring, M. G. Bose, R. De Geronimo, G. Dowkontt, P. Errando, M. Guarino, V. Hattori, K. Hayashida, K. Imazato, F. Ishida, M. Iyer, N. K. Kislat, F. Kiss, M. Kitaguchi, T. Krawczynski, H. Lisalda, L. Matake, H. Maeda, Y. Matsumoto, H. Mineta, T. Miyazawa, T. Mizuno, T. Okajima, T. Pearce, M. Rauch, B. F. Ryde, F. Shreves, C. Spooner, S. Stana, T. -A. Takahashi, H. Takeo, M. Tamagawa, T. Tamura, K. Tsunemi, H. Uchida, N. Uchida, Y. West, A. T. Wulf, E. A. Yamamoto, R. |
author_facet |
Abarr, Q. Awaki, H. Baring, M. G. Bose, R. De Geronimo, G. Dowkontt, P. Errando, M. Guarino, V. Hattori, K. Hayashida, K. Imazato, F. Ishida, M. Iyer, N. K. Kislat, F. Kiss, M. Kitaguchi, T. Krawczynski, H. Lisalda, L. Matake, H. Maeda, Y. Matsumoto, H. Mineta, T. Miyazawa, T. Mizuno, T. Okajima, T. Pearce, M. Rauch, B. F. Ryde, F. Shreves, C. Spooner, S. Stana, T. -A. Takahashi, H. Takeo, M. Tamagawa, T. Tamura, K. Tsunemi, H. Uchida, N. Uchida, Y. West, A. T. Wulf, E. A. Yamamoto, R. |
author_sort |
Abarr, Q. |
title |
XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission |
title_short |
XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission |
title_full |
XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission |
title_fullStr |
XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission |
title_full_unstemmed |
XL-Calibur -- a second-generation balloon-borne hard X-ray polarimetry mission |
title_sort |
xl-calibur -- a second-generation balloon-borne hard x-ray polarimetry mission |
publisher |
arXiv |
publishDate |
2020 |
url |
https://dx.doi.org/10.48550/arxiv.2010.10608 https://arxiv.org/abs/2010.10608 |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
https://dx.doi.org/10.1016/j.astropartphys.2020.102529 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.2010.10608 https://doi.org/10.1016/j.astropartphys.2020.102529 |
_version_ |
1766278726379634688 |