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The design and performance of the XL-Calibur anticoincidence shield
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics. The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, 106 91 Stockholm, Sweden..ORCID iD: 0000-0001-6134-8105
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics. The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, 106 91 Stockholm, Sweden..ORCID iD: 0000-0001-5191-9306
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics. The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, 106 91 Stockholm, Sweden..ORCID iD: 0000-0001-7011-7229
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics. The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, 106 91 Stockholm, Sweden..ORCID iD: 0000-0002-1165-6166
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2023 (English)In: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, ISSN 0168-9002, E-ISSN 1872-9576, Vol. 1048, article id 167975Article in journal (Refereed) Published
Abstract [en]

The XL-Calibur balloon-borne hard X-ray polarimetry mission comprises a Compton-scattering polarimeter placed at the focal point of an X-ray mirror. The polarimeter is housed within a BGO anticoincidence shield, which is needed to mitigate the considerable background radiation present at the observation altitude of ∼40 km. This paper details the design, construction and testing of the anticoincidence shield, as well as the performance measured during the week-long maiden flight from Esrange Space Centre to the Canadian Northwest Territories in July 2022. The in-flight performance of the shield followed design expectations, with a veto threshold <100 keV and a measured background rate of ∼0.5 Hz (20–40 keV). This is compatible with the scientific goals of the mission, where %-level minimum detectable polarisation is sought for a Hz-level source rate.

Place, publisher, year, edition, pages
Elsevier BV , 2023. Vol. 1048, article id 167975
Keywords [en]
Anticoincidence, BGO scintillator, Monte Carlo, Photomultiplier tube, Qualification testing, Scientific ballooning, X-ray polarimetry
National Category
Astronomy, Astrophysics and Cosmology Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-330081DOI: 10.1016/j.nima.2022.167975ISI: 000995686300001Scopus ID: 2-s2.0-85146099547OAI: oai:DiVA.org:kth-330081DiVA, id: diva2:1775174
Note

QC 20230626

Available from: 2023-06-26 Created: 2023-06-26 Last updated: 2023-11-29Bibliographically approved

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Iyer, NirmalKiss, MózsiPearce, MarkStana, Theodor-Adrian

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Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Astronomy, Astrophysics and CosmologySubatomic Physics

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