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Systematic effects on a Compton polarimeter at the focus of an X-ray mirror
Osaka University, Department of Earth and Space Science, Graduate School of Science, and Project Research Center for Fundamental Sciences, 1-1 Machikaneyama-cho, Toyonaka, Osaka 560-0043, Japan, 1-1 Machikaneyama-cho, Toyonaka.
Physics Department, Washington University in St. Louis, 1 Brookings Drive, CB 1105, St. Louis, MO 63130, USA, 1 Brookings Drive, CB 1105; McDonnell Center for the Space Sciences, Washington University in St. Louis, 1 Brookings Drive, CB 1105, St. Louis, MO 63130, USA, 1 Brookings Drive, CB 1105.
Physics Department, Washington University in St. Louis, 1 Brookings Drive, CB 1105, St. Louis, MO 63130, USA, 1 Brookings Drive, CB 1105; McDonnell Center for the Space Sciences, Washington University in St. Louis, 1 Brookings Drive, CB 1105, St. Louis, MO 63130, USA, 1 Brookings Drive, CB 1105.
Physics Department, Washington University in St. Louis, 1 Brookings Drive, CB 1105, St. Louis, MO 63130, USA, 1 Brookings Drive, CB 1105; McDonnell Center for the Space Sciences, Washington University in St. Louis, 1 Brookings Drive, CB 1105, St. Louis, MO 63130, USA, 1 Brookings Drive, CB 1105.
Vise andre og tillknytning
2024 (engelsk)Inngår i: Astroparticle physics, ISSN 0927-6505, E-ISSN 1873-2852, Vol. 158, artikkel-id 102944Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

XL-Calibur is a balloon-borne Compton polarimeter for X-rays in the ∼15–80 keV range. Using an X-ray mirror with a 12 m focal length for collecting photons onto a beryllium scattering rod surrounded by CZT detectors, a minimum-detectable polarization as low as ∼3% is expected during a 24-hour on-target observation of a 1 Crab source at 45° elevation. Systematic effects alter the reconstructed polarization as the mirror focal spot moves across the beryllium scatterer, due to pointing offsets, mechanical misalignment or deformation of the carbon-fiber truss supporting the mirror and the polarimeter. Unaddressed, this can give rise to a spurious polarization signal for an unpolarized flux, or a change in reconstructed polarization fraction and angle for a polarized flux. Using bench-marked Monte-Carlo simulations and an accurate mirror point-spread function characterized at synchrotron beam-lines, systematic effects are quantified, and mitigation strategies discussed. By recalculating the scattering site for a shifted beam, systematic errors can be reduced from several tens of percent to the few-percent level for any shift within the scattering element. The treatment of these systematic effects will be important for any polarimetric instrument where a focused X-ray beam is impinging on a scattering element surrounded by counting detectors.

sted, utgiver, år, opplag, sider
Elsevier BV , 2024. Vol. 158, artikkel-id 102944
Emneord [en]
Balloon-borne telescope, Bench-marking, Compton polarimetry, Modulation response, Monte-Carlo simulations, Offset correction, X-ray optics
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Identifikatorer
URN: urn:nbn:se:kth:diva-344000DOI: 10.1016/j.astropartphys.2024.102944ISI: 001198087900001Scopus ID: 2-s2.0-85185398384OAI: oai:DiVA.org:kth-344000DiVA, id: diva2:1841370
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QC 20240229

Tilgjengelig fra: 2024-02-28 Laget: 2024-02-28 Sist oppdatert: 2024-04-29bibliografisk kontrollert

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Iyer, NirmalKiss, MózsiKlepper, Kassiaf Malmborg, FilipPearce, Mark

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