Back to Search Start Over

Systematic effects on a Compton polarimeter at the focus of an X-ray mirror

Authors :
Aoyagi, M.
Bose, R. G.
Chun, S.
Gau, E.
Hu, K.
Ishiwata, K.
Iyer, N. K.
Kislat, F.
Kiss, M.
Klepper, K.
Krawczynski, H.
Lisalda, L.
Maeda, Y.
Malmborg, F. af
Matsumoto, H.
Miyamoto, A.
Miyazawa, T.
Pearce, M.
Rauch, B. F.
Cavero, N. Rodriguez
Spooner, S.
Takahashi, H.
Uchida, Y.
West, A. T.
Wimalasena, K.
Yoshimoto, M.
Source :
Astropart. Phys. 158 (2024) 102944
Publication Year :
2024

Abstract

XL-Calibur is a balloon-borne Compton polarimeter for X-rays in the $\sim$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 $\sim$3% is expected during a 24-hour on-target observation of a 1 Crab source at 45$^{\circ}$ 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.<br />Comment: Submitted to Astroparticle Physics

Details

Database :
arXiv
Journal :
Astropart. Phys. 158 (2024) 102944
Publication Type :
Report
Accession number :
edsarx.2402.15229
Document Type :
Working Paper
Full Text :
https://doi.org/10.1016/j.astropartphys.2024.102944