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

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
M. Aoyagi , R.G. Bose , S. Chun , E. Gau , K. Hu , K. Ishiwata , N.K. Iyer , F. Kislat , M. Kiss , K. Klepper , H. Krawczynski , L. Lisalda , Y. Maeda , F. af Malmborg , H. Matsumoto , A. Miyamoto , T. Miyazawa , M. Pearce , B.F. Rauch , N. Rodriguez Cavero , M. Yoshimoto
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Abstract

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.

X 射线镜焦点处的康顿偏振计的系统效应
XL-Calibur 是一个气球载康普顿偏振计,用于探测 15-80 千伏范围内的 X 射线。利用一个焦距为 12 米的 X 射线反射镜将光子收集到一个铍散射棒上,该散射棒周围装有 CZT 探测器,在对 1 蟹源进行仰角为 45°的 24 小时目标观测时,预计可探测到的最小偏振低至 3%。如果不加以解决,就会导致非偏振通量出现虚假偏振信号,或偏振通量的重建偏振分数和角度发生变化。利用同步辐射光束线的基准蒙特卡洛模拟和精确的镜面点展函数,对系统效应进行了量化,并讨论了缓解策略。通过重新计算偏移光束的散射点,可以将散射元件内任何偏移的系统误差从百分之几十降低到百分之几的水平。在任何偏振测量仪器中,聚焦的 X 射线光束都会撞击到由计数探测器包围的散射元件上。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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