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X-ray polarimetry on-board HXMT

机译:机上X射线极化仪HXMT

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摘要

The development of micropixel gas detectors, capable to image tracks produced in a gas by photoelectrons, makes possible to perform polarimetry of X-ray celestial sources in the focus of grazing incidence X-ray telescopes. HXMT is a mission by the Chinese Space Agency aimed to survey the Hard X-ray Sky with Phoswich detectors, by exploitation of the direct demodulation technique. Since a fraction of the HXMT time will be spent on dedicated pointing of particular sources, it could host, with moderate additional resources a pair of X-ray telescopes, each with a photoelectric X-ray polarimeter (EXP~2, Efficient X-ray Photoelectric Polarimeter) in the focal plane. We present the design of the telescopes and the focal plane instrumentation and discuss the performance of this instrument to detect the degree and angle of linear polarization of some representative sources. Notwithstanding the limited resources, the proposed instrument can represent a breakthrough in X-ray Polarimetry.
机译:通过光电子在气体中产生的微泛素气检测器的开发能够在气体中产生的轨道,使得可以在放牧入射X射线望远镜的焦点中执行X射线天体源的偏振基。 HXMT是中国太空机构的使命,旨在通过开采直接解调技术来调查用福斯旺斯探测器的硬X射线天空。由于HXMT时间的一部分将在专用的特定来源指向上,因此它可能托管,以适度的额外资源一对X射线望远镜,每个X射线望远镜都有光电X射线偏振仪(Exp〜2,高效X射线光电偏振仪)在焦平面。我们展示了望远镜和焦平面仪器的设计,并讨论了这种仪器的性能,以检测一些代表源的线性极化的程度和角度。尽管有限的资源,所提出的仪器可以代表X射线偏振基的突破。

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