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arXiv 1701.04536astro-ph.IM
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球载X射线偏振计X-Calibur望远镜桁架和吊舱的设计

Design of the telescope truss and gondola for the balloon-borne X-ray polarimeter X-Calibur

Fabian Kislat, Banafsheh Beheshtipour, Paul Dowkontt, Victor Guarino, R. James Lanzi, Takashi Okajima, Dana Braun, Scott Cannon, Gialuigi De Geronimo, Scott Hea… 展开作者

Fabian Kislat, Banafsheh Beheshtipour, Paul Dowkontt, Victor Guarino, R. James Lanzi, Takashi Okajima, Dana Braun, Scott Cannon, Gialuigi De Geronimo, Scott Heatwole, Janie Hoorman, Shaorui Li, Hideyuki Mori, Christopher M. Shreves, David Stuchlik, Henric Krawczynski

摘要:

近年来,X射线偏振测量法受到越来越多的关注。探测器技术和聚焦X射线光学器件的改进现在使灵敏的天体物理学X射线偏振测量成为可能。这些测量将为黑洞吸积过程、中子星和磁星的X射线发射以及活动星系核喷流的结构提供新的见解。X-Calibur是一种球载硬X射线散射偏振仪。焦距为8 m的X射线镜将X射线聚焦到探测器上,探测器由塑料散射元件组成,周围是吸收和记录散射X射线的碲锌镉探测器。由于X射线优先地垂直于其偏振方向散射,因此X射线束的偏振性质可以从散射X射线的方位角分布推断。要求X射线焦斑与探测器的中心紧密对准,以减少系统不确定性并保持高光子探测效率。这对望远镜结构的机械和热稳定性提出了严格的要求。在同温层气球上飞行期间,X-Calibur利用Wallops弧秒指针(WASP)将望远镜指向天体物理源。在本文中,我们描述了望远镜结构的设计,建造和测试,以及它在25小时的飞行中的性能。新墨西哥州萨姆纳碳纤维-铝复合材料结构符合X-Calibur的要求,其设计可以很容易地适用于其他类型的实验,如X射线成像或光谱望远镜。

英文摘要:

X-ray polarimetry has seen a growing interest in recent years. Improvements in detector technology and focusing X-ray optics now enable sensitive astrophysical X-ray polarization measurements. These measurements will provide new insights into the processes at work in accreting black holes, the emission of X-rays from neutron stars and magnetars, and the structure of AGN jets. X-Calibur is a balloon-borne hard X-ray scattering polarimeter. An X-ray mirror with a focal length of 8 m focuses X-rays onto the detector, which consists of a plastic scattering element surrounded by Cadmium-Zinc-Telluride detectors, which absorb and record the scattered X-rays. Since X-rays preferentially scatter perpendicular to their polarization direction, the polarization properties of an X-ray beam can be inferred from the azimuthal distribution of scattered X-rays. A close alignment of the X-ray focal spot with the center of the detector is required in order to reduce systematic uncertainties and to maintain a high photon detection efficiency. This places stringent requirements on the mechanical and thermal stability of the telescope structure. During the flight on a stratospheric balloon, X-Calibur makes use of the Wallops Arc-Second Pointer (WASP) to point the telescope at astrophysical sources. In this paper, we describe the design, construction, and test of the telescope structure, as well as its performance during a 25-hour flight from Ft. Sumner, New Mexico. The carbon fiber-aluminum composite structure met the requirements set by X-Calibur and its design can easily be adapted for other types of experiments, such as X-ray imaging or spectroscopic telescopes.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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