IXPE上成像x射线偏振仪的在轨监测

A. Di Marco, F. Muleri, S. Fabiani, F. La Monaca, J. Rankin, P. Soffitta, L. Baldini, E. Costa, E. Del Monte, R. Ferrazzoli, C. Lefevre, L. Maiolo, F. Maita, A. Manfreda, A. Morbidini, S. O’Dell, B. Ramsey, A. Ratheesh, C. Sgro’, A. Trois, A. Tennant, M. Weisskopf
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引用次数: 4

摘要

成像x射线偏振探测器(IXPE)于2021年12月9日从卡纳维拉尔角发射到近地赤道轨道。该任务由美国国家航空航天局(NASA)与意大利航天局(ASI)合作领导,以三个相同的望远镜为特色,每个望远镜在x射线反射镜组件的焦点处都有一个成像x射线光电偏振计。每个焦平面探测器包括一组四个校准源,由55Fe核素供电,以监测探测器的性能。在这些光源中,一个产生两种能量的偏振x射线,其余三个产生非偏振辐射。在这里,我们介绍了这一监测计划的现状,从安装飞行核素到对天文台进行地面环境测试,再到最近在科学操作期间的在轨测量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
In-orbit monitoring of the imaging x-ray polarimeters on-board IXPE
The imaging x-ray polarimetry explorer (IXPE) was launched on December 9, 2021, from Cape Canaveral into a low-Earth equatorial orbit. The mission, led by NASA in collaboration with the Italian Space Agency (ASI), features three identical telescopes, each with an imaging x-ray photoelectric polarimeter at the focus of an x-ray mirror assembly. Each focal-plane detector includes a set of four calibration sources powered by a 55Fe nuclide to monitor the detector’s performance. Of these sources, one produces polarized x-rays at two energies and the remaining three generate unpolarized radiation. Here we present the status of this monitoring program, starting from installation of the flight nuclides before on-ground environmental testing of the observatory through recent on-orbit measurements during science operations.
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