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An Overview of X-Ray Polarimetry of Astronomical Sources

机译:天文来源的X射线极化法概述

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We review the history of astronomical X-ray polarimetry based on the author’s perspective, beginning with early sounding-rocket experiments by Robert Novick at Columbia University and his team, of which the author was a member. After describing various early techniques for measuring X-ray polarization, we discuss the polarimeter aboard the Orbiting Solar Observatory 8 (OSO-8) and its scientific results. Next, we describe the X-ray polarimeter to have flown aboard the ill-fated original Spectrum-X mission, which provided important lessons on polarimeter design, systematic effects, and the programmatics of a shared focal plane. We conclude with a description of the Imaging X-ray Polarimetry Explorer (IXPE) and its prospective scientific return. IXPE, a partnership between NASA and ASI, has been selected as a NASA Astrophysics Small Explorers Mission and is currently scheduled to launch in April of 2021.
机译:我们从作者的角度回顾了天文学X射线极化技术的历史,首先是哥伦比亚大学的罗伯特·诺维克及其团队的早期探空火箭实验,作者是其中的一员。在描述了各种用于测量X射线极化的早期技术之后,我们讨论了轨道太阳天文台8号(OSO-8)上的旋光仪及其科学成果。接下来,我们描述X射线旋光仪已经搭乘了命运多f的原始Spectrum-X任务,该任务为旋光仪的设计,系统效果以及共享焦平面的程序设计提供了重要的经验教训。我们以成像X射线极化仪(IXPE)及其预期的科学回报作为结尾。 IXPE是NASA与ASI之间的合作伙伴关系,已被选为NASA天体物理学小探险家任务,目前计划于2021年4月发射。

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