成像x射线偏振探测器(IXPE)

R. Ferrazzoli
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引用次数: 4

摘要

在高能多波长研究的难题中,x射线偏振法是一个长期缺失的部分。成像x射线偏振测量探测器(IXPE)将填补我们知识上的这一空白,它将偏振测量添加到目前可用的观测数据中:能量、时间和位置。IXPE最初是为了响应2014年发布的机会公告而提出的,于2017年1月在美国宇航局天体物理小型探测器(SMEX)计划的背景下被选中,并与意大利航天局(ASI)合作。由于其具有气体像素探测器成像能力的偏振计,IXPE将在理解粒子加速过程,高磁化致密物体和散射诱导极化特性方面打开新的窗口。在这里,将重点介绍该任务的技术方面和IXPE将探索的一些科学案例。将特别注意IXPE将能够研究的扩展源的选择,这得益于其成像能力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Imaging X-ray Polarimetry Explorer (IXPE)
X-ray polarimetry is a long-standing missing piece in the puzzle of multiwavelenght study of high energy sources. The Imaging X-ray Polarimetry Explorer (IXPE) will fill this gap in our knowedge by adding polarization measurements to observables currently avaiable: energy, time, and position. IXPE, first proposed in response of an Announcement of Opportunity issued on 2014, was selected in the context of the NASA Astrophysics Small Explorer (SMEX) program in January 2017, and is a collaboration with the Italian Space Agency (ASI). Thanks to its Gas Pixel Detector imaging-capable polarimeter, IXPE will open new a new window in the understanding of particle acceleration processes, higly magnetized compact objects and the properties of scattering induced polarization. Here, the thecnical aspects of the mission and some of the scientific cases that IXPE will explore will be highlighted. Special attenton will be given to a selection of extended sources that IXPE will be able to study thanks its imaging capabilities.
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