The encircled energy function of the IXPE determined from data of the crab pulsar

Masaki Kamikobayashi, S. Gunji, L. Baldini, B. Ramsey, E. Watanabe, Masanobu Terashima, Yuuma Kan, Manato Mori
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Abstract

The Imaging X-ray Polarimetry Explorer (IXPE) is the unprecedented satellite capable of obtaining the x-ray polarization map. To obtain the accurate polarization map for extended sources, the measurements of the Encircled Energy Function (EEF) in flight is necessary. Though it has been often carried out using point-like source, the background may affect the accurate measurements. So, we have investigated the EEF using the data of the Crab pulsar with the nebula, because the background can be accurately removed by subtracting the off-pulse component from the on-pulse component. With the method, we succeeded in obtaining the energy dependence of the EEF.
由蟹状脉冲星数据确定的IXPE的环能量函数
成像x射线偏振探测卫星(IXPE)是前所未有的能够获得x射线偏振图的卫星。为了获得精确的扩展源偏振图,需要在飞行中测量环绕能量函数(EEF)。虽然通常使用点状光源进行测量,但背景会影响测量的准确性。因此,我们使用蟹状星云脉冲星的数据来研究EEF,因为通过从脉冲分量中减去非脉冲分量可以准确地去除背景。利用该方法,我们成功地获得了电场的能量依赖关系。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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