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Mission Overview and Initial Observation Results of the X-Ray Pulsar Navigation-I Satellite

机译:任务概述和X射线Pulsar导航 - 我卫星的初始观察结果

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摘要

The newly launched X-ray pulsar navigation-I (XPNAV-1) is an experimental satellite of China that is designed for X-ray pulsar observation. This paper presents the initial observation results and aims to recover the Crab pulsar’s pulse profile to verify the X-ray instrument’s capability of observing pulsars in space. With the grazing-incidence focusing type instrument working at the soft X-ray band (0.5–10 keV), up to 162 segments of observations of the Crab pulsar are fulfilled, and more than 5 million X-ray events are recorded. Arrival times of photons are corrected to the solar system barycentre, and the 33 ms pulse period is sought out for Crab. Epoch folding of all the corrected photon times generates the refined pulse profile of Crab. The characteristic two-peak profile proves that the Crab pulsar has been clearly seen, so that the conclusion is made that XPNAV-1’s goal of being capable of observing pulsars is achieved.
机译:新推出的X射线Pulsar Navigation-I(XPNAV-1)是中国的实验卫星,专为X射线Pulsar观察而设计。本文介绍了初始观察结果,旨在恢复螃蟹脉冲脉冲曲线,以验证X射线仪器观察太空中脉冲条件的能力。通过在软X射线带(0.5-10keV)的放牧发生型聚焦仪器,满足高达162个观察的观察,并记录了超过500万X射线事件。光子的到达时间被校正到太阳系BaryCentre,并寻求螃蟹的33毫秒脉冲周期。 EPOCH折叠所有校正的光子次数产生螃蟹的精细脉冲曲线。特征的双峰配置文件证明了螃蟹脉冲结果已经清楚地看到,因此结论是实现了XPNAV-1能够观察脉冲条的目标。

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