A Localization Method of High Energy Transients for All-sky Gamma-ray Monitor

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Yi Zhao, Wangchen Xue, Shaolin Xiong, Qi Luo, Yuanhao Wang, Jiacong Liu, Heng Yu, Xiaoyun Zhao, Yue Huang, Jinyuan Liao, Jianchao Sun, Xiaobo Li, Qibin Yi, Ce Cai, Shuo Xiao, Shenglun Xie, Chao Zheng, Yanqiu Zhang, Chenwei Wang, Wenjun Tan, Zhiwei Guo, Chaoyang Li, Zhenghua An, Gang Chen, Yanqi Du, Min Gao, Ke Gong, Dongya Guo, Jiang He, Jianjian He, Bing Li, Gang Li, Xinqiao Li, Jing Liang, Xiaohua Liang, Yaqing Liu, Xiang Ma, Rui Qiao, Liming Song, Xinying Song, Xilei Sun, Jin Wang, Ping Wang, Xiangyang Wen, Hong Wu, Yanbing Xu, Sheng Yang, Dali Zhang, Fan Zhang, Hongmei Zhang, Peng Zhang, Shu Zhang, Zhen Zhang, Shijie Zheng, Keke Zhang, Xingbo Han, Haiyan Wu, Hu Tai, Hao Geng, Gaopeng Lu, Wei Xu, Fanchao Lyu, Hongbo Zhang, Fangjun Lu, Shuangnan Zhang
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引用次数: 0

Abstract

Fast and reliable localization of high-energy transients is crucial for characterizing the burst properties and guiding the follow-up observations. Localization based on the relative counts of different detectors has been widely used for all-sky gamma-ray monitors. There are two major methods for this count distribution localization: χ 2 minimization method and the Bayesian method. Here we propose a modified Bayesian method that could take advantage of both the accuracy of the Bayesian method and the simplicity of the χ 2 method. With comprehensive simulations, we find that our Bayesian method with Poisson likelihood is generally more applicable for various bursts than the χ 2 method, especially for weak bursts. We further proposed a location-spectrum iteration approach based on the Bayesian inference, which could alleviate the problems caused by the spectral difference between the burst and location templates. Our method is very suitable for scenarios with limited computation resources or time-sensitive applications, such as in-flight localization software, and low-latency localization for rapidly follow-up observations.
用于全天空伽马射线监测的高能瞬变定位方法
对高能瞬变进行快速可靠的定位,对于描述爆发特性和指导后续观测至关重要。基于不同探测器相对计数的定位方法已被广泛用于全天空伽马射线监测。这种计数分布定位有两种主要方法:χ2最小化法和贝叶斯法。在这里,我们提出了一种改进的贝叶斯方法,它既能利用贝叶斯方法的精确性,又能利用χ2方法的简便性。通过综合模拟,我们发现我们的泊松似然贝叶斯方法比 χ2 方法更适用于各种突发,尤其是弱突发。我们进一步提出了一种基于贝叶斯推理的位置-频谱迭代方法,它可以缓解突发和位置模板之间的频谱差异所带来的问题。我们的方法非常适合计算资源有限或时间敏感的应用场景,如飞行定位软件和快速跟踪观测的低延迟定位。
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来源期刊
Research in Astronomy and Astrophysics
Research in Astronomy and Astrophysics 地学天文-天文与天体物理
CiteScore
3.20
自引率
16.70%
发文量
2599
审稿时长
6.0 months
期刊介绍: Research in Astronomy and Astrophysics (RAA) is an international journal publishing original research papers and reviews across all branches of astronomy and astrophysics, with a particular interest in the following topics: -large-scale structure of universe formation and evolution of galaxies- high-energy and cataclysmic processes in astrophysics- formation and evolution of stars- astrogeodynamics- solar magnetic activity and heliogeospace environments- dynamics of celestial bodies in the solar system and artificial bodies- space observation and exploration- new astronomical techniques and methods
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