A Localization Method of High Energy Transients for All-sky Gamma-ray Monitor
/ Authors
Yi Zhao, W. Xue, Shaolin Xiong, Qiumin Luo, Yuanhao Wang, Jia-Cong Liu, Heng Yu, Xiao-Yun Zhao, Yue Huang, Jin-yuan Liao
and 55 more authors
Jianchao Sun, Xiaobo Li, Q. Yi, C. Cai, S. Xiao, Sheng Q. Xie, C. Zheng, Yan-Qiu Zhang, Chenwei Wang, Wen-Hai Tan, Zhiwei Guo, Chaoyang Li, Z. An, Gang Chen, Yanqi Du, M. Gao, K. Gong, D. Guo, Jiang He, Jian-Jian He, Bing Li, Gang Li, Xinqiao Li, J. Liang, Xiaohua Liang, Ya-qing Liu, Xiang Ma, Rui Qiao, Liming Song, Xinying Song, Xilei Sun, Jin Wang, Ping Wang, X. Wen, Hong-jie Wu, Yan-Bing Xu, Sheng Yang, Dali Zhang, Fan Zhang, Hongmei Zhang, P. Zhang, Shu Zhang, Zhen Zhang, Shijie Zheng, Keke Zhang, Xing Han, Haiyan Wu, T. Hu, Haobo Geng, Gao-na Lu, Wei Xu, F. Lyu, Hongbo Zhang, F. Lu, Shuangnan Zhang
/ 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.
Journal: Research in Astronomy and Astrophysics