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
{"title":"用于全天空伽马射线监测的高能瞬变定位方法","authors":"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","doi":"10.1088/1674-4527/ad683b","DOIUrl":null,"url":null,"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: <italic toggle=\"yes\">χ</italic>\n<sup>2</sup> 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 <italic toggle=\"yes\">χ</italic>\n<sup>2</sup> method. With comprehensive simulations, we find that our Bayesian method with Poisson likelihood is generally more applicable for various bursts than the <italic toggle=\"yes\">χ</italic>\n<sup>2</sup> 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.","PeriodicalId":54494,"journal":{"name":"Research in Astronomy and Astrophysics","volume":"162 1","pages":""},"PeriodicalIF":1.8000,"publicationDate":"2024-09-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A Localization Method of High Energy Transients for All-sky Gamma-ray Monitor\",\"authors\":\"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\",\"doi\":\"10.1088/1674-4527/ad683b\",\"DOIUrl\":null,\"url\":null,\"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: <italic toggle=\\\"yes\\\">χ</italic>\\n<sup>2</sup> 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 <italic toggle=\\\"yes\\\">χ</italic>\\n<sup>2</sup> method. With comprehensive simulations, we find that our Bayesian method with Poisson likelihood is generally more applicable for various bursts than the <italic toggle=\\\"yes\\\">χ</italic>\\n<sup>2</sup> 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.\",\"PeriodicalId\":54494,\"journal\":{\"name\":\"Research in Astronomy and Astrophysics\",\"volume\":\"162 1\",\"pages\":\"\"},\"PeriodicalIF\":1.8000,\"publicationDate\":\"2024-09-03\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Research in Astronomy and Astrophysics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1088/1674-4527/ad683b\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research in Astronomy and Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1088/1674-4527/ad683b","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
A Localization Method of High Energy Transients for All-sky Gamma-ray Monitor
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: χ2 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 χ2 method. With comprehensive simulations, we find that our Bayesian method with Poisson likelihood is generally more applicable for various bursts than the χ2 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.
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