The GECAM ground search system for gamma-ray transients

IF 6.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY
Ce Cai, Yan-Qiu Zhang, Shao-Lin Xiong, Ping Wang, Jian-Hui Li, Xiao-Bo Li, Cheng-Kui Li, Yue Huang, Shi-Jie Zheng, Li-Ming Song, Shuo Xiao, Qi-Bin Yi, Yi Zhao, Sheng-Lun Xie, Rui Qiao, Yan-Qi Du, Zhi-Wei Guo, Wang-Chen Xue, Chao Zheng, Jia-Cong Liu, Chen-Wei Wang, Wen-Jun Tan, Yue Wang, Jin-Peng Zhang, Chao-Yang Li, Guo-Ying Zhao, Xiao-Yun Zhao, Xiao-Lu Zhang, Zhen Zhang, Wen-Xi Peng, Xiang Ma, Jing-Yan Shi, Dong-Ya Guo, Jin Wang, Xin-Qiao Li, Xiang-Yang Wen, Zheng-Hua An, Fan Zhang
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Abstract

In the era of time-domain, multi-messenger astronomy, the detection of transient events on the high-energy electromagnetic sky has become more important than ever. The gravitational wave high-energy electromagnetic counterpart all-sky monitor (GECAM) is a dedicated mission to monitor gamma-ray transients, launched in December, 2020. A real-time on-board trigger and location software, using the traditional signal-to-noise ratio (SNR) method for blind search, is constrained to relatively bright signals due to the limitations in on-board computing resources and the need for real-time search. In this work, we developed a ground-based pipeline for GECAM to search for various transients, especially for weak bursts missed by on-board software. This pipeline includes both automatic and manual mode, offering options for blind search and targeted search. The targeted search is specifically designed to search for interesting weak bursts, such as gravitational wave-associated gamma-ray bursts (GRBs). From the ground search of the data in the first year, GECAM has been triggered by 54 GRBs and other transients, including soft gamma-ray repeaters, X-ray binaries, solar flares, terrestrial gamma-ray flashes. We report the properties of each type of triggers, such as trigger time and light curves. With this search pipeline and assuming a soft Band spectrum, the GRB detection sensitivity of GECAM is increased to about 1.1 × 10−8 erg cm−2 s−1 (10–1000 keV, burst duration of 20 s). These results demonstrate that the GECAM ground search system (both blind search and targeted search) is a versatile pipeline to recover true astrophysical signals which were too weak to be found in the on-board search.

GECAM伽马射线瞬变地面搜索系统
在时域、多信使天文学时代,探测高能电磁天空中的瞬态事件变得比以往任何时候都更加重要。引力波高能电磁对应物全天监测仪(GECAM)是一项专门监测伽马射线瞬变的任务,于2020年12月发射。实时星载触发与定位软件采用传统的信噪比(SNR)法进行盲搜索,由于星载计算资源的限制和实时搜索的需要,只能选择相对明亮的信号。在这项工作中,我们为GECAM开发了一个地面管道,用于搜索各种瞬态,特别是机载软件遗漏的弱突发。该管道包括自动和手动模式,提供盲搜索和目标搜索选项。目标搜索是专门为寻找有趣的弱爆发而设计的,比如引力波相关的伽马射线爆发(GRBs)。从第一年的地面数据搜索来看,GECAM已经被54次grb和其他瞬变触发,包括软伽马射线中继器、x射线双星、太阳耀斑、地面伽马射线闪光。我们报告了每种类型的触发器的性质,如触发时间和光曲线。GECAM的GRB探测灵敏度提高到1.1 × 10−8 erg cm−2 s−1 (10 - 1000 keV,突发持续时间为20 s)。这表明GECAM地面搜索系统(包括盲搜索和目标搜索)是一种通用的管道,可以恢复在机载搜索中过于微弱而无法发现的真实天体物理信号。
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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来源期刊
Science China Physics, Mechanics & Astronomy
Science China Physics, Mechanics & Astronomy PHYSICS, MULTIDISCIPLINARY-
CiteScore
10.30
自引率
6.20%
发文量
4047
审稿时长
3 months
期刊介绍: Science China Physics, Mechanics & Astronomy, an academic journal cosponsored by the Chinese Academy of Sciences and the National Natural Science Foundation of China, and published by Science China Press, is committed to publishing high-quality, original results in both basic and applied research. Science China Physics, Mechanics & Astronomy, is published in both print and electronic forms. It is indexed by Science Citation Index. Categories of articles: Reviews summarize representative results and achievements in a particular topic or an area, comment on the current state of research, and advise on the research directions. The author’s own opinion and related discussion is requested. Research papers report on important original results in all areas of physics, mechanics and astronomy. Brief reports present short reports in a timely manner of the latest important results.
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