_version_ 1866915183011561472
author Cai, Ce
Zhang, Yan-Qiu
Xiong, Shao-Lin
Wang, Ping
Li, Jian-Hui
Li, Xiao-Bo
Li, Cheng-Kui
Huang, Yue
Zheng, Shi-Jie
Song, Li-Ming
Xiao, Shuo
Yi, Qi-Bin
Zhao, Yi
Xie, Sheng-Lun
Qiao, Rui
Du, Yan-Qi
Guo, Zhi-Wei
Xue, Wang-Chen
Zheng, Chao
Liu, Jia-Cong
Wang, Chen-Wei
Tan, Wen-Jun
Wang, Yue
Zhang, Jin-Peng
Li, Chao-Yang
Zhao, Guo-Ying
Zhao, Xiao-Yun
Zhang, Xiao-Lu
Zhang, Zhen
Peng, Wen-Xi
Ma, Xiang
Shi, Jing-Yan
Guo, Dong-Ya
Wang, Jin
Li, Xin-Qiao
Wen, Xiang-Yang
An, Zheng-Hua
Zhang, Fan
author_facet Cai, Ce
Zhang, Yan-Qiu
Xiong, Shao-Lin
Wang, Ping
Li, Jian-Hui
Li, Xiao-Bo
Li, Cheng-Kui
Huang, Yue
Zheng, Shi-Jie
Song, Li-Ming
Xiao, Shuo
Yi, Qi-Bin
Zhao, Yi
Xie, Sheng-Lun
Qiao, Rui
Du, Yan-Qi
Guo, Zhi-Wei
Xue, Wang-Chen
Zheng, Chao
Liu, Jia-Cong
Wang, Chen-Wei
Tan, Wen-Jun
Wang, Yue
Zhang, Jin-Peng
Li, Chao-Yang
Zhao, Guo-Ying
Zhao, Xiao-Yun
Zhang, Xiao-Lu
Zhang, Zhen
Peng, Wen-Xi
Ma, Xiang
Shi, Jing-Yan
Guo, Dong-Ya
Wang, Jin
Li, Xin-Qiao
Wen, Xiang-Yang
An, Zheng-Hua
Zhang, Fan
contents 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 1.1E-08 erg cm-2 s-1 (10 keV - 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.
format Preprint
id arxiv_https___arxiv_org_abs_2503_03161
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The GECAM Ground Search System for Gamma-ray Transients
Cai, Ce
Zhang, Yan-Qiu
Xiong, Shao-Lin
Wang, Ping
Li, Jian-Hui
Li, Xiao-Bo
Li, Cheng-Kui
Huang, Yue
Zheng, Shi-Jie
Song, Li-Ming
Xiao, Shuo
Yi, Qi-Bin
Zhao, Yi
Xie, Sheng-Lun
Qiao, Rui
Du, Yan-Qi
Guo, Zhi-Wei
Xue, Wang-Chen
Zheng, Chao
Liu, Jia-Cong
Wang, Chen-Wei
Tan, Wen-Jun
Wang, Yue
Zhang, Jin-Peng
Li, Chao-Yang
Zhao, Guo-Ying
Zhao, Xiao-Yun
Zhang, Xiao-Lu
Zhang, Zhen
Peng, Wen-Xi
Ma, Xiang
Shi, Jing-Yan
Guo, Dong-Ya
Wang, Jin
Li, Xin-Qiao
Wen, Xiang-Yang
An, Zheng-Hua
Zhang, Fan
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
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 1.1E-08 erg cm-2 s-1 (10 keV - 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.
title The GECAM Ground Search System for Gamma-ray Transients
topic High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2503.03161