Overview of Ground-based Wide-Angle Cameras array
Abstract
As one of the key ground-based facilities of the Chinese-French SVOM mission, the main scientific objectives of the Ground-based Wide Angle Camera array (GWAC) are to detect prompt optical emission of gamma-ray bursts or other short duration astronomical transients on a second-scale temporal resolution. GWAC is located at Xinglong observatory, China, and consists of 10 mounts and 40 cameras, providing a joint field of view of about 3600 square degrees.The detection ability is 16 magnitude in 10 seconds of exposure time in the visual band under the condition of the new moon phase. Here, we give an overview of GWAC and introduce the science motivation of the project, as well as the performance of the hardware and the software. The observation strategies and the data processing are briefly presented. The early sciences in the last 5 years since the first light are summarized.
Keywords
Cite
@article{arxiv.2604.24260,
title = {Overview of Ground-based Wide-Angle Cameras array},
author = {Liping Xin and Lei Huang and Hongbo Cai and Xuhui Han and Yang Xu and Xiaomeng Lu and Huali Li and Jing Wang and Yulei Qiu and Chao Wu and Ruosong Zhang and Pinpin Zhang and Yujie Xiao and Guangwei Li and Jingsong Deng and Dawei Xu and Linjun Wang and Jinran Xu and Yinuo Ma and Yangtong Zheng and Wenlong Dong and Zhuheng Yao and Enwei Liang and Xianggao Wang and Xiangyu Wang and Zigao Dai and Yuangui Yang and Jianyan Wei},
journal= {arXiv preprint arXiv:2604.24260},
year = {2026}
}
Comments
Accepted fro publication in the SVOM special issue in Research in Astronomy and Astrophysics; 14 pages, 11 figures