A low-latency pipeline for GRB light curve and spectrum using FermilGBM near real-time data
A low-latency pipeline for GRB light curve and spectrum using FermilGBM near real-time data
复制标题
使用 FermilGBM 近实时数据的 GRB 光变曲线和光谱的低延迟管道
DOI：
10.1088/1674-4527/18/5/57
复制
发表时间：
2018
影响因子：
1.8
通讯作者：
Shao Jian-Xiong
中科院分区：
文献类型：
--
作者：
Zhao Yi;Zhang Bin-Bin;Xiong Shao-Lin;Long Xi;Zhang Qiang;Song Li-Ming;Sun Jian-Chao;Wang Yuan-Hao;Li Han-Cheng;Bu Qing-Cui;Feng Min-Zi;Li Zheng-Heng;Wen Xing;Wu Bo-Bing;Zhang Lai-Yu;Zhang Yong-Jie;Zhang Shuang-Nan;Shao Jian-Xiong
Rapid response and short time latency are very important for Time Domain Astronomy, such as the observations of Gamma-ray Bursts (GRBs) and electromagnetic (EM) counterparts of gravitational waves (GWs). Based on near real-time Fermi/GBM data, we developed a low-latency pipeline to automatically calculate the temporal and spectral properties of GRBs. With this pipeline, some important parameters can be obtained, such as T 90 and fluence, within∼ 20 min after the GRB trigger. For∼ 90% of GRBs, T 90 and fluence are consistent with the GBM catalog results within 2σ errors. This pipeline has been used by the Gamma-ray Bursts Polarimeter (POLAR) and the Insight Hard X-ray Modulation Telescope (Insight-HXMT) to follow up the bursts of interest. For GRB 170817A, the first EM counterpart of GW events detected by Fermi/GBM and INTEGRAL/SPI-ACS, the pipeline gave T 90 and spectral information 21 min after the GBM trigger, providing important information for POLAR and Insight-HXMT observations.
