Year: 2022
Type: article
Abstract: Fast radio bursts (FRBs) are highly dispersed millisecond-duration radio bursts,[1,2] of which the physical origin is still not fully understood. FRB 20201124A is one of the most actively repeating FRBs. In this paper, we present the collection of 1863 burst dynamic spectra of FRB 20201124A measured with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The current collection, taken from the observation during the FRB active phase from April to June 2021, is the largest burst sample detected for any FRB so far. The standard PSRFITs format is adopted, including dynamic spectra of the burst, and the time information of the dynamic spectra, in addition, mask files help readers to identify the pulse positions are also provided. The dataset is available in Science Data Bank, with the link https://www.doi.org/10.57760/sciencedb.j00113.00076 .
Source: Chinese Physics B
Authors: Bo-Jun Wang, Heng Xu, Jin-Chen Jiang, Jiang-Wei Xu, Jia-Rui Niu, Ping Chen, Ke-Jia Lee, Bing Zhang, Wei-Wei Zhu, Su-Bo Dong, Chun-Feng Zhang, Hai Fu, De-Jiang Zhou, Yong-Kun Zhang, Pei Wang, Yi Feng, Ye Li, Dong-Zi Li, Wen-Bin Lu, Yuan-Pei Yang, R. N. Caballero, Ce Cai, Mao-Zheng Chen, Zi-Gao Dai, A. Esamdin, Heng-Qian Gan, Jin-Lin Han, Long-Fei Hao, Yu-Xiang Huang, Peng Jiang, Cheng-Kui Li, Di Li, Hui Li, Xin-Qiao Li, Zhi-Xuan Li, Zhi-Yong Liu, Rui Luo, Yun-Peng Men, Chen-Hui Niu, Wen-Xi Peng, Lei Qian, Li-Ming Song, Jing-Hai Sun, Fa-Yin Wang, Min Wang, Na Wang, Wei-Yang Wang, Xue-Feng Wu, Shuo Xiao, Shao-Lin Xiong, Yong-Hua Xu, Ren-Xin Xu, Jun Yang, Xuan Yang, Rui Yao, Qi-Bin Yi, You-Ling Yue, Dong-Jun Yu, Wen-Fei Yu, Jian-Ping Yuan, Bin-Bin Zhang, Song-Bo Zhang, Shuang-Nan Zhang, Yi Zhao, Wei-Kang Zheng, Yan Zhu, Jin-Hang Zou
Institutions: Chinese Academy of Sciences, Peking University, National Astronomical Observatories, University of Chinese Academy of Sciences, Weizmann Institute of Science, University of Nevada, Las Vegas, Nanjing University, University of Iowa, Zhejiang Lab, Purple Mountain Observatory, California Institute of Technology, Guizhou Normal University, University of California, Berkeley, Yunnan University, Institute of High Energy Physics, Xinjiang Astronomical Observatory, University of Science and Technology of China, Yunnan Observatories, Commonwealth Scientific and Industrial Research Organisation, Max Planck Institute for Radio Astronomy, State Key Laboratory of Nuclear Physics and Technology, Shanghai Astronomical Observatory, Hebei Normal University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Awards: G1178317537, G1192735915, G1438537086, 天体高能爆发的物理机制和地球环境, G1986983526, G208852609, G2393958023, G2424786454, G2500546165, G270816197, G3344751404, G3519253691, G3635049790, G3950889893, G433490822, G4516183393, G4559515314, G5557302724, G5579061841, G5636501495, G5665470415, G5753704908, G6248463922, G7465896656, G7619885634, G7724300976, G8128137341, 短伽玛射线暴及其天体物理问题研究, G859119811, G8892125080
OpenAlex ID: W4311116302