Atlas of dynamic spectra of fast radio burst FRB 20201124A  

作　　者：王铂钧 胥恒 姜金辰 徐江伟 牛佳瑞 陈平 李柯伽 张冰 朱炜玮 东苏勃 张春风 傅海 周德江 张永坤 王培 冯毅 李晔 李冬子 鲁文宾 杨元培 RNCaballero 蔡策 陈卯蒸 戴子高 艾力·伊沙木丁 甘恒谦 韩金林 郝龙飞 黄玉祥 姜鹏 李承奎 李菂 李辉 李新乔 李志玄 刘志勇 罗睿 门云鹏 牛晨辉 彭文溪 钱磊 宋黎明 孙京海 王发印 汪敏 王娜 王维扬 吴雪峰 肖硕 熊少林 徐永华 徐仁新 杨俊 杨轩 姚蕊 易祁彬 岳友岭 于东俊 余文飞 袁建平 张彬彬 张松波 张双南 赵一 郑伟康 朱岩 邹金航 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;RNCaballero;Ce Cai;Mao-Zheng Chen;Zi-Gao Dai;AEsamdin;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(Kavli Institute for Astronomy and Astrophysics,Peking University,Beijing 100871,China;National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;Department of Astronomy,Peking University,Beijing 100871,China;University of Chinese Academy of Sciences,Chinese Academy of Sciences,Beijing 100049,China;Department of Particle Physics and Astrophysics,Weizmann Institute of Science,Rehovot 76100,Israel;Nevada Center for Astrophysics,University of Nevada,Las Vegas,NV 89154,USA;Department of Physics and Astronomy,University of Nevada,Las Vegas,NV 89154,USA;Department of Physics&Astronomy,University of Iowa,Iowa City,IA 52242,USA;Zhejiang Laboratory,Hangzhou,Zhejiang 311121,China;Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China;TAPIR,Walter Burke Institute for Theoretical Physics,Mail Code 350-17,Caltech,Pasadena,CA 91125,USA;Department of Astronomy,University of California at Berkeley,Berkeley,CA 94720,USA;South-Western Institute For Astronomy Research,Yunnan University,Yunnan 650504,China;Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China;Xinjiang Astronomical Observatory,Chinese Academy of Sciences,Urumqi 830011,China;University of Science and

机构地区：[1]Kavli Institute for Astronomy and Astrophysics,Peking University,Beijing 100871,China [2]National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China [3]Department of Astronomy,Peking University,Beijing 100871,China [4]University of Chinese Academy of Sciences,Chinese Academy of Sciences,Beijing 100049,China [5]Department of Particle Physics and Astrophysics,Weizmann Institute of Science,Rehovot 76100,Israel [6]Nevada Center for Astrophysics,University of Nevada,Las Vegas,NV 89154,USA [7]Department of Physics and Astronomy,University of Nevada,Las Vegas,NV 89154,USA [8]Department of Physics&Astronomy,University of Iowa,Iowa City,IA 52242,USA [9]Zhejiang Laboratory,Hangzhou,Zhejiang 311121,China [10]Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China [11]TAPIR,Walter Burke Institute for Theoretical Physics,Mail Code 350-17,Caltech,Pasadena,CA 91125,USA [12]Department of Astronomy,University of California at Berkeley,Berkeley,CA 94720,USA [13]South-Western Institute For Astronomy Research,Yunnan University,Yunnan 650504,China [14]Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China [15]Xinjiang Astronomical Observatory,Chinese Academy of Sciences,Urumqi 830011,China [16]University of Science and Technology of China,Anhui 230026,China [17]Yunnan Observatories,Chinese Academy of Sciences,Kunming 650216,China [18]Guizhou Normal University,Guiyang 550001,China [19]CSIRO Space and Astronomy,Epping,NSW 1710,Australia [20]Max-Planck institut fur Radioastronomie,Auf Dem Hugel,Bonn,53121,Germany [21]School of Astronomy and Space Science,Nanjing University,Nanjing 210093,China [22]State Key Laboratory of Nuclear Physics and Technology,School of Physics,Peking University,Beijing 100871,China [23]Shanghai Astronomical Observatory,Chinese Academy of Sciences,Shanghai 200030,China [24]Key Laboratory of Modern Astronomy and Astrophysics(Nanjing University),Ministry of Education,Nanjing 210093,China [25]College

出　　处：《Chinese Physics B》2023年第2期1-4,共4页中国物理B（英文版）

基　　金：supported by the National SKA Program of China (Grant Nos. 2020SKA0120100 and 2020SKA0120200);the National Natural Science Foundation of China (Grant Nos. 12041304, 11873067, 11988101, 12041303, 11725313, 11725314, 11833003, 12003028, 12041306, 12103089, U2031209, U2038105, and U1831207);the National Key Research and Development Program of China (Grant Nos. 2019YFA0405100, 2017YFA0402602, 2018YFA0404204, and 2016YFA0400801);Key Research Program of the Chinese Academy of Sciences (Grant No. QYZDJ-SSW-SLH021);Natural Science Foundation of Jiangsu Province (Grant No. BK20211000);Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS, the Strategic Priority Research Program on Space Science, the Western Light Youth Project of Chinese Academy of Sciences (Grant Nos. XDA15360000, XDA15052700, and XDB23040400);funding from the MaxPlanck Partner Group, the science research grants from the China Manned Space Project (Grant Nos. CMS-CSST2021-B11 and CMS-CSST-2021-A11);PKU development (Grant No. 7101502590);support from the XPLORER PRIZE;supported by Fundamental Research Funds for the Central Universities (Grant No. 14380046);the Program for Innovative Talents, Entrepreneur in Jiangsu。

摘　　要：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.

关 键 词：fast radio burst FAST 

分 类 号：P16[天文地球—天文学]