A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism
Weiwei Zhu(Zhejiang Lab), Yongkun Zhang(Chinese Academy of Sciences), Youling Yue(Chinese Academy of Sciences), C. Kouveliotou(George Washington University), Mingyu Ge(Chinese Academy of Sciences), Jiarui Niu(Chinese Academy of Sciences), Yuan-Pei Yang(Yunnan University), Kejia Lee(Chinese Academy of Sciences), Renxin Xu(Peking University), Cheng-Kui Li(University of Science and Technology of China), Shuang‐Nan Zhang(Netherlands Institute for Radio Astronomy), Xing Guan(Chinese Academy of Sciences), Mao Yuan(Chinese Academy of Sciences), Yi Feng(Chinese Academy of Sciences), D. J. Zhou(Chinese Academy of Sciences), Heng Xu(Beijing Institute of Technology), Weiyang Wang(Chinese Academy of Sciences), Yunpeng Men(Max Planck Institute for Radio Astronomy), Ersin Göğüş(Sabancı Üniversitesi), Mengyao Xue(Curtin University), Lingqi Meng(Chinese Academy of Sciences), Jinchen Jiang(Chinese Academy of Sciences), Wenfei Yu(Shanghai Astronomical Observatory), Bojun Wang(Chinese Academy of Sciences), Lin Lın(National Center for Chronic and Noncommunicable Disease Control and Prevention), Bing Zhang(University of Nevada, Las Vegas), Di Li(Physical Research Laboratory), Pei Wang(Chinese Academy of Sciences), Chunfeng Zhang(Peking University), Peng Jiang(George Washington University), Zhengli Wang(Guangxi University), Jiangwei Xu(Chinese Academy of Sciences), Yutong Chen(Dalian Ocean University), Chenchen Miao(Chinese Academy of Sciences), J. L. Han(Chinese Academy of Sciences), Chenghui Niu(Chinese Academy of Sciences), Xueli Miao(Chinese Academy of Sciences)
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