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A Possible Periodic Rotation Measure Evolution in the Repeating FRB 20220529

  • Authors: Yi-Fang Liang, Ye Li, Zhen-Fan Tang, Xuan Yang, Song-Bo Zhang, Yuan-Pei Yang, Fa-Yin Wang, Bao Wang, Di Xiao, Qing Zhao, Jun-Jie Wei, Jin-Jun Geng, Jia-Rui Niu, Jun-Shuo Zhang, Guo Chen, Min Fang, Xue-Feng Wu, Zi-Gao Dai, Wei-Wei Zhu, Peng Jiang, Bing Zhang

Yi-Fang Liang et al 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure 1.

Temporal evolution of RM, DM, and burst rate in FRB 20220529. (A) FRB daily burst rate. Grey vertical dashed lines indicate observation days (bursts detected and undetected). The y-axis of the plot is logarithmic. (B) DM of bursts. The blue points represent the detected DM values with their uncertainties. (C) RM of bursts. The filled blue region delineates the RM variation range excluding the RM flare epoch, with the y-axis range scaled to compress the RM flare region and enhance the visibility of the primary dataset. The red points correspond to the daily-binned RM values. The orange lines mark the phases corresponding to the peak of the 200 day period, approximately at phase 0.25.

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