20200120E

 

This figure shows normalised dirty images of individual bursts (a-c) and of their combinations (d-e); panel (f) shows the resulting localisation as derived from the combined data sets with respect to the optical Subaru image of the region (from Kirsten et al. https://arxiv.org/abs/2105.11445).

We published two papers on the localisation and the origin of the repeating FRB 20200120E. Please check the following works:

  1. A repeating fast radio burst source in a globular cluster, Kirsten et al. 2022, Nature (arxiv, ads, journal)

  2. Burst timescales and luminosities link young pulsars and fast radio bursts, Nimmo et al. 2022, Nature Astronomy 6, 393 (arxiv, ads, journal)