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. 2022 Jun 8;606(7916):873–877. doi: 10.1038/s41586-022-04755-5

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© The Author(s) 2022, corrected publication 2022

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

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Extended Data Fig. 1 — The observation were performed at 1.5, 3, and 5.5 GHz. They were shown as offsets from the best-fit position of the ensemble of bursts, at RA = 16h02m04.272s, dec. = −11° 17′ 17.32″ (J2000). The uncertainties on the positions of the bursts are indicated with shaded ellipses, and those for the PRS are shown with error bars. These uncertainties include 1σ statistical errors and estimates for systematic errors added in quadrature.