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Abstract
This paper reports the detection and localization of the repeating fast radio burst (FRB) 20190520B, which is co-located with a compact, persistent radio source and associated with a dwarf host galaxy. The high host-galaxy dispersion measure suggests caution in inferring FRB redshifts without accurate host-galaxy identifications. The FRB exhibits a high burst rate and complex frequency-time intensity structure. Its properties are compared to other repeating FRBs, particularly FRB 20121102A.
Publisher
Nature
Published On
Jun 30, 2022
Authors
C.-H. Niu, K. Aggarwal, D. Li, X. Zhang, S. Chatterjee, C.-W. Tsai, W. Yu, C. J. Law, S. Burke-Spolaor, J. M. Cordes, Y.-K. Zhang, S. K. Ocker, J.-M. Yao, P. Wang, Y. Feng, Y. Niino, C. Bochenek, M. Cruces, L. Connor, J.-A. Jiang, S. Dai, R. Luo, G.-D. Li, C.-C. Miao, J.-R. Niu, R. Anna-Thomas, J. Sydnor, D. Stern, W.-Y. Wang, M. Yuan, Y.-L. Yue, D.-J. Zhou, Z. Yan, W.-W. Zhu, B. Zhang
Tags
fast radio burst
FRB 20190520B
localization
host galaxy
dispersion measure
persistence
radio source
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