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Fast radio bursts (FRBs) are millisecond-timescale bursts of coherent radio emission that are luminous enough to be detectable at cosmological distances.
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2015
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2016
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D. J. Champion, et al. , Five new fast radio bursts from the HTRU high-latitude survey at Parkes: first evidence for two-component bursts. Mon. Not. R. Astron. Soc. 460
2016
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V. Ravi, et al. , The magnetic field and turbulence of the cosmic web measured using a brilliant fast radio burst. Science 354
2016
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L. G. Spitler, et al. , A repeating fast radio burst. Nature 531
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2020
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2020
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2021
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2021
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2021
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2022
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2022
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2022
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2022
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2041
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S. P. Tendulkar, et al. , The Host Galaxy and Redshift of the Repeating Fast Radio Burst FRB 121102. Astrophys. J. Lett. 834
2041
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B. Marcote, et al. , The Repeating Fast Radio Burst FRB 121102 as Seen on Milliarcsecond Angular Scales. Astrophys. J. Lett. 834
2041
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K. Gourdji, et al. , A Sample of Low-energy Bursts from FRB 121102. Astrophys. J. Lett. 877
2041
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G. H. Hilmarsson, et al. , Rotation Measure Evolution of the Repeating Fast Radio Burst Source FRB 121102. Astrophys. J. Lett. 908
2041
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H. Cho, et al. , Spectropolarimetric Analysis of FRB 181112 at Microsecond Resolution: Implications for Fast Radio Burst Emission Mechanism. Astrophys. J. Lett. 891
2041
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CHIME/FRB Collaboration, et al. , CHIME/FRB Discovery of Eight New Repeating Fast Radio Burst Sources. Astrophys. J. Lett. 885
2041
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E. Fonseca, et al. , Nine New Repeating Fast Radio Burst Sources from CHIME/FRB. Astrophys. J. Lett. 891
2041
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M. Lyutikov, M. V. Barkov, D. Giannios, FRB Periodicity: Mild Pulsars in Tight O/B-star Binaries. Astrophys. J. Lett. 893
2041
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Z. Pleunis, et al. , LOFAR Detection of 110-188 MHz Emission and Frequency-dependent Activity from FRB 20180916B. Astrophys. J. Lett. 911
2041
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B. Zhang, A “Cosmic Comb” Model of Fast Radio Bursts. Astrophys. J. Lett. 836
2041
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B. Margalit, B. D. Metzger, A Concordance Picture of FRB 121102 as a Flaring Magnetar Embedded in a Magnetized Ion-Electron Wind Nebula. Astrophys. J. Lett. 868
2041
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W. Zhu, et al. , A Fast Radio Burst Discovered in FAST Drift Scan Survey. Astrophys. J. Lett. 895
2041
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