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Structure Functions of Rotation Measures Revealing the Origin of Fast Radio Bursts
Published 2025-01-01“…Here, we report that the SFs of the binary PSR B1744–24A and the repeating fast radio burst (FRB) 20201124A exhibit both a periodic geometric component, caused by binary orbital motion, and a flat statistical component. …”
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A Universal Break in Energy Functions of Three Hyperactive Repeating Fast Radio Bursts
Published 2025-01-01“…Fast radio bursts (FRBs) are millisecond-duration pulses occurring at cosmological distances with a mysterious origin. …”
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Morphology of 137 Fast Radio Bursts Down to Microsecond Timescales from the First CHIME/FRB Baseband Catalog
Published 2025-01-01“…We present a spectro-temporal analysis of 137 fast radio bursts (FRBs) from the first CHIME/FRB baseband catalog, including 125 one-off bursts and 12 repeat bursts, down to microsecond resolution using the least-squares optimization fitting routine fitburst . …”
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3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
Published 2025-01-01“…Fast radio bursts (FRBs) are high-energy, short-duration phenomena in radio astronomy. …”
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Intrinsic Pulse Widths of FRB 20121102A and Calculation of Broadening from Propagation and Instrumental Effects
Published 2025-01-01“…The pulse widths of fast radio bursts are always broadened due to the scattering of the plasma medium through which the electromagnetic wave passes. …”
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The Timing and Spectral Properties of the 2022 Outburst of SGR J1935+2154 Observed with NICER
Published 2025-01-01“…While a flare is evident on the light curve, a fast radio burst (FRB) was detected immediately following the peak of this flare. …”
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A New X-Ray and Radio Burst Activity from the Magnetar SGR 1935+2154
Published 2025-01-01“…SGR 1935+2154 has emerged as the most active magnetar in recent years, exhibiting X-ray burst activity nearly annually and emitting a fast radio burst (FRB 200428 (FRB1)) in its 2020 April activity, for the first time from a Milky Way source, accompanied by an X-ray burst (X _FRB1 ). …”
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