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20232026
most citedTera-Hertz Counterparts to Fast Radio Bursts from Coherent Cherenkov Radiation by Tilted Bunches

1 citations · 2 across the 6 of their papers we have counts for

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astro-ph.HE2026

X-rays breaking out of pre-explosion ejecta mark a supernova's first light

Weimin Yuan, Qiu-Ju Huang, Jin-Ping Zhu +130

Massive stars die as core-collapse supernovae, whose optical light emerges days after the implosion. Theory predicts that the initial collapse-driven shock, upon breaking through t…

astro-ph.HE20261 cited

Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm

Zhengyan Liu, Zelin Xu, Ji-an Jiang +35

The gravitational wave (GW) event S250206dm, as the first well-localized neutron star merger candidate potentially located in the mass gap, presented a unique opportunity to probe…

astro-ph.HE2025

A Deep VLA Search for a Persistent Radio Counterpart to the One-off FRB 20250316A

Tao An, Ailing Wang, Yu-Chen Huang +4

Fast Radio Burst (FRB) 20250316A, detected by CHIME on 2025 March 16 with a fluence of and a dispersion measure of , r…

astro-ph.HE20251 cited

Tera-Hertz Counterparts to Fast Radio Bursts from Coherent Cherenkov Radiation by Tilted Bunches

Ze-Nan Liu, Wei-Yang Wang, Yu-Chen Huang +1

Fast radio bursts (FRBs) are millisecond-duration extragalactic transients characterized by ultrahigh brightness temperatures, suggesting coherent emission mechanisms in extreme as…

astro-ph.HE2025

A universal break in energy functions of three hyperactive repeating fast radio bursts

Q. Wu, F. Y. Wang, Z. Y. Zhao +16

Fast radio bursts (FRBs) are millisecond-duration pulses occurring at cosmological distances with a mysterious origin. Observations show that at least some FRBs are produced by mag…

astro-ph.HE2023

A bright burst from FRB 20200120E in a globular cluster of the nearby galaxy M81

S. B. Zhang, J. S. Wang, X. Yang +9

Fast radio bursts (FRBs) are immensely energetic millisecond-duration radio pulses. Observations indicate that nearby FRBs can be produced by old stellar populations, as suggested…