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19982022
most citedThe radio to X-ray spectrum of GRB 970508 on May 21.0 UT

115 citations · 1k across the 23 of their papers we have counts for

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astro-ph.HE2022★ 16 cited

Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation

Xiang-Han Cui, Cheng-Min Zhang, Di Li +9

Fast radio bursts (FRBs) are extremely strong radio flares lasting several micro- to milliseconds and come from unidentified objects at cosmological distances, most of which are on…

astro-ph.HE2021★ 7 cited

Statistical properties of fast radio bursts elucidate their origins: magnetars are favoured over gamma-ray bursts

Xiang-Han Cui, Cheng-Min Zhang, Shuang-Qiang Wang +11

Fast radio bursts (FRBs) are extremely strong radio flares lasting several milliseconds, most of which come from unidentified objects at a cosmological distance. They can be appare…

astro-ph.HE2020★ 18 cited

Periodic and Phase-locked Modulation in PSR B1929+10 Observed with FAST

F. F. Kou, W. M. Yan, B. Peng +17

We present a detailed single-pulse analysis for PSR B1929+10 based on observations with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The main pulse and interpu…

astro-ph.HE2020★ 29 cited

Fast radio bursts: do repeaters and non-repeaters originate in statistically similar ensembles

Xiang-Han Cui, Cheng-Min Zhang, Shuang-Qiang Wang +9

Fast Radio Bursts (FRBs) are the short, strong radio pulses lasting several milliseconds. They are subsequently identified, for the most part, as emanating from unknown objects at…

astro-ph.HE2014★ 19 cited

Detailed Afterglow Modeling and Host Galaxy Properties of the Dark GRB 111215A

A. J. van der Horst, A. J. Levan, G. G. Pooley +13

Gamma-ray burst (GRB) 111215A was bright at X-ray and radio frequencies, but not detected in the optical or near-infrared (nIR) down to deep limits. We have observed the GRB afterg…

astro-ph.HE2014★ 83 cited

A Comprehensive Radio View of the Extremely Bright Gamma-Ray Burst 130427A

A. J. van der Horst, Z. Paragi, A. G. de Bruyn +11

GRB 130427A was extremely bright as a result of occurring at low redshift whilst the energetics were more typical of high-redshift gamma-ray bursts (GRBs). We collected well-sample…