activity
20172021
most citedNo pulsed radio emission during a bursting phase of a Galactic magnetar

140 citations · 389 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2021

Energy and waiting time distributions of FRB 121102 observed by FAST

G. Q. Zhang, P. Wang, Q. Wu +4

The energy and waiting time distributions are important properties for understanding the physical mechanism of repeating fast radio bursts (FRBs). Recently, the Five-hundred-meter…

astro-ph.HE2021★ 14 cited

Possible periodic activity in the short bursts of SGR 1806-20: connection to fast radio bursts

G. Q. Zhang, Zuo-Lin Tu, F. Y. Wang

Magnetars are highly magnetized neutron stars that are characterized by recurrent emission of short-duration bursts in soft gamma-rays/hard X-rays. Recently, FRB 200428 were found…

astro-ph.CO2020★ 78 cited

Intergalactic medium dispersion measures of fast radio bursts estimated from IllustrisTNG simulation and their cosmological applications

Z. J. Zhang, K. Yan, C. M. Li +2

Fast radio bursts (FRBs) are millisecond-duration radio transients and can be used as a cosmological probe. However, the dispersion measure (DM) contributed by intergalactic medium…

astro-ph.HE2020★ 29 cited

Dispersion and Rotation Measures from the Ejecta of Compact Binary Mergers: Clue to the Progenitors of Fast Radio Bursts

Z. Y. Zhao, G. Q. Zhang, Y. Y. Wang +2

Since the discovery of FRB 200428 associated with the Galactic SGR 1935+2154, magnetars are considered to power fast radio bursts (FRBs). It is widely believed that magnetars could…

astro-ph.HE2020

Understanding FRB 200428 in the synchrotron maser shock model: consistency and possible challenge

Q. Wu, G. Q. Zhang, F. Y. Wang +1

Recently, the discovery of Galactic FRB 200428 associated with a X-ray burst (XRB) of SGR 1935+2154 has built a bridge between FRBs and magnetar activities. In this paper, we assum…

astro-ph.HE2020★ 4 cited

Dispersion measures of fast radio burst host galaxies derived from IllustrisTNG simulation

G. Q. Zhang, Hai Yu, J. H. He +1

We calculate the dispersion measures (DMs) contributed by host galaxies of fast radio bursts (FRBs). Based on a few host galaxy observations, a large sample of galaxy with similar…

astro-ph.HE2020★ 140 cited

No pulsed radio emission during a bursting phase of a Galactic magnetar

L. Lin, C. F. Zhang, P. Wang +45

Fast radio bursts (FRBs) are mysterious millisecond-duration radio transients of unknown origin observed at extragalactic distances. It has been long speculated that magnetars are…

astro-ph.HE2020★ 14 cited

The rarity of repeating fast radio bursts from binary neutron star mergers

G. Q. Zhang, S. X. Yi, F. Y. Wang

Fast radio bursts (FRBs) are extragalactic, bright pulses of emission at radio frequency with milliseconds duration. Observationally, FRBs can be divided into two classes, repeatin…

astro-ph.HE2019★ 5 cited

Consequences of Energetic Magnetar-Like Outbursts of Nearby Neutron Stars: C Events and the Cosmic Electron Spectrum

F. Y. Wang, Xinyu Li, D. O. Chernyshov +3

Four significant events of rapid C increase have taken place within the past several thousand years. The physical origin of these rapid increases is still a mystery but must…

astro-ph.HE2019★ 23 cited

Energy function, formation rate and low-metallicity environment of fast radio bursts

G. Q. Zhang, F. Y. Wang

In this paper, we investigate the energy function, formation rate and environment of fast radio bursts (FRBs) using Parkes sample and Australian Square Kilometer Array Pathfinder (…

astro-ph.HE2019★ 24 cited

Galactic and cosmological fast radio bursts as scaled-up solar radio bursts

F. Y. Wang, G. Q. Zhang, Z. G. Dai

Fast radio bursts (FRBs) are bright milliseconds radio transients with large dispersion measures. Recently, FRB 200428 was detected in temporal coincidence with a hard X-ray flare…

astro-ph.HE2017★ 58 cited

The formation rate of short gamma-ray bursts and gravitational waves

G. Q. Zhang, F. Y. Wang

In this paper, we study the luminosity function and formation rate of short gamma-ray bursts (sGRBs). Firstly, we derive the correlation using 16 sGRBs with redshift meas…