activity
20172022
most citedA bimodal burst energy distribution of a repeating fast radio burst source

287 citations · 430 across the 8 of their papers we have counts for

collaborators

12 papers

astro-ph.HE202213 cited

Detection of strong scattering close to the eclipse region of PSR B1957+20

J. T. Bai, S. Dai, Q. J. Zhi +14

We present the first measurement of pulse scattering close to the eclipse region of PSR B1957+20, which is in a compact binary system with a low-mass star. We measured pulse scatte…

astro-ph.HE202141 cited

FAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252

Pei Wang, Di Li, Colin J. Clark +23

High sensitivity radio searches of unassociated -ray sources have proven to be an effective way of finding new pulsars. Using the Five-hundred-meter Aperture Spherical radio Tel…

astro-ph.HE2021287 cited

A bimodal burst energy distribution of a repeating fast radio burst source

D. Li, P. Wang, W. W. Zhu +29

The event rate, energy distribution, and time-domain behaviour of repeating fast radio bursts (FRBs) contains essential information regarding their physical nature and central engi…

astro-ph.CO2021

Investigating X-ray sources during the epoch of reionization with the 21 cm signal

Qing-Bo Ma, Benedetta Ciardi, Marius B. Eide +3

Heating of neutral gas by energetic sources is crucial for the prediction of the 21 cm signal during the epoch of reionization (EoR). To investigate differences induced on statisti…

astro-ph.HE20207 cited

Wideband Monitoring Observations of PSR J1803-3002A in the Globular Cluster NGC 6522

Lei Zhang, Richard N. Manchester, Andrew D. Cameron +10

We report the first wideband monitoring observations of PSR J1803-3002A, a relatively bright millisecond pulsar in the globular cluster NGC 6522 with a spin period of 7.1 ms and no…

astro-ph.CO20199 cited

Observing the redshifted 21 cm signal around a bright QSO at

Qing-Bo Ma, Benedetta Ciardi, Koki Kakiichi +3

We use hydrodynamics and radiative transfer simulations to study the 21~cm signal around a bright QSO at . Due to its powerful UV and X-ray radiation, the QSO quickly in…