activity
20032023
most citedA bright millisecond-duration radio burst from a Galactic magnetar

745 citations · 3k across the 30 of their papers we have counts for

collaborators
Showing 2021Show all

9 papers · 1 filter

astro-ph.HE2021★ 22 cited

Unusual Emission Variations Near the Eclipse of A Black Widow PSR J17200533

S. Q. Wang, J. B. Wang, N. Wang +15

We report on an {unusually} bright observation of PSR J17200533 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The pulsar is in a black widow system tha…

astro-ph.HE2021★ 19 cited

Long and Short Fast Radio Bursts are Different from Repeating and Non-repeating Transients

X. J. Li, X. F. Dong, Z. B. Zhang +1

We collect 133 Fast Radio Bursts (FRBs), including 110 non-repeating and 23 repeating ones, and systematically investigate their observational properties. To check the frequency de…

astro-ph.HE2021★ 298 cited

A repeating fast radio burst associated with a persistent radio source

C. -H. Niu, K. Aggarwal, D. Li +32

The dispersive sweep of fast radio bursts (FRBs) has been used to probe the ionized baryon content of the intergalactic medium, which is assumed to dominate the total extragalactic…

astro-ph.SR2021★ 145 cited

Kink oscillations of coronal loops

V. M. Nakariakov, S. A. Anfinogentov, P. Antolin +13

Kink oscillations of coronal loops, i.e., standing kink waves, is one of the most studied dynamic phenomena in the solar corona. The oscillations are excited by impulsive energy re…

astro-ph.HE2021★ 14 cited

A broadband radio study of PSR J0250+5854: the slowest-spinning radio pulsar known

C. H. Agar, P. Weltevrede, L. Bondonneau +19

We present radio observations of the most slowly rotating known radio pulsar PSR J0250+5854. With a 23.5 s period, it is close, or even beyond, the - diagram region tho…

astro-ph.HE2021★ 75 cited

Polarization properties of FRB 20201124A from detections with the 100-m Effelsberg Radio Telescope

G. H. Hilmarsson, L. G. Spitler, R. A. Main +1

The repeating FRB source, FRB 20201124A, was found to be highly active in March and April 2021. We observed the source with the Effelsberg 100-m radio telescope at 1.36 GHz on 9 Ap…