activity
20072026
most citedNo pulsed radio emission during a bursting phase of a Galactic magnetar

140 citations · 330 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

7 papers · 1 filter

astro-ph.HE2026

Mass measurements of the double neutron star system PSR J0641+0448

Z. L. Yang, J. L. Han, P. F. Wang +8

Pulsar timing of double neutron star (DNS) systems is one of the best methodologies to study the neutron star masses distribution. Here we report the discovery of a double neutron…

astro-ph.HE2023★ 9 cited

The FAST Galactic Plane Pulsar Snapshot survey: IV. Discovery of five fast radio bursts

D. J. Zhou, J. L. Han, W. C. Jing +8

We report five new fast radio bursts (FRBs) discovered from the Galactic Plane Pulsar Snapshot (GPPS) survey by the Five-hundred-meter Aperture Spherical radio Telescope (FAST): FR…

astro-ph.HE2023★ 14 cited

Distance of PSR B0458+46 indicated by FAST HI absorption observations

W. C. Jing, J. L. Han, Tao Hong +6

The pulsar B0458+46 was previously believed to have a distance of about 1.3kpc and to be associated with a nearby supernova remnant, SNR HB9 (G160.9+2.6). We observe the neutral…

astro-ph.HE2023★ 22 cited

Strong and weak pulsar radio emission due to thunderstorms and raindrops of particles in the magnetosphere

X. Chen, Y. Yan, J. L. Han +14

Pulsars radiate radio signals when they rotate. However, some old pulsars often stop radiating for some periods. The underlying mechanism remains unknown, while the magnetosphere d…

astro-ph.HE2021★ 12 cited

Fast radio burst detection in the presence of coloured noise

C. F. Zhang, J. W. Xu, Y. P. Men +17

In this paper, we investigate the impact of correlated noise on fast radio burst (FRB) searching. We found that 1) the correlated noise significantly increases the false alarm prob…

astro-ph.HE2020★ 43 cited

Jiamusi pulsar observations: III. Nulling of 20 pulsars

P. F. Wang, J. L. Han, L. Han +12

Most of pulsar nulling observations were conducted at frequencies lower than 1400~MHz. We aim to understand the nulling behaviors of pulsars at relatively high frequency, and to ch…