activity
20192021
most citedPSR J1926-0652: A Pulsar with Interesting Emission Properties Discovered at FAST

45 citations · 127 across the 7 of their papers we have counts for

collaborators

10 papers

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.HE2021

Revisiting Pulsar Velocities Using Gaia Data Release 2

Meng Yang, Shi Dai, Di Li +3

Precise measurements of neutron star (NS) velocities provide critical clues to the supernova physics and evolution of binary systems. Based on Gaia Data Release 2 (DR2), we selecte…

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.HE2020

On the Circular Polarisation of Repeating Fast Radio Bursts

Shi Dai, Jiguang Lu, Chen Wang +9

Fast spinning (e.g., sub-second) neutron star with ultra-strong magnetic fields (or so-called magnetar) is one of the promising origins of repeating fast radio bursts (FRBs). Here…

astro-ph.HE2020

The two emission states of PSR B1534+12

S. Q. Wang, G. Hobbs, J. B. Wang +10

We have observed PSR~B1534+12 (J1537+1155), a pulsar with a neutron star companion, using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). We found that this pulsa…

astro-ph.IM202011 cited

Applying saliency-map analysis in searches for pulsars and fast radio bursts

C. Zhang, C. Wang, G. Hobbs +9

To investigate the use of saliency-map analysis to aid in searches for transient signals, such as fast radio bursts and individual pulses from radio pulsars. We aim to demonstrate…