activity
19982023
most citedAn ultra-wide bandwidth (704 to 4032 MHz) receiver for the Parkes radio telescope

229 citations · 1.2k across the 32 of their papers we have counts for

collaborators

32 papers

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★ 2 cited

Distinct polarization properties for two emission states of four pulsars

Yi Yan, P. F. Wang, J. L. Han

Four pulsars, PSRs J1838+1523, J1901+0510, J1909+0007 and J1929+1844, are found to exhibit bright and weak emission states from sensitive FAST observations. New FAST observations h…

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.GA2023★ 4 cited

More relaxed intracluster gas than galaxies in clusters in quasi-equilibrium

Z. S. Yuan, J. L. Han, H. Böhringer +2

During cluster mergers, the intracluster gas and member galaxies undergo dynamic evolution, but at different timescales and reach different states. We collect 24 galaxy clusters in…

astro-ph.GA2023★ 4 cited

Three New Spiral Galaxies with Active Nuclei Producing Double Radio Lobes

Xuyang Gao, Zhongsheng Yuan, Jinlin Han +2

Double radio lobes are generally believed to be produced by active nuclei of elliptical galaxies. However, several double-lobed radio sources have been solidly found to be associat…

astro-ph.HE2023★ 3 cited

Jiamusi pulsar observations: IV. The core-weak pattern of PSR B0329+54

Tao Wang, J. L. Han, C. Wang +2

The bright pulsar PSR B0329+54 was previously known for many years to have two emission modes. Sensitive observations of individual pulses reveal that the central component of puls…