activity
20022026
most citedThe spatial energy spectrum of magnetic fields in our Galaxy

102 citations · 780 across the 26 of their papers we have counts for

collaborators

27 papers

astro-ph.HE2026

Radio eclipse of the slowest spinning Galactic-field spider pulsar PSR J1932+2121 and its X-ray emission prospect

Ze-Xin Du, Yun-Wei Yu, Zong-Lin Yang +5

PSR J19322121 is a newly discovered spider pulsar with a pronounced radio eclipse identified by the Five-hundred-meter Aperture Spherical radio Telescope (FAST); it provides an…

astro-ph.IM2026★ 1 cited

HiFAST: An HI data calibration and imaging pipeline for the FAST IV: The stray-radiation correction

Qingze Chen, Jie Wang, Yingjie Jing +12

Stray radiation is a considerable challenge for radio telescopes, requiring careful assessment due to its effects. This is crucial when the strong background flux from side lobes s…

astro-ph.HE2025

Search for Radio Pulsations from Neutron Star Candidates in Detached Binaries

Shi-Jie Gao, Xiang-Dong Li, Song Wang +7

Recent optical astrometric and spectroscopic surveys have identified numerous neutron star (NS) candidates in non-accreting detached binary systems, but their compact-object nature…

astro-ph.GA2020★ 10 cited

Discovery of a new supernova remnant G21.8-3.0

X. Y. Gao, P. Reich, W. Reich +2

Sensitive radio continuum surveys of the Galactic plane are ideal for discovering new supernova remnants (SNRs). From the Sino-German λ6 cm polarisation survey of the Galactic plan…

astro-ph.HE2018★ 16 cited

Jiamusi Pulsar Observations: II. Scintillations of 10 Pulsars

P. F. Wang, J. L. Han, Lei Han +6

Context. Pulsars scintillate. Dynamic spectra show brightness variation of pulsars in the time and frequency domain. Secondary spectra demonstrate the distribution of fluctuation p…

astro-ph.GA2016★ 27 cited

Radio polarization and magnetic field structure in M 101

E. M. Berkhuijsen, M. Urbanik, R. Beck +1

We observed total and polarized radio continuum emission from the spiral galaxy M 101 at 6.2 cm and 11.1 cm wavelengths with the Effelsberg telescope. We use these data to study va…