collaborators

8 papers

astro-ph.HE2026

Pulsar electrodynamics inferred from frequency-dependent circular polarization diversity

Shunshun Cao, Yanjun Guo, Jinchen Jiang +3

The nature of coherent radio emission is still challenging even after more than half a century of pulsar discovery, but it is generally a consensus that single-pulse observations a…

astro-ph.HE2026

Improved proper motion and gravity tests with PSR J1913+1102

Xueli Miao, Paulo C. C. Freire, Norbert Wex +11

PSR J1913+1102 is a highly asymmetric double neutron star system and an excellent laboratory for testing scalar-tensor gravity theories, as well as a potential progenitor analogue…

astro-ph.HE2025

The double neutron star PSR J1946+2052 I. Masses and tests of general relativity

Lingqi Meng, Paulo C. C. Freire, Kevin Stovall +28

We conducted high-precision timing of PSR J1946+2052 to determine the masses of the two neutron stars in the system, test general relativity (GR) and assessed the system's potentia…

astro-ph.HE2025

Detecting Intermediate-mass Black Holes Using Miniature Pulsar Timing Arrays in Globular Clusters

Xian Chen, Verónica Vázquez-Aceves, Siyuan Chen +3

Theoretical models predict that intermediate-mass black holes (IMBHs) exist in globular clusters (GCs), but observational evidence remains elusive. Millisecond pulsars (MSPs), whic…

astro-ph.HE2025

The Chinese Pulsar Timing Array data release I. Single pulsar noise analysis

Siyuan Chen, Heng Xu, Yanjun Guo +23

The Chinese Pulsar Timing Array (CPTA) has collected observations from 57 millisecond pulsars using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST) for close to th…

astro-ph.HE2025

Periodic variation of magnetoionic environment of a fast radio burst source

Jiangwei Xu, Heng Xu, Yanjun Guo +8

Fast radio bursts (FRBs) are luminous, dispersed millisecond-duration radio bursts whose origin is poorly known. Recent observations suggest that some FRBs may reside in binary sys…