Showing 1–20 of 56 results
/ Date/ Name
Jun 28, 2023Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release IAug 16, 2010Detecting massive gravitons using pulsar timing arraysApr 19, 2012The optimal schedule for pulsar timing array observationsApr 8, 2014Model-based asymptotically optimal dispersion measure correction for pulsar timingDec 2, 2009Lower bounds of altitudes for pulsar $γ$-ray radiationDec 13, 2021Repeating Fast Radio Burst: Coherent Circular Polarization By BunchesAug 19, 2024AXPs/SGRs: strange stars with crusts?Mar 5, 2025A Linear Decomposition Method to Analyze and Study Pulsar Mode ChangesFeb 28, 2025The Chinese pulsar timing array data release I. Polarimetry for 56 millisecond pulsarsDec 22, 2025On the Diversity of Pulsar's Frequency-Dependent Circular PolarizationDec 18, 2025The SKAO Pulsar Timing ArrayOct 11, 2023The Qitai Radio TelescopeJul 10, 2025Detecting Intermediate-mass Black Holes Using Miniature Pulsar Timing Arrays in Globular ClustersSep 9, 2019Advancing Pulsar Science with the FASTSep 24, 2019FRB 171019: An event of binary neutron star merger?Oct 11, 2024Is the Gum Nebula an Important Interstellar Scattering Disk of Background Pulsars?Aug 23, 2018Verifying and Reporting Fast Radio BurstsNov 28, 2017Large magnetic field variations towards the Galactic Centre magnetar, PSR J1745-2900Jul 3, 2025Multi-year Polarimetric Monitoring of Four CHIME-Discovered Repeating Fast Radio Bursts with FASTApr 1, 2025Polarization Position Angle Swing and the Rotating Vector Model of Repeating Fast Radio Bursts