Relativistic reflection features are commonly observed in the X-ray spectra of accreting black
holes. In the presence of high quality data and with the correct astrophysical model, X-ray …

The megajansky radio burst, FRB 20200428, and other bright radio bursts detected from the
Galactic source SGR J1935+ 2154 suggest that magnetars can make fast radio bursts …

Fast radio bursts (FRBs) are short pulses observed in the radio band from cosmological
distances. One class of models invokes soft gamma-ray repeaters (SGRs), or magnetars, as …

This article provides a review on X-ray pulsar-based navigation (XNAV). The review starts
with the basic concept of XNAV, and briefly introduces the past, present and future projects …

Fast radio bursts are millisecond-duration, bright radio signals (fluence 0.1–100 Jy ms)
emitted from extragalactic sources of unknown physical origin. The recent CHIME/FRB and …

Fast radio bursts (FRBs) are millisecond-duration radio transients of unknown physical
origin observed at extragalactic distances,–. It has long been speculated that magnetars are …

Low-frequency quasiperiodic oscillations (LFQPOs) are commonly found in black hole X-ray
binaries, and their origin is still under debate. The properties of LFQPOs at high energies …

Accreting X-ray pulsars (XRPs) are presumed to be ideal targets for polarization
measurements, as their high magnetic field strength is expected to polarize the emission up …

We report the X-ray timing results of the black hole candidate MAXI J1820+ 070 during its
2018 outburst using the Hard X-ray Modulation Telescope (Insight-HXMT) and Neutron Star …

We present the calibration of the Insight-Hard X-ray Modulation Telescope (Insight-HXMT) X-
ray satellite, which can be used to perform timing and spectral studies of bright X-ray …