Songbo Zhang

TL;DR: In this article, the authors describe the International Pulsar Timing Array second data release, which includes recent pulsar timing data obtained by three regional consortia: the European Pulsars Timing array, the North American Nanohertz Observatory for Gravitational Waves, and the Parkes pulsar timing array, and find that the timing precisions of pulsars are generally improved compared to the previous data release.

TL;DR: In this paper, the Parkes Pulsar Timing Array (PTA) data were used to detect the spatial correlation of the Hellings-downs signature of the gravitational wave background.

TL;DR: In this article, the authors reported the detection of a non-thermal X-ray burst in the 1-250 keV energy band with the Insight-HXMT satellite, which they identify as having been emitted from SGR J1935+2154.

TL;DR: 14 yr of public data from the Parkes Pulsar Timing Array is described, an ongoing project that is producing precise measurements of pulse times of arrival from 26 millisecond pulsars using the 64-m Parkes radio telescope with a cadence of approximately 3 weeks in three observing bands.

TL;DR: Polarization observations of the fast radio burst FRB-180301 with the FAST radio telescope show diverse polarization angle swings, consistent with a magnetospheric origin of the emission as discussed by the authors.