The Advanced LIGO [1] and Advanced Virgo [2] detectors have made numerous detections
of gravitational waves (GWs), to date consisting of short-duration (transient) GWs emitted …

The field of gravitational-wave astronomy is now firmly established, with the detection of
multiple compact binary coalescences by the LIGO and Virgo observatories. These …

We report here on the first results of a systematic monitoring of southern glitching pulsars at
the Argentine Institute of Radioastronomy that started in the year 2019. We detected a major …

The stability of the spin of pulsars and the precision with which these spins can be
determined, allows many unique tests of interest to physics and astrophysics. Perhaps the …

ABSTRACT High-resolution, pulse-to-pulse observation of the 2016 Vela glitch and its
relaxation provided an opportunity to probe the neutron star internal structure and dynamics …

ABSTRACT A systematic, semi-automated search for pulsar glitches in the first UTMOST
public data release is presented. The search is carried out using a hidden Markov model …

The frequency evolution behavior of radio pulse profiles is an important clue for the radiation
mechanism of a pulsar. Combined with the latest results of the European Pulsar Network …

We study individual pulses of Vela (PSR B0833− 45/J0835− 4510) from daily observations
of over 3 h (around 120 000 pulses per observation), performed simultaneously with the two …

Noise characterization for pulsar-timing applications accounts for interstellar dispersion by
assuming a known frequency dependence of the delay it introduces in the times of arrival …

Noise characterization for pulsar-timing applications accounts for interstellar dispersion by
assuming a known frequency dependence of the delay it introduces in the times of arrival …