The rotation of more than 700 pulsars has been monitored using the 76-m Lovell Telescope
at Jodrell Bank. Here we report on a new search for glitches in the observations, revealing …

With the aim of constraining the structural properties of neutron stars and the equation of
state of dense matter, we study sudden spin-ups, glitches, occurring in the Vela pulsar and …

Timing observations from the Parkes 64-m radio telescope for 165 pulsars between 1990
and 2011 have been searched for period glitches. Data spans for each pulsar ranged …

Shemar & Lyne have previously presented observations and an analysis of 32 glitches and
their subsequent relaxations observed in a total of 15 pulsars. These data are brought …

We report on more than 7 yr of monitoring of PSR J0537-6910, the 16 ms pulsar in the LMC,
using data acquired with RXTE. During this campaign the pulsar experienced 23 sudden …

Timing observations of 40 mostly young pulsars using the ATNF Parkes radio telescope
between 1990 January and 1998 December are reported. In total, 20 previously unreported …

Pulsars are rotating neutron stars, sweeping the emission regions from the magnetic poles
across our line of sight. Isolated neutron stars lose angular momentum through dipole …

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 …

Context. Glitches are rare spin-up events that punctuate the smooth slow-down of the
rotation of pulsars. For the Vela pulsar and PSR J0537− 6910, their large glitch sizes and …

IN the past ten years, the Vela pulsar PSR 0833–45 has undergone several large,
discontinuous changes—glitches—in its pulsation period. On 24 December 1988, we were …