R. M. Shannon

Detection of 107 glitches in 36 southern pulsars

Timing observations from the Parkes 64-m radio telescope for 165 pulsarsbetween 1990 and 2011 have been searched for period glitches. Data spansfor each pulsar ranged between 5.3 and 20.8 yr. From the total of 1911yr of pulsar rotational history, 107 glitches were identified in 36pulsars. Out of these glitches, 61 have previously been reported whereas46 are new discoveries. Glitch parameters, both for the previously knownand the new glitch detections, were measured by fitting the timingresidual data. Observed relative glitch sizes{

Measurement and correction of variations in interstellar dispersion in high-precision pulsar timing

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A fast radio burst in the direction of the Carina dwarf spheroidal galaxy

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Development of a pulsar-based time-scale

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Pulsed Gamma Rays from the Original Millisecond and Black Widow Pulsars: A Case for Caustic Radio Emission?

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temponest: a Bayesian approach to pulsar timing analysis

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Radio properties of the magnetar near sagittarius A* from observations with the Australia telescope compact array

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Binary supermassive black hole environments diminish the gravitational wave signal in the pulsar timing band

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Limitations in timing precision due to single-pulse shape variability in millisecond pulsars

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Six millisecond pulsars detected by the Fermi Large Area Telescope and the radio/gamma-ray connection of millisecond pulsars

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