activity
20082023
most citedHigh-Resolution Timing Observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope

48 citations · 149 across the 6 of their papers we have counts for

collaborators

7 papers

gr-qc2023★ 7 cited

Search for gravitational wave signals from known pulsars in LIGO-Virgo O3 data using the 5n-vector ensemble method

Luca D'Onofrio, Rosario De Rosa, Cristiano Palomba +16

The 5n-vector ensemble method is a multiple test for the targeted search of continuous gravitational waves from an ensemble of known pulsars. This method can improve the detection…

astro-ph.HE2020★ 1 cited

Flickering of the Vela pulsar during its 2016 glitch

Gregory Ashton, Paul D. Lasky, Rowina Nathan +1

The first pulse-to-pulse observations of a neutron star glitch in the Vela pulsar identified a null pulse hinting at the sudden disruption of the neutron star's magnetosphere. The…

astro-ph.HE2019

Rotational evolution of the Vela pulsar during the 2016 glitch

Gregory Ashton, Paul D. Lasky, Vanessa Graber +1

The 2016 Vela glitch observed by the Mt Pleasant radio telescope provides the first opportunity to study pulse-to-pulse dynamics of a pulsar glitch, opening up new possibilities to…

gr-qc2019★ 39 cited

First search for long-duration transient gravitational waves after glitches in the Vela and Crab pulsars

David Keitel, Graham Woan, Matthew Pitkin +7

Gravitational waves (GWs) can offer a novel window into the structure and dynamics of neutron stars. Here we present the first search for long-duration quasi-monochromatic GW trans…

astro-ph.HE2011★ 12 cited

Consecutive Bright Pulses in the Vela Pulsar

Jim L. Palfreyman, Aidan W. Hotan, John M. Dickey +2

We report on the discovery of consecutive bright radio pulses from the Vela pulsar, a new phenomenon that may lead to a greater understanding of the pulsar emission mechanism. This…

astro-ph.HE2010★ 42 cited

Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

A. Pellizzoni, A. Trois, M. Tavani +68

Pulsars are known to power winds of relativistic particles that can produce bright nebulae by interacting with the surrounding medium. These pulsar wind nebulae (PWNe) are observed…