activity
20082020
most citedSearching for gravitational waves from Cassiopeia A with LIGO

122 citations · 341 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2020★ 30 cited

Transient gravitational waves from pulsar post-glitch recoveries

Garvin Yim, D. I. Jones

This work explores whether gravitational waves (GWs) from neutron star (NS) mountains can be detected with current 2nd-generation and future 3rd-generation GW detectors. In particu…

astro-ph.HE2018★ 88 cited

Evidence for a minimum ellipticity in millisecond pulsars

G. Woan, M. D. Pitkin, B. Haskell +2

Neutron stars spin down over time due to a number of energy-loss processes. We provide tantalizing population-based evidence that millisecond pulsars (MSPs) have a minimum elliptic…

astro-ph.HE2018

Advances in our understanding of the free precession candidate PSR B1828-11

Gregory Ashton, David Ian Jones, Reinhard Prix

We highlight the advances and difficulties in understanding PSR B1828-11, which undergoes long-term periodic modulations in its timing and pulse shape over several years. A model c…

astro-ph.HE2016★ 20 cited

Implications of the Occurrence of Glitches in Pulsar Free Precession Candidates

D. I. Jones, G. Ashton, R. Prix

The timing properties of radio pulsars provide a unique probe of neutron star interiors. Recent observations have uncovered quasiperiodicities in the timing and pulse properties of…

astro-ph.HE2016★ 15 cited

On the free-precession candidate PSR B1828-11: Evidence for increasing deformation

G. Ashton, D. I. Jones, R. Prix

We observe that the periodic variations in spin-down rate and beam-width of the radio pulsar PSR B1828-11 are getting faster. In the context of a free precession model, this corres…

astro-ph.SR2015★ 40 cited

Comparing models of the periodic variations in spin-down and beam-width for PSR B1828-11

G. Ashton, D. I. Jones, R. Prix

We build a framework using tools from Bayesian data analysis to evaluate models explaining the periodic variations in spin-down and beam-width of PSR B1828-11. The available data c…