activity
20102026
most citedThe second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

1k citations · 4k across the 53 of their papers we have counts for

collaborators

56 papers

astro-ph.IM2026

Evaluating the effectiveness of radio frequency interference removal algorithms for single pulse searches

R. S. Hombal, L. Levin, B. W. Stappers +10

Radio Frequency Interference (RFI), the presence of artificial and/or terrestrial signals in astronomical data, poses a great challenge to the search for pulsars and radio transien…

astro-ph.HE2026

Twenty-four thousand hours of GREENBURST observations with the GBT

J. W. Kania, S. Paine, G. M. Doskoch +23

In addition to fast radio burst (FRB) searches carried out using dedicated surveys, a number of radio observatories take advantage of commensal opportunities with large facilities…

astro-ph.HE2024

The impact on astrometry by solar-wind effect in pulsar timing

K. Liu, A. Parthasarathy, M. Keith +16

Astrometry of pulsars, particularly their distances, serves as a critical input for various astrophysical experiments using pulsars. Pulsar timing is a primary approach for determi…

astro-ph.CO2024

Searches for signatures of ultra-light axion dark matter in polarimetry data of the European Pulsar Timing Array

N. K. Porayko, P. Usynina, J. Terol-Calvo +74

Ultra-light axion-like particles (ALPs) can be a viable solution to the dark matter problem. The scalar field associated with ALPs, coupled to the electromagnetic field, acts as an…

astro-ph.HE2024★ 10 cited

Measuring glitch recoveries and braking indices with Bayesian model selection

Yang Liu, Michael J. Keith, Danai Antonopoulou +6

For a selection of 35 pulsars with large spin-up glitches (), which are monitored by the Jodrell Bank Observatory, we analyse 157 glitches and their recoveries. Al…

astro-ph.IM2024★ 4 cited

Improving pulsar timing precision through superior Time-of-Arrival creation

J. Wang, J. P. W. Verbiest, G. M. Shaifullah +6

The measurement of pulsar pulse times-of-arrival (ToAs) is a crucial step in detecting low-frequency gravitational waves. To determine ToAs, we can use template-matching to compare…