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20092024
most citedThe second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

1k citations · 5.8k across the 54 of their papers we have counts for

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12 papers · 1 filter

astro-ph.IM2021★ 6 cited

Removal and replacement of interference in tied-array radio pulsar observations using the spectral kurtosis estimator

M. Purver, C. G. Bassa, I. Cognard +10

We describe how to implement the spectral kurtosis method of interference removal (zapping) on a digitized signal of averaged power values. Spectral kurtosis is a hypothesis test,…

astro-ph.IM2021

MeerTRAP in the era of multi-messenger astrophysics

Kaustubh Rajwade, Benjamin Stappers, Christopher Williams +9

Real-time detections of transients and rapid multi-wavelength follow-up are at the core of modern multi-messenger astrophysics. MeerTRAP is one such instrument that has been deploy…

astro-ph.IM2020★ 11 cited

Real-time triggering capabilities for Fast Radio Bursts at the MeerKAT telescope

F. Jankowski, M. Berezina, B. W. Stappers +9

Fast Radio Bursts (FRBs) are bright enigmatic radio pulses of roughly millisecond duration that come from extragalactic distances. As part of the MeerTRAP project, we use the MeerK…

astro-ph.IM2019★ 98 cited

A pulsar-based timescale from the International Pulsar Timing Array

G. Hobbs, L. Guo, R. N. Caballero +56

We have constructed a new timescale, TT(IPTA16), based on observations of radio pulsars presented in the first data release from the International Pulsar Timing Array (IPTA). We us…

astro-ph.IM2018★ 45 cited

Single-pulse classifier for the LOFAR Tied-Array All-sky Survey

D. Michilli, J. W. T. Hessels, R. J. Lyon +7

Searches for millisecond-duration, dispersed single pulses have become a standard tool used during radio pulsar surveys in the last decade. They have enabled the discovery of two n…

astro-ph.IM2017

The beamformer and correlator for the Large European Array for Pulsars

R. Smits, C. G. Bassa, G. H. Janssen +10

The Large European Array for Pulsars combines Europe's largest radio telescopes to form a tied-array telescope that provides high signal-to-noise observations of millisecond pulsar…

astro-ph.IM2016

Pulsar observations with European telescopes for testing gravity and detecting gravitational waves

D. Perrodin, C. G. Bassa, G. H. Janssen +20

A background of nanohertz gravitational waves from supermassive black hole binaries could soon be detected by pulsar timing arrays, which measure the times-of-arrival of radio puls…

astro-ph.IM2016★ 123 cited

From Spin Noise to Systematics: Stochastic Processes in the First International Pulsar Timing Array Data Release

L. Lentati, R. M. Shannon, W. A. Coles +80

We analyse the stochastic properties of the 49 pulsars that comprise the first International Pulsar Timing Array (IPTA) data release. We use Bayesian methodology, performing model…

astro-ph.IM2016★ 457 cited

The International Pulsar Timing Array: First Data Release

J. P. W. Verbiest, L. Lentati, G. Hobbs +89

The highly stable spin of neutron stars can be exploited for a variety of (astro-)physical investigations. In particular arrays of pulsars with rotational periods of the order of m…

astro-ph.IM2015★ 102 cited

LEAP: the large European array for pulsars

C. G. Bassa, G. H. Janssen, R. Karuppusamy +9

The Large European Array for Pulsars (LEAP) is an experiment that harvests the collective power of Europe's largest radio telescopes in order to increase the sensitivity of high-pr…

astro-ph.IM2015★ 74 cited

The noise properties of 42 millisecond pulsars from the European Pulsar Timing Array and their impact on gravitational wave searches

R. N. Caballero, K. J. Lee, L. Lentati +36

The sensitivity of Pulsar Timing Arrays to gravitational waves depends on the noise present in the individual pulsar timing data. Noise may be either intrinsic or extrinsic to the…

astro-ph.IM2014★ 25 cited

Gravitational wave astronomy with the SKA

G. H. Janssen, G. Hobbs, M. McLaughlin +12

On a time scale of years to decades, gravitational wave (GW) astronomy will become a reality. Low frequency (nanoHz) GWs are detectable through long-term timing observations of the…