activity
20032018
most citedPlacing limits on the stochastic gravitational-wave background using European Pulsar Timing Array data

272 citations · 569 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2018★ 49 cited

Internal gas models and central black hole in 47 Tucanae using millisecond pulsars

F. Abbate, A. Possenti, A. Ridolfi +4

Despite considerations of mass loss from stellar evolution suggesting otherwise, the content of gas in globular clusters seems poor and hence its measurement very elusive. One way…

astro-ph.CO2011★ 272 cited

Placing limits on the stochastic gravitational-wave background using European Pulsar Timing Array data

R. van Haasteren, Y. Levin, G. H. Janssen +16

Direct detection of low-frequency gravitational waves ( Hz) is the main goal of pulsar timing array (PTA) projects. One of the main targets for the PTAs is to me…

astro-ph.HE2011★ 2 cited

Status and Prospects of Fermi LAT Pulsar Blind Searches

P. M. Saz Parkinson

Blind Searches of Fermi Large Area Telescope (LAT) data have resulted in the discovery of 24 gamma-ray pulsars in the first year of survey operations, most of which remain undetect…

astro-ph.HE2010★ 119 cited

The European Pulsar Timing Array: current efforts and a LEAP toward the future

Robert D. Ferdman, Rutger van Haasteren, Cees G. Bassa +22

The European Pulsar Timing Array (EPTA) is a multi-institutional, multi-telescope collaboration, with the goal of using high-precision pulsar timing to directly detect gravitationa…

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…

astro-ph2003★ 18 cited

The chemical composition of the peculiar companion to the millisecond pulsar in NGC 6397

E. Sabbi, R. G. Gratton, A. Bragaglia +4

We present the chemical composition of the bright companion to the millisecond pulsar J1740-5340 in NGC 6397, based on high resolution spectra. Though the large rotation velocity o…