activity
20002008
most citedUpper limits on gravitational wave emission from 78 radio pulsars

195 citations · 352 across the 7 of their papers we have counts for

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8 papers · 1 filter

astro-ph20074 cited

Quark core formation in spinning-down pulsars

G. F. Marranghello, T. Regimbau, J. A. de Freitas Pacheco

Pulsars spin-down due to magnetic torque reducing its radius and increasing the central energy density. Some pulsar which are born with central densities close to the critical valu…

astro-ph200613 cited

Stochastic background from inspiralling double neutron stars

Tania Regimbau

We review the contribution of extra galactic inspiralling double neutron stars, to the LISA astrophysical gravitational wave foreground. Using recent fits of the star formation rat…

astro-ph200631 cited

Detection regimes of the cosmological gravitational wave background from astrophysical sources

David Coward, Tania Regimbau

Key targets for gravitational wave (GW) observatories, such as LIGO and the next generation interferometric detector, Advanced LIGO, include core-collapse of massive stars and the…

astro-ph200614 cited

Capture Rates of Compact Objects by Supermassive Black Holes

José Antonio de Freitas Pacheco, Charline Filloux, Tania Regimbau

Capture rates of compact objects were calculated by using a recent solution of the Fokker-Planck equation in energy-space, including two-body resonant effects. The fraction of comp…

astro-ph2005

Upper Limits on a Stochastic Background of Gravitational Waves

LIGO Scientific Collaboration, B. Abbott

The Laser Interferometer Gravitational Wave Observatory (LIGO) has performed a third science run with much improved sensitivities of all three interferometers. We present an analys…

astro-ph2003

Observational evidence for a correlation between peak-luminosities and beaming in GRBs

Maurice H. P. M. van Putten, Tania Regimbau

We calculate the unseen-but-true GRB-event rate from a current flux-limited sample of 33 GRBs with individually measured redshifts. We consider a GRB-event rate which is proportion…