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F

F. Antonucci

Researcher at University of Trento

Publications -  67
Citations -  4912

F. Antonucci is an academic researcher from University of Trento. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 27, co-authored 67 publications receiving 4700 citations.

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Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors

J. Abadie, +722 more
TL;DR: In this paper, Kalogera et al. presented an up-to-date summary of the rates for all types of compact binary coalescence sources detectable by the initial and advanced versions of the ground-based gravitational-wave detectors LIGO and Virgo.
Journal ArticleDOI

Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

J. Abadie, +709 more
TL;DR: In this article, the authors present an up-to-date summary of the rates for all types of compact binary coalescence sources detectable by the Initial and Advanced versions of the ground-based LIGO and Virgo Astrophysical estimates for compact-binary coalescence rates depend on a number of assumptions and unknown model parameters.
Journal ArticleDOI

An upper limit on the stochastic gravitational-wave background of cosmological origin

B. P. Abbott, +667 more
- 20 Aug 2009 - 
TL;DR: In this paper, the authors reported limits on the amplitude of the stochastic gravitational-wave background using the data from a two-year science run of the Laser Interferometer Gravitational-wave Observatory (LIGO).
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Virgo: a laser interferometer to detect gravitational waves

T. Accadia, +341 more
TL;DR: Virgo as discussed by the authors is a very large Michelson interferometer with 3 km-long arms, built at Cascina, near Pisa (Italy), with a detailed description of all its different elements is given.
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Searches for gravitational waves from known pulsars with science run 5 LIGO data

B. P. Abbott, +705 more
TL;DR: In this article, an updated search for gravitational waves from 116 known millisecond and young pulsars using data from the fifth science run of the LIGO detectors was presented, where ephemerides overlapping the run period were obtained using radio and X-ray observations.