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Silvio Pardi

Researcher at University of Naples Federico II

Publications -  254
Citations -  6158

Silvio Pardi is an academic researcher from University of Naples Federico II. The author has contributed to research in topics: Gravitational wave & Interferometry. The author has an hindex of 33, co-authored 138 publications receiving 5876 citations. Previous affiliations of Silvio Pardi include University of Salerno.

Papers
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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.
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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.
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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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Status of VIRGO

Fausto Acernese, +128 more
TL;DR: The Virgo detector has now finished its first science run; a science mode duty cycle of more than 80% and a 4.5 Mpc horizon distance for binary neutron star inspiral sources were achieved.