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P. Astone

Researcher at Istituto Nazionale di Fisica Nucleare

Publications -  464
Citations -  80969

P. Astone is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 96, co-authored 444 publications receiving 65350 citations. Previous affiliations of P. Astone include Sapienza University of Rome & Max Planck Society.

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All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run

J. Abadie, +878 more
- 20 Jun 2012 - 
TL;DR: In this paper, the authors presented results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010.
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Directional Limits on Persistent Gravitational Waves from Advanced LIGO’s First Observing Run

B. P. Abbott, +1018 more
TL;DR: Directed searches for narrowband gravitational waves from astrophysically interesting objects yield median frequency-dependent limits on strain amplitude at the most sensitive detector frequencies between 130-175 Hz, which represents a mean improvement of a factor of 2 across the band compared to previous searches of this kind.
Journal ArticleDOI

Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data

J. Aasi, +865 more
TL;DR: A search for the stochastic background with the latest data from the LIGO and Virgo detectors shows no evidence of a stochastically gravitational-wave signal, and the limits in these four bands are the lowest direct measurements to date on the stoChastic background.

Search for gravitational waves from binary black hole inspiral, merger, and ringdown

J. Abadie, +720 more
Journal ArticleDOI

Implementation and testing of the first prompt search for gravitational wave transients with electromagnetic counterparts

J. Abadie, +815 more
TL;DR: In this paper, a low-latency analysis pipeline was used to identify and localize GW event candidates and to request images of targeted sky locations, where a catalog of nearby galaxies and Milky Way globular clusters were used to select the most promising sky positions to be imaged.