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V. Necula

Researcher at University of Florida

Publications -  197
Citations -  26848

V. Necula is an academic researcher from University of Florida. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 64, co-authored 197 publications receiving 23699 citations.

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Gravitational waves from known pulsars: Results from the initial detector era

J. Aasi, +906 more
TL;DR: The results of searches for gravitational waves from a large selection of pulsars using data from the most recent science runs (S6, VSR2 and VSR4) of the initial generation of interferometric gravitational wave detectors LIGO (Laser Interferometric Gravitational-wave Observatory) and Virgo as discussed by the authors.
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Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3

J. Abadie, +890 more
TL;DR: The results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) were detected by satellite-based gamma ray experiments in 2009-2010, during the sixth LIGO science run and the second and third Virgo science runs as mentioned in this paper.
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Observation of Exclusive Charmonium Production and gamma gamma -> mu(+)mu(-) in p(p)over-bar Collisions at root s=1.96 TeV

T. Aaltonen, +617 more
TL;DR: An upper limit is put on the cross section for Odderon exchange in exclusive J/psi production in hadron-hadron collisions and the continuum is consistent with QED.
Journal ArticleDOI

Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

J. Aasi, +896 more
- 04 Sep 2013 - 
TL;DR: In this paper, a selection of simulated signals added either in hardware or software to the data collected by the two LIGO instruments and the Virgo detector during their most recent joint science run, including a "blind injection" where the signal was not initially revealed to the collaboration.
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Implementation and testing of the first prompt search for gravitational wave transients with electromagnetic counterparts

J. Abadie, +901 more
TL;DR: In this paper, a low-latency analysis pipeline was used to identify and localize GW event candidates and to reconstruct maps of possible sky locations, and a catalog of nearby galaxies and Milky Way globular clusters were used to select the most promising sky positions to be imaged.