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G. Gemme

Researcher at Joint Institute for Nuclear Research

Publications -  291
Citations -  48771

G. Gemme is an academic researcher from Joint Institute for Nuclear Research. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 77, co-authored 262 publications receiving 40003 citations.

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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, +807 more
TL;DR: The results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that 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 are presented in this article.
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Noise from scattered light in Virgo's second science run data

T. Accadia, +171 more
TL;DR: Virgo is one of the large, ground-based interferometers aimed at detecting gravitational waves as mentioned in this paper, but its sensitivity is limited by light in the output beams which is backscattered by seismically excited surfaces and couples back into the main beam of the interferometer.
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Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817

B. P. Abbott, +1138 more
TL;DR: In this paper, the authors revisited the binary neutron star coalescence with a focus on longer signal durations up until the end of the Second Advanced LIGO-Virgo Observing run, 8.5 days after the coalescence of GW170817.
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An improved analysis of GW150914 using a fully spin-precessing waveform model

B. P. Abbott, +970 more
TL;DR: In this paper, a 15-dimensional precessing-spin waveform model (precessing EOBNR) was developed within the EOB formalism for GW150914.
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Constraints on cosmic strings from the ligo-virgo gravitational-wave detectors

J. Aasi, +893 more
TL;DR: New constraints on cosmic string parameters are derived, which complement and improve existing limits from previous searches for a stochastic background of GWs from cosmic microwave background measurements and pulsar timing data.