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G

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 High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Arnauld Albert, +1990 more
TL;DR: In this paper, the authors search for high-energy neutrinos from the binary neutron star merger in the GeV-EeV energy range using the Antares, IceCube, and Pierre Auger Observatories.
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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.
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A Standard Siren Measurement of the Hubble Constant from GW170817 without the Electromagnetic Counterpart

Maya Fishbach, +325 more
TL;DR: In this paper, a statistical standard siren analysis of GW170817 is presented, which considers all galaxies brighter than 0.626{L}_{B}^{\star }$ as equally likely to host a binary neutron star merger.
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A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo

B. P. Abbott, +1276 more
TL;DR: In this article, the first and second observing runs of the Advanced LIGO and Virgo detector network were used to obtain the first standard-siren measurement of the Hubble constant (H 0).
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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.