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J.-M. Isac

Researcher at Pierre-and-Marie-Curie University

Publications -  112
Citations -  43055

J.-M. Isac is an academic researcher from Pierre-and-Marie-Curie University. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 65, co-authored 112 publications receiving 36162 citations. Previous affiliations of J.-M. Isac include PSL Research University & Paris-Sorbonne University.

Papers
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

B. P. Abbott, +1144 more
TL;DR: The total background may be detectable with a signal-to-noise-ratio of 3 after 40 months of total observation time, based on the expected timeline for Advanced LIGO and Virgo to reach their design sensitivity.
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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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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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Search for post-merger gravitational waves from the remnant of the binary neutron star merger GW170817

B. P. Abbott, +1103 more
TL;DR: In this paper, the authors presented a search for gravitational waves from the remnant of the binary neutron star merger GW170817 using data from Advanced LIGO and Advanced Virgo and found no signal from the post-merger remnant.
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Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run

B. P. Abbott, +955 more
TL;DR: In this article, the authors reported the non-detection of gravitational waves from the merger of binary neutron star systems and neutron-star-black-hole systems during the first observing run of Advanced LIGO.