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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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Constraints on cosmic strings using data from the first Advanced LIGO observing run

B. P. Abbott, +1042 more
- 08 May 2018 - 
TL;DR: In this article, an analysis conducted to specifically search for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO 2015-2016 observing run (O1) was conducted.
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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

B. P. Abbott, +1225 more
- 08 Jul 2019 - 
TL;DR: In this article, the results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast spinning neutron stars with an asymmetry around their rotation axis, were presented.
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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, +1932 more
TL;DR: In this article, 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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Effects of data quality vetoes on a search for compact binary coalescences in Advanced LIGO's first observing run

B. P. Abbott, +983 more
TL;DR: The systematic removal of noisy data from analysis time is shown to improve the sensitivity of searches for compact binary coalescences, and the output of the PyCBC pipeline is used as a metric for improvement.
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Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background

B. P. Abbott, +1143 more
TL;DR: Using data recorded by Advanced LIGO during its first observing run, no evidence for a background of any polarization is found, and the first direct bounds on the contributions of vector and scalar polarizations to the stochastic background are placed.