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E. L. Merilh

Researcher at National Science Foundation

Publications -  156
Citations -  54523

E. L. Merilh is an academic researcher from National Science Foundation. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 71, co-authored 145 publications receiving 43074 citations.

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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, +981 more
TL;DR: In this paper, the authors reported that 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 the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO).
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Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817

B. P. Abbott, +1144 more
TL;DR: In this paper, the mass of the dynamical ejecta can be estimated without a direct electromagnetic observation of the kilonova, using GW measurements and a phenomenological model calibrated to numerical simulations of mergers with dynamical ejecteda.
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Sensitivity and performance of the Advanced LIGO detectors in the third observing run

Aaron Buikema, +208 more
- 15 Sep 2020 - 
TL;DR: In 2019, the Advanced Laser Interferometer Gravitational-wave Observatory (aLIGO), joined by the Advanced Virgo detector, began the third observing run, a year-long dedicated search for gravitational radiation as discussed by the authors.
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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).