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V

V. Brisson

Researcher at Université Paris-Saclay

Publications -  535
Citations -  75299

V. Brisson is an academic researcher from Université Paris-Saclay. The author has contributed to research in topics: Gravitational wave & HERA. The author has an hindex of 100, co-authored 532 publications receiving 65072 citations. Previous affiliations of V. Brisson include RWTH Aachen University & University of Hamburg.

Papers
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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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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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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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Status of the Virgo project

T. Accadia, +182 more
TL;DR: In this article, the authors describe the current state and future evolution of the Virgo gravitational wave detector, realized by the European Gravitational Observatory in Cascina near Pisa in Italy.
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Combination and QCD analysis of charm production cross section measurements in deep-inelastic ep scattering at HERA

Halina Abramowicz, +489 more
TL;DR: In this article, the effect of different heavy flavour schemes on the parton distribution functions was investigated. And the running mass of the charm quark was determined using the fixed flavour number scheme.