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F

F. Clara

Researcher at National Science Foundation

Publications -  216
Citations -  60804

F. Clara 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 82, co-authored 205 publications receiving 48814 citations.

Papers
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Journal ArticleDOI

Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817

B. P. Abbott, +1140 more
TL;DR: In this paper, the authors presented a search for GWs from the remnant of the binary neutron star merger GW170817 using data from Advanced LIGO and Advanced Virgo.
Journal Article

GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

B. P. Abbott, +979 more
TL;DR: A matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors from September 12 to October 20, 2015.
Journal ArticleDOI

Search for gravitational waves from low mass compact binary coalescence in LIGO's sixth science run and Virgo's science runs 2 and 3

J. Abadie, +884 more
- 19 Apr 2012 - 
TL;DR: In this paper, the authors report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo observations between July 7, 2009, and October 20, 2010.
Journal ArticleDOI

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).
Journal ArticleDOI

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.