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M

M. Agathos

Researcher at University of Cambridge

Publications -  282
Citations -  77714

M. Agathos is an academic researcher from University of Cambridge. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 91, co-authored 263 publications receiving 62049 citations. Previous affiliations of M. Agathos include VU University Amsterdam & Max Planck Society.

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

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.