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H. Overmier

Researcher at California Institute of Technology

Publications -  274
Citations -  67398

H. Overmier is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 91, co-authored 263 publications receiving 55260 citations.

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Journal ArticleDOI

Tests of General Relativity with GW170817

B. P. Abbott, +1240 more
TL;DR: In this paper, the authors place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime of a binary neutron star inspiral.
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Quantum-Enhanced Advanced LIGO Detectors in the Era of Gravitational-Wave Astronomy

Maggie Tse, +210 more
TL;DR: During the ongoing O3 observation run, squeezed states are improving the sensitivity of the LIGO interferometers to signals above 50 Hz by up to 3 dB, thereby increasing the expected detection rate by 40% and 50% respectively.
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Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy

Denis Martynov, +262 more
- 02 Jun 2016 - 
TL;DR: The first observation run of the Advanced LIGO detectors started in September 2015 and ended in January 2016 as discussed by the authors, which achieved a strain sensitivity of better than 10^(−23)/√Hz around 100 Hz.
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GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

B. P. Abbott, +980 more
- 07 Jun 2016 - 
TL;DR: In this paper, the results of 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 were reported.
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Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

Richard J. Abbott, +1695 more
TL;DR: In this article, the authors reported the observation of gravitational waves from two compact binary coalescences in LIGO's and Virgo's third observing run with properties consistent with neutron star-black hole (NSBH) binaries.