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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 Article

Search for transient gravitational waves in coincidence with short-duration radio transients during 2007–2013

B. P. Abbott, +997 more
TL;DR: In this article, an archival search for transient gravitational-wave bursts in coincidence with 27 single-pulse triggers from Green Bank Telescope pulsar surveys, using the LIGO, Virgo, and GEO interferometer network, was presented.
Journal ArticleDOI

Erratum: “First Search for Gravitational Waves from Known Pulsars with Advanced LIGO” (2017, ApJ, 839, 12)

B. P. Abbott, +995 more
TL;DR: In this article, the authors present the results of searches for gravitational waves from 200 pulsars using data from the first observing run of the Advanced LIGO detectors, and they find no significant evidence for a gravitational-wave signal from any of these pulsars, but they are able to set the most constraining upper limits yet on their gravitationalwave amplitudes and ellipticities.
Journal Article

Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data

B. P. Abbott, +959 more
Book ChapterDOI

Observation of Gravitational Waves from a Binary Black Hole Merger

B. P. Abbott, +1010 more
TL;DR: The first direct detection of gravitational waves and the first observation of the collision and merger of a pair of black holes were reported in this paper, which was observed on September 14, 2015 by the two detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO), arguably the most sensitive scientific instruments ever constructed.
Journal ArticleDOI

Hydraulic External Pre-Isolator System for LIGO

TL;DR: The Hydraulic External Pre-Isolator (HEPI) as discussed by the authors is the first 6 degrees of freedom active seismic isolation system implemented at the LIGO and has been successfully used at the National Institute of Aeronautics and Astronautics (NICA).