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Martin M. Fejer

Researcher at Stanford University

Publications -  1227
Citations -  104666

Martin M. Fejer is an academic researcher from Stanford University. The author has contributed to research in topics: Lithium niobate & Gravitational wave. The author has an hindex of 123, co-authored 1190 publications receiving 88708 citations. Previous affiliations of Martin M. Fejer include Laser Interferometer Gravitational Wave Observatory & University of Florida.

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Journal ArticleDOI

Binary Black Hole Mergers in the first Advanced LIGO Observing Run

B. P. Abbott, +972 more
TL;DR: The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2016, saw the first detections of gravitational waves from binary black hole mergers as discussed by the authors.
Journal ArticleDOI

A gravitational-wave standard siren measurement of the Hubble constant

B. P. Abbott, +1322 more
- 02 Nov 2017 - 
TL;DR: A measurement of the Hubble constant is reported that combines the distance to the source inferred purely from the gravitational-wave signal with the recession velocity inferred from measurements of the redshift using the electromagnetic data.
Journal ArticleDOI

GW190521: A Binary Black Hole Merger with a Total Mass of 150 M

R. Abbott, +1335 more
TL;DR: It is inferred that the primary black hole mass lies within the gap produced by (pulsational) pair-instability supernova processes, with only a 0.32% probability of being below 65 M⊙, which can be considered an intermediate mass black hole (IMBH).
Journal ArticleDOI

Properties of the Binary Black Hole Merger GW150914

B. P. Abbott, +987 more
TL;DR: The data around the time of the event were analyzed coherently across the LIGO network using a suite of accurate waveform models that describe gravitational waves from a compact binary system in general relativity.
Journal ArticleDOI

GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence

B. P. Abbott, +1101 more
TL;DR: In this paper, the authors show that the signal waveform is consistent with the predictions of general relativity and verify that the signals from the merger of two stellar-mass black holes in the LIGO detectors are consistent with these predictions.