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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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Search for gravitational waves from binary inspirals in S3 and S4 LIGO data

B. P. Abbott, +463 more
- 07 Mar 2008 - 
TL;DR: In this paper, a search for gravitational waves from the coalescence of compact binary systems during the third and fourth LIGO science runs was reported, which focused on gravitational waves generated during the inspiral phase of the binary evolution.
Journal ArticleDOI

Photovoltaic spatial solitons

TL;DR: In this paper, the authors analyze self-trapping of one-dimensional optical beams in photorefractive, photovoltaic media for open-and closed-circuit realizations.
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Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors

B. P. Abbott, +376 more
- 15 Apr 2004 - 
TL;DR: In this article, a model emission mechanism is used to interpret the limits as a constraint on the pulsar's equatorial ellipticity, and two independent analysis methods are used and are demonstrated in two independent methods: a frequency domain method and a time domain method.
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Observation of a kilogram-scale oscillator near its quantum ground state

B. P. Abbott, +454 more
TL;DR: In this paper, the resonant frequency of a 2.7 kg pendulum mode was dynamically shifted to lie within this optimal band, where its effective temperature falls as low as 1.4 μK and its occupation number reaches about 200 quanta.
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A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo

B. P. Abbott, +1276 more
TL;DR: In this article, the first and second observing runs of the Advanced LIGO and Virgo detector network were used to obtain the first standard-siren measurement of the Hubble constant (H 0).