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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

Multiple-channel wavelength conversion by use of engineered quasi-phase-matching structures in LiNbO(3) waveguides.

TL;DR: Different frequency generation-based wavelength converters with multiple phase-matching wavelengths that use engineered quasi-phase- matching structures in LiNbO(3) waveguides that can be used to perform wavelength broadcasting.
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Second-harmonic generation of green light in periodically poled planar lithium niobate waveguide

TL;DR: In this article, a periodically poled, planar waveguide in lithium niobate was used to generate 532 nm radiation at room temperature by continuous-wave frequency doubling with a conversion efficiency of 5% per Wcm2.
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Search for the isotropic stochastic background using data from Advanced LIGO's second observing run

B. P. Abbott, +1133 more
- 15 Sep 2019 - 
TL;DR: In this article, a cross-correlation analysis on the data from Advanced LIGO's second observing run (O2) is presented, which combines with the results of the first observing run, and upper limits on the normalized energy density in gravitational waves at the 95% credible level of ΩGW < 6.0 × 10−8 at 25 Hz for a background of compact binary coalescences.
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All-optical signal processing using /spl chi//sup (2)/ nonlinearities in guided-wave devices

TL;DR: Integrated structures that will allow for improvements of current signal-processing functions as well as the implementation of novel device concepts are presented.
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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.