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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.

Papers
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Journal ArticleDOI

First search for gravitational waves from known pulsars with advanced LIGO

B. P. Abbott, +1039 more
TL;DR: In this paper, the results of searches for gravitational waves from 200 pulsars using data from the first observing run of the Advanced LIGO detectors were presented, and they were able to set the most constraining upper limits yet on their gravitational-wave amplitudes and ellipticities.
Journal ArticleDOI

Constraints on cosmic strings using data from the first Advanced LIGO observing run

B. P. Abbott, +1042 more
- 08 May 2018 - 
TL;DR: In this article, an analysis conducted to specifically search for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO 2015-2016 observing run (O1) was conducted.
Journal ArticleDOI

Thermo-optic noise in coated mirrors for high-precision optical measurements

TL;DR: In this paper, thermal fluctuations in the coatings used to make high reflectors are becoming significant noise sources in precision optical measurements and are particularly relevant to advanced gravitational-wave detectors.
Proceedings ArticleDOI

Photothermal common-path interferometry (PCI): new developments

TL;DR: In this article, a 3.39 μm probe was used for testing and studying various semiconductor materials, such as p-doped GaAs, that can exhibit non-thermal response to the pump beam in addition to the thermal one.
Journal ArticleDOI

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

B. P. Abbott, +1225 more
- 08 Jul 2019 - 
TL;DR: In this article, the results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast spinning neutron stars with an asymmetry around their rotation axis, were presented.