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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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Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data

J. Aasi, +911 more
- 21 Jan 2015 - 
TL;DR: In this paper, the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data are presented.
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A cryogenic silicon interferometer for gravitational-wave detection

Rana X. Adhikari, +114 more
TL;DR: In this paper, the authors designed a new instrument able to detect gravitational waves at distances 5 times further away than possible with Advanced LIGO, or at greater than 100 times the event rate.
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Experimental measurements of mechanical dissipation associated with dielectric coatings formed using SiO2, Ta2O5 and Al2O3

TL;DR: In this paper, the authors quantified the mechanical dissipation associated with dielectric thin films formed from alternating layers of ion-beam-sputtered SiO2 and Ta2O5 and concluded that such dissipation could lead to potentially significant levels of thermally induced displacement noise in proposed advanced gravitational wave detectors.
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Laser‐induced photochromic damage in potassium titanyl phosphate

TL;DR: In this article, photochromic damage induced in KTiOPO4 single crystals by ultraviolet (UV) irradiation with peak intensities from 3 to 40 MW/cm2 was reported.
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Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during Their First and Second Observing Runs

B. P. Abbott, +1255 more
TL;DR: In this article, the authors present the results of a search for BBH mergers that inspiral in eccentric orbits using data from the first and second observing runs (O1 and O2) of Advanced LIGO and Advanced Virgo.