Frequency-Dependent Squeezing for Advanced LIGO.

@article{McCuller2020FrequencyDependentSF,
  title={Frequency-Dependent Squeezing for Advanced LIGO.},
  author={Lee McCuller and Chris Whittle and D. Ganapathy and Kentaro Komori and M. Tse and {\'A}lvaro Fern{\'a}ndez-Galiana and Lisa Barsotti and P. Fritschel and Matthew MacInnis and F. Matichard and Kenneth R Mason and Nergis Mavalvala and Rachel Mittleman and Haocun Yu and Michael Edward Zucker and Matthew Evans},
  journal={Physical review letters},
  year={2020},
  volume={124 17},
  pages={
          171102
        }
}
The first detection of gravitational waves by the Laser Interferometer Gravitational-Wave Observatory (LIGO) in 2015 launched the era of gravitational-wave astronomy. The quest for gravitational-wave signals from objects that are fainter or farther away impels technological advances to realize ever more sensitive detectors. Since 2019, one advanced technique, the injection of squeezed states of light, is being used to improve the shot-noise limit to the sensitivity of the Advanced LIGO… 

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