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Source of Noise Curves

WARNING: Some of these may not (yet) be correct.

If you alter or add any curves to this directory please edit this file appropriately.

AdLIGO

https://dcc.ligo.org/LIGO-P1200087-v42/public

AdVirgo

https://dcc.ligo.org/LIGO-P1200087-v42/public

KAGRA

https://dcc.ligo.org/LIGO-P1200087-v42/public

Cosmic Explorer

https://dcc.ligo.org/LIGO-P1600143/public

A+

https://dcc.ligo.org/LIGO-T1500293

ET

http://www.et-gw.eu/index.php/etsensitivities

LISA

http://www.srl.caltech.edu/~shane/sensitivity/

High-frequency detector.

Generated from Rob Ward: 9/2/2018: 'here’s a sensitivity for an aLIGO-like detector with a few non-crazy (but still possibly tough) modifications: 5% SRM, 15dB free-independent squeezing, 250W input power. With this sensitivity, we can increase the surface loss of the test-masses by a factor of 50 to help tame parametric instabilities, but I think PI may remain the single biggest challenge'

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