LIGO-T0900288-v3
12 Jun 2018, 11:07 |
These curves represent the incoherent sum of the principal noise sources as we best understand them at this time. There will be, in addition, technical noise sources. This is not a guaranteed performance, but a good guide to the overall curve and an early approximation to the anticipated sensitivity. These caveats need to be mentioned when describing these curves in presentations and publications.
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