LIGO Document T2300300-v5
- Since O3 we haven t been able to increase the CLF power without destroying the amount of squeezing. Low CLF power results in a marginal SQZ 3MHz LO loop. A squeezer laser intensity noise measurement showed that our laser intensity noise was not as good as the Mephisto documentation claimed to be (alog68991). We then injected a frequency dependent squeezing with a high CLF power and showed that the squeezer laser intensity noise could
indeed be the limiting factor (alog69084). Hence, we proposed adding a mode cleaner on the SQZT0 to mitigate the CLF intensity noise.
- - Added Vicky's PMC measurements from MIT
- Added LHO table layout (Fig.16)
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