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Reports until 12:04, Thursday 06 October 2016
H1 CAL (DetChar)
jeffrey.kissel@LIGO.ORG - posted 12:04, Thursday 06 October 2016 - last comment - 12:59, Thursday 06 October 2016(30269)
PCALX Roaming Calibration Line Frequency Changed
J. Kissel, S. Karki

As we've done in O1, we're creating a high-frequency ( > 1 kHz ) excitation via PCALX whose frequency is changed over long-duration in order to map out the interferometer's sensing function out to as high as is needed for burst and binary neutron star coalescence searches. For quite some time now (since July! see LHO aLOG 28301), this line has been gathering data at 3501.3 [Hz]. We haven't moved it because the IFO's duty cycle has been low, the power level has been inconsistent, and our person power has been limited.

Today is the day!

I've resumed moving this line, following the schedule posted by Sudarshan in LLO aLOG 28070, which I repeat here for convenience:

Frequency    Planned Amplitude        Planned Duration      Actual Amplitude    Start Time                 Stop Time                    Achieved Duration
(Hz)         (ct)                     (hh:mm)                   (ct)               (UTC)                    (UTC)                         (hh:mm)
---------------------------------------------------------------------------------------------------------------------------------------------------------
1001.3       35k                      02:00      
1501.3       35k                      02:00     
2001.3       35k                      02:00     
2501.3       35k                      05:00      
3001.3       35k                      05:00                   39322.0           Oct 06 2016 18:39:26 UTC
3501.3       35k                      05:00                   39322.0           Jul 06 2016 18:56:13 UTC    Oct 06 2016 18:39:26 UTC      months
4001.3       40k                      10:00
4301.3       40k                      10:00       
4501.3       40k                      10:00
4801.3       40k                      10:00  
5001.3       40k                      10:00

Several things to note: 
- The line frequency was changed in the middle of the lock stretch.
- This lock stretch has been with the PSL power at 58.7W (we hope to run ER10 / O2 at 50 W).
- Alignment of SRC optics is being slowly changed by commissioners
- Robert has also been playing with Intensity Noise coupling, which is currently limiting the sensitivity at these high frequencies, so the SNR of the line may be varying quite wildly.
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jeffrey.kissel@LIGO.ORG - 12:59, Thursday 06 October 2016 (30271)
The past and current lock stretches at 60 W were unintentional consequences of a readjustment of the PSL HPO output waveplate without changing the power request back to 50 W (which had been changed to be 60 W yesterday when it was identified that the HPO wasn't putting out enough juice; see LHO aLOG 30239 and LHO aLOG 30260).

We've now, mid-lock readjusted the power back down to 50W, so we expect to return to normal ER10/O2-like operation. So the CAL lines should be measured beyond this point.
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