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Reports until 16:11, Thursday 05 January 2017
H1 General
cheryl.vorvick@LIGO.ORG - posted 16:11, Thursday 05 January 2017 (32995)
Ops Day Summary:

TITLE: 01/05 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 68.9378Mpc
INCOMING OPERATOR: None
SHIFT SUMMARY:

Images attached to this report
H1 ISC
sheila.dwyer@LIGO.ORG - posted 14:48, Thursday 05 January 2017 (32994)
quick jitter measurement,

While LLO was down, Cheryl took the interferometer to commisioning at 22:10 UTC do the jitter measurements described in WP 6384  This took about 7 minutes.  

We had not redone a jitter injection since the model rates were increased to 16kHz.  I redid the injections, and got good measurements to about 2kHz where the sensor noise of the IMC WFS limits the measurement.  

The new measurements are included in the attached noise budget plot, which is still missing some noises but has an estimate of the noise from the ITM elliptical baffles based on data that Annamaria and Robert took durring PEM injections in December.  

Images attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 13:39, Thursday 05 January 2017 (32992)
Ops Day Transition and Mid-Day Update:

TITLE: 01/05 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 64.9223Mpc
OUTGOING OPERATOR: Nutsinee
CURRENT ENVIRONMENT:
    Wind: 10mph Gusts, 9mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.17 μm/s
QUICK SUMMARY:

LHO FMCS
bubba.gateley@LIGO.ORG - posted 11:24, Thursday 05 January 2017 (32991)
Heat Changes in the LVEA and EY chilled water pump trip
Early this morning I noticed the LVEA temperature falling. Around 8:00 A M local time, I brought in 1 stage of heat in Zone 3A, this brought the temperature up. 3A is currently not one of the four zones controlled by the VARIAC transformers so I am reducing this zone and will slightly increase Zone 4 and 5 from 8 to 9 ma, which are controlled by the VARIACS. This should help stabilize the temperatures.

Around that same time this morning Nutsinee informed me that she had critical alarm at EY chiller yard. I looked into the alarm and found that CWP-1 had tripped. Fortunately, this trip occurred during one of the chiller off cycles. I started CWP-2 and reset CWP-1, all seems to be good so far.   
H1 CAL (ISC)
jeffrey.kissel@LIGO.ORG - posted 09:47, Thursday 05 January 2017 - last comment - 14:02, Sunday 08 January 2017(32989)
Calibration Reference Measurement Analysis; Old (2016-11-12) vs. New (2017-01-04) with Updated AA/AI Filter Gain
J. Kissel

I've analyzed the reference data taken from 2017-01-03, and re-analyzed the data from 2016-11-12 with updated matlab analysis code that includes the LHO-only bug-fix regarding the gain of the AA/AI filter model (see LHO aLOG 32907). The results are tabulated below. 
                                                                           MAP     (68% C.I.)  MAP       (68% C.I.)

 Date                                                  2016-11-12          2016-11-12          2017-01-03
                                                   (former analysis)       (new analysis)       (new analysis)
 Optical Gain                K_C         [ct/m]        1.15e6              1.164e6 (0.09%)     1.086e6   (0.07%)
 Couple Cav. Pole Freq.      f_c         [Hz]          346.7               346.7   (0.4%)      360.4     (0.4%)
 Residual Sensing Delay      tau_C       [us]          2.3                 2.3     (50%)       0.65      (200%)
 SRC Detuning Spring Freq.   f_s         [Hz]          7.4                 7.4     (1.1%)      6.9       (0.5%)
 Inv. Spring Qual. Factor    1/Q_s       [ ]           0.05                0.05    (8.7%)      0.03      (12%)

 UIM/L1 Actuation Strength   K_UIM       [N/ct]        8.164e-8            8.104e-8  (0.2%)    8.091e-8  (0.2%)
 PUM/L2 Actuation Strength   K_PUM       [N/ct]        6.841e-10           6.773e-10 (0.03%)   6.768e-10 (0.02%)
 UIM/L3 Actuation Strength   K_TST       [N/ct]        4.389e-12           4.389e-12 (0.04%)   4.357e-12 (0.02%)


As expected, with the 2016-11-12 reference measurements re-analyzed, the estimated sensing function gain has increased by ~1%, and the actuation function have decreased by a few %.

Further, we see that -- also as expected -- the 2017-01-04 reference measurements show some evolution of the optical sensing parameters, no evolution of the UIM and PUM stage actuation strengths, and a few % change in TST actuation strength change due to charge evolution.

The steps forward from here:
- Convert the actuation strength in [N/ct] to [N/A] or [N/V^2] so we can create an updated reference parameter set for the DARM loop model
- Compare the new open loop gain model against measurements
- Use the loop model tp push new reference values to the front end CAL-CS model (changing the optical plant compensation, and the gain of the actuator compensation, L2/L3 change has already been pushed)
- Use the loop model to push new EPICs records that document model values at calibration line frequencies (the biggest change will be from the L2/L3 cross-over upgrade)   << this is the major problem that's causing bad h(t) calibration flag
- Use the new loop model to push a new set of GDS FIR correction filters (small changes due to better AA/AI model)
- Confirm that time-dependent correction factors are within an expected range  << if/when in range, this should green light the h(t) calibration flag
- Use the new loop model to generate DCS FIR filters to recalibrate the all data from the post-winter break from raw DARM_ERR and DARM_CTRL.
- Push hard for uncertainty estimations for both the first part of O2 and data post-winter break.

There's a ton of librarian information that I need to post that documents where all this data came from and what scripts were used, but I'll post as a comment later today.
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:02, Sunday 08 January 2017 (33090)
J. Kissel

I repost the table, without typos in the (new analysis) columns in actuation:
                                                                           MAP     (68% C.I.)  MAP       (68% C.I.)

 Date                                                  2016-11-12          2016-11-12          2017-01-03
                                                   (former analysis)       (new analysis)       (new analysis)
 Optical Gain                K_C         [ct/m]        1.15e6              1.164e6 (0.09%)     1.086e6   (0.07%)
 Couple Cav. Pole Freq.      f_c         [Hz]          346.7               346.7   (0.4%)      360.4     (0.4%)
 Residual Sensing Delay      tau_C       [us]          2.3                 2.3     (50%)       0.65      (200%)
 SRC Detuning Spring Freq.   f_s         [Hz]          7.4                 7.4     (1.1%)      6.9       (0.5%)
 Inv. Spring Qual. Factor    1/Q_s       [ ]           0.05                0.05    (8.7%)      0.03      (12%)

 UIM/L1 Actuation Strength   K_UIM       [N/ct]        8.164e-8            8.104e-8  (0.2%)    8.091e-8  (0.2%)
 PUM/L2 Actuation Strength   K_PUM       [N/ct]        6.841e-10           6.773e-10 (0.03%)   6.768e-10 (0.02%)
 UIM/L3 Actuation Strength   K_TST       [N/ct]        4.389e-12           4.347e-12 (0.04%)   4.357e-12 (0.02%)
Note that (new analysis) sensing function parameter fits are MCMC results, not nlinfit results, which are what is used for updating the DARM loop model. However, MCMC results are consistent with the uncertainty of the nlinfit results, so we consider the results interchangeable. Rather, we use the MCMC results for response function uncertainty, where we use nlinfit results to update the DARM loop model -- we should and will use MCMC results for updating the DARM loop model in the future such that we have a self-consistent pipeline from reference measurement analysis to response function uncertainty estimation. 

I attach an update to the sensing function plot for each reference data set which improves the MCMC fit results vs. measurement plot to show residuals and parameter values with uncertainties, such that it can now be directly compared to the same plot produced by the nlinfit code.

As promised, a complete description of how these results were generated:

            :::: How I generated 2016-11-12 (new analysis) ::::
---------
- Updated measurement base-level processing scripts and DARM model, which fixes the AA/AI filter gain analysis bug identified in LHO aLOG 32907),
${CalSVN}/aligocalibration/trunk/Runs/O2/DARMmodel/src/
    DARMmodel.m        (r4093, lc: r3511)
    computeActuation.m (r4093, lc: r4003)
    computeSensing.m   (r4093, lc: r4025)

---------
- Generated a new fit for actuation parameters using MCMC analysis:
pre-process actuation measurements using
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/FullIFOActuatorTFs/
        actuatorCoefficients_Npct.m (r4065, lc: r4065)
which spits out text files of the actuation function for each stage with portions known to negligible uncertainty removed (e.g. frequency dependence of SUS dynamics, AI filter shape, etc.),
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Measurements/FullIFOActuatorTFs/2016-11-12/
        2016-11-12_H1SUSETMY_L1_actuationStrength_Npct.txt (r4111, lc: r4111)
        2016-11-12_H1SUSETMY_L2_actuationStrength_Npct.txt (r4111, lc: r4111)
        2016-11-12_H1SUSETMY_L3_actuationStrength_Npct.txt (r4111, lc: r4111)
which are then loaded into
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/FullIFOActuatorTFs/
        fitActCoefs_Npct.m (r3977, lc: r3977)
where each stage is fit independently, so you have to switch the variable "stage" between 'L1', 'L2', or 'L3'.
Running on ONLY the 2016-11-12 reference measurement time (instead of two days of measurements, as Darkhan originally did)
   dateListRef = {'2016-11-12'};
   gpsListRef = [1162969230];

yields the above results. 

There's a typo in the above table: the new analysis of L3/TST actuator coefficient is 4.347e-12 [N/ct], as shown in the above attachement https://alog.ligo-wa.caltech.edu/aLOG/uploads/32989_20170105090730_2016-11-12_H1_SUSETMY_ACT_COEF_REF_fitCorner.pdf

---------
- Generated a new fit for the sensing function parameters using nlinfit and MCMC analysis:
pre-process sensing function measurements with
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/PCAL/
        fitDataToC_20161116.m (r4040, lc: r4028)
which produces an nlinfit list of parameters on the IFO optical plant (i.e. with stuff known to negligible uncertainty removed, like frequency dependence of OMC DCPD high frequency electronics), and also spits out a text file of that IFO optical plant for MCMC fitting,
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Results/Sensing
        2016-11-12_H1_meas_sensingTF_withoutDCPDTFs_ctpm.txt (r4079, lc: 4072)
This is loaded into 
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/PCAL/
        fitCTF_mcmc.m (r4112, lc: r4112)
to produce the MCMC maximum a posteriori (MAP).

Even though all MCMC results are repeated using python code, the sensing function parameter's posterior distribution from the above matlab MCMC code are exported to text:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Results/Sensing/
2016-11-12_H1_sensing_burn80p_nWalk100_output.txt      (r4079, lc: r4077)
2016-11-12_H1_sensing_burn80p_nWalk100_posteriors.txt  (r4079, lc: r4079)
Actuator parameter posterior distributions are not yet exported from the matlab code.

            :::: How I generated 2017-01-03 (new analysis) ::::
--------
- Used the updated versions of same the base-level processing scripts described above for 2016-11-12 (new analysis)

--------
- Generated a fit for actuation parameters using MCMC analysis:
Above mentioned actuation function pre-processing script copied from ER10 directory to O2 directory (prior to making aesthetic changes to the script in rev 4065),
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/FullIFOActuatorTFs/
        actuatorCoefficients_Npct.m (r3811, lc: r3811)
became
    ${CalSVN}/aligocalibration/trunk/Runs/O2/H1/Scripts/FullIFOActuatorTFs/
        fitDataToA_20170103.m (r4095, ls: r4061)                                (Note the intentional name change to match sensing function scripts)
which produces text files of actuation functions with frequency dependence known to negligible uncertainty removed,
    ${CalSVN}/aligocalibration/trunk/Runs/O2/H1/Results/FullIFOActuatorTFs/    (Note change in location because the text files are a result,
        2017-01-03_H1SUSETMY_L1_actuationStrength_Npct.txt (r4095, lc: r4056)    not a part of the measurements)
        2017-01-03_H1SUSETMY_L2_actuationStrength_Npct.txt (r4095, lc: r4056)
        2017-01-03_H1SUSETMY_L3_actuationStrength_Npct.txt (r4095, lc: r4056)
which are analysized by the MCMC code copied over from ER10 to O2,
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/FullIFOActuatorTFs/
        fitActCoefs_Npct.m (r3977, lc: r3977)
became
    ${CalSVN}/aligocalibration/trunk/Runs/O2/H1/Scripts/FullActuatorTFs/
        fitATF_mcmc_20170103.m                                                  (Note the intentional name change to match sensing function scripts)
and again, run individually for each stage on 2017-01-03 reference measurement.

--------
- Generated a fit for sensing function parameters using nlinfit and MCMC analysis,
pre-process sensing function measurements with a new copy of
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/PCAL/
        fitDataToC_20161116.m (r4040, lc: r4028)
now named
    ${CalSVN}/aligocalibration/trunk/Runs/O2/H1/Scripts/SensingFunctionTFs/     (Note folder change to match actuator scripts and the rest
        fitDataToC_20170103.m (r4095, ls: r4090)                              of O2 directory structure)
which produces an nlinfit list of parameters on the IFO optical plant (i.e. with stuff known to negligible uncertainty removed, like frequency dependence of OMC DCPD high frequency electronics), and also spits out a text file of that IFO optical plant for MCMC fitting,
    ${CalSVN}/aligocalibration/trunk/Runs/O2/H1/Results/Sensing
        2017-01-03_H1_meas_sensingTF_withoutDCPDTFs_ctpm.txt (r4095, lc: 4056)
This is loaded into a copy of
    ${CalSVN}/aligocalibration/trunk/Runs/ER10/H1/Scripts/PCAL/
        fitCTF_mcmc.m (r4041, lc: r4041)
    (copied prior to aesthetic changes to fit vs. measurement plot which now shows residuals in r4112 as described above)
which is now
    ${CalSVN}/aligocalibration/trunk/Runs/O2/H1/Scripts/PCAL/
        fitCTF_mcmc_20170103.m (r4095, lc: r4091)
to produce the MCMC maximum a posteriori (MAP) (and also has the same aesthetic changes as the ER10 version, r4112).

Even though all MCMC results are repeated using python code, the sensing function parameter's posterior distribution from the above matlab MCMC code are exported to text:
${CalSVN}/aligocalibration/trunk/Runs/O2/H1/Results/SensingFunctionTFs/
2017-01-03_H1_sensing_burn80p_nWalk100_output.txt       (r4095, lc: 4058)
2017-01-03_H1_sensing_burn80p_nWalk100_posteriors.txt   (r4095, lc: 4058)
Actuator parameter posterior distributions are not yet exported from the matlab code.
     
----------
A super-duper thanks to Darkhan, Kiwamu, and Evan for writing the brunt of these functions. It took a while to find everything, how the analysis flow was to go, and how to correctly into file names, but it otherwise works like a charm with very reproducible results. I look forward to making the functions even more streamlined, and potentially merging functionality so there's not so many functions of which to keep track. 
----------
Non-image files attached to this comment
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 08:01, Thursday 05 January 2017 (32988)
Ops Owl Shift Summary

TITLE: 01/05 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC

STATE of H1: Observing at 68.823Mpc

INCOMING OPERATOR: Cheryl

SHIFT SUMMARY: Locked and observe the entire shift. Low frequency noise (10-20Hz) also has been apparent all night. a2l didn't seem to help. 

LOG:

15:30 out of observe to run a2l

15:46 Back to observe.

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 04:49, Thursday 05 January 2017 (32985)
Ops OWL mid-shift summary

Still up and observing. Low wind, low useism. LLO is down.

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 01:43, Thursday 05 January 2017 (32984)
Late Ops Owl Shift Transition

TITLE: 01/05 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC

STATE of H1: Observing at 68.6153Mpc

OUTGOING OPERATOR: Ed

CURRENT ENVIRONMENT: Wind: 13mph Gusts, 10mph 5min avg Primary useism: 0.02 μm/s Secondary useism: 0.15 μm/s

QUICK SUMMARY: Not much. Verbal alarm complains about TCSY low flow. This is a known issue. The chiller on the mezzanine reported nomal flow rate.

H1 General
edmond.merilh@LIGO.ORG - posted 00:03, Thursday 05 January 2017 (32983)
Shift Summary - Day Transition
TITLE: 01/05 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 67.6951Mpc
INCOMING OPERATOR: Nutsinee
SHIFT SUMMARY:
Pretty quiet shift.
Darm is showing some low frequency noise and no improvement in range after I ran the a2l script. Perhaps it's the EY HVAC?
LOG:

02:49 H1 back to NLN

02:59 a2l. PIT out a little. YAW out a lot

03:14 Intention Bit set to Observing

04:32 Prop airplane flyover. 

LHO FMCS
john.worden@LIGO.ORG - posted 21:18, Wednesday 04 January 2017 (32980)
EY HVAC

I think our fan flow rates at EY are bogus - In order to improve temperature control Bubba and I adjusted flows on SF1 and after no response decided to turn on SF2.

Plot of the idicated flows attached - SF2 (red trace) shows 7 days of somewhat uniform flow even though we just turned it on today. Blue trace does not show expected results of adjusting pitch control as we did today.

If temperature control has improved by tomorrow we will leave the second fan running (two fans operating). Please let us know if there is evidence of increased vibration or noise due to this fan addition.

Changes were made between 4:45  pm and 5:00 pm local time.

Images attached to this report
H1 General
edmond.merilh@LIGO.ORG - posted 21:17, Wednesday 04 January 2017 - last comment - 10:07, Thursday 05 January 2017(32979)
Dropping from Observing Intent to run a2l

I was left instructions to run a2l a few hours into the new lock. It's a bit early but the range has deteriorated too much for my pleasure and the YAW coherence is coming apart pretty bad. I've informed LLO of my action and will also inform them when I'm finished and back in the game.

Comments related to this report
edmond.merilh@LIGO.ORG - 21:19, Wednesday 04 January 2017 (32981)

Incidentally, running the a2l script from th MEDM launch screen seems to crash all of the MEDM screens. I thought, at first that it was only the new Ops workstation but I now see it happening on the other workstation as well.

edmond.merilh@LIGO.ORG - 22:01, Wednesday 04 January 2017 (32982)

back to Observing @ 05:23UTC

jim.warner@LIGO.ORG - 10:07, Thursday 05 January 2017 (32990)OpsInfo

Re: running a2l from sitemap->sus->a2l screen crashes medm screens

There was a typo on the a2l button that I must have added before the break. There was an apostrophe at the end of the command for running the a2l script, this obviously was doing something bad. It was actually my punctuation all out of order.  Needed to be ' &  not  & '  .  It's fixed now, a2l should run normally from this screen.

H1 General
edmond.merilh@LIGO.ORG - posted 20:15, Wednesday 04 January 2017 (32978)
Mid-Shift Summary
H1 General (DetChar)
edmond.merilh@LIGO.ORG - posted 19:57, Wednesday 04 January 2017 (32977)
PEM Corner Station MIC Data Spanning Accidental Fire Alarm ACtivation

All times in UTC:

 The attached plot shows that the fier alarm activated at approximately 2 minutes after 00:00UTC.  Lockloss occurred approx 3 minutes after the alarm had been silenced.

It seems that the PSL Mic detected the alarm at roughly 00:02:23 until 00:09:12. The duration of it was approx 7 minutes.

I picked a common, control room StripTool channel, H1:LSC-TR_X_NORM_INMON,  to represent the time of lockloss which seemed to have occurred at approx 00:12:16. Most all of the other mics show a spike feature at the same time as the TR_X plot indicating some correlation. 

Images attached to this report
H1 General
edmond.merilh@LIGO.ORG - posted 19:36, Wednesday 04 January 2017 (32976)
H1 Intention Bit Set To Observing

03:14UTC

LHO VE
kyle.ryan@LIGO.ORG - posted 16:51, Wednesday 04 January 2017 - last comment - 13:39, Monday 09 January 2017(32972)
~1625 hrs. local -> Isolated PT180 from rotating shaft vacuum pumps and exposed PT180 to YBM
~1625 - 1630 hrs. local -> Kyle in and out of LVEA

Shut down rotating shaft vacuum pumps which had been pumping PT180 (BSC8) for the past 8 days.  Also, removed ladder which had been leaning against BSC8.  We should now have enough data to compare and contrast PT180's behavior between when it is exposed/pumped by the YBM to that of when exposed/pumped by a locally mounted turbo.  

Recall that the post-detect era installed Bayard-Alpert gauges PT170, PT180 and PT140 all exhibit a slow upward drift that the iLIGO era Cold Cathode gauges (sampling same vacuum volume) do not.  Understanding/believing our gauges is critical.  

We will decouple the vacuum pumps from PT180 on the next maintenance day.   
Comments related to this report
chandra.romel@LIGO.ORG - 14:43, Thursday 05 January 2017 (32993)

Pressure reading from PT180 is once again rising after being valved into main volume. We suspect the water load is causing this. End stations show no sign but also get 2.5x more pumping speed from cyropumps due to smaller volume.

PT140 pressure reading on diagonal volume (no crypopump) started dropping this week after a three month incline. These changes are due to LVEA temperature fluctuations.

Images attached to this comment
chandra.romel@LIGO.ORG - 13:39, Monday 09 January 2017 (33109)

Correction:  water pumping speed is more like 1.8x more at end stations. 

Corner volume = 445,000 liters

End volume = 88,000 liters

Corner cyropumping = [100,000 - 3,000] x 2 (L/s)

End cryopuming = 100,000 - 30,000 (L/s)

H1 CAL (CAL)
aaron.viets@LIGO.ORG - posted 14:43, Wednesday 04 January 2017 - last comment - 18:05, Wednesday 11 January 2017(32965)
DCS filters for LHO data for early O2 A (2016)
I have produced filters for offline calibration of Hanford data from the beginning of O2 A until the end of 2016. The filters can be found in the calibration SVN at this location:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/GDSFilters/H1DCS_1163173888.npz

For information on the calibration model, see
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=31693
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=32329
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=32907

For suggested command line options to use when calibrating this data, see:
https://wiki.ligo.org/Calibration/GDSCalibrationConfigurationsO2

The filters were produced using this Matlab script in SVN revision 4050:
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/Scripts/TDfilters/H1_run_td_filters_1163173888.m

The parameters files used (all in revision 4050) were:
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/Common/params/IFOindepParams.conf
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/params/H1params.conf
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/params/2016-11-12/H1params_2016-11-12.conf
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/params/H1_TDparams_1163173888.conf
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Scripts/CAL_EPICS/D20161122_H1_CAL_EPICS_VALUES.m

Several plots are attached. The first four (png files) are spectrum comparisons between CALCS, GDS, and DCS. Kappas were applied in both GDS and DCS plots with a coherence uncertainty threshold of 0.4%. Time domain vs. frequency domain comparison plots of the filters are also attached. Lastly, brief time series of the kappas and coherences are attached, for comparison with CALCS.
Images attached to this report
Non-image files attached to this report
Comments related to this report
aaron.viets@LIGO.ORG - 06:25, Thursday 05 January 2017 (32986)
More plots from beginning of O2 (Nov 30) to show that these filters still have the right model and EPICS.
Images attached to this comment
Non-image files attached to this comment
aaron.viets@LIGO.ORG - 07:01, Thursday 05 January 2017 (32987)
Same set of plots one more time, this time in early ER10 (Nov 16). Note that kappas were not applied in the GDS pipeline this time, leading to a notable difference in the spectra.
Images attached to this comment
Non-image files attached to this comment
aaron.viets@LIGO.ORG - 18:05, Wednesday 11 January 2017 (33169)CAL
These filters have been updated to account for corrections made to the DARM loop parameters since the AA/AI filter bug fixes. For information on the model changes, see:
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=33153

The updated filters were produced using all the same files (updated versions) in SVN revision #4133. The only exception is that the EPICS file and the parameters file to produce it were:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Scripts/CAL_EPICS/DCS20161112_H1_CAL_EPICS_VALUES.m
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Scripts/CAL_EPICS/callineParams_20161118.m

Note from the plots the slight discrepancy between GDS and DCS, presumably due to the corrections to the model. Also note that DCS and CALCS do not agree on the kappas. This is likely not cause for concern, as the model used to compute them was different. The EPICS and pcal correction factors were produced using the same parameter files as the filters, so they should be correct.
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