Displaying reports 20621-20640 of 87740.Go to page Start 1028 1029 1030 1031 1032 1033 1034 1035 1036 End
Reports until 12:16, Friday 28 April 2023
H1 ISC
elenna.capote@LIGO.ORG - posted 12:16, Friday 28 April 2023 (69153)
ADS gain increased

The ADS gain has been doubled so we can converge the ADS faster and move to camera servos. I updated the ads gains in LSC params to be 20. The LSC params value is used by the ISC_LOCK guardian in Lownoise ASC and by the Camera servo guardian. We should keep an eye on this for the next few locks and check that this doesn't rail the ADS at any point.

H1 ISC
elenna.capote@LIGO.ORG - posted 12:15, Friday 28 April 2023 - last comment - 16:36, Monday 01 May 2023(69152)
CARM gain increased

We have determined we want to operate with higher carm gain. Instead of slowly increasing the carm gain during thermalization, we decided to try increasing it from the start and avoid causing glitches. The SERVO gain for REFL A and B will both be set to 9 dB instead of 6 dB in LASER NOISE SUPPRESSION.

Comments related to this report
gabriele.vajente@LIGO.ORG - 12:22, Friday 28 April 2023 (69154)

The CARM gain adjustment in the THERMALIZATION guardian has been disabled yesterday

elenna.capote@LIGO.ORG - 16:36, Monday 01 May 2023 (69225)

I measured the CARM gain today 30 minutes and 1 hour into the lock stretch to see the effect of the 3 dB increase. See attached plot. I think this plot shows, as predicted, we start with the UGF around 25 kHz, which is a bit high. However, we thermalize back to about where we want the UGF to be. We have not completely suppressed the high frequency "tail" shape in DARM with this gain increase, but we are unlikely to win much more by increasing the gain further. Daniel and I ran a long coherence from the long lock this weekend, see plot, that shows that we are not limited very much at 1 kHz by frequency noise (this time stretch comes well after thermalization is complete). The high coherence around 100 Hz is probably coming from PRCL or SRCL. We think this is a decent place to run for O4. I declare our CARM adjustments complete! I will unplug the SR785 at the next possible opportunity.

Images attached to this comment
Non-image files attached to this comment
H1 CDS (CDS)
jennifer.wright@LIGO.ORG - posted 11:55, Friday 28 April 2023 (69150)
Issue with labutils conda environment

Jennie, Craig, Erik

I've been having trouble importing functions into python scripts from the labutils packages while on the control room workstations, even while in the labutils conda environment.

For some reason I can still run thermal_state_capture from the command line though...

Just putting this here in case anyone else is having this issue in the future.

The temporary fix (from Erik) is to manually add labutils to your path before activating the environment each time from the command line:

export PYTHONPATH=/ligo/gitcommon/labutils
 

H1 ISC
marc.pirello@LIGO.ORG - posted 11:34, Friday 28 April 2023 (69107)
Power Supply Survey

We had a look at the next set of power supplies that likely have siezed fans and we found the following,

EY - All supplies register less than 80 degrees on input with sufficient air flow, no issues.

EX - VDD-1 LHS U12 24V H1-PCAL registers at 115F in the front, lower in the back.  Low temperature gradient & high temperature vs ambient = bad fan

EX - Remaining supplies regiseter 80 degrees no issues.

CER - C2 U34 RHS 92F front, 93F back, hard to feel air flow ISC-C3 -24V S1201927.  Low temperature gradient & moderate temperature vs ambient = bad fan

CER - C2 U30 RHS 90F front 115F back, low air flow, high heat on front mount, ISC-C2 -18V S1201978.  Moderate temperature gradient & moderate temperature vs ambient = failing fan (not failed yet)

CER - C3 U22 RHS 101F front, 104F back, low air flow, SEI-C4 BSC1, S1201989.  Low temperature graidnet & high temperature vs ambient = bad fan

CER - Remaining supplies regiseter 80 degrees no issues.

There are a few supplies in the CER which are not easily measured in the front.  These supplies have obstructed input vents so it is hard to tell if the fan is bad, or the supply is starved for fresh air.

M. Pirello, F. Mera

 

H1 SEI
ryan.crouch@LIGO.ORG - posted 10:51, Friday 28 April 2023 (69145)
BRS Drift Trends - Monthly - FAMIS

Closes FAMIS 17558

Both figures look nominal

Images attached to this report
H1 CAL (CAL, ISC, OpsInfo)
jeffrey.kissel@LIGO.ORG - posted 10:30, Friday 28 April 2023 (69147)
Quick Broadband PCAL Injection
J. Kissel, E. Goetz

   /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O3/H1/Measurements/FullIFOSensingTFs/
       2023-04-28_1702UTC_H1_PCALY2DARMTF_BB_3min.xml

More later.
H1 CAL
evan.goetz@LIGO.ORG - posted 09:58, Friday 28 April 2023 (69143)
Changed/installed CALCS demod bandpass filters
J. Kissel, E. Goetz

We have changed and updated CALCS bandpass filters for LINE4, LINE10 so that they could read temporary CAL_AWG_LINES thermalization line (see LHO aLOG 68947) (24.5 Hz) and the X comparison line (410.2 Hz). In addition, we installed bandpass filters on the EXT DEMOD in the PCAL X and PCAL Y comparison demods:
CS_TDEP_PCAL_LINE4_ERR_DEMOD_SIG 0 butter("BandPass",6,24.45,24.55)
CS_TDEP_PCAL_LINE4_EXT_DEMOD_SIG 0 butter("BandPass",6,24.45,24.55)
CS_TDEP_PCAL_LINE4_PCAL_DEMOD_SIG 0 butter("BandPass",6,24.45,24.55)
CS_TDEP_PCAL_LINE10_ERR_DEMOD_SIG 0 butter("BandPass",6,410.17,410.23)
CS_TDEP_PCAL_LINE10_EXT_DEMOD_SIG 0 butter("BandPass",6,410.17,410.23)
CS_TDEP_PCAL_LINE10_PCAL_DEMOD_SIG 0 butter("BandPass",6,410.17,410.23)
CS_TDEP_PCAL_X_COMPARE_EXT_DEMOD_SIG 0 butter("BandPass",6,410.19,410.21)
CS_TDEP_PCAL_Y_COMPARE_EXT_DEMOD_SIG 0 butter("BandPass",6,410.29,410.31)

Also in the PCAL X and PCAL Y comparison demods, we installed the same 300 s low-pass filter to the EXT demod:
CS_TDEP_PCAL_X_COMPARE_EXT_DEMOD_I 0 butter("LowPass",4,0.0033)
CS_TDEP_PCAL_X_COMPARE_EXT_DEMOD_Q 0 butter("LowPass",4,0.0033)
CS_TDEP_PCAL_Y_COMPARE_EXT_DEMOD_I 0 butter("LowPass",4,0.0033)
CS_TDEP_PCAL_Y_COMPARE_EXT_DEMOD_Q 0 butter("LowPass",4,0.0033)
H1 General
ryan.crouch@LIGO.ORG - posted 08:04, Friday 28 April 2023 (69139)
OPS day shift start

TITLE: 04/28 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Commissioning
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 13mph Gusts, 10mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.13 μm/s
QUICK SUMMARY:

H1 General (ISC, SEI)
austin.jennings@LIGO.ORG - posted 00:03, Friday 28 April 2023 - last comment - 16:44, Friday 28 April 2023(69121)
Thursday Eve Shift Summary

TITLE: 04/27 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Commissioning
SHIFT SUMMARY:

- IFO is locked at NLN, but not in Observing Mode due to unreconciled observe SDFs, attached below, so I am leaving it in Commissioning mode - Tagging ISC

- Lock #1:

- Lock #2:

Other Notes:

- 2:14 UTC - inc EQ from South Georgia - 5.8 mag eq

- 3:25 UTC - EX saturation, IFO was a little unstable, seeing ringups in INP1_P_INMON, MICH_Y_INMON, CSOFT_P_OUT, CHARD_Y_OUT, and DHARD_Y_OUT

LOG:                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                           

Start Time System Name Location Lazer_Haz Task Time End
19:56 LVEA LAZER HAZARD LVEA YES THE LVEA IS LASER HAZARD 19:55
23:45 ISC Elenna CR N Switching over camera filters 23:52
23:51 ISC Elenna CR N QUIET TIME Measurement 00:07
01:52 GAINS Rick S Y Arm N Bike ridin 03:00
Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 16:44, Friday 28 April 2023 (69173)SQZ

I've added some lines to the SQZ_FC guardian DOWN state to return the (currently unused) H1:SQZ-FC_LSC_DOF{3,4}_TRAMP to 5 seconds, rather than either 0 or 5 seconds, depending on the state of FC2. This to avoid the sdf diffs Austin found: FC_LSC sdf diffs. The guardian shows at some point we planned to send WFS_A_I to DOF3 for Laser AOM feedback...

H1 General (OpsInfo)
austin.jennings@LIGO.ORG - posted 21:47, Thursday 27 April 2023 (69137)
Mid Shift Eve Report

All was going well until we had what I believe to be a ground motion related lockloss. Then when reacquiring lock, I ran into the same issue I did last night, despite resetting all the values to their working state from Ryan's alog. I'll keep trying...

 

EDIT: For sanities sake, I have attached a screen shot of the changes I implemented, which are the exact same as the ones noted in the alog.

 

EDIT 2: I have also screenshotted the SDF changes to show that they're actually there and that they're the correct channels, but for some reason it doesn't seem to be working.

 

EDIT 3: On the 5th(6th?) attempt it finally caught, and was able to go up ISC. This might need to be looked into more tomorrow

Images attached to this report
H1 General (DetChar)
austin.jennings@LIGO.ORG - posted 18:47, Thursday 27 April 2023 - last comment - 19:52, Thursday 27 April 2023(69132)
O4 Officially Observing!!

Thanks to the hard work from everyone at LHO, we have reconciled all observing.snap SDFs and have flipped the intention bit and LHO is now...

officially 🥳 OBSERVING FOR THE FIRST TIME IN O4 🥳

👏👏👏👏🙌🙌🙌

The mode was acquired at 00:53 UTC, Apr 28th and I intend on leaving it in this mode to allow for some offsite data analysis.

Congratulations to all!!

Comments related to this report
michael.landry@LIGO.ORG - 19:52, Thursday 27 April 2023 (69136)

Terrific work all to get to this state early in the engineering phase!

H1 ISC
jenne.driggers@LIGO.ORG - posted 18:00, Thursday 27 April 2023 (69130)
Several guardian nodes excluded - must fix

I have added 3 more nodes to the guardian exclude list for tonight.  This is not at all what we want, but they need further thought tomorrow.  This lets us flip the Observing Bit tonight.

The DIAG_EXC node is not happy, since there are 2 calibration lines that it is flagging as going on.  We will have these lines on for at least through our calibration week to monitor the SRCL detuning, but then they'll (I think) be turned off.  So, it's excluded.

Also, the THERMALIZATION guardian needs to be reworked so that it can return OK some time sooner than many hours after we've locked. I've excluded it, and I've also excluded ISC_LOCK since it won't return OK until Thermalization is OK.  We must re think these and fix them tomorrow or ASAP.  For these two, this will be the state of things during the observing run, and we clearly need to be able to set the observing bit earlier than many hours after having locked.

Attached is the list of excluded nodes, with my comments on our needing to deal with these three nodes.

Images attached to this report
H1 ISC
jenne.driggers@LIGO.ORG - posted 17:49, Thursday 27 April 2023 (69129)
Yet more SDFs - SDF is clear

I've accepted the last few SDF diffs we've got.  Some still need review tomorrow, but for the most part I think these are now matching what we have in safe.snaps. 

SDF is now clear, and so we are one major step closer to pushing the Intent Bit!

Images attached to this report
H1 ISC (OpsInfo)
ryan.short@LIGO.ORG - posted 17:46, Thursday 27 April 2023 - last comment - 11:42, Friday 28 April 2023(69128)
E{X,Y}_ISC SDF Observe.snap files are Linked to Safe.snap

R. Short, J. Driggers, T. Shaffer

We've learned that the main issue with locking last night and this morning stemmed from whitening gains and gain steps for the TR_A/B channels in the EX/Y_ISC models being accepted as all zeros (see TJ's alog 69103 for details). I've also discovered that the OBSERVE.snap file is in fact symlinked to a SAFE.snap, which means these two tables are the same. We assume someone accepting SDFs at NLN had accepted these to zero not knowing about the linked tables. TJ and I plan to reconcile this issue tomorrow morning and double-check other models that have recently been added to the SDF_REVERT state.

In the effort to be able to use the Observation intent bit tonight -- meaning all SDF differences must be cleared -- I have accepted these differences, knowing they are incorrect for the locking process. If we are attempting to relock before we can fix the table issue, these values must be changed back to the listed setpoints (see attached screenshots).

Images attached to this report
Comments related to this report
betsy.weaver@LIGO.ORG - 11:42, Friday 28 April 2023 (69149)

Yep, that was me, sorry. Not loving the symbolically linked SDF files now! Sounds like there are more work arounds in process, thanks TJ, Ryan, and Ryan.

H1 SQZ (SQZ)
nutsinee.kijbunchoo@LIGO.ORG - posted 16:35, Thursday 27 April 2023 - last comment - 10:43, Friday 28 April 2023(69116)
Added fudge factor to SQZ BLRMS

I added fudge factors to squeezer BLRMS NULL gain so the monitors read 0dB when we are not squeezing. All of the changes have been accepted in SDF.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 10:43, Friday 28 April 2023 (69144)
BLRMS 30mins after NLN (brown trace) 3 hours after NLN (mint trace) Comment
# center freq BLRMs calc DARM calc BLRMs calc DARM calc
1 80Hz n/a (new lines) -0.9 n/a -0.4 Check for lines
2 135Hz -1.2 -1.4 -0.8 -1.4 A bit off
3 325Hz -1.5 -1.9 -1.8 -2.3 Underestimated
4 750Hz -2.4 -2.5 -3.0 -3.1 Great
5 1700Hz -2.2 -2.1 -3.2 -3.0 Great
6 4650Hz 0 0 -1.8 -1.8 Great

Checking on the reliability of these BLRMs by comparing the BLRMs H1:SQZ-DCPD_RATIO_{1-6}_DB_MON with DARM SQZ vs No SQZ. Above 750Hz, BLRMS#4,5,6 exactly agree with whats seen in DARM.

#1 80Hz BLRM isn't making sense, maybe we're not taking into account the PCALX 77.7Hz line (alog68289). #3 325Hz seems like the scaling is underestimating SQZ in the BLRMS and something is off with #2 135Hz but this is a region we've ben seeing varying noise.

"BLRMS calc" is the mean of H1:BLRMs H1:SQZ-DCPD_RATIO_{1-6}_DB_MON at the time. Note the attached plot is just the mean and not showing the min/max which is quite noisy.
"DARM calc" is me, by eye using DTT cursors, seeing the difference in dB (SQZ overview > DARM FDS template) between SQZ and no SQZ centered in the BLRMS frequency in the attached DARM plot.
Images attached to this comment
H1 ISC
gabriele.vajente@LIGO.ORG - posted 15:38, Thursday 27 April 2023 - last comment - 22:53, Thursday 27 April 2023(69108)
Improved ASC-INP1 loops

Elenna, Gabriele

We noticed coherence between DARM and INP1_P and INP1_Y. So we redesigned the loops to have a much larger roll-off at 10 Hz and above, for both P and Y

Images attached to this report
Comments related to this report
gabriele.vajente@LIGO.ORG - 16:50, Thursday 27 April 2023 (69118)

Elenna, Gabriele

Same treatment for PRC2 PIT adn PRC2 YAW, sicne those showed coherence too. Attached plots compare the old and new controllers.

Images attached to this comment
elenna.capote@LIGO.ORG - 16:57, Thursday 27 April 2023 (69123)

We have adjusted the new filters for PRC2 and INP1 to be used by the guardian from Engage ASC for Full IFO onward. We are using probably a factor 10 less gain for INP1 P now than normal for powering up. This may be a problem, so please keep an eye on ASC stability during power up. Normally we would have the factor 10 gain for INP1 all the way through Max Power, and then the gain would be lowered in Lownoise ASC.

I have accepted these new filters in the observe SDF.

elenna.capote@LIGO.ORG - 17:07, Thursday 27 April 2023 (69125)

Looks like some low frequency improvement from this change!

Images attached to this comment
gabriele.vajente@LIGO.ORG - 17:14, Thursday 27 April 2023 (69126)

Comparison of ASC control signals with the old (RED) and new (BLUE) controllers. CHARD controllers are the same, but the noise improved probably due to the reduction in the other loops' noise

I think we don't see an improvement in INP1_P because we are hitting the numerical limit of the PSD computation

Images attached to this comment
elenna.capote@LIGO.ORG - 22:53, Thursday 27 April 2023 (69138)

We have successfully powered up with these new loops.

H1 SQZ
camilla.compton@LIGO.ORG - posted 12:54, Thursday 27 April 2023 - last comment - 09:39, Friday 28 April 2023(69096)
ADF angle and RMS change while Thermalizing

SQZ Team. Last night we left the ADF on at 1300Hz while the IFO thermalized. See attached plot for how ADF calculated phase changes 25degrees over the first 5 hours of the IFO lock. We plan to repeat this tonight with the ADF nearer 100Hz (where H1 range is effected by SQZ changes more) and expect less change. See alog 69055 for optimizing SQZ angle during first ~1hour of lock. SQZ angle H1:SQZ-CLF_REFL_RF6_PHASE_PHASEDEG = 140.33 throughout.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 09:39, Friday 28 April 2023 (69142)

Nutsinee left the ADF at 90Hz last night (alog69127) and I've attached the 90Hz thermalization plot. At 90Hz SQZ changes <5 degrees within the first hour so is much more stable than the high frequency squeezing.

I'm unsure what is happening in the first ~10 minutes of NLN when both frequencies change +/-10degrees.

Images attached to this comment
H1 CAL (CAL, DetChar, GRD, ISC, OpsInfo)
jeffrey.kissel@LIGO.ORG - posted 13:58, Wednesday 26 April 2023 - last comment - 12:13, Friday 28 April 2023(69047)
CAL-CS and GDS Calibration Updated
J. Betzwieser, L. Dartez, E. Goetz, J. Kissel, J. Rollins

The details are happening all too fast in order to write them all down here but at the 10000 foot level, as of 2024-04-26 19:54 UTC, we've updated
   - the primary CAL-CS variables that create CAL-DELTAL_EXTERNAL_DQ, which correspond to the interferometrically-measured free parameters (optical gain, cavity pole, actuation gains for TST, PUM, and UIM changes)
       :: Values are informed by last Thursday's 2023-04-20 IFO measurement. No major change here, just pushing these to get them consistent with the rest of the pipeline. Not informed yet by the current state of the IFO, especially the TCS settings and SRCL offsets

   - The "DARM model transfer function function values at calibration line frequencies" EPICs records
       :: Importantly, this comes with changes that are the fall out of LHO:68880 and the solution pyDARM Merge Request 234

   - The GDS-CALIB_STRAIN pipeline has new filters, and importantly its got a configuration change that now using the corner station copy of the PCAL, H1:CAL-DELTAL_REF_PCAL_DQ, as it's measure of the PCAL system rather than the end-station.
       :: Again, this is the fall out of LHO:68880

Many details to come in the comments.
Comments related to this report
jeffrey.kissel@LIGO.ORG - 15:37, Wednesday 26 April 2023 (69054)
Here's a blow-by-blow of what happened:

- Had been locked and powered up to 76W PSL input power for ~3:30 hours

- Louis walked us through the calibration report for what would be pushed upon update from
    /ligo/groups/cal/data/H1/reports/20230420T014029Z/H1_calibration_report_20230420T014029Z.pdf

- Took ISC_LOCK to NLN_CAL_MEAS

- Took a "before change" PCAL broadband injection, 
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O3/H1/Measurements/FullIFOSensingTFs/
        2023-04-26_1925UTC_H1_PCALY2DARMTF_BB_3min.xml
    

- While the broadband was going, took inventory of what filter modules were available for us to place the new IFO-measured free parameters in the 
    H1:CAL-CS_DARM_ERR
    H1:CAL-CS_DARM_ANALOG_ETMX_L1
    H1:CAL-CS_DARM_ANALOG_ETMX_L2
    H1:CAL-CS_DARM_ANALOG_ETMX_L3
filter banks. Found that FM1 and FM2 were available in DARM_ERR, and FM4s were available in the L1, L2, and L3 banks.

- Edited the pydarm command line interface configuration / parameter file,
    /ligo/groups/cal/ifo/H1/pydarm_cmd_H1.yaml
  to chose these filter banks, and a new name for the filter. For the sensing function we chose "ER15_Gain" and "ER15_NoD2N" for the optical gain and cavity pole frequency in FM1 and FM2 of DARM_ERR. For the actuation strengths for the L1, L2, and L3 stages, we chose "Npct_ER15" in FM4.

- Ran the command line interface for exporting the calibration model to the front end (currently using a curated path and pydarm branch)
    :: First, without actually pushing, aka a dry run, which spits out everything it's *going* to push as it stands. The first couple of lines of that output are the IFO-measured free parameters, copied here for future searchability
        Hc: 3.1796e+06 :: 1/Hc: 3.1450e-07
        Fcc: 4.3371e+02 Hz
        Hau: 1.6072e+00 N/A :: 7.5454e-08 N/ct
        Hap: 3.0579e-02 N/A :: 6.2634e-10 N/ct
        Hat: 2.5464e-11 N/A :: 9.6474e-13 N/ct
        These are not that different from what was installed on 2023-04-20 01:15 UTC, see LHO:68856, so we don't expect that much change here.

     :: Then, we actually pushed those values, 
        PYTHONPATH=/ligo/home/louis.dartez/repos/pydarm pydarm export --push
        which spit out to the commanding what it was changing, when it was changing it (but lacked any "done!" message)

- Went CAL-CS model's GDS_TP screen, waited ~5 seconds until the "Modified Filter File Detected" message to appear, then hit "LOAD COEFFICIENTS" (i.e. pressed the H1:FEC-117_LOAD_NEW_COEFF button), and waited another ~10 seconds for it to complete

- Went to each of the above mentioned filter banks and switched over to each of the new filters by hand; FM1 & FM2 in the DARM_ERR, and FM4s in ANALOG_ETMX_L1, ANALOG_ETMX_L2, and ANALOG_ETMX_L3. 

- Took another post-calibration update broad-band injection in order to see how much better / different the calibration is/was, 
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O3/H1/Measurements/FullIFOSensingTFs/
        2023-04-26_1950UTC_H1_PCALY2DARMTF_BB_3min.xml

- Louis, on the side, created / updated new PCAL and DELTAL calibrations for the DTT template, and put them in 
    /ligo/home/louis.dartez/projects/20230426/
        pcal_calib_dtt.txt
        deltal_external_calib_dtt.txt
    
  so, we loaded these in to the 1950UTC DTT template. Hopefully this gives us a more accurate answer for what the systematic error is without all the extra caveats we've had in recent history about "well, the DTT calibration is some old crap, that has an outdated version of the super-Nyquist corrections for DELTAL, so you can't trust the answer *exactly*." While we're not yet confident that you can trust the answer "exactly," we are confident it's at least better. To load in these files,
        :: Hit "Calibration" button to open calibration pop-up window
        :: Select H1:CAL-PCALY_RX_PD_OUT_DQ
        :: Hit "New" to open the labeling pop-up.
            . Enter in a name for the Teference (can be anything, "asdfsdf" for eg)
            . Enter in a Unit of "m"
            . Enter in a Time that's much earlier that now (hold down CTRL and click the down arrow once to change the year to 2022)
            . Hit OK to return to the calibration pop-up
        :: Unselect the check box in every other tab besides "Trans. Func."
        :: Under the "Trans. Func." tab, 
            . Check the box
            . Hit Edit... to open up the transfer function editing window
            . From the toolbar, select File > Open...
            . Navigate to pcal_calib_dtt.txt, and double click it to select, close the pop-up, and have it populate in the TF editing window.
            . Hit "OK" to accept the new TF and close the TF editing window
        :: Hit "Set" to make sure this new calibration sticks.
        :: Repeat the process for H1:CAL-DELTAL_EXTERNAL_DQ using deltal_external_calib_dtt.txt

See 2023-04-26_1950UTC_CalibrationUpdate_BBInjection.png which shows the change between the BB taken after the last calibration update on 2023-04-23, just before this update on 2023-04-26 19:25 UTC, and just after at 2023-04-23 19:50 UTC. This is after we've updated the calibration within the DTT template, so for the first time in a long time, the low-frequency end of phase of this transfer function makes sense "starting" at 0 deg.

- We then went back to nominal low noise, turning the calibration lines back on so as to start measuring the TDCFs again. Even though we've moved around some delays and got rid of some DEMOD phase rotations, the TDCF answers remain about the same before and after the calibration change, as expected. This gives us confidence in what changes we made to pydarm as a result of last week's solutions to long standing mysteries about the EPICs records.

Satisfied with this "first brush" answer, 

- Went to the SDF screen for the CALCS model, and accepted all the new settings (including all the changes to the "DARM model transfer function values at calibration line frequencies") -- see 2023-04-26_1950UTC_CalibrationUpdate_SDFAccept.png.

- Jamie then used the FIR filters generated in that 2023-04-20 report, 
    /ligo/groups/cal/data/H1/reports/20230420T014029Z/
        gstlal_compute_strain_C00_filters_H1.npz
to inform and restart the GST-LAL calibration pipeline, in some way that hopefully he'll document in further comments below.
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jeffrey.kissel@LIGO.ORG - 12:13, Friday 28 April 2023 (69151)
In order to update the pydarm_H1.ini parameter file value for the CALCS foton export of the sensing function, i.e. the "foton_invsensing_tf" parameter in the "[calcs]" section, I've followed the instructions in LHO:47948 to create
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O3/H1/Measurements/Foton/
        2023-04-20_H1CALCS_InverseSensingFunction_Foton_ER15_NoD2N_tf.txt

for future use.
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