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Reports until 16:53, Friday 24 October 2025
LHO General
ryan.short@LIGO.ORG - posted 16:53, Friday 24 October 2025 (87731)
Ops Day Shift Summary

TITLE: 10/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY: Busy day of continuous troubleshooting of H1. Things have been learned and progress has been made, but currently still waiting to relock after discovering an incorrect whitening setting and swapping a sat amp to see if those help with some of our instabilities. We've had some locklosses at DRMI_3F, but waiting for DRMI ASC to fully converge on this most recent try seemed to work. Currently relocking up to MOVE_SPOTS.

LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:32 FAC Randy Y-arm N Caulking BTE 17:17
17:03 VAC Travis MX, MY N Checking pumps 17:34
17:20 FAC Randy CS, EX N Moving boom lift to EX 17:48
17:44 ISC Keita, Rahul Opt Lab Local ISS array work 18:43
20:27 VAC Travis MY N Pump measurement 20:43
H1 CDS
david.barker@LIGO.ORG - posted 16:10, Friday 24 October 2025 - last comment - 16:20, Friday 24 October 2025(87732)
New SDF settings differences lists

My first SDF post today, which was based on getting archive files from subversion commits, doesn't appear to be complete and in addition may have some false positives.

I have generated new lists, this time getting the archived OBSERVE.snap files from the CDS backups of userapps by the file server.

In the directory /ligo/home/david.barker/tuesdaymaintenance/24oct2025/sdf/observe there are:

mon20oct2025/ Directory of backups as of 00:39 early monday morning

wed22oct2025/ Directory of backups as of 00:39 early wednesday morning

thu23oct2025/ Directory of snaps as of 00:39 ealy thursday morning

mon-wed_diffs.txt Text file of settings changed between the monday and wednesday backups

mon-thu_diffs.txt Text file of settings changed between the monday and thursday backups

snap_diffs.bsh Shell script to generate the diffs files

snapfiles Text file of the userapps "OBSERVE.snap" files as symbolically linked from the target directories

 

Comments related to this report
jennifer.wright@LIGO.ORG - 16:20, Friday 24 October 2025 (87733)

Didn't find any other smoking guns, just the LSC-POP_A filter selection being wrong, making the anti-whitening gain wrong (see alog #87728), which we already knew about from the commit comparison Dave did previously (see alog #87718):

-H1:LSC-POP_A_RF45_I_SW1S 1 4.12400000000000000000e+03 0xffffffff
+H1:LSC-POP_A_RF45_I_SW1S 1 1.05200000000000000000e+03 0xffffffff

-H1:LSC-POP_A_RF45_Q_SW1S 1 4.12400000000000000000e+03 0xffffffff
+H1:LSC-POP_A_RF45_Q_SW1S 1 1.05200000000000000000e+03 0xffffffff

 

H1 General
ryan.crouch@LIGO.ORG - posted 15:50, Friday 24 October 2025 (87730)
OPS Friday EVE shift start

TITLE: 10/24 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM
    Wind: 9mph Gusts, 6mph 3min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.53 μm/s 
QUICK SUMMARY:

H1 ISC
elenna.capote@LIGO.ORG - posted 14:11, Friday 24 October 2025 (87728)
POP A RF45 whitening set wrong

We (Sheila, Jennie, Ryan, Oli) have found that the POP A RF45 antiwhitening gain was set incorrectly. We tracked this problem down to the SDF being saved incorrectly Monday night along with with various dark offsets (87598). The antiwhitening gain should be -15 dB but was set to -21 dB. Additionally, the new dark offsets were doubled. We think this problem explains why the MICH gain needed to be doubled this week (87645).

I reset the safe SDF to have the correct LSC POP antiwhitening filters, and reverted the dark offsets as well.

Extra kudos to Jennie for scrolling through Dave's SDF difference file (400 settings!) to find this mismatch, 87718.

Sheila edited the guardian to remove the MICH gain doubling.

Images attached to this report
H1 SUS
oli.patane@LIGO.ORG - posted 11:39, Friday 24 October 2025 - last comment - 12:48, Friday 24 October 2025(87722)
ETMY L2 satamp reinstated (reswapped) to try and solve locking issues

Marc, Oli

In 87713 it's noted that some of the strange behavior we've been seeing with the locks seem to be related to the ETMY L2 stage. The ETMY L2 satamp was swapped out on Oct 14th from S1100137 to S1100127 as part of the ECR E2400330 upgrade (87469). So, even though we were seemingly doing fine with this ETMY L2 satamp, we decided to swap it out this morning to see if that is the cause of our issues. Coincidentally, the spare satamp that we have available that was modified for ECR E2400330 and that Jeff had characterized was the satamp that had come from ETMY L2, S1100137. So we decided to put that one back in - it was fine before, although it obviously has now been modified for the satamp upgrade. So it's not been swapped back to exactly what it was before, but this is the closest we can get!

Marc and I took S1100137 down to EY and swapped out S1100127 with S1100137. I edited the fitresults file for S1100137 to work for ETMY L2 and replaced the previous OSEMINF 5.3:0.1 compensation filters to be the best possible compensation filters for this new satamp. 

Updating compensation filters
$ py satampswap_bestpossible_filterupdate_ECR_E2400330.py -o ETMY_L2
All updated filters grabbed for ETMY
ETMY L2 UL compensation filter updated to zpk([5.25],[0.0959],1,"n")
ETMY L2 LL compensation filter updated to zpk([5.21],[0.0953],1,"n")
ETMY L2 UR compensation filter updated to zpk([5.18],[0.0949],1,"n")
ETMY L2 LR compensation filter updated to zpk([5.21],[0.0955],1,"n")
write /opt/rtcds/userapps/release/sus/h1/filterfiles/H1SUSETMY.txt
Done writing updated filters for ETMY

Swap timeline

Date Serial Number Whitening zp
Before Oct 14th 2025 S1100137 10:0.4
Oct 14th 2025 S1100127 5.3:0.1
Oct 24th 2025 S1100137 5.3:0.1

Satamp characterization data

Here's the characterization data and fit results for S1100137, assigned to ETMY L2's ULLLURLR OSEMs.

This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.

The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100137_ETMY_L2_20251020.m

Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:

Optic  Stage  Serial_Number  Channel_Number  OSEM_Name  Zero_Pole_Hz  R_TIA_kOhm  Foton_Design 
ETMY L2 S1100137 CH1 UL 0.0959:5.25 120.875 zpk([5.25],[0.0959],1,"n")
      CH2 LL 0.0953:5.21 121.625 zpk([5.21],[0.0953],1,"n")
      CH3 UR 0.0949:5.18 121.625 zpk([5.18],[0.0949],1,"n")
      CH4 LR 0.0955:5.21 121.5 zpk([5.21],[0.0955],1,"n")

The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100137_D0901284-v5_fitresults.txt

Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.

Non-image files attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 12:48, Friday 24 October 2025 (87726)

This swap seems to have fixed the saturation problems, great work!

LHO VE
david.barker@LIGO.ORG - posted 10:45, Friday 24 October 2025 (87719)
Fri CP1 Fill

Fri Oct 24 10:10:02 2025 INFO: Fill completed in 9min 58secs

 

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 10:26, Friday 24 October 2025 - last comment - 11:28, Friday 24 October 2025(87718)
SDF settings changes since Monday

To continue with the "what has changed since Monday" I have created the SDF reports. For now I've just concentrated on the OBSERVE.snap settings changes.

Models with changed settings over this time period: h1alsex  h1alsey  h1asc  h1ascimc  h1iscex  h1iscey  h1isietmy  h1lsc  h1omc  h1suspr3  h1sussr3

There are approximately 400 settings changes.

Full details available in /ligo/home/david.barker/tuesdaymaintenance/23oct2025/sdf/observe

Comments related to this report
jennifer.wright@LIGO.ORG - 11:28, Friday 24 October 2025 (87721)

I can only see dark offset updates except for:

inp1 gain changed from 2 to 1 (which Elenna said was reverted):

-H1:ASC-INP1_P_GAIN 1 -2.00000000000000000000e+00 1
+H1:ASC-INP1_P_GAIN 1 -1.00000000000000000000e+00 1

 

changes to ISI-ETMY_ST2_BLND which I assume are to do with BRSY not working, 

 

The following changes in h1lsc:

-H1:LSC-POP_A_RF45_I_SW1S 1 4.12400000000000000000e+03 0xffffffff
+H1:LSC-POP_A_RF45_I_SW1S 1 1.05200000000000000000e+03 0xffffffff

-H1:LSC-POP_A_RF45_Q_SW1S 1 4.12400000000000000000e+03 0xffffffff
+H1:LSC-POP_A_RF45_Q_SW1S 1 1.05200000000000000000e+03 0xffffffff


-H1:LSC-MICH2_GAIN 1 1.00000000000000000000e+00 1
+H1:LSC-MICH2_GAIN 1 2.00000000000000000000e+00 1
-H1:OMC-REFL_A_LF_SW2S 1 1.55600000000000000000e+03 0xffffffff
+H1:OMC-REFL_A_LF_SW2S 1 1.55200000000000000000e+03 0xffffffff

 

Changes related to PR3 amd SR3 estimator that Olli is not suspicious of as it it all off.

Edit: Don't think any of this is suspicious.

H1 ISC (Lockloss)
elenna.capote@LIGO.ORG - posted 10:10, Friday 24 October 2025 (87717)
More DARM

We had a lockloss at 17:03 UTC that has the same "pulse" behavior noted by Jennie and Oli yesterday. This pulses can be seen in the DARM loop, on the L3 master out, and in the EX and EY L2 master outs. These pulses are about 5.8 Hz in frequency.

Images attached to this report
H1 ISC
elenna.capote@LIGO.ORG - posted 10:05, Friday 24 October 2025 - last comment - 10:47, Friday 24 October 2025(87716)
1 Hz instability investigations

I'm going to use this post to keep running notes of the 1 Hz investigations:

DHARD P at 1 Hz attached.

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 10:47, Friday 24 October 2025 (87720)

We edited the thermalization guardian so that it should set the csoft p gain to 20 only once, after 30 minutes (as before), then after that a user can change it as they wish.

H1 SUS
elenna.capote@LIGO.ORG - posted 09:04, Friday 24 October 2025 - last comment - 12:47, Friday 24 October 2025(87713)
ETMY reaction chain length tracking causing saturations

We have been getting saturation warnings on EY after going through the lownoise coil drivers state. We finally tracked it down to the R0 F2 and F3 drivers. The reaction chain length drive (aka reaction chain tracking) is causing these saturations. This servo is run using the L2 OSEMs as a witness to then drive the R0 chain to follow the main chain. I turned off the length drive and the saturations stopped. When I turn it back on it continues to saturate.

The only recent change I can think of is the L2 satamp swap on all the test masses.

Comments related to this report
sheila.dwyer@LIGO.ORG - 09:25, Friday 24 October 2025 (87714)

Adding a comment:  We've only had these saturations intermittently the last few days, in this lock it is now contiuous if the R0 tracking is on.  The sat amp swap happened Oct 14th, so perhaps this is some delayed consequence of the swap. 

elenna.capote@LIGO.ORG - 09:51, Friday 24 October 2025 (87715)

I was also reminded that the EY tiltmeter is possibly not performing as well as it can either as of Tuesday this week.

elenna.capote@LIGO.ORG - 12:47, Friday 24 October 2025 (87725)

After the ETMY L2 satamp was swapped back, we no longer get saturations on EY with R0 tracking on!

H1 ISC
elenna.capote@LIGO.ORG - posted 08:38, Friday 24 October 2025 (87712)
Lownoise DHARD P commented out of guardian

Because we continue to have issues with the lownoise state of DHARD P (1 Hz ring up), I have commented out both DHARD P lownoise steps in LOWNOISE_ASC. This includes the engagement of FM4 (lownois reshape with low pass) and FM8 (boost). These steps are done separately. This means that we can safely run the LOWNOISE_ASC guardian state, there will just be a little more noise until we can resolve the DHARD P issues.

LHO General
ryan.short@LIGO.ORG - posted 07:34, Friday 24 October 2025 - last comment - 13:28, Friday 24 October 2025(87710)
Ops Day Shift Start

TITLE: 10/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM
    Wind: 8mph Gusts, 6mph 3min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.62 μm/s 
QUICK SUMMARY: H1 was down overnight due to ongoing locking issues. I'll start by running through an initial alignment while I get caught up on events of the past couple days.

Comments related to this report
ryan.crouch@LIGO.ORG - 13:28, Friday 24 October 2025 (87727)SUS

After confirming it was damping well over mulitple locks I added the new settings of ITMX13 to lscparams and reloaded the GRD, -30 phase with a gain of -1.0.

H1 SUS
filiberto.clara@LIGO.ORG - posted 13:11, Tuesday 14 October 2025 - last comment - 11:42, Friday 24 October 2025(87469)
Sat Amps Modified: L2 (PUM) Stages for ETMX, ETMY, ITMX, and ITMY

WP 12836
ECR E2400330
Modified List T2500232

The following SUS SAT Amps were upgraded per ECR E2400330. Modification improves the whitening stage to reduce ADC noise from 0.05 to 10 Hz.

Suspension Old New OSEM
ETMX L2 (PUM) S1100146 S1100119 ULLLURLR
ETMY L2 (PUM) S1100137 S1100127 ULLLURLR
ITMX L2 (PUM) S1100135 S1100118 ULLLURLR
ITMY L2 (PUM) S1000277 S1100148 ULLLURLR


F. Clara, J. Kissel, O. Patane

Comments related to this report
oli.patane@LIGO.ORG - 17:22, Tuesday 14 October 2025 (87481)

Here's the characterization data and fit results for S1100148, assigned to ITMY L2's ULLLURLR OSEMs.

This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.

The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100148_ITMY_L2_ULLLURLR_20250917.m

Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:

Optic  Stage  Serial_Number  Channel_Number  OSEM_Name  Zero_Pole_Hz  R_TIA_kOhm  Foton_Design 
ITMY L2 S1100148 CH1 UL 0.095:5.19 120.5 zpk([5.19],[0.095],1,"n")
      CH2 LL 0.0957:5.24 120.0 zpk([5.24],[0.0957],1,"n")
      CH3 UR 0.0958:5.24 120.125 zpk([5.24],[0.0958],1,"n")
      CH4 LR 0.0967:5.28 120.375 zpk([5.28],[0.0967],1,"n")

The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-09-17_UKSatAmp_S1100148_D0901284-v5_fitresults.txt

Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.

Non-image files attached to this comment
oli.patane@LIGO.ORG - 17:19, Tuesday 14 October 2025 (87478)

Here's the characterization data and fit results for S1100119, assigned to ETMX L2's ULLLURLR OSEMs.

This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.

The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100119_ETMX_L2_ULLLURLR_20250916.m

Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:

Optic  Stage  Serial_Number  Channel_Number  OSEM_Name  Zero_Pole_Hz  R_TIA_kOhm  Foton_Design 
ETMX L2 S1100119 CH1 UL 0.0949:5.19 120 zpk([5.19],[0.0949],1,"n")
      CH2 LL 0.0971:5.32 120 zpk([5.32],[0.0971],1,"n")
      CH3 UR 0.0964:5.27 120 zpk([5.27],[0.0964],1,"n")
      CH4 LR 0.0957:5.23 120 zpk([5.23],[0.0957],1,"n")

The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-09-16_UKSatAmp_S1100119_D0901284-v5_fitresults.txt

Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.

Non-image files attached to this comment
oli.patane@LIGO.ORG - 17:18, Tuesday 14 October 2025 (87480)

Here's the characterization data and fit results for S1100118, assigned to ITMX L2's ULLLURLR OSEMs.

This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.

The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100118_ITMX_L2_ULLLURLR_20250916.m

Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:

Optic  Stage  Serial_Number  Channel_Number  OSEM_Name  Zero_Pole_Hz  R_TIA_kOhm  Foton_Design 
ITMX L2 S1100118 CH1 UL 0.0966:5.27 120 zpk([5.27],[0.0966],1,"n")
      CH2 LL 0.0961:5.25 120 zpk([5.25],[0.0961],1,"n")
      CH3 UR 0.0963:5.26 120 zpk([5.26],[0.0963],1,"n")
      CH4 LR 0.097:5.3 120 zpk([5.3],[0.097],1,"n")

The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-14_UKSatAmp_S1100118_D0901284-v5_fitresults.txt

Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.

Non-image files attached to this comment
oli.patane@LIGO.ORG - 17:21, Tuesday 14 October 2025 (87479)

Here's the characterization data and fit results for S1100127, assigned to ETMY L2's ULLLURLR OSEMs.

This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.

The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100127_ETMY_L2_ULLLURLR_20250916.m

Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:

Optic  Stage  Serial_Number  Channel_Number  OSEM_Name  Zero_Pole_Hz  R_TIA_kOhm  Foton_Design 
ETMY L2 S1100127 CH1 UL 0.0963:5.26 121.25 zpk([5.26],[0.0963],1,"n")
      CH2 LL 0.0958:5.24 121.25 zpk([5.24],[0.0958],1,"n")
      CH3 UR 0.0952:5.2 121.25 zpk([5.2],[0.0952],1,"n")
      CH4 LR 0.0954:5.21 121.25 zpk([5.21],[0.0954],1,"n")

The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-09-16_UKSatAmp_S1100127_D0901284-v5_fitresults.txt

Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.

Non-image files attached to this comment
filiberto.clara@LIGO.ORG - 11:26, Thursday 23 October 2025 (87685)

ITMY L2 (PUM) Sat Amp S1100148 installed on 10/14/2025. Replaced on 10/16/2024 with S1100080.

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=87515

oli.patane@LIGO.ORG - 11:42, Friday 24 October 2025 (87723)

Note that the satamp for ETMY L2 has now been swapped back to a S1100137, which has been modified for ECR E2400330

alog: 87722

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