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Reports until 17:33, Thursday 24 July 2025
H1 General
matthewrichard.todd@LIGO.ORG - posted 17:33, Thursday 24 July 2025 (85979)
A-la-Mode Modeling Efforts to understand the IFO

M. Todd, E. Capote, C. Compton, S. Dwyer


After the vent, beam profiles were taken at REFL and POP (single-bounce) which are of interest to modeling efforts to gain some confidence in model parameters. Using a-la-mode to model the beam throughout the IFO and compare it to the measurements, we are able to confirm most of the parameters in the finesse yamlfile for the IFO model. See Figure 1 and Figure 2 for measured profiles of REFL and POP compared to the model beam parameters.

Now that we have more confidence in the model, we feel more comfortable looking at figures of merit that the model can provide -- such as the beam overlaps of different modes. Of particular interest was the input beam overlap with the PRC and ARM eigenmodes -- it seems the input beam is not super well mode-matched the PRC.

Table 1: Overlaps calculated using model for vertical and horizontal directions.
Mode1 Mode2 Overlap: v, h [%]
Input beam [IMC] PRCx 94.98 ,  97.00
Input beam [IMC] PRCy 96.99 , 98.32
Input beam [IMC] ARMx 98.57 , 98.91
Input beam [IMC] ARMy 99.03 , 99.31
PRCx ARMx 96.71 , 98.11
PRCy ARMy 97.96 , 98.87

There are plenty of interesting figures of merit that we can calculate using this model that help us understand more about the mode-matching state of our interferometer, and hopefully inform steps to correct mismatch.


The code used in this modeling is held in the 'ligo-commissioning-modeling' repo folder:

/ligo/home/matthewrichard.todd/repos/ligo-commissioning-modeling/analysis/O4/LHO/mode_matching/alm/main.m
Images attached to this report
H1 SUS
oli.patane@LIGO.ORG - posted 17:26, Thursday 24 July 2025 - last comment - 13:32, Tuesday 29 July 2025(85980)
TMSX F1/F2/F3/LF satamp box swapped

Fil, Elenna, Oli

In an effort to find and solve the ASC excursion locklosses that seem to be linked to TMSX (85973), Fil swapped out the satellite amplifier that he had installed last Tuesday (85770) that had serial number S1100150 with another modified satamp that he had on hand, S1100122 (originally meant for OMC T1 T2 T3 LF). We are hoping this fixes the problem. Since this is partially for testing and since we originally were planning to use this satellite amplifier for the OMC, for now I've replaced the OSEMINF compensation filters for TMSX (which had the specific tuned filters) with the generic 5.31:0.0969 zp filters. We can update these later when we figure out which satamp will be staying there. I've loaded these filters in and brought TMSX back.

 

taken out: S1100150

put in: S1100122 (originally meant for OMC T1 T2 T3 LF)

Images attached to this report
Comments related to this report
oli.patane@LIGO.ORG - 13:32, Tuesday 29 July 2025 (86072)

Filters updated to best possible for this new satamp: 86071

LHO General
thomas.shaffer@LIGO.ORG - posted 16:35, Thursday 24 July 2025 (85965)
Ops Day Shift End

TITLE: 07/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Earthquake
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY: Calibration and commissioning time today. We had one lock loss that ended a 21 hour lock, and now an earthquake is rolling through delaying relocking.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
21:06 SAF LVEA IS LASER HAZARD LVEA Y LVEA IS LASER HAZARD 22:03
16:29 - Corey Opt Lab n Parts hunt 16:48
17:01 - Corey MX n Parts hunt 17:23
17:06 VAC Janos, Anna MX n Looking around, checks 18:28
21:50 CDS Dave Mech room N Take down temporary camera 22:58
22:45 VAC Gerardo, Jordan FCTE n Checking on vac things 23:05
H1 CAL
elenna.capote@LIGO.ORG - posted 16:27, Thursday 24 July 2025 (85974)
Mistake in push of calibration report 20250719T225835Z

I reported in a comment to alog 85961 that I pushed a new calibration today based on report 20250719T225835Z. However, I made a mistake: I did not load the CAL CS model after this push. This load includes changes to gains and filters in the CAL CS model that are important for the calibration. We went back into observing because an unloaded model does not prevent us from observing, and I was not aware that I needed to do this! I found out about this mistake when Dave brought the unloaded filter changes to my attention.

Overall, the differences were small, but they were clearly enough to make a difference. With permission, we left observing, loaded the model, and TJ ran a broadband PCAL measurement. I have attached a comparison of the three broadbands from today. Green is the failed push of the 6/28 report, blue was what I thought was a successful push of the 7/19 report, and then red shows the result after we loaded the model.

Therefore, the 2% uncertainty at 20 Hz that I noted in my previous alog was due to having the wrong filters in CAL CS, and we don't have any problems with the L2/L3 crossover.

So, as a note to myself for the future, make sure to load the CAL CS model before observing.

Images attached to this report
H1 SUS (ISC, Lockloss)
elenna.capote@LIGO.ORG - posted 16:15, Thursday 24 July 2025 (85973)
ASC yaw excursion locklosses appear to be due to TMSX osems

We have been reporting in various alogs about locklosses where the yaw ASC signals have a large motion right before lockloss (85935, 85841, 85948). I have narrowed it down to the TMSX suspension moving largely in yaw. TMSX yaw moves first, and the ASC signals follow. The TMS servo, which adjusts the TMSX TEST offsets to center the beam on the TMS QPDs follows the TMSX yaw motion. We can see that the F2, F3 and F1 oseminf outputs move by about a half a micron just before these locklosses. However, the MASTER OUTs don't see a large drive, so this is something that the sensor is seeing.

There is also no movement in the HEPI IPS, ISI GS13 or ISI CPSs, which leads us to believe this is due to something at the suspension level.

Images attached to this report
H1 General
ryan.crouch@LIGO.ORG - posted 16:12, Thursday 24 July 2025 (85972)
OPS Thursday EVE shift start

TITLE: 07/24 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Earthquake
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: EARTHQUAKE
    Wind: 22mph Gusts, 12mph 3min avg
    Primary useism: 1.49 μm/s
    Secondary useism: 0.24 μm/s
QUICK SUMMARY:

LHO VE
david.barker@LIGO.ORG - posted 16:08, Thursday 24 July 2025 (85971)
Thu CP1 Fill

Thu Jul 24 10:09:37 2025 INFO: Fill completed in 9min 33secs

 

Images attached to this report
H1 General
thomas.shaffer@LIGO.ORG - posted 15:41, Thursday 24 July 2025 (85970)
Lock loss 2237 UTC

1437431869

Ending a 21 hour lock. No obvious cause, lock loss tool analyzing.

H1 SEI
ryan.short@LIGO.ORG - posted 15:29, Thursday 24 July 2025 (85969)
ISI CPS Noise Spectra Check - Weekly

FAMIS 26053, last checked in alog85829

The script reports BSC high frequency noise is elevated for the following sensors:

ITMY_ST1_CPSINF_H3

Non-image files attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 15:15, Thursday 24 July 2025 (85967)
PSL 10-Day Trends

FAMIS 31095

Late to this check this week, but not too much to report. Jason's incursion last week for an FSS tuneup (alog85769) is clearly seen, and generally things have been stable since. Only strangeness is a noisier FSS TPD signal as of about 2 days ago, which I looked a little closer into.

Zooming in on the FSS TPD signal during an observing period (see second to last attachment), these look to be brief jumps in power on the TPD on the order of 20-30mV that I don't see evidence of anywhere else; AMP2 output, PMC output, and ISS actuation all seem nominal during these times. These jumps look to be happening constantly any time the IFO is at or above the 'LOCKING_ALS' steps, and it was during this step during relocking after Tuesday maintenance when the jumps first started. The only thing that changed during Tuesday's maintenance period that might have an effect is the sat amp modifications to MC1 and MC3 (alog85922), possibly changing something about the IMC's feedback to the FSS? See final attachment for behavior while the IFO is unlocked and the FSS TPD signal goes quiet. I've been watching the RefCav REFL camera spot while these jumps happen, and I do notice a very slight shift of the spot, but not a change in shape. I'm not sure how to explain this behavior or why it would have started, but at least so far it hasn't seemed to be much of a "problem," although I'll be keeping an eye on it.

Images attached to this report
H1 ISC
jennifer.wright@LIGO.ORG - posted 14:47, Thursday 24 July 2025 - last comment - 18:04, Tuesday 19 August 2025(85966)
Stepping OMC ASC loop offsets to improve optical gain

Summary: I didn't see any conclusive difference that showed we could get an improvement from a change in a particular direction. Since the optical gain moves around so much its hard to see the effect of small or quick changes. It might be worth doing a longer test were we step these offsets in sets of three different values per dof (3*4 steps) and do each for five mins (~ 1 hour).


 

I orginally was trying to use the results of our last injection (2025-06-16 20:41:15 UTC to2025-06-16 21:01:57 UTC ) to determine how to change the OMC ASC alignment.

Using /ligo/home/jennifer.wright/git/2025/OMC_Alignment/20250116_OMC_Alignment_EXC.xml we injected four low frequency lines into H1:OMC-ASC_{POS,ANG}_{X,Y}_EXC - these channels come after the filter banks (ASC-OMC_A_PIT_OFFSET, then ASC-OMC_B_PIT_OFFSET, then ASC-OMC_A_YAW_OFFSET, then ASC-OMC_B_YAW_OFFSET) where the nominal offsets are set. The injection is at four different frequencies (0.0113, 0.0107, 0.0097 and 0.0103 Hz).

 

The analysis then involves looking at the 410 Hz line height on the OMC DCPD SUM to interpret the effect on optical gain.

 

However it is not clear from this plot that the full range of phase space has been looked at - ie we have not changed the offset with a large enough amplitude to check their current position is optimal.


 

Thus today I stepped ASC-OMC_A_PIT_OFFSET, then ASC-OMC_B_PIT_OFFSET, then ASC-OMC_A_YAW_OFFSET, then ASC-OMC_B_YAW_OFFSET - these filter banks are before the ones used above in the model and are the ones where the offset for the QPDs is set. In the

Towards the last three measurements we realised that we need to do larger changes ~0.04 counts to see a change in kappa C then wait for 3-4 mins. On the long term trend none of these changes seemed to produce any meausurable gain, but it would be good to repeat this measurement with longer times spent at each step and perhaps go in slightly larger steps.

The ndscope template is in /ligo/home/jennifer.wright/git/2025/OMC_Alignment/20250724_change _offsets_by_hand.yaml

Images attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 18:04, Tuesday 19 August 2025 (86468)

Jennie, Elenna,

 

The other day Elenna noticed some coherence between DARM and the light reflected from the OMC (OMC-REFL_A_LF_OUT_DQ) and wondered if this implies our mode-matching or OMC alignment is bad.

So I took some times from above when one of the offsets was non-nominal and we compared the coherence between these times, since it shows some small change maybe there is still some tuning we could do of these offsets to recover some optical gain.

 

The measurement is saved in /ligo/home/jennifer.wright/git/2025/OMC_Alignment/Jennie_OMC_offsets.xml

Each was around 3 minutes long apart from the starting measurement which we took from a quiet time before the measurements.

The measurement times are:

nominal settings: 16:29:21 UTC

PITCH A: 17:54:11:UTC

PITCH B: 18:39:57 UTC

YAW A :18:58:10 UTC

YAW B :19:23:20 UTC

 

Images attached to this comment
H1 ISC (ISC, Lockloss)
camilla.compton@LIGO.ORG - posted 14:42, Thursday 24 July 2025 - last comment - 17:07, Thursday 24 July 2025(85968)
Amount of Locklosses per day and percentage of ETM GLITCH Locklosses has not significantly increased
Between Dec 2024 and Feb 2025, 20% of our Observe locklosses were tagged ETM_GLITCH, see 82609.
Since then we've roughly had the same amount of OBSERVE locklosses per day, and the same percentage of ETM_GLICH locklossses. 
The amount of locklosses per day in the last 10 days is slightly increased, but not much.

Looking just in the last 10 days where we feel we've been having more locklosses:

Comments related to this report
oli.patane@LIGO.ORG - 17:07, Thursday 24 July 2025 (85977)
Images attached to this comment
H1 CAL
elenna.capote@LIGO.ORG - posted 11:47, Thursday 24 July 2025 (85963)
L2 Calibration line height lowered

I lowered the L2 calibration line height by a factor of 2.2- the measurement uncertainty was around 0.0007, and our target is 0.002. Now the uncertainty seems to lie around 0.0016. I updated the guardian and SDF with the new injection amplitude- 3.5.

H1 CAL
thomas.shaffer@LIGO.ORG - posted 10:47, Thursday 24 July 2025 - last comment - 10:55, Thursday 24 July 2025(85961)
Calibration Sweep

Ran a broad band (171106UTC), then a simulines. This was after running a serparate bb and start of a simulines that I had to bail out of because I had not gone back to NLN_CAL_MEAS. This allowed Elenna and Sheila to decide on something else and we reran after they made some changes.

Simulines start:

PDT: 2025-07-24 10:16:43.573765 PDT
UTC: 2025-07-24 17:16:43.573765 UTC
GPS: 1437412621.573765

Simulines end:
PDT: 2025-07-24 10:40:03.824053 PDT
UTC: 2025-07-24 17:40:03.824053 UTC
GPS: 1437414021.824053

Files:

2025-07-24 17:40:03,654 | INFO | File written out to: /ligo/groups/cal/H1/measurements/DARMOLG_SS/DARMOLG_SS_20250724T1
71644Z.hdf5
2025-07-24 17:40:03,661 | INFO | File written out to: /ligo/groups/cal/H1/measurements/PCALY2DARM_SS/PCALY2DARM_SS_2025
0724T171644Z.hdf5
2025-07-24 17:40:03,666 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L1_SS/SUSETMX_L1_SS_2025
0724T171644Z.hdf5
2025-07-24 17:40:03,670 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L2_SS/SUSETMX_L2_SS_2025
0724T171644Z.hdf5
2025-07-24 17:40:03,675 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L3_SS/SUSETMX_L3_SS_2025
0724T171644Z.hdf5

Images attached to this report
Non-image files attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 10:55, Thursday 24 July 2025 (85962)

I (with help and input from Sheila and Joe B) pushed a new calibration today before this report was run.

First, we tried pushing the 20250628T190643Z report, but again that "failed" because the broadband showed a higher uncertainty than expected, again. The kappa C value also dropped from 0.993 before the push to 0.985 after the push and TDCF burn in. We puzzled over this for a bit, until I brought up that maybe this report is too out of date to be useful. We also had to make minor ring heater changes to avoid PIs just after this report had been generated. Sheila trended the optical gain and saw that it did decrease by about 1% after we changed the ring heater.

So, I took a look at the report from 20250719T225835Z, and it looked very promising. The sensing function fit residual showed it was much more flat than the 6/28 report. I pushed this report next, and after burn in kappa C returned to be about 0.993. The broadband also showed this was a better calibration. We think this is improved, and we will stick with this calibration!

Open questions: why is the error still at 2% at 20 Hz? Can we improve the optical gain further?

Images attached to this comment
H1 ISC (Lockloss)
camilla.compton@LIGO.ORG - posted 08:47, Wednesday 23 July 2025 - last comment - 17:00, Thursday 24 July 2025(85935)
Locklosses with YAW ASC Excursion

In 85846 on Friday 18th, Elenna notes a lockloss after YAW ASC excursion, we have been having very short locks and I see evidence of two more of these yaw excursion in the last 24 hours:

Seen in CSOFT, SRC1, PRC2 and mainly on the L2 stage of quads. In the last 1-2 seconds before LL.

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 17:48, Wednesday 23 July 2025 (85950)

The lockloss that Ryan S. reports as being from a sitewide power glitch in this alog had a similar behavior in the suspension channels and yaw loops. Apparently the power glitch that caused the lockloss also tripped the HEPI pumps, but I'm not sure how that relates to the control loop behavior. I'm not sure if this is useful to link with these other locklosses or not.

Generally, every yaw ASC loops sees this behavior, but it's hard to tell what is moving first, or the most, since the channels are not calibrated into useful units. As a note, the soft loops are not DC coupled, so I imagine they are just following the other loops. Our lockloss scopes plot the very slow ASC channels, so here is a faster plot of some of the ASC channels before one of these locklosses. The centering loop signals are moving away from zero, but not large enough that the beam is at the edge of the WFS.

I broke out my old TMS servo scope to see if we are being pulled off the TMS QPDs. Clearly the X TR B yaw signal is increasing, but it may be because it's trying to follow a large movement in the hard loops. TMS X yaw moves about 1 urad before the lockloss as well.

In the first yaw excursion lockloss Camilla notes above, the ETMX HEPI RZ appears to oscillate in the two seconds before lockloss. I don't see that in the other yaw excursion lockloss though.

Images attached to this comment
ryan.crouch@LIGO.ORG - 20:32, Wednesday 23 July 2025 (85955)

Both of these YAW ASC locklosses saw TMSX_Y start oscillating a few seconds before the lockloss.

Images attached to this comment
elenna.capote@LIGO.ORG - 17:00, Thursday 24 July 2025 (85976)

Follow up to add that although the lockloss that Ryan S noted on 7/13 had an ASC excursion, the TMSX yaw suspension did not have the similar strange behavior that these other few locklosses have (ndscope). It's possible that this TMSX yaw behavior is linked to the sat amp change on 7/15, 85770.

Images attached to this comment
H1 DetChar (DetChar, PEM)
derek.davis@LIGO.ORG - posted 17:22, Friday 18 July 2025 - last comment - 11:20, Thursday 24 July 2025(85856)
20.2 Hz line appeared Jun 9, turns on and off

Prompted by me noticing on-off behaviors in the daily strain spectrogram for today at around 20.2 Hz, I've done some additional investigations into the source and behavior of this line: 

The 20.2 Hz line, which is currently prominent in DARM, first appeared in accelerometer and microphone data from the corner station on June 9. The first appearance of this line that I found was in the PSL mics, as shown in this spectrogram. This line then appeared in DARM in the first post-vent locks a few days later. The summary of work from June 9 does not show anything obvious to me that would be the source of this new noise.

This feature also turns off and on multiple times during the day. An example from today can be seen in this spectrogram. Most corner station microphones and accelerometers exhibit this feature, but it is most pronounced visually in the PSL microphone spectrograms. I was unable to identify any other non-PEM channels that showed the same on-off behavior, but this does reveal many change points that should aid in tracking down the source. Almost every day, this line exhibits abrupt on-off features at different times of the day and for varying durations. Based on my initial review, these change points appear to be more likely during the local daytime (although not at any specific time).  When the line first appeared, it was usually in the "off" state and then turned on for short periods. However, this has slowly changed, so that now the line is generally in the "on" state and turns off for brief periods. 

  

Images attached to this report
Comments related to this report
derek.davis@LIGO.ORG - 09:24, Monday 21 July 2025 (85887)

Looking into past alogs, I noticed that I reported this same issue last summer in alog 79948. Additional discussion about this line can be found in the detchar-requests repository (requires authentication). In this case, the line appeared in late spring and disappeared in early autumn of 2024. No source was identified before the line disappeared. 

Going back further, I also see the same feature appearing in late spring and disappearing in early autumn of 2023. The presence of the line is hence correlated with the outside temperature, likely related to some aspect of the air conditioning system that is only needed when it is (roughly) hotter outside than inside. This also means that we can expect this line to remain present in the data until autumn unless mitigation measures are taken.

timothy.ohanlon@LIGO.ORG - 11:20, Thursday 24 July 2025 (85959)

I looked briefly into the 20 Hz Noise without much success. Comparing the floor accelerometers, the noise is louder in the EBAY than the LVEA (although the signal of the EBAY accelerometer doesn't look good since the vent). The next closest is HAM1 followed by BS. So the noise is around the -X-Y corner of the LVEA, likely in the EBAY, Transition Area or Optics Lab because HAM6 sees less motion than HAM1 and EBAY sees the most.

Images attached to this comment
H1 AOS (DetChar)
preeti.sharma@LIGO.ORG - posted 10:46, Friday 18 July 2025 - last comment - 15:57, Tuesday 29 July 2025(85848)
Investigation of Lock losses due to Earthquakes

Preeti, Gaby

With the help of Ashley Patron's Eqlock script, we calculated the locklosses caused due to EQs for each observing runs. This is a part of the study of investigating the correlation between the microseism and duty-cycle (alog), so we chose winter months (Nov, Dec, Jan and Feb) of each observing run and calculated the vertical velocity of the ground from z-channel and horizontal velocity which is the quadrature sum of x and y channels at the time of locklost due to an EQ. We also did the same study for LLO (alog). 

Conclusion:

Images attached to this report
Comments related to this report
preeti.sharma@LIGO.ORG - 12:04, Thursday 24 July 2025 (85964)

After removing EQ events which happend during the locklosses, the probability of surviving lock during an EQ in O2 winter was found to be 54%, O3b winter was 64%, O4a winter was 73% and O4b winter was 41%. 

preeti.sharma@LIGO.ORG - 15:57, Tuesday 29 July 2025 (86082)

Some corrections have been done in the script after getting Derek's feedback and have attached the updated scatter plot between peak horizontal ground motion and peak vertical ground motion of Earthquake events, also data table including total number of EQs and lock probability in each observing runs' winters. Although, the number of surviving EQ events are still lower in O4 than O3. 

Images attached to this comment
H1 SUS
filiberto.clara@LIGO.ORG - posted 13:02, Tuesday 15 July 2025 - last comment - 15:19, Monday 28 July 2025(85770)
Top Sat Amps Modified: MC2/PR2/ETMX (MO, RO, UIM, and TMS)

WP 12675
WP 12676
ECR E2400330
Drawing D0901284-v5
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. The EX PUM SAT Amp was NOT upgraded. 

Suspension Old New OSEM
ETMX MO S1100128 S1100075 F1F2F3SD
ETMX MO/RO S1100079 S1100163 RTLF/RTLF
ETMX RO S1100149 S1100132 F1F2F3SD
ETMX UIM S1000297 S1100140 ULLLURLR
TMSX S1100098 S1100150 F1F2F3LF
TMSX S1000292 S1100058 RTSD
MC2 S1100107 S1100071 T1T2T3LF
MC2/PR2 S1100087 S1100147 RTSD/T1T2
PR2 S1100172 S1100121 T3LFRTSD


F. Clara,  J. Kissel

Comments related to this report
oli.patane@LIGO.ORG - 17:29, Thursday 24 July 2025 (85981)

As of 2025/07/25 00:00 UTC, the TMSX satamp box for F1/F2/F3/LF has been swapped from S1100150 to S1100122

See 85980 for more info

jeffrey.kissel@LIGO.ORG - 14:16, Monday 28 July 2025 (86028)
Here's the characterization data and fit results for  S1100075 , assigned to ETMX M0's F1F2F3SD OSEMs (Fil refers to this as ETMX MO F1F2F3SD).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100075_ETMX_M0_F1F2F3SD_20250710.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     M0       S1100075         CH1                F1           0.0971:5.31     120           zpk([5.31],[0.0971],1,"n")
                                   CH2                F2           0.0973:5.33     120           zpk([5.33],[0.0973],1,"n")
                                   CH3                F3           0.0979:5.36     120           zpk([5.36],[0.0979],1,"n")
                                   CH4                SD           0.0953:5.21     120           zpk([5.21],[0.0953],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/Scripts/

As LHO:85626 discusses, I'm intentionally excluding the fit of transimpedance gain from the foton design string, and so I've stopped using the R_TIA_kOhm as a knob in my by-hand fitting of the zeros and poles. Hence, you'll find that from here on, R_TIA_kOhm will almost always be the default 120 kOhm value I've found that works with the measured data and changing only the zero:pole frequency.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 14:16, Monday 28 July 2025 (86029)
Here's the characterization data and fit results for  S1100163 , assigned to ETMX M0/R0's LFRT/LFRT OSEMs (Fil refers to this as ETMX MO/RO RTLF/RTLF above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100163_ETMX_M0R0_LFRTLFRT_20250710.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     M0R0      S1100163        CH1                LF           0.0948:5.18     120           zpk([5.18],[0.0948],1,"n")
                                   CH2                RT           0.0954:5.21     120           zpk([5.21],[0.0954],1,"n")
                                   CH3                LF           0.0969:5.30     120           zpk([5.30],[0.0969],1,"n")
                                   CH4                RT           0.0947:5.17     120           zpk([5.17],[0.0947],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/Scripts/

As LHO:85626 and the above LHO:86028 discusses, R_TIA_kOhm is the default 120 kOhm.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 14:33, Monday 28 July 2025 (86030)
Here's the characterization data and fit results for  S1100132 , assigned to ETMX R0's F1F2F3SD OSEMs (Fil refers to this as ETMX RO F1F2F3SD above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100132_ETMX_R0_F1F2F3SD_20250710.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     R0        S1100132        CH1                F1           0.0943:5.17     120.75        zpk([5.17],[0.0943],1,"n")
                                   CH2                F2           0.0960:5.25     121.00        zpk([5.25],[0.0960],1,"n")
                                   CH3                F3           0.0963:5.28     121.25        zpk([5.28],[0.0963],1,"n")
                                   CH4                SD           0.0970:5.33     120.75        zpk([5.33],[0.0970],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/Scripts/

This sat amp actually needed some fit transimpedance gain, so I report it here. But, again, it's not used in the compensation filter.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 14:50, Monday 28 July 2025 (86031)
Here's the characterization data and fit results for  S1100140 , assigned to ETMX L1's ULLLURLR OSEMs (Fil refers to this as ETMX UIM ULLLURLR above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100140_ETMX_L1_ULLLURLR_20250715.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     L1       S1100140         CH1                UL           0.0943:5.14     120.5         zpk([5.14],[0.0943],1,"n")
                                   CH2                LL           0.0965:5.26     120.5         zpk([5.26],[0.0965],1,"n")
                                   CH3                UR           0.0943:5.14     120.5         zpk([5.14],[0.0943],1,"n")
                                   CH4                LR           0.0961:5.24     120.5         zpk([5.24],[0.0961],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/Scripts/

Similar to S1100132, I found I needed to slightly adjust the transimpedance to get a good phase fit of the zero frequency while getting magnitude scale to the ~1.000 +/- 0.005 level. Again, this won't be used in the compensation filter.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 14:55, Monday 28 July 2025 (86032)
Here's the characterization data and fit results for  S1100122 , which -- per LHO:85981, LHO:85980 and after 2025-07-25, has been assigned to TMSX M1's F1F2F3LF OSEMs (Fil refers to this as just TMSX F1F2F3LF above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100122_TMSX_M1_F1F2F3LF_20250724.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
TMSX     M1       S1100122         CH1                F1           0.0962:5.26     120           zpk([5.26],[0.0962],1,"n")
                                   CH2                F2           0.0971:5.31     120           zpk([5.31],[0.0971],1,"n")
                                   CH3                F3           0.0957:5.24     120           zpk([5.24],[0.0957],1,"n")
                                   CH4                LF           0.0951:5.20     120           zpk([5.20],[0.0951],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/Scripts/

As LHO:85626 and the above LHO:86028 discusses, R_TIA_kOhm is the default 120 kOhm.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 15:06, Monday 28 July 2025 (86033)
Here's the characterization data and fit results for  S1100058 , assigned to TMSX M1's RTSD OSEMs and CH3CH4 are not connected to any OSEM in-vacuum, hence the "xxxx" place holders (Fil refers to this as just TMSX RTSD above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100058_TMSX_M1_RTSDxxxx_20250708.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
TMSX     M1       S1100058         CH1                RT           0.0939:5.11     121           zpk([5.11],[0.0939],1,"n")
                                   CH2                SD           0.0960:5.25     120           zpk([5.25],[0.0960],1,"n")
                                   CH3                xx           0.0955:5.23     120           zpk([5.23],[0.0955],1,"n")
                                   CH4                xx           0.0961:5.25     120           zpk([5.25],[0.0961],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/Scripts/

As LHO:85626 and the above LHO:86028 discusses, R_TIA_kOhm is (mostly) the default 120 kOhm, save for CH1.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 15:11, Monday 28 July 2025 (86034)
Here's the characterization data and fit results for  S1100071 , assigned to MC2 M1's T1T2T3LF OSEMs (Fil refers to this as just MC2 T1T2T3LF above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100071_MC2_M1_T1T2T3LF_20250710.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
MC2      M1       S1100071         CH1                T1           0.0977:5.34     120           zpk([5.34],[0.0977],1,"n")
                                   CH2                T2           0.0956:5.23     120           zpk([5.23],[0.0956],1,"n")
                                   CH3                T3           0.0948:5.18     120           zpk([5.18],[0.0948],1,"n")
                                   CH4                LF           0.0958:5.22     120           zpk([5.22],[0.0958],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/Scripts/

As LHO:85626 and the above LHO:86028 discusses, R_TIA_kOhm is the default 120 kOhm.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 15:15, Monday 28 July 2025 (86035)
Here's the characterization data and fit results for  S1100147 , assigned to MC2/PR2 M1's RTSD/T1T2 OSEMs (Fil refers to this as just MC2/PR2 RTSD/T1T2 above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100147_MC2PR2_M1_RTSDT1T2_20250710.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
MC2      M1       S1100147         CH1                RT           0.0975:5.33     120           zpk([5.33],[0.0975],1,"n")
MC2      M1                        CH2                SD           0.0947:5.18     120           zpk([5.18],[0.0947],1,"n")
PR2      M1                        CH3                T1           0.0969:5.29     120           zpk([5.29],[0.0969],1,"n")
PR2      M1                        CH4                T2           0.0962:5.25     120           zpk([5.25],[0.0962],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/Scripts/

As LHO:85626 and the above LHO:86028 discusses, R_TIA_kOhm is the default 120 kOhm.
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 15:19, Monday 28 July 2025 (86036)
Here's the characterization data and fit results for  S1100121 , assigned to PR2 M1's T3LFRTSD OSEMs (Fil refers to this as just PR2 T3LFRTSD above).
The data was taken per methods described in T080062-v3.
The data was processed and fit using 
    ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
         plotresponse_S1100121_PR2_M1_T3LFRTSD_20250710.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
PR2      M1       S1100121         CH1                T3           0.0979:5.37     120           zpk([5.37],[0.0979],1,"n")
                                   CH2                LF           0.0967:5.29     120           zpk([5.29],[0.0967],1,"n")
                                   CH3                RT           0.0958:5.24     120           zpk([5.24],[0.0958],1,"n")
                                   CH4                SD           0.0969:5.31     120           zpk([5.31],[0.0969],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/Scripts/

As LHO:85626 and the above LHO:86028 discusses, R_TIA_kOhm is the default 120 kOhm.
Non-image files attached to this comment
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 02:14, Wednesday 25 June 2025 - last comment - 16:55, Thursday 24 July 2025(85317)
Annulus Ion Pump for BSC1 Rails

Signal railed about 5:18 PM local time, I checked trend data for PT120 and PT180 and no pressure rise noted inside the main volume.  Attached is 3 day trend of the pump behavior, very glitchy for a long while already.

System will be evaluated as soon as possible.  AIP last replaced on 2015, see aLOG 18261.

Images attached to this report
Comments related to this report
gerardo.moreno@LIGO.ORG - 04:00, Friday 27 June 2025 (85382)VE

Well, it appears as if the pump still has some life, just a few minutes ago started to pump the annulus system, for now.

Images attached to this comment
gerardo.moreno@LIGO.ORG - 16:55, Thursday 24 July 2025 (85975)VE

(Jordan V., Gerardo M.)

Late entry, activity took place last Tuesday 07/22/2025.

The annulus ion pump signal railed again, so this time we decided to replace the controller.  It does not seem like the controller improved the ion pump behavior, since the current signal is swinging more than before, see attached plot.  We are keeping an eye on this system.

Images attached to this comment
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