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Reports until 16:31, Wednesday 20 August 2025
LHO General
thomas.shaffer@LIGO.ORG - posted 16:31, Wednesday 20 August 2025 (86476)
Ops Day Shift End

TITLE: 08/20 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY: Locked for 1 hour after a fast lock loss (alog86483). Reacquisition was straight forward but I did need to run an initial alignment.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:54 FAC Kim Opt Lab n Tech clean 17:54
16:27 FAC Tyler, HFD Vertex n Hydrant fix 17:55
17:55 FAC Kim MX n Tech clean 18:33
18:35 ISC Camilla Opt Lab n Parts bin 19:26
20:03 FAC Tyler Vertex n Taking photos of the leaky hydrant 20:08
21:02 SPI Jeff Opt Lab n Inventory 21:17
21:05 SPI Rick, Dripta, Tony PCAL lab yes SPI BS meas. 22:41
LHO General
corey.gray@LIGO.ORG - posted 16:28, Wednesday 20 August 2025 (86487)
Wed EVE Ops Transition

TITLE: 08/20 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 14mph Gusts, 7mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.10 μm/s
QUICK SUMMARY:

H1's been locked almost an hr (and TJ reported reacquisition was straightforward---good to know after yesterday's post-Maintenance locking issues!).  Winds low, microseism is low (below 50th percentile' here's to smooth sailing!

X1 SEI
jeffrey.kissel@LIGO.ORG - posted 14:34, Wednesday 20 August 2025 (86484)
Picomotor Science: Dimensions of Glenair MightMouse Connector
J. Kissel

Dimensions of Glenair picomotor mightmouse connector for Science.
Images attached to this report
H1 General
thomas.shaffer@LIGO.ORG - posted 14:11, Wednesday 20 August 2025 (86483)
Lock Loss 2055UTC

1439758519

No obvious cause, looks very fast.

H1 ISC
elenna.capote@LIGO.ORG - posted 13:56, Wednesday 20 August 2025 - last comment - 10:51, Wednesday 03 September 2025(86482)
Recent measurements of ASC calibrations

Since the HAM1 vent, I have done a few different measurements of the ASC that provide information on how to calibrate WFS signals from counts to microradians. Here is a summary:

CHARD, INP1 and PRC2 results come from this alog

DHARD results come from this alog

SRM results come from this alog (if you are comparing values, I made a power normalization error in the linked alog)

BS results were taken but never alogged (shame on me)

All of these measurements were taken by notching all ASC loops at 8.125 Hz and injecting an 8.125 Hz line in the desired DoF. The osem wits provide the urad reference.

Unless otherwise specified, the witness channels are the bottom stage osems

DoF Input Matrix Calibration Notes
CHARD P -1 * REFL A 45 I + 0.6 * REFL B 45 I

0.0161 urad [ETMY L2] / ct [REFL A 45 I]

0.0109 urad [ETMY L2] / ct [REFL B 45 I]

measured as ETMY L2 wit, must transform to L3 urad, can also convert to cavity angle

coherence near 1

CHARD Y -1 * REFL A 45 I + 0.8 * REFL B 45 I

0.0113 urad [ETMY L2] / ct [REFL A 45 I]

0.00965 urad [ETMY L2] / ct [REFL B 45 I]

measured as ETMY L2 wit, must transform to L3 urad, can also convert to cavity angle

coherence near 1

DHARD P 0.5 * AS A 45 Q - 0.5 * AS B 45 Q

0.00312 urad [ETMX L2] / ct [AS A 45 Q]

0.00312 urad [ETMX L2] / ct [AS B 45 Q]

measured as ETMX L2 wit, must transform to L3 urad, can also convert to cavity angle

coherence = 0.8, 10 averages

DHARD Y 0.5 * AS A 45 Q - 0.5 * AS B 45 Q

0.00612 urad [ITMY L2] / ct [AS A 45 Q]

0.02 urad [ITMY L2] / ct [AS B 45 Q]

measured as ITMY L2 wit, must transform to L3 urad, can also convert to cavity angle

coherence = 0.5, 10 averages

PRC2 P (PR2) 1 * POP X RF I 0.00033 urad / ct coherence 1
PRC2 Y (PR2) 1 * POP X RF I 0.000648 urad / ct coherence 1
INP1 P (IM4)

1.5 * REFL A 45 I + 1 * REFL B 45 I

0.0104 urad / ct [REFL A 45 I]

0.00988 urad / ct [REFL B 45 I]

coherence 1
INP1 Y (IM4) 2 * REFL A 45 I + 1 * REFL B 45 I

0.0141 urad/ct [REFL A 45 I]

0.00608 urad/ct [REFL B 45 I]

coherence 1
MICH P (BS) 1 * AS A 36 Q 0.0161 urad [M2]/ct measured as BS M2 WIT/AS A 36 Q, must transform into M3 urad, coherence near 1
MICH Y (BS) 1 * AS A 36 Q   data not taken
SRC1 P (SRM) 1 * AS A 72 Q 16.9 urad/ct coherence near 1
SRC1 Y (SRM) 1 * AS A 72 Q 10.6 urad/ct coherence near 1

 

Comments related to this report
elenna.capote@LIGO.ORG - 10:51, Wednesday 03 September 2025 (86713)

Here is data for MICH yaw and SRC2:

DoF Input Matrix Calibration Notes
MICH Y 1 * AS A 36 Q 0.00248 urad [BS M2] / ct measured as BS M2 WIT/AS A 36 Q, must transform into M3 urad
SRC2 P (SRM + SR2) 1 * AS_C

33.4 urad [SR2 M3] / ct

44.7 urad [SRM M3] / ct

SRC2 drive matrix is a combination of SRM and SR2:

-7.6 * SRM + 1 * SR2

SRC2 Y (SRM + SR2) 1 * AS_C

20.9 [SR2 M3] / ct

48.8 [SRM M3] /ct

SRC2 drive matrix is a combination of SRM and SR2:

7.1 * SRM + 1 * SR2

 

H1 ISC
elenna.capote@LIGO.ORG - posted 11:57, Wednesday 20 August 2025 (86481)
More SRCL FF updates

Continuing my efforts to check and update the LSC coupling (see 86423 and 86370) I ran yet another bruco, which showed that now the dominant low frequency coherence is coming from SRCL.

In review, I have:

I think we can do better. The main challenge is fitting the <100 Hz coupling while fitting the >100 Hz coupling, or at least not significantly worsening it. I think the fit would be easier if we made use of the parallel SRCLFF banks to fit a low and high frequency feedforward. This would require fitting the low frequency coupling, engaging it, and then remeasuring the high frequency coupling to fit separately.

I have what I think is a better fit to the low frequency coupling, currently saved in FM5 of the SRCLFF1 bank. To test this new filter:

Time permitting, if the new filter works, taking a better measurementing of the coupling from 100 Hz and up while on the new filter would be a useful next step, which may require adjusting the excitation shape or increasing the excitation gain.

To motivate the use of commissioning time on this, I did a very simple coherence based subtraction of the SRCL noise to see what it could get us in range improvement. I used the same time as the bruco I linked above, so this time includes the PRCL and MICH improvements. I copied some of Oli's range compare code to help me generate this nice plot comparing 1 hour of strain with coherence subtraction of the SRCL noise. Even if we can't improve the feedforward above 100 Hz, there is possible a 2 Mpc improvement from below 100 Hz.

Non-image files attached to this report
LHO VE
david.barker@LIGO.ORG - posted 11:00, Wednesday 20 August 2025 (86479)
Wed CP1 Fill

Wed Aug 20 10:09:36 2025 INFO: Fill completed in 9min 32secs

Gerardo confirmed a good fill curbside.

Images attached to this report
LHO FMCS (DetChar)
thomas.shaffer@LIGO.ORG - posted 10:55, Wednesday 20 August 2025 (86478)
Fire pump 1 turned on while in Observing 1725-1742UTC

While fixing a hydrant on the backside of the OSB/vertex area, fire pump 1 was activate from 1725-1742UTC. Hanford FD pickup truck and our F150 were also back in that area. Their driving to and from that area, as well as some of their work showed up on our ITMY seismometer.

Images attached to this report
LHO General
thomas.shaffer@LIGO.ORG - posted 07:33, Wednesday 20 August 2025 - last comment - 10:35, Wednesday 20 August 2025(86474)
Ops Day Shift Start

TITLE: 08/20 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 3mph Gusts, 1mph 3min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.07 μm/s
QUICK SUMMARY: Locked for 11.5 hours, no alarms, calm environment. Looks like we dropped Observing at 1053-1057UTC because the SQZr lost lock and relocked.

Our range isn't as stable as it has been lately, and the Omicron glitch gram FOM shows some extra SNR around 20-30Hz during those times.

Comments related to this report
david.barker@LIGO.ORG - 10:35, Wednesday 20 August 2025 (86477)

HFD are working on a hydrant, Tyler has requested the fire_pump alarms be bypassed for the next two hours.

Bypass will expire:
Wed Aug 20 12:31:32 PM PDT 2025
For channel(s):
    H0:FMC-CS_FIRE_PUMP_1
    H0:FMC-CS_FIRE_PUMP_2
 

LHO General
corey.gray@LIGO.ORG - posted 22:00, Tuesday 19 August 2025 (86465)
Tues EVE Ops Summary

TITLE: 08/19 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY:

Shift started out with Elenna & Jenne troubleshooting H1 due to locklosses at DHARD WFS post-Maintenance.  Elenna was eventually able to get H1 past the rough DHARD/CARM Offset steps of ISC_LOCK.  H1 was then able to get back to Observing (please see Elenna's alog for more info---Elenna mentioned, as she was leaving for the night, that this was an issue similar to what she saw after the recent HAM1 vent.).

Violins were elevated on this lock, but once High Power Damping settings were started, most modes were damped down pretty fast.  ETMy M1 was slow, so I helped it out a little (nominal gain is -0.1 for ETMy Mode1, and I have it at -0.2 and will leave it here for the night since it continues to damp this one nicely.
LOG:

H1 SUS
corey.gray@LIGO.ORG - posted 21:38, Tuesday 19 August 2025 (86471)
Weekly In-Lock SUS Charge Measurement - FAMIS 28419

This morning the In-Lock SUS Charge Measurements ran.  Attached are the plots for all four Test Masses.  Closing FAMIS 28419.

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 21:37, Tuesday 19 August 2025 - last comment - 21:38, Tuesday 19 August 2025(86472)
HAM1 Gauge PT100 VACSTAT alarm 20:17:24 PDT due to sensor glitch

We had a 2 second square wave sensor glitch in PT100. Its pressure jumped from 1.7e-07 to 3.7e-07 Torr for 2 seconds and then jumped back.

VACSTAT sent cell phone texts to team-VAC due to this single gauge event, because HAM1 is separated from the rest of the vertex and is therefore exempt from the 2-gauges-in-alarm filter.

VACSTAT was restarted at 21:26 and I took the opportunity to bring MY's PT124B back into the system.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 21:38, Tuesday 19 August 2025 (86473)

VACSTAT all green again.

Images attached to this comment
H1 ISC
corey.gray@LIGO.ORG - posted 19:58, Tuesday 19 August 2025 (86470)
Back To Observing

After Elenna left (and made a summary alog), H1 made it to OBSERVING.  To get here, I ACCEPTED new ASC SDFs (see attached).

Violins are elevated after today's Maintenance, but once DAMPING came on, they are mostly all sharply dropping.

Images attached to this report
H1 ISC
anthony.sanchez@LIGO.ORG - posted 19:37, Tuesday 19 August 2025 (86466)
Bi-Weekly Locking Histograms

Bi-weekliy stats for a few locking sequences for the bast 14 days.
ALS: max Duration 28 Min
Average 4.79 Min
% above 5 minutes 32.07
Date range: 2025-08-06 02:28:40 to 2025-08-20 02:28:40

DRMI [18-101]: max Duration 57 Min
Average 13.68 Min
% above 5 minutes 54.90

Date range: 2025-08-06 02:29:42  to  2025-08-20 02:29:42

 

CARM: [120 -428] - max Duration 29 Min
Average 5.28 Min
% above 5 minutes 18.42

Date range: 2025-08-06 02:30:51  to 2025-08-20 02:30:51

Powerup [429-590]: max Duration 46 Min
Average 21.633 Min
% above 30 minutes 63.33

Date range: 2025-08-06 02:32:18  to  2025-08-20 02:32:18

 

Images attached to this report
H1 ISC
elenna.capote@LIGO.ORG - posted 19:36, Tuesday 19 August 2025 - last comment - 07:57, Wednesday 20 August 2025(86469)
Problem with DHARD WFS, CARM offset reduction

We kept losing lock at DHARD WFS, and Jenne and I spent a lot of time figuring out why. Here are some notes about things that we tried:

How I solved the problem:

Some final notes about minor mistakes I made after:

Comments related to this report
elenna.capote@LIGO.ORG - 07:57, Wednesday 20 August 2025 (86475)

Apologies for missing this detail in my original alog, but we had run two successful initial alignments. The first was run as usual after the end of the maintenance day. Green alignment converged properly, arm alignment looked good. We ran a second after the early problems with DHARD, thinking that maybe the alignment was poor. Same results, good green convergence, but problems with DHARD.

In general, the alignment of the arms and corners looked very good through this whole process. When I stepped in DHARD P and Y, I was making very small steps overall to correct the alignment, steps on the order of 0.01 or 0.03. In general, the buildups and the camera showed good alignment. The green arms also stayed well aligned when the DHARD signal engaged properly, which is telling me that our initial alignment was doing the correct thing for the ITMS. Is it possible that the CARM offset was too large? I have been wondering this, because if the alignment was decent but the WFS signal was junk because we were too far from resonance that might explain this behavior, and it lines up with the fact that the better fix was reducing the carm offset more before moving to REFL. I'm not sure if that makes sense though.

As a side note, DRMI was mostly locking very quickly throughout the night.

H1 ISC
elenna.capote@LIGO.ORG - posted 14:09, Tuesday 19 August 2025 - last comment - 11:13, Wednesday 20 August 2025(86456)
PRC1 returned to PRMI ASC

TJ, Ryan S, Elenna

Today we (once again) took some time to try to commission the PRM ASC loop in PRMI ASC.

We locked PRMI, and I engaged the beamsplitter ASC. I was able to see by moving PRM pitch around, and watching the buildups, that the "old" error signal, REFL A RF9 I, was a great error signal and only required a sign flip.

However, PRM yaw was harder. I checked REFL A and B RF9 I and neither signal worked. I checked POP X I next, and saw that the signal worked just fine. This doesn't make a lot of sense, but it works. I updated the guardian accordingly.

To test that the guardian changes work, we brought the ISC_DRMI guardian down, which unlocked PRMI, and re-requested PRMI ASC. We fixed a few guardian errors and tried again. It worked fine.

These are the changes made:

Loaded and tested!

Comments related to this report
elenna.capote@LIGO.ORG - 11:13, Wednesday 20 August 2025 (86480)

Rereading this, I realized that saying it "didn't work" is very vague.

More words:

I stepped around with the PRM slider, watching both the POP18 and POP90 buildups. While watching the buildups, I looked to see when various signals crossed zero. For PRM pitch, REFL A 9 I clearly had a good zero crossing at the maximized buildup. The difference was the sign flip, which I tested by turning on the loop and seeing the error signal go the wrong direction (away from zero), and then the right direction (towards zero) when the gain sign was flipped. To maintain the gain sign as set by the guardian, I flipped the sign on the input matrix value from positive (pre-vent value) to negative.

For PRM yaw, the REFL signals did not cross zero when the buildups were maximized. However, the POP X RF signal did cross zero. I also watched the POP QPDs, which are sensitive to PRM, but also require some offset. I decided setting some offset and trying to use the REFL WFS was probably a bad idea, so I chose POP X RF yaw as the error signal. I calibrated it by measuring the signal difference in counts compared to the sliders steps I took, which are in urad. I checked the overall sign using the similar loop engagement test I described above.

H1 SQZ
camilla.compton@LIGO.ORG - posted 12:38, Tuesday 19 August 2025 - last comment - 13:23, Friday 22 August 2025(86445)
PSAMS adjustments for SQZ-OMC mode matching

Leo, Jennie, Camilla

Followed setup instructions from 80010, with 75mW injected in the SEED beam, we had 1mW on OPO_IR_PD_DC slightly lower than last time. Also took SQZ_FC to FC_MISALIGNED.  And opened SQZ beam divertor and fast shutter. Have counts of ~60 on ASC-AS_A and B and 7e-4 on ASC-OMC-A and B NSUMs. Jennie took the OMC PZT down to zero to start and then ran a template userapps/../omc/h1/templates/OMC_scan_sqz_beam.xml.

Repeated mode scans with different ZM PSAMs offsets, the DC centering loops could account for the pitch change for PSAMs, for the extreme PSAMS values, I increased the servo limiter from 85 to 95. 

Jennie and Leo have the data to analyze. 

Comments related to this report
jennifer.wright@LIGO.ORG - 17:42, Tuesday 19 August 2025 (86467)

See the ndscope with the channels we used to monitor attached.

This template is saved in /ligo/home/jennifer.wright/Documents/OMC_scan/20250819_SQZ_beam_scan_with_ZM_changes.yaml

leendert.schrader@LIGO.ORG - 15:10, Wednesday 20 August 2025 (86485)
Following up on these OMC scans: attached is the table with all computed mode-mismatch values.
Non-image files attached to this comment
leendert.schrader@LIGO.ORG - 13:23, Friday 22 August 2025 (86520)
Leo, Jennie W., Camilla

Below is a plot of the OMC scans fitted with a surface polynomial.
The plot is from the presentation in T2500228, so the labels on axes will be different.
This can be plotted on Matlab simply using the following code block (requires Curve Fitting Toolbox to use fit()).

OMCX = [5.5, 4, 2.3, 3, 8.1, 2.3, 2.3, 6, 9.5, 6, 6, 9, 3, 8, 4, 9.5, 9.5];
OMCY = [-0.8, 0.34, 0.2, 0.85, -0.4, -0.1, 0.2,    -0.4, -0.6, -4.5, -5.3, 2, 2, -2, -2, -5, -0.6];
OMCdata = [1-4.048/100, 1-3.412/100, 1-3.074/100, 1-3.234/100, 1-5.073/100, ...
        1-3.176/100, 1-2.884/100, 1-2.174/100, 1-3.343/100, 1-9.490/100, 1-11.865/100, 1-6.282/100, 1-2.313/100, ...
        1-3.013/100, 1-3.021/100, 1-9.179/100, 1-3.243/100];

omc = fit([transpose(OMCX), transpose(OMCY)], transpose(OMCdata), 'poly22');
    
p = plot(omc);
Images attached to this comment
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