Had issues with FAMIS, so was not able to check this until today. Looks like the SUS Charge measurements ran this past Tuesday morning.
(A procedure note: when I ran the printing command, it would generate the ETMx plot, but that was it.....until I saved the plot to the desktop and then closed the generated .png plot. Then it would continue with the other plots (one at a time)---took me a bit to figure that out!)
Attached are the plots for all four Test Masses. Closing FAMIS 28425.
TITLE: 10/03 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 156Mpc
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 3mph Gusts, 2mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.21 μm/s
QUICK SUMMARY: H1 has been locked for over 10 hours. S251003at earlier this morning at 13:23 UTC.
S251003at from this morning was retracted.
Also ran range comparison checks comparing this lock stretch to the last as our range is a bit better. Seems like DARM looks better overall above ~60Hz; Sheila says this is probably just because the squeezer is "better" today. Report attached.
TITLE: 10/03 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 155Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY: Observing at 155 Mpc and have been locked for over 30 minutes. We recovered from the lockloss really quickly (59 minutes!) and I didn't need to intervene.
LOG:
23:30 UTC Observing and locked for almost 4 hours
01:59 GRB-Short E606552
03:22 Lockloss
04:21 NOMINAL_LOW_NOISE
04:24 Observing
Lockloss at 2025-10-03 03:22 UTC after just over 7.5 hours locked. It looks like it was caused by a very sudden localish event between 0.3 - 3 Hz (0.3-3 Hz, 1-3 Hz CS).
picket fence, build-ups, LSC, QUADs, peakmon, CS movement vs LL
10/03/2025 04:24 UTC Back to Observing
We are still Observing and have been Locked for over 7 hours now. Nothing to report.
TITLE: 10/02 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 12mph Gusts, 6mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.29 μm/s
QUICK SUMMARY: Observing at 149 Mpc and have been Locked for almost 4 hours. Secondary microseism is going back down and wind is low.
TITLE: 10/02 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY: Locked for almost 4 hours. Both relocks today needed an initial alignment, and took their time to lock DRMI, but eventually got there. No calibration measurement was run today due to the lock losses around commissioning time. We will need to get one on Saturday.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 22:52 | LASER | LVEA IS LASER HAZARD | LVEA | YES | LVEA IS LASER HAZARD \u0d26\u0d4d\u0d26\u0d3f(\u239a_\u239a) | 13:52 |
| 14:53 | FAC | Randy | Xarm | n | Xarm BTE inspections | 18:53 |
| 14:53 | PEM | Robert | LVEA | YES | Setup measurements | 16:27 |
| 17:42 | FAC | Kim | MX | n | Tech clean | 18:42 |
| 19:38 | Cheeta | Camilla | Opt Lab | n | Optics dropoff | 19:52 |
| 19:39 | FAC | Randy | Xarm | n | BTE inspection, near MX | 21:52 |
| 20:29 | FAC | Tyler | Mids | n | Checking on and signs | 21:14 |
| 21:09 | ISS | Keita, Jennie | Opt Lab | LOCAL | ISS array work | 00:09 |
| 21:19 | PCAL | Dripta | PCAL Lab | LOCAL | Taking pictures | 21:28 |
We lost lock during commissioning for unknown reasons at 1800UTC. Relocking required an initial alignment, and DRMI took 12 minutes to lock, but it got there and we are now Observing at 1944UTC.
Today I began calibrating the camera servo signals into spot positions. I ran the A2L script at the nominal camera spot positions. Then, I changed the camera offset and waited for the camera servo to converge. Then I remeasured the A2L gain. Using the a2l_lookup function in /opt/rtcds/userapps/release/isc/common/scripts/decoup/BeamPosition the A2L gain can be converted into a spot position in mm. This is a slow process so it will take time to get the conversions for all.
| Camera offset | A2L gain | Conversion | |
| ETMY Pitch | start: -230, end: -231 | start: 5.62, end: 5.92 |
(-23.2 mm - -21.8 mm)/-1ct = 1.4 mm/ct |
| ITMX Pitch | start: -230, end: -231 | start: -0.45, end: -0.56 |
(6.46 mm - 5.96 mm)/-1ct = -0.5 mm/ct |
I continued today following the same process stated above.
| Camera offset | A2L gain | Conversion | |
| ETMX P | start: -173, end: -172 | start: 3.04, end: 2.92 |
(-9.38 mm - -9.93 mm)/ 1ct = 0.55 mm/ct |
| ETMY Y | start: -349.5, end: -348.5 | start: 1.41, end: 1.06 |
(3.90 mm - 5.18 mm) / 1ct = -1.28 mm/ct |
| ETMX Y | start: -422, end: -421 | start: 4.85, end: 4.68 |
(17.22 mm - 17.84 mm) = -0.62 mm/ct |
I reran the ITMX beam spot calibration following the same method described above, but this time I checked how the beam spot moved on both ITMX and ITMY when I changed the BS camera offset. Turns out, they give the same answer, so that's good.
| Camera Offset | A2L gain | Conversion | |
| ITMX P (ITMY P) | start: -230 ct, end: -231 ct | start: -0.45 (0.19), end: -0.55 (0.09) |
(6.41 mm - 5.96 mm)/-1 ct = -0.45 mm/ct |
| ITMX Y (ITMY Y) | start: -236 ct, end: -237 ct | start: 3.18 (-2.75), end: 3.06 (-2.63) |
(11.26 mm - 11.70 mm)/ -1ct = 0.44 mm/ct (-0.44 mm/ct for ITMY) |
Thu Oct 02 10:07:28 2025 INFO: Fill completed in 7min 24secs
Matt, Camilla
After TJ and Dave fixed the HWS Live GUI 87252, Matt and I checked on it and re-centered the origin crosses which are meant to mark the center of where the IFO beam is heating the ITM, before and after, sdf diff. We moved them both down but we hadn't updated them in a few years so this isn't too surprising.
Also attached is a HWS image of the test masses comparing getting to 60W in to 180s later, plot. As usual, ITMY looks clean and ITMX has it's known point absorbers. There is some edge effects on ITMX that should be ignored.
TITLE: 10/02 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
SEI_ENV state: USEISM
Wind: 12mph Gusts, 8mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.41 μm/s
QUICK SUMMARY: Looks like we lost lock 2 hours ago. An initial alignment was done an hour ago, but DRMI is not catching despite high flashes.
Planned calibration and commissioning today, but we need to get back up first.
TITLE: 10/01 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
INCOMING OPERATOR: Ibrahim
SHIFT SUMMARY:
H1 has been locked over 18hrs with no issues this shift.
I took some more histograms of our locking sequences today.
ALS
DRMI-BiWeekly
DRMI-Monthly
DRMI-Daily Average
Carm
Powerup
& NLN
Checking in on our DARM lockloss status after the second month of having our higher bias. At the end of August I put some comparison plots in to show how the doubling of the bias had significantly decreased the number of locklosses we had, as well as also significantly decreasing the amount of those locklosses that were due to the DARM glitch(86678). I remade those plots again now that we've gone through September.
In my usual lockloss vs DARM lockloss plot, we see that we've actually had no locklosses due to the DARM glitch between September 3rd - September 30th, which is the longest we've gone in all of O4 without that lockloss cause!
The average lock length has gone down a bit compared to August (10.8 vs 13.3 hours), but that's still double the average lock length of February, March, June, and July (table, plot). The number of lockloses is still also much lower than the pre-ESD-doubling months.
WP 12813
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 |
| PR2 M2 | S1100174 | S1100159 | ULLLURLR |
| PR2 M3 | S1100093 | S1100141 | ULLLURLR |
| SR2 M2 | S1100169 | S1100070 | ULLLURLR |
| SR2 M3 | S1100134 | S1000295 | ULLLURLR |
F. Clara, J. Kissel, O. Patane
(Since Jeff is out of town, I'm putting these in for these swaps.)
Here's the characterization data and fit results for S1100159, assigned to PR2 M2'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_S1100159_PR2_M2_ULLLURLR_20250924.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 M2 S1100159 CH1 UL 0.0956:5.22 120.25 "zpk([5.22],[0.0956],1,""n"")" CH2 LL 0.0967:5.28 120 "zpk([5.28],[0.0967],1,""n"")" CH3 UR 0.0978:5.34 120 "zpk([5.34],[0.0978],1,""n"")" CH4 LR 0.0969:5.3 120 "zpk([5.3],[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/Results/ 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), I 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.
(Since Jeff is out of town, I'm putting these in for these swaps.)
Here's the characterization data and fit results for S1100141, assigned to PR2 M3'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_S1100141_PR2_M3_ULLLURLR_20250924.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 M3 S1100141 CH1 UL 0.0957:5.22 120.25 "zpk([5.22],[0.0957],1,""n"")" CH2 LL 0.0949:5.17 120.5 "zpk([5.17],[0.0949],1,""n"")" CH3 UR 0.0977:5.33 120.375 "zpk([5.33],[0.0977],1,""n"")" CH4 LR 0.0946:5.16 120.25 "zpk([5.16],[0.0946],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/ 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), I 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.
(Since Jeff is out of town, I'm putting these in for these swaps.)
Here's the characterization data and fit results for S1100070, assigned to SR2 M2'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_S1100070_SR2_M2_ULLLURLR_20250924.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 SR2 M2 S1100070 CH1 UL 0.0961:5.24 120.25 "zpk([5.24],[0.0961],1,""n"")" CH2 LL 0.0965:5.27 120.375 "zpk([5.27],[0.0965],1,""n"")" CH3 UR 0.0961:5.23 120.5 "zpk([5.23],[0.0961],1,""n"")" CH4 LR 0.0963:5.26 120.75 "zpk([5.26],[0.0963],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/ 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), I 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.
(Since Jeff is out of town, I'm putting these in for these swaps.)
Here's the characterization data and fit results for S1000295, assigned to SR2 M3'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_S1000295_SR2_M3_ULLLURLR_20250924.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 SR2 M3 S1000295 CH1 UL 0.0964:5.27 121.75 "zpk([5.27],[0.0964],1,""n"")" CH2 LL 0.0954:5.21 121.625 "zpk([5.21],[0.0954],1,""n"")" CH3 UR 0.0955:5.22 121.375 "zpk([5.22],[0.0955],1,""n"")" CH4 LR 0.0964:5.26 122 "zpk([5.26],[0.0964],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/ 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), I 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.