TITLE: 09/05 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY: Mostly quiet shift with one lock acquisition early on and observing since. H1 has now been locked for 4 hours.
LOG:
H1 is back to observing as of 00:55 UTC after a day of commissioning and a lockloss late this afternoon.
After running an alignment, DRMI locked easily, but DRMI ASC pulled things away from good alignment and there was a lockloss during DHARD_WFS. The next attempt needed a run through PRMI, which caught and PRMI ASC worked well. No other issues during the locking process. The only SDF diff I needed to address was the SQZT0 picomotor driver was left on (and is now off).
Yesterday during commissioning, I did some injections on the HAM1 ISI to try to measure the coupling of table motion at that chamber to DARM. Consistent with the multiple logs Elenna has put in the last few days, I don't see much evidence for coupling above 10hz. First 4 attached images show results for the X, Z, RY and RZ dofs. I didn't do Y or RX, I suspect from these results there's not a lot of reason to pursue those, but the each measurement is only 90s and are relatively low risk.
For each injection, I sent a bandpassed (butter("BandPass",8,10,100) in diaggui) the input of the iso loops, with amplitudes between 2 and 4 (I think 4 would have been fine for all dofs, as far as the IFO was concerned). I then made dtt templates for each excitation dof with spectra for the relevant BLND GS13 dof and CAL_DELTAL, put those filenames and locations in the coupling_plot.py and used the coupling_util.py function attached here, as well as the darm calibration txt. I'm sure these exist somewhere in the svn or something (couldn't find them) but it's taken several days to get this sorted on my own and want half a chance of figuring it out again in the future. I got some help from Huyen, but also used some older copies I had from previous measurements.
TITLE: 09/04 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 153Mpc
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY:
For today...we only observed for 15min--rest of the day was for commissioning (1445 until past 0000utc when H1 gets back to NLN); the 42hr lock ended right after Commissioning started. (apologies for handing you an unlocked H1, RyanS....but did get to do some locking for the first time in weeks (due to long H1 locks)!).
LOG:
TITLE: 09/04 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
SEI_ENV state: SEISMON_ALERT
Wind: 10mph Gusts, 5mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.08 μm/s
QUICK SUMMARY: H1 has been commissioning pretty much all day, but just had a lockloss at 22:51. H1 is starting an initial alignment now.
This morning at 16:03UTC, Corey heated up OM2 by setting H1:AWC-OM2_TSAMS_POWER_SET to 4.6, plot attached.
I switched off the heater by changing H1:AWC-OM2_TSAMS_POWER_SET back to 0 count at 21:59:37 UTC.
Attached is a plot showing the two thermistors on the OM2 heater (top plots) and kappa C on the bottom right to monitor the optical gain (while doing the darm offset step or before we get to NLN this value is flat as the PCAL line that is used in the calculation is not at its nominal settings).
At 22:00 UTC, Jennie turned this OM2 heater back off.
We plan to stay in commissioning until 23:00UTC to avoid contaminating Observing data with the 78618 "bike chain" glitches from OM2 slipping.
Sheila, Camilla
Camilla then noticed that my angle tuning for FDS above wasn't very good, so she repeated that. 86737
camilla.compton/Documents/sqz/templates/dtt/20250904_SRCLSQZdata.xml
and
attached.Type | Time (UTC) | SRCL Offset | Angle | DTT Ref |
FIS SQZ | 21:09:30 - 21:12:30 | -382 | (-)125.4 | ref 1 |
FIS SQZ | 21:14:45 - 21:17:45 | -200 | (-)151.0 | ref 2 |
FIS SQZ | 21:19:30 - 21:22:30 | 0 | (-)211.7 | ref 3 |
Took above data at NLG of 24.0, measaured a few hours ago 86729.
Type | Time (UTC) | SRCL Offset | Angle | DTT Ref |
FIS SQZ | 21:44:00 - 21:47:00 | -235 | (-)143.4 | ref 4 |
FIS Mid + SQZ (tuned to no sqz) | 21:48:00 - 21:51:00 | -235 | (-)151.0 | ref 5 |
FIS Mid - SQZ (tuned to no sqz) | 21:51:45 - 21:54:45 | -235 | (-)122.6 | ref 6 |
Mean SQZ (ADF off) | 21:56:00 - 21:59:00 | -235 | N/A | ref 7 |
I used this data and the no sqz data from here to run the so-called "brontosaurus" plot.
The results indicate that the SRCL offset is significantly decreased. The fit gives an offset of -235 ct for the hot OM2, compared to our current -382 ct offset.
at 19:25:38-19:56:30 UTC we went to no sqz with OM2 hot.
There was a 29Hz peak injected by Robert, and this was 1 hour 30 minutes after power up.
In this alog, I showed a plot that compares the CHARD P and INP1 P noise before and after the HAM1 ISI install. Last night, I took the measured CHARD P coupling function and calculated the CHARD P contribution to DARM just before the vent to install the HAM1 ISI, and from a high range time this past weekend, with the HAM1 ISI installed. The attached plot compares DARM before and after the vent and the CHARD P contribution to DARM before and after the vent.
Turns out the change in CHARD noise may have actually directly reduced some noise in DARM. The DARM/CHARD coupling function remained the same before and after the vent, so the improvement is directly due to the reduction of noise in CHARD.
We were running HAM1 feedforward to the pitch ASC before the install, but it varied in performance. My plot in the linked alog shows the best performance achieved, but looking at the data closer to the vent, the noise in CHARD P may have been higher than the best performance I show in the linked alog above.
The low frequency noise in DARM has also changed for other reasons:
Closes FAMIS#37256, last checked 86348
Things to note:
Possible issues:
CS_DUST_LAB1_{300,500}NM both stalled at a value 16 days ago
CS_DUST_DR1_300NM has been at zero for the past four days
CS_DUST_DR1_500NM has been at zero for the past six days
Not an issue:
CS_DUST_LVEA5_300NM has been at 0 for three months - since we turned it off after the vent
CS_DUST_LAB2_{300,500}NM both off as expected (comparing to last month when Ryan C didn't mention it as an issue)
Thu Sep 04 10:05:52 2025 INFO: Fill completed in 5min 48secs
Gerardo confirmed a good fill curbside.
15:59:33 Wed 03sep2025 PDT power glitch. H1 was in lock throughout and no impact on range.
H1 lockloss a few after hitting the 42hr mark for a lock (42hrs03min). At this time we were in at the beginning of 6hr commissioning period and at the time of the lockloss we were about ~10min into running the DARM Offset script for OM2 heating set-up.
Not sure that the DARM offset step caused this as we were almost back at our nominal offset when we lost lock (step 6 out of 7 with H1:OMC-READOUT_X0_OFFSET = 9) which is ~27 mA, nominal is 40 mA.
We checked the lockloss ndscopes and couldn't see any smoking guns when the offset was changing from 8 to 9.
FAMIS 28464, last checked in alog86272
Nothing much out of the ordinary here that I can see aside from the fact that the ITMX SLED is getting awfully close to the 1mW lower power threshold and will likely hit it in the next month.
Two issues I'm seeing in these plots 1) The ITMX HWS SLED is degrading faster than previous SLEDs and 2) There is some weirdness going on with the ITMX CO2 flow meter a week and a half ago.
The rate of degradation of these sleds is often on the order of roughly 2mW/yr. This is why we can generally get about a year's worth out of each SLED. Comparing the last ITMX SLED and the one that we just installed in May (alog84417), the old SLED decayed at a rate of 2.43mW/yr and the new one is 4.2mW/yr. This is just from making some lines in ndscope, so it's pretty rough, but we can definitey say that it is degrading about 2x as fast as the last SLED (attachment 1). The ITMY SLEDs are a bit more consistent at: previous = 2.7mW/yr and new = 2.2mW/yr.
We saw that on the ITMY SLED this last time around that we were still able to see spherical power changes from lock to lock even with the SLED power reporting 0.5mW, and ring heater changes were tough to see (alog84408). Let's consider 0.5mW to be our limit we can take these, but really it should be before we can't see anything, at our current rate this SLED would finish the run at ~0.3mW. Looks like we will need to swap this one before the end of the run.
In Ryan's alog I noticed that the usual change in flow, as reported by the paddle wheel flow meter on the floor, became much more stable on Sunday Aug. 24th. Looking back over two years (attachment 2), it actually looks like the flow has been unusually unstable since returning from the spring vent, and whatever happened on the 24th brought us back to normal. Being a Sunday, there wasn't much going on (alog86540), we were in the middle of a 40+ hour long lock. Zooming into the event doesn't show the laser doing anything during that time, as if it didn't actually see a change in flow. Not sure what's going on here.
Tried to measure NLG (following 76542) at different ISS setpoints (by changing the SHG waveplate to adjust how much power is incident on the AOM), with the same OPO TRANS power. Because in 86363 we were confused that the NLG increased significantly when we realigned Pump fiber, with the same OPO Trans setpoint.
This was confusing and I'd like to repeat next week. I initially thought we were getting pump depletion so decreased the seed power, but later noticed the ISS was just unable to keep up and the control voltage was dropping to -5 for the low values of ISS setpoint, see attached, it could hold in LOCKED_CLF_DUAL with 80uW OPO_TRANS fine but not with the SEED beam.
OPO Setpoint | ISS Setpoint when locked on | Amplified | Unamplified | NLG | Notes | |||
CLF DUAL | SEED | Max | Min | UnAmp | Dark | |||
80 | 4.9 | 3.2 | 0.192924 | 0.002389 | 0.0079612 | -2.1e-5 | 24.2 | |
80 | 2.9 | 2.9 | 0.045037 | -2.2e-5 | 39 ?(using below unamp) | Pump deplation? Reduced SEED power from 0.7 to 0.3 to keep it locked on SEED (still didn't work first time). | ||
80 | 6.3 | 6.3 | 0.0430464 | 0.000546 | 0.0011063 | -2.2e-5 | 38 ? | Unamp signal decreased from SEED power change. |
80 | 4.8 | 4.7 | 0.0454944 | 0.0005378 | 0.0018533 | -2.7e-5 | 24.2 | |
80 | 2.9 | -5 ? | Noticed ISS Controlmon at -5. | |||||
80 | 3.5 | 3.5 | 0.0452317 | 0.00054049 | 0.0018636 | -2.4e-5 | 24.0 | |
80 | 4.95 | 0.04523 | 24.0 | Leaving here. |
Repeated while Corey was relocking today. We had one strange measurement when the ISS setpoint at 3.3V where the un-amplified signal was much lower but when later repeating at 3.1V, we didn't see this.
OPO Setpoint | ISS Setpoint when locked on | Amplified | Unamplified | NLG | |||
CLF DUAL | SEED | Max | Min | UnAmp | Dark | ||
80 | 5.0 | 5.0 | 0.042961 | 0.00051437 | 0.00176935 | -2.1e-5 | 24.0 |
80 | 2.8 | ISS Setpoint dropped to -5, so OPO TRANS not at 80uW | |||||
80 | 3.3 | 3.2 | 0.043273 | 0.0005247 | 0.00106713 | -2.1e-5 | 39.7 |
80 | 6.2 | 6.2 | 0.041031 | 0.00051677 | 0.0017658 | -2.1e-5 | 23.0 |
80 | 6.5 | 6.4 | 0.0409285 | 0.00051425 | 0.00175578 | -2.1e-5 | 23.0 |
80 | 3.6 | 3.5 | 0.0429806 | 0.00051216 | 0.00175932 | -2.7e-5 | 24.1 |
80 | 3.1 | 3.0 | 0.0431685 | 0.000516166 | 0.0017296 | -2.7e-5 | 24.5 |
80 | 2.8 | ISS Setpoint dropped to -5, so OPO TRANS not at 80uW | |||||
80 | 4.9 | 4.8 | 0.0429243 | 0.0005134 | 0.0017627 | -2.7e-7 | 24.0 |