I just took some No SQZing time (starting at 2025-06-25 15:01 UTC (1427040078)) and compared it to the pre-vent No SQZ Time of 2025-03-26 16:01 UTC (1427040078). I used the command python3 range_compare.py 1427040078 1434898893 --span 600. I originally wanted to use a time span of half an hour instead of 10 minutes, but the March time had some sort of glitch that messed up its range calculation, and the range calculation for today's time was the same, so I went with 10 minutes. Here's the range comparison.
TITLE: 06/25 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 145Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 5mph Gusts, 2mph 3min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.06 μm/s
QUICK SUMMARY:
Observing and have been Locked for almost 2.5 hours. Range is okay at 145Mpc, it looks like its been drifting a bit down since the lock started.
Looking at the lockloss from last night (2025-06-25 11:02 UTC - note that the 'refined lockloss time' is one whole second early than the actual lockloss time), it's immediately clear that we lost lock due to a quick ringup, but it is unclear where that ringup came from or what frequency it was actually at. We can see an 8Hz oscillation in DARM one second before the lockloss, but looking at the LSC channels, SRCL sees a 1.5 Hz oscillation right before the lockloss, and PRCL has a 4.5 Hz oscillation (although the PRCL oscillation could be unrelated, although it does look like it grows a bit larger). In the ASC channels, MICH P OUT has a ringup at ~3.8 Hz in that last second, and some of the other ASC channels look like they maybe also have some sort of excursion right before the lockloss.
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.
Lockloss From Nominal_Low_Noise @ 03:01:08 UTC.
I'm not exactly sure what caused this LL .
With the HAM1 ion pump performing nobly, the HAM1 turbo pump was spooled down and the associated SS-500 pump cart was disconnected from the HAM1 volume. All mechanical sources of vacuum equipment noise should be in nominal observing mode.
The HAM1 pressure gauge, PT-100, was connected via a standard gauge pigtail cable, directly from gauge body sub-D to supply CPC. All of the temporary cabling was removed including the breakout board and analog voltage readout pigtail, so PT-100 is solely on Ethercat communication.
Famis 28411 Weekly In-Lock SUS Charge Measurement.
This command is very useful to determine if the SUS charge measurements ran in the last week:
ls /opt/rtcds/userapps/release/sus/common/scripts/quad/InLockChargeMeasurements/rec_LHO -lt | head -n 6
Coherence for bias_drive_bias_off is 0.06426009151210332, which is below the threshold of 0.1. Skipping this measurement
Cannot calculate beta/beta2 because some measurements failed or have insufficient coherence!
Cannot calculate alpha/gamma because some measurements failed or have insufficient coherence!
Something went wrong with analysis, skipping ITMX_13_Hz_1434811847
TITLE: 06/25 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 145Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY:
Currently Observing at 150Mpc and have been Locked for just over 2 hours. Relocking went pretty smooth, with the only issue being DRMI/PRMI taking very long to catch still. During maintenance today, the auxiliary pumps around HAM1 were turned off, and the jitter noise that we had been seeing around 550-600Hz is basically almost fully gone.
LOG:
14:30 Observing at 145Mpc and have been Locked for almost 4 hours
14:45 Out of Observing to run SUS Charge measurements
15:00 Lockloss during SWAP_BACK_ETMX
- It doesnt look like it was due to anything that was happening with the swap
19:31 Started relocking
- Initial alignment
- Lockloss from MOVE_SPOTS
22:33 NOMINAL_LOW_NOISE
22:34 Observing
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
15:03 | FAC | Chris, Eric | XARM | n | Bee-am sealing | 17:32 |
15:09 | FAC | Randy | LVEA | n | Drilling holes in a pipe | 16:17 |
15:10 | FAC | Nellie, Kim | LVEA | n | Tech clean | 16:27 |
15:21 | VAC | Gerardo, Jordan | LVEA, FCETube | n | Turning off HAM1 pump, replacing gauge in FCETube, craning onto termination slab | 19:25 |
15:33 | VAC | Janos | EX, EY | n | Pumping line parts collection | 18:40 |
15:39 | FAC | Tyler | XARM | n | Driving Big Red to move spool | 16:39 |
15:45 | SQZ | Camilla, Sheila | LVEA | y(local) | SQZT7 work | 18:49 |
15:45 | PSL | Jason | LVEA | n | Inventory | 17:32 |
15:46 | FAC | Mitchell | LVEA | n | Inventory | 16:09 |
15:53 | CDS | Jonathan | remote | n | Rebuilding camera software | 16:01 |
15:54 | VAC | Travis | LVEA | n | Helping Gerardo and Jordan | 17:21 |
16:07 | SUS | RyanC | CR | N | OPLEV charge measurements, EY & EX | 17:38 |
16:14 | FAC | Richard, Ken | LVEA | n | Looking at cable tray near HAM6 | 16:27 |
16:15 | Christina | LVEA | n | Inventory | 16:33 | |
16:16 | VAC | Jackie | FCETube | n | Joining Jordan and Gerardo | 17:14 |
16:18 | CDS | Patrick | remote | n | Reimaging VAC Beckhoff computer | 19:05 |
16:33 | FAC | Randy | MX | n | Craning | 18:20 |
16:33 | Christina | MY | n | Taking a photo | 17:01 | |
16:36 | SEI | Jim | remote | n | HAM1 ISI measurements | 19:05 |
16:52 | FAC | Mitchell | FCETube | n | Inventory | 17:59 |
16:52 | FAC | Tyler | XARM | n | Meeting up with Chris, Eric, and the bees | 17:07 |
16:57 | Keita | LVEA | n | Checking analog camera inventory | 17:33 | |
16:59 | FAC | Kim, Nellie | HAM Shack | n | Tech clean | 17:27 |
17:05 | EE | Fil, Marc | LVEA | n | Fixing BSC temp sensor | 18:35 |
17:11 | Jennie, Leo, Tooba | LVEA | n | Tour | 17:42 | |
17:24 | Betsy, Brian O, LIGO India people | LVEA | n | LIGO India planning | 18:09 | |
17:24 | Christina | LVEA | n | Inventory | 17:33 | |
17:27 | FAC | Kim | MX | n | Tech clean | 18:28 |
17:28 | FAC | Nellie | MY | n | Tech clean | 18:58 |
17:34 | Christina | HAM Shack | n | Looking for a forklift | 18:17 | |
17:42 | SQZ | Jennie, Leo | LVEA | y(local) | Joining on SQZT7 | 18:31 |
18:16 | Betsy + others | EY | n | Looking at stuff | 19:05 | |
18:18 | Christina | LVEA | n | Still looking for a forklift | 18:48 | |
18:49 | Camilla | OpticsLab | n | 18:51 | ||
19:11 | RyanC | LVEA | n | Sweep | 19:35 | |
19:37 | Matt | LVEA | n | Unplugging a cable | 19:40 | |
19:48 | EE | Fil | MX | n | Dropping stuff off | 20:18 |
20:19 | FAC | Chris | MY, EY | n | Checking filters | 21:16 |
20:23 | FAC | Tyler | XARM | n | Checking out more bees | 20:51 |
20:36 | VAC | Gerardo, Jordan | FCETube | n | Opening FC gate valve | 21:09 |
22:10 | PCAL | Tony | PCAL Lab | y(local) | Taking stuff | 22:16 |
Ryan S., Elenna
Ryan and I are still trying to speed up the MOVE_SPOTS state. Today, Ryan implemented new code that checks the convergence of the loops and only ramps up the ADS gains of loops that are not yet converged to help them converge faster. This appeared to work well, although the state is still slow. We are now taking the spots to the FINAL spots that the camera servos go to, instead of some old spot, so it's possible that which loops that are far off have changed.
Ryan also pointed out that the ENGAGE_ASC_FOR_FULL_IFO state is taking a while because it is limited by the convergence of the PIT3 ADS. This is likely because the POP A offset used in DRMI ASC is not quite right, so I adjusted it for pitch so the PRM should be closer to the full lock position. SDFed.
The last work that was done for the estimator was back on May 21st 84548. The data that I got then was of the Open Loop TFs for when SR3 OSEMINF gains were nominal (aka what they are now) vs our 'more calibrated' values that are shown in 84367. I then wrote a script that takes in the OLTF traces that were exported from diaggui and divides them for each DOF (results). The average between the two divided traces is what we are going to be using as the gain values needed to counter the 'more calibrated' values. I put these gains in as FM7(previously had old unused gains in) in the DAMP filter bank.
Today I changed the M1 coil driver state to 1, set the OSEMINF gains to the ones listed in 84367, turned on FM7 for all degrees of freedom in the DAMP filter bank to turn on the gain corrections, changed the gain for DAMP Y to be -0.1 instead of the nominal -0.5, and then took SUSPOINT to M1 transfer function measurements.The measurements can be found in: /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/Common/Data/2025-06-24_1700_H1ISIHAM5_ST1_WhiteNoise_SR3SusPoint_{L,T,V,R,P,Y}_0p02to50Hz.xml, in svn as r12356.
After that, I took regular transfer functions with damping on for SR3 M1 to M1. Unfortunately I accidentally took the transfer functions for Pitch with the wrong bin width, so the original xml file there has double the values as the other ones. The saved .mat file, though, has the data all the same size. The measurements can be found in: /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/SAGM1/Data/2025-06-24_1900_H1SUSSR3_M1_WhiteNoise_{L,T,V,R,P,Y}_0p02to50Hz.xml, in svn as r12359. The results are found in: /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/SAGM1/Results/2025-06-24_1900_H1SUSSR3_M1_ALL_TFs.pdf, also r12359.
After these measurements, everything was put back to how it was before, including the OSEMINF gains, the DAMP Y gain, and the DAMP FM7 filters turned back off.
Range comparison plot:
Command Ran: python3 range_compare.py 1396833438 1434842418 --span 1800
time 1 is April 11th 2024
time 2 is today at 23:20 UTC June 24th 2025
I ran two brucos, one on NOLINES and one on CLEAN.
Overall, the message of Tony's alog is that, relative to our best range, we have lost 10 Mpc by the time we reach 100 Hz, and an additional 5 Mpc by the time we reach 1 kHz. The brucos above show a lot of low level coherence with: MICH, SRCL, PRCL, REFL RIN. There is a chance that making additional improvements to the feedforward can help. Right now it's hard to tell how many Mpc that gets us back, but it's where we should start.
I made a range comparison with a time form last night when we got up to 155Mpc (Jun 25, 2025 05:07:30 UTC (1434863268)) and compared it to a time of good range before the vent, Apr 01, 2025 03:05:42 UTC (1427511960). Here's the range comparison.
(Jordan V., Gerardo M.)
Today we replaced the MKS gauge at FC-C-1, this is the first 6 way cross inside the filter cavity tube enclosure, we installed serial number 390F00490, twice, yes two times. It turns out that the flange has some scratches on the knife edge, and it was not going to seal regardless of the effort that we put into it. Once the gauge was removed the scratches transferred to the copper gasket. We replaced it with serial number 390F00495, this one seems to be doing good. New conflat was leak tested and no leak was detectable above 2.42e-10 torr*l/sec.
The old gauge serial number is 390F00406 with a date code of June 2021.
TITLE: 06/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 148Mpc
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 11mph Gusts, 7mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.06 μm/s
QUICK SUMMARY:
H1 has been Locked for close to an hour.
Note:
CDS Alarm H0:VAC-LY_Y3_PT114B_PRESS_TOUR alarmed at 1434843240. Oli metioned that Davis said this is nothing to worry about, I'm just documenting it here.
Everything else looks fine.
Sheila, Camilla. WP#12573
Sheila and I realigned the Homodyne after it needed to be touched to re-seat one of the PDs in 85116. Sheila balanced powers using the LO waveplate and measured visibility to be 98.4% (11.4mV min 1.46 V max).
We then used SQZ_MANAGER SQZ_READY_HD (needed to change LO gain, see sdf). Attached plot.
Last done by Kevin/Vicky in 84661, they got 6.4 to 7 dB of SQZ, 14.6 dB of anti-SQZ, and 12.1 dB of mean squeezing.
Type | NLG | Angle | SQZ (@300Hz) | DTT Ref |
LO shot noise | N/A | N/A | Used as 0dB | ref 1 |
ASQZ | 10 | (+) 204 | 14.3dB | ref 2 |
SQZ | 10 | (-) 114 | -7dB | ref 3 |
Mean SQZ | 10 | N/A | 10.7dB | ref 4 |
OPO Setpoint | Amplified Max | Amplified Min | UnAmp | Dark | NLG | OPO Gain |
95uW | 0.0530 | 0.001913 | 0.005307 | 9.1e-5 | 10.16 | -8 |
After Sheila and Camilla realigned the homodyne, I tried estimating the NLG by looking at the ADF beatnote while varying the squeezing angle to map out the ADF-LO ellipse as described in the ADF paper.
The channels used to measure the beatnote were H1:SQZ-ADF_HD_DIFF_NORM_{I,Q}. The squeeze angle was varied by sweeping H1:SQZ-CLF_REFL_RF6_PHASE_PHASEDEG from 0 to 275 degrees with both polarities of the CLF servo (H1:SQZ-CLF_SERVO_IN2POL).
I then fit the data to an ellipse. The ratio of the semi-major to semi-minor axes is denoted by G in the ADF paper and was then used to compute the NLG. This results in
G: 5
NLG: 8.8
By comparison, an NLG of 10.2 is equivalent to G=5.4, which is consitent with the accuracy of this data. This kind of measurement could probably be improved in the future by taking more data near the anti-squeezing points on the ellipse.
It's not obvious from the ADF paper how to convert from G to NLG and back. For posterity, the functions I used for these conversions are also attached. These use the "alternative OPO configuration" shown in Fig 6(a) of the ADF paper.
The data is located at /ligo/gitcommon/squeezing/sqzutils/data/NLG_HD_06_24_2025.h5.
WP12623 h1asc add fast channels to DAQ
Elenna, Dave:
A new h1asc model was rev-locked and installed. Four new fast DQ channels were added to the DAQ (channel, rate):
> H1:ASC-DC6_P_IN1_DQ, 256
> H1:ASC-DC6_P_OUT_DQ, 512
> H1:ASC-DC6_Y_IN1_DQ, 256
> H1:ASC-DC6_Y_OUT_DQ, 512
DAQ restart needed.
WP12570 Restart Digivideo Cameras with latest pylon
Patrick, Jonathan, Dave:
Jonathan updated pylon on h1digivideo[4,5,6] and restarted all the camera servers on these machines. This should fix the bug of stuck open files accumulating when the camera connection is interrupted.
No DAQ restart needed.
Add PID SMOO channels to vacuum SDF
Dave:
Prior to today's h0vacly restart I added the missing CP PID-control SMOO channels to the vacuum SDF monitor.req and safe.snap files. SDF was restarted 08:29. No DAQ restart needed.
WP12577, 12608, 12615 Upgrade LY Vacuum Controls
Janos, Gerardo, Patrick, Jonathan, Erik, Dave:
Patrick installed a new h0vacly system this morning. Main items are:
Pleae see Patrick's alog for details.
A extended DAQ restart was required, renaming Ion Pump raw minute trend files for uninterrupted lookback and construcing new PT100 (HAM1) raw minute trends following the upgrade of h0vaclx last Tuesday (17th June 2025).
DAQ Restart
Jonathan, Erik, Patrick, Dave:
Immediately following the restart of h1asc at 11:52, the DAQ was restarted using the following procedure:
It was at this late point that I remembered that the temporary H1 version of PT100B is no longer needed, and indeed this channel has no data following the removal of the PT100B Volts channel from h0vacly. However since it is still in the EDC, we need to continue running the temporary IOC until the next DAQ restart. I've removed it from edcumaster.txt as a reminder.
GPS Leap Seconds Updates
Jonathan, Erik, Dave:
Erik's FAMIS task reminded us that the leapseonds files expiration date of 30 June 2025 is rapidly approaching. Although no leap seconds are to be applied, the files need to be updated to reset their expiration dates. Please see Erik and Jonathan's alog for more details.
DNS testing
Erik:
ns1 (backup DNS server) was used by Erik to see if we can reproduce the error whereby loss of connection to GC caused internal CDS name resolution issues. It did not.
Vacuum Ion Pump channel name changes (old-name, new-name)
H0:VAC-FCES_IP23_II123_AIP_IC_VOLTS | H0:VAC-FCES_IPFCC9_IIC9_AIP_IC_VOLTS |
H0:VAC-FCES_IP23_II123_AIP_IC_VOLTS_ERROR | H0:VAC-FCES_IPFCC9_IIC9_AIP_IC_VOLTS_ERROR |
H0:VAC-FCES_IP23_II123_AIP_IC_MA | H0:VAC-FCES_IPFCC9_IIC9_AIP_IC_MA |
H0:VAC-FCES_IP23_II123_AIP_IC_MA_ERROR | H0:VAC-FCES_IPFCC9_IIC9_AIP_IC_MA_ERROR |
H0:VAC-FCES_IP23_II123_AIP_IC_LOGMA | H0:VAC-FCES_IPFCC9_IIC9_AIP_IC_LOGMA |
H0:VAC-FCES_IP23_II123_AIP_IC_LOGMA_ERROR | H0:VAC-FCES_IPFCC9_IIC9_AIP_IC_LOGMA_ERROR |
H0:VAC-FCES_IP23_VI123_AIP_PRESS_TORR | H0:VAC-FCES_IPFCC9_VIC9_AIP_PRESS_TORR |
H0:VAC-FCES_IP23_VI123_AIP_PRESS_TORR_ERROR | H0:VAC-FCES_IPFCC9_VIC9_AIP_PRESS_TORR_ERROR |
H0:VAC-FCES_IP24_II124_AIP_IC_VOLTS | H0:VAC-FCES_IPFCD1_IID1_AIP_IC_VOLTS |
H0:VAC-FCES_IP24_II124_AIP_IC_VOLTS_ERROR | H0:VAC-FCES_IPFCD1_IID1_AIP_IC_VOLTS_ERROR |
H0:VAC-FCES_IP24_II124_AIP_IC_MA | H0:VAC-FCES_IPFCD1_IID1_AIP_IC_MA |
H0:VAC-FCES_IP24_II124_AIP_IC_MA_ERROR | H0:VAC-FCES_IPFCD1_IID1_AIP_IC_MA_ERROR |
H0:VAC-FCES_IP24_II124_AIP_IC_LOGMA | H0:VAC-FCES_IPFCD1_IID1_AIP_IC_LOGMA |
H0:VAC-FCES_IP24_II124_AIP_IC_LOGMA_ERROR | H0:VAC-FCES_IPFCD1_IID1_AIP_IC_LOGMA_ERROR |
H0:VAC-FCES_IP24_VI124_AIP_PRESS_TORR | H0:VAC-FCES_IPFCD1_VID1_AIP_PRESS_TORR |
H0:VAC-FCES_IP24_VI124_AIP_PRESS_TORR_ERROR | H0:VAC-FCES_IPFCD1_VID1_AIP_PRESS_TORR_ERROR |
H0:VAC-FCES_IP25_CS187_STATUS | H0:VAC-FCES_IPFCH8A_CSH8A_STATUS |
H0:VAC-FCES_IP25_II187_IC_VOLTS | H0:VAC-FCES_IPFCH8A_IIH8A_IC_VOLTS |
H0:VAC-FCES_IP25_II187_IC_VOLTS_ERROR | H0:VAC-FCES_IPFCH8A_IIH8A_IC_VOLTS_ERROR |
H0:VAC-FCES_IP25_II187_IC_AMPS | H0:VAC-FCES_IPFCH8A_IIH8A_IC_AMPS |
H0:VAC-FCES_IP25_II187_IC_AMPS_ERROR | H0:VAC-FCES_IPFCH8A_IIH8A_IC_AMPS_ERROR |
H0:VAC-FCES_IP25_VI187_PRESS_TORR | H0:VAC-FCES_IPFCH8A_VIH8A_PRESS_TORR |
H0:VAC-FCES_IP25_VI187_PRESS_TORR_ERROR | H0:VAC-FCES_IPFCH8A_VIH8A_PRESS_TORR_ERROR |
Ansel, Sheila, Camilla
Last week, Ansel noticed that there is a 2Hz comb in DARM since the break, similar to that that we've seen from the HWS camera sync frequency and power supplies and fixed in 75876. The cabling has not been changed since, the camera sync frequency has been changed.
Our current camera sync frequencies are: ITMX = 2Hz, ITMY = 10Hz. We have typically seen these combs in H1:PEM-CS_MAG_LVEA_OUTPUTOPTICS_Y_DQ. With a 0.0005Hz BW on DTT I can't easily see these combs, see attached.
It may be difficult to see in a standard spectrum, but can be clearly seen in Fscan plots linked off of the summary pages. For the "observing" Fscan, the interactive spectrum plot shows the 2 Hz comb marked automatically. See the attached image of H1:GDS-CALIB_STRAIN_CLEAN
Verifed that the cabling has not changed since 75876.
Next steps we should follow, as listed in 75876 would be to try using a different power supply or lowering the voltage to +12V. Or, there is a note suggesting Fil could make a new cable to power both the camera and CLink's via the external supply (14V is fine for both).
Thanks Camilla. If anything can be done more rapidly than waiting another week, it would be very much appreciated. Continuing to collect contaminated data is bad for CW searches.