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Reports until 12:19, Wednesday 25 June 2025
H1 SQZ
camilla.compton@LIGO.ORG - posted 12:19, Wednesday 25 June 2025 - last comment - 14:27, Wednesday 25 June 2025(85329)
SQZ HD Dataset

Yesterday 85295 we took HD data just at the nominal 95uW OPO trans setpoint, today we changed the NLG and retook data, saved at /camilla.compton/Documents/sqz/templates/dtt/20250625_HD.xml

Strangely, when I started checking the NLG with 95uW, once the seed was injected, this dropped to 65uW, I then increased injected seed power form 0.5mW to 0.6mW, I also  increased the pump power as we were close to the edge of the AOM range.

Used SQZ_MANAGER SQZ_READY_HD (needed to change LO gain, see sdf).

Type NLG Angle SQZ (@500Hz) DTT Ref
LO shot noise N/A N/A Used as 0dB ref 1
ASQZ 10 (+) 206 14.3dB ref 2
SQZ 10 (-) 112 6.9dB ref 3
Mean SQZ 10 N/A 11.3dB ref 4
ASQZ 18 (+) 210 17.2dB ref 5
SQZ 18 (-) 112 7.3dB ref 6
Mean SQZ 18 N/A 14.1dB ref 7
ASQZ 21 (+) 210 17.5dB ref 8
SQZ 21 (-) 110 7.4dB ref 9
Mean SQZ 21 N/A 14.7dB ref 10
ASQZ 14 (+) 206 15.6dB ref 11
SQZ 14 (-) 113 7.4dB ref 12
Mean SQZ 14 N/A 12.7dB ref 13
 
OPO Setpoint Amplified Max Amplified Min UnAmp Dark NLG OPO Gain
95uW 0.0730506 0.002413 0.006841 8.4e-5 10.81 -8
115uW 0.122166 0.002215     18.08 -8
120uW 0.141799 0.0021763     20.99 -8
105uW 0.0942627 0.0023351     13.95 -8
Comments related to this report
camilla.compton@LIGO.ORG - 12:28, Wednesday 25 June 2025 (85331)

Plot attached, we think that the SQZ is worse at NLG 10 that the other NLGs and we are considering running with NLG = 14.

Images attached to this comment
sheila.dwyer@LIGO.ORG - 12:52, Wednesday 25 June 2025 (85332)

Here's a fit of Camilla's data, it shows that our OPO threshold has increased compared to 83070, and we still have the same efficiency for squeezing, which implies 6% unexplained loss, which hasn't been fixed by moving the crystal. 

This plot was made using this script

Images attached to this comment
camilla.compton@LIGO.ORG - 14:27, Wednesday 25 June 2025 (85337)OpsInfo

We decided that an OPO TRANS setpoint of 105uW for an NLG of 14 gave us slightly better squeezing, see attached BLRMS. Leaving this in.

If the Operators have any issues keeping the OPO locked at this higher output power, they could lower it slightly following the instructions in 70050 to drop it down to 100uW or 95uW.

Images attached to this comment
H1 ISC
sheila.dwyer@LIGO.ORG - posted 11:38, Wednesday 25 June 2025 (85328)
OMC QPD offsets updated

Matt Todd, Sheila Dwyer

We moved the OMC alignment a bit in pitch while watching for a response in kappa C. The attached screenshots show the updated pitch offsets that have been accepted in safe and observe.   The next screenshot shows us stepping this around. 

Overall, we improved the optical gain by something like 0.5 %.  We would like to return to the yaw offsets to see if we can recover the 1% optical gain that we lost during the vent.

Images attached to this report
H1 General (Lockloss)
oli.patane@LIGO.ORG - posted 10:54, Wednesday 25 June 2025 - last comment - 13:47, Wednesday 25 June 2025(85327)
Lockloss

Lockloss during commissioning at 2025-06-25 17:52UTC after over 5.5 hours Locked. Cause not known, but probably not commissioning related.

Comments related to this report
oli.patane@LIGO.ORG - 12:56, Wednesday 25 June 2025 (85334)

18:48 Back to NOMINAL_LOW_NOISE

camilla.compton@LIGO.ORG - 13:47, Wednesday 25 June 2025 (85335)TCS

Within the same ~15 seconds of the lockloss, we turned the CO2 powers down form 1.7W each to 0.9W each. In the hope of doing the thermalization tests we tried last week 85238.

We checked the lockloss today and LSC channels at the time last week we turned the CO2s down and see no glitches corresponding with the CO2 waveplate (out of vac) change, we think the lockloss was unrelated.

LHO VE
david.barker@LIGO.ORG - posted 10:26, Wednesday 25 June 2025 (85325)
Wed CP1 Fill

Wed Jun 25 10:12:58 2025 INFO: Fill completed in 12min 55secs

 

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 10:05, Wednesday 25 June 2025 - last comment - 10:41, Wednesday 25 June 2025(85323)
Update Vacuum MEDM and VACSTAT following yesterday's vacuum changes

MEDM

Confusingly we have been running with two separate copies of the vacuum overview MEDM.

CDS_OVERVIEW has been using /ligo/lho/h0/ve/medm/beckhoff/H0_VAC_SITE_OVERVIEW_CUSTOM.adl (not under any version control)

SITEMAP has been using /opt/rtcds/userapps/release/vacuum/h0/medm/Target/H0_VAC_SITE_OVERVIEW_CUSTOM.adl (under git version control)

It is the second one, which is git controlled, which should be used. I took the opportunity when fixing the MEDMs to remove use of the /ligo files and move CDS_OVERVIEW over to using the Target file.

Changes made to the site overview and committed to git (see attachment) are:

RED - HAM1 now only shows the new PT100_MOD2 gauge

YELLOW - IP24,IP25 have new names

PURPLE - text to show the local git working directory and git repo information

VACSTAT

I added the new HAM1 PT100_MOD2 gauge to VACSTAT last night. Initially I also removed the temporary H1 PT100B gauge, but then remembered this has channels in H1EPICS_VACSTAT.ini which caused EDC disconnects.

So for now VACSTAT has the new H0 PT100_MOD2 (not in DAQ) and the old H1 PT100B (in DAQ, but needs to be removed)

Trip levels were returned to pre-vent values.

 

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 10:12, Wednesday 25 June 2025 (85324)

NOTE that PT114 is currently disabled in VACSTAT, this cold-cathode is yet to "catch" following yesterday's restart of h0vacly

david.barker@LIGO.ORG - 10:41, Wednesday 25 June 2025 (85326)

The control room FOM caqtdm version of the vacuum overview was upgraded and nuc22 rebooted at 10:35

Images attached to this comment
H1 SQZ
oli.patane@LIGO.ORG - posted 08:53, Wednesday 25 June 2025 (85320)
No SQZ Range Comparison

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.

Non-image files attached to this report
H1 General
oli.patane@LIGO.ORG - posted 07:34, Wednesday 25 June 2025 - last comment - 08:24, Wednesday 25 June 2025(85318)
Ops Day Shift Start

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.

Comments related to this report
oli.patane@LIGO.ORG - 08:24, Wednesday 25 June 2025 (85319)ISC, Lockloss

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.

Images attached to this comment
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 02:14, Wednesday 25 June 2025 - last comment - 04:00, Friday 27 June 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
H1 General (Lockloss)
anthony.sanchez@LIGO.ORG - posted 21:23, Tuesday 24 June 2025 (85315)
Lockloss from NLN

Lockloss From Nominal_Low_Noise @ 03:01:08 UTC.

I'm not exactly sure what caused this LL .

Images attached to this report
LHO VE (VE)
travis.sadecki@LIGO.ORG - posted 20:35, Tuesday 24 June 2025 (85314)
HAM1 turbo off, pump cart removed, and PT-100 gauge pigtail installed

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.  

H1 SUS (SUS)
anthony.sanchez@LIGO.ORG - posted 17:59, Tuesday 24 June 2025 (85311)
Weekly In-Lock SUS Charge Measurement

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

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 17:41, Tuesday 24 June 2025 (85310)
Ops Day Shift End

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
H1 ISC
anthony.sanchez@LIGO.ORG - posted 17:09, Tuesday 24 June 2025 - last comment - 09:31, Wednesday 25 June 2025(85307)
Range Comparison: April 2024 vs Today.

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
 

Non-image files attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 17:25, Tuesday 24 June 2025 (85308)

I ran two brucos, one on NOLINES and one on CLEAN.

bruco NOLINES

bruco 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.

oli.patane@LIGO.ORG - 09:21, Wednesday 25 June 2025 (85321)

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.

Non-image files attached to this comment
elenna.capote@LIGO.ORG - 09:31, Wednesday 25 June 2025 (85322)

This is interesting because it indicates that the range loss at low frequency in DARM now versus right before the vent is much smaller, only 3 Mpc. But looking back to our best range in April 2024, there is even more loss in sensitivity at low frequency.

H1 SQZ
camilla.compton@LIGO.ORG - posted 15:31, Tuesday 24 June 2025 - last comment - 19:51, Tuesday 24 June 2025(85295)
7dB on SQZ HD with New Spot in OPO Crystal

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
Images attached to this report
Comments related to this report
kevin.kuns@LIGO.ORG - 19:51, Tuesday 24 June 2025 (85313)

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.

Images attached to this comment
Non-image files attached to this comment
H1 TCS (DetChar-Request)
camilla.compton@LIGO.ORG - posted 13:20, Monday 23 June 2025 - last comment - 11:58, Thursday 26 June 2025(85247)
2Hz Comb in DARM from ITMX HWS Camera?

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.

Images attached to this report
Comments related to this report
evan.goetz@LIGO.ORG - 13:31, Monday 23 June 2025 (85254)DetChar
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
Images attached to this comment
camilla.compton@LIGO.ORG - 17:04, Tuesday 24 June 2025 (85306)

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). 

evan.goetz@LIGO.ORG - 18:30, Tuesday 24 June 2025 (85312)DetChar
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.
camilla.compton@LIGO.ORG - 15:11, Wednesday 25 June 2025 (85341)

Matt and I turned down the Voltage supplied from 14V to 12V for each camera at ~22:00UTC when the IFO was relocking. Verified HWS cameras and code still running.

We also will plan to have Dave reimpliemnt the hws_camera_control.py script he wrote in 74951 to turn the HWS's off in Observing until we fix this issue.

kiet.pham@LIGO.ORG - 11:58, Thursday 26 June 2025 (85361)

The 2 Hz comb is still present in H1:GDS-CALIB_STRAIN_CLEAN after the voltage change (before the software update)

Images attached to this comment
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