I ran a noise budget injection into DC6 (centering loop for POP WFS), using a broadband excitation from 10-100 Hz. Based on the results in the DTT template (attached), there is not any measureable contribution to noise in DARM when injecting about 100x above ambient in the DC6 P control (bottom left plot, ref trace shows quiet time, live trace shows injection). We can include this channel in the ASC noise budget, but our code won't even generate a trace since the reference DARM and injection DARM shown here are exactly the same (top left plot, blue reference trace shows quiet time, red live trace shows injection time).
At a later time I will check DC6 Y.
Ran A2L script for all sus during comissioning today. Screenshot attached.
Wed Jun 18 10:11:15 2025 INFO: Fill completed in 11min 11secs
H1 ISI CPS Noise Spectra Check - FAMIS 26048
NEW and IMPROVED H1 ISI CPS Noise Spectra check Now includes HAM1 !
HAM1 currently have some very loud VAC equipment attached to it which is running and may be why HAM1 looks so terible relative to the rest of the othe HAMs.
Sheila, Camilla
We can see large SQZ changes dependent on the OPO PZT value, we;vee seen this before, some alignment changes from this PZT should be adjusted for by FC AS and FC beamspot control. The FC beamspot control has been off since the vent, but we're turned FC beamspot control on again in the hope to reduce this dependency.
Yesterday we needed to turn the ASC on to improve high freq sqz 85147 and since we've started using the THERMALIZATION guardian 85083 to slowly adjust SRCL Offset, our squeezing and ASC error signals are reduced slightly (see below). We have turned back on the SQZ ASC as expect this new guardian will stop the ASC running away.
Now we have the THERMALIZATION guardian working, the ADF measured sqz ang change has reduced (see below), we want to try turning back on SQZ_ANG_SERVO which will take a little tuning of settings. You can see in this plot that when the OPo PZT changed, the servo would have adjusted the sqz angle too.
Also touched the SHG launch waveplates to decrease the rejected power in H1:SQZ-SHG_FIBR_REJECTED_DC_POWER.
SQZ ASC was running away at the start of the lock so I've turned SQZ ASC off again.
I tried re-measureing the sensing matrix, the result was different to that measrue in September 80373 with the YAW sensor swapped (see output of /sqz/h1/scripts/ASC/python AS42_sensing_matrix_cal.py below) but when I tried it later the sensing matrix seemed to be different, I expect you need to start in good squeezing for it to work well which we were not when I tried it.
Plan to remeasure the sensing matrix more carefully (as in 80373) and then try a new one again.
Also tried today the SQZ_ANG_ADJUST servo using ADF, as the ASC was running away this was confusing, left off.
Jonathan, Erik, Dave, Ibrahim, Tony:
Following the front end restarts yesterday there has been a spate of Guardian AWG connection issues e.g. alog85130
Erik recommended that we reboot h1guardian1 at the next opportunity to force new front end connections for all Guardian nodes, rather than restart each node as the problem arises.
Following a lock loss this morning, the control room gave us the go ahead to reboot h1guardian1 at 08:49 Wed18jun2025PDT. Like TJs last reboot 12 days ago, h1guardian came back and restarted all of its nodes quickly and without any problems.
However our two guesses are:
Reminder that for the past month HAM1 pressure was being reported by a temporary "H1" version of the old cold-cathode PT100A (called H1:VAC-LY_X0_PT100B_PRESS_TORR) which uses an ADC in h0vacly and calcuates the pressure from the raw voltage signal.
Yesterday Patrick installed the h0vaclx full Beckhoff readout of this gauge via an ethernet connection. The channel name for this gauge from now onwards is H0:VAC-LX_X0_PT100_MOD2_PRESS_TORR
For now I'm showing both channels on the Vacuum MEDM and FOMs, H1:VAC-LY_X0_PT100B_PRESS_TORR upper, H0:VAC-LX_X0_PT100_MOD2_PRESS_TORR lower.
Note the H1 channel is a bigger number, the voltage signal increased slightly when Gerardo plugged the ethernet cable into h0vaclx yesterday.
TITLE: 06/18 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 146Mpc
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 3mph Gusts, 1mph 3min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.05 μm/s
QUICK SUMMARY:
IFO is in NLN and OBSERVING as of 11:57 UTC
Looks like we were able to recover from a 5.8 Mexico quake fully automatically last night.
TITLE: 06/18 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 145Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY:
Currently Observing at 145 Mpc and have been Locked for almost 2 hours.Everything looking good.
Two hours into our previous lock, our range was slowly dropping and we could see that SQZ wasn't looking very good, and trending back the optic allignments Camilla saw that ZM4 and ZM6 weren't where they were supposed to be because the ASC hadn't been offloaded before all the updates earlier today(ndscope1). To fix this, we popped out of Observing and turned on the SQZ ASC for three minutes, which made the sqzing better(ndscope2)! This better sqzing has persisted to this next lock stretch.
After the 01:30 lockloss (85145), I sat in DOWN for a couple minutes while restarting a few Guardian nodes since awg was restarted earlier today and this should help with the guardian node error (like in 85130) (these are the ones I could think of that probably all use awg): ALS_{X,Y}ARM, ESD_EXC_{I,E}TM{X,Y}, SUS_CHARGE, PEM_MAG_INJ Tagging Guardian
LOG:
23:30 Observing and have been Locked for over 1 hour
00:24 Popped out of Observing quickly to run the SQZ ASC for a few minutes
00:27 Back into Observing
01:30 Lockloss
- Sat in DOWN for a couple minutes while I restarted some Guardian nodes
- We ended up in CHECK_MICH_FRINGES but that didn't help, so I started an IA
03:05 NOMINAL_LOW_NOISE
03:08 Observing
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
15:22 | SAF | LASER SAFE | LVEA | SAFE | LVEA is LASER SAFE ദ്ദി( •_•) | 15:37 |
20:49 | ISS | Keita, Rahul | Optics lab | LOCAL | ISS array work (Rahul out 23:45) | 00:28 |
03:08 Observing
The DAQ was restarted for a second time today at 12:41 (0-leg) and 12:50 (1-leg) for three reasons:
1) h1psldbb had a bad DAQ status following model change at 09:15 to remove an IPC sender
2) H0EPICS_VACLX.ini has new PT100 HAM1 gauge channels
3) H1EPICS_DIGVIDEO.ini has new CAM37 ISCT1-REFL channels (camera was added recently)
I regenerated H1EPICS_DIGVIDEO.ini using generate_camera_daq_ini.py, which correctly added CAM37 channels as a new server machine, but reverted CAMs[21, 23, 24, 26] back to "old" server settings. Remember these cameras were moved to a new server, but lack of masking forced them back to the old server (digivideo2). At this point the EDC was expecting a new set of channels, so as a work around I built a dummy ioc to simulate these channels to keep EDC happy. So to make a long story short, these cameras are back with their original PV set and digivideo_dummy_ioc is no longer needed. To test this I shut down the IOC with no loss of EDC connections, and verified tha the Guardian CDS_COPY "from" list was still functioning.
Detailed list of DAQ channel changes (9097 additions, 91 removals)
To run the test that calculates how much loss we have between the ASC-AS_C (anti-symmetric port) and the DCPDs at the output of the OMC (where strain is derived from).
conda activate labutils
python auto_darm_offset_step.py
The script turns on one notch in the DARM LSC loop, then changes the PCAL line heights so all the power is in just two frequencies.
At the end it reverses both these changes.
It can be stopped using Crtl-C but this will not restore the PCAL line heights back to their default values so you may have to use time machine.
After setting up the PCAL the script steps the DARM offset level in 120 s steps, I think it takes about 21 minutes to run.
After the script finishes, please put the OMC ASC MASTER GAIN back to its original value.
TITLE: 06/17 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 142Mpc
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 10mph Gusts, 4mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.07 μm/s
QUICK SUMMARY:
We are Observing and have been Locked for almost 1.5 hours. SQZ doesn't look good, so I might pop out of Observing in another hour to run sqz scan align. Also, if we lose lock I will be restarting a couple guardian nodes that use AWG since that was restarted earlier today, and we've already had one awg error pop up in ALS_YARM (85130).
TITLE: 06/17 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 140Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY:
IFO is in NLN and OBSERVING as of 22:26 UTC
TUES Maintenance Activities:
We had a very productive maintenance day during which the following was completed
LVEA was swept - alog 85128
*Only listing completed WP’s - close your permits if work is done.
Lock Reacquisition:
Lock recovery was quite rough due to a few issues
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
15:22 | SAF | LASER SAFE | LVEA | SAFE | LVEA is LASER SAFE \u0d26\u0d4d\u0d26\u0d3f( \u2022_\u2022) | 15:37 |
15:07 | FAC | Kim, Nellie | LVEA | N | Technical Cleaning | 16:12 |
15:40 | VAC | Jordan, Gerardo | LVEA | N | Anchor Drill work | 17:31 |
15:42 | OPS' | Camilla | LVEA | N | Laser SAFE transition, ISCT1 check | 16:14 |
15:42 | 3:00 | Christina | LVEA | N | Walkabout | 17:08 |
16:05 | FAC | Randy | LVEA | N | Inventory | 20:49 |
16:12 | FAC | Kim | EX | N | Technical Cleaning | 17:58 |
16:13 | FAC | Nellie | EX | N | Technical Cleaning | 17:15 |
16:19 | PSL | Jason | LVEA | N | PSL Inventory + Cable pull | 17:08 |
16:23 | 3IFO | Betsy, Mitchell, LIGO India Delegation | LVEA | N | Tour, 3IFO Walkabout + Rick | 18:20 |
16:28 | VAC | Richard | LVEA | N | Check on vac | 18:48 |
16:30 | AOS | Jennie | Optics Lab | Local | ISS Array | 17:21 |
16:42 | ISS | Kieta | Optics lab | Local | Joining Jennie W in he optics lab | 19:15 |
16:43 | CDS | Erik | Remote | N | Restarting EndX IOC | 16:53 |
16:57 | EE | Fil | LVEA & Both Ends | N | Looking for Scopes & Talkign to Richard. | 18:55 |
17:08 | FAC | Christina | End stations | N | Getting Pictures of hardware | 18:25 |
17:13 | ISC | Sheila, Matt, Camilla | LVEA | N | ISCT1 Laser Panels | 17:41 |
17:27 | Bee | Tyler | LVEA | N | Being a Busy Bee keeper and intercepting Betsy | 17:35 |
17:27 | ISS | Rahul | Optics Lab | Local | Helping Keita with ISS work | 19:15 |
17:28 | ISS | Jennie W | Optics Lab | Local | Working on ISS with Keita | 19:15 |
17:42 | ISC | Camilla | ISCT table | N | ISCT table work | 17:58 |
17:44 | PEM | Ryan C | LVEA | n | Checking Dust mons | 18:18 |
17:45 | VAC | Gerardo | Mid & EY | N | Guage replacements | 18:56 |
17:58 | FAC | Nellie, Kim | FCES | N | Technical Cleaning | 18:32 |
18:20 | 3IFO | Mitchell, Jim, 3IFO team member | LVEA | N | 3IFO inventory check | 18:23 |
18:25 | 3IFO | Brijesh, Jim | LVEA | N | 3IFO Inventory | 18:43 |
18:34 | TCS | Camilla | LVEA | N | TCS Part Search | 18:45 |
18:57 | VAC | Gerardo | LVEA | N | Vac Gauge Reconnection | 19:06 |
19:58 | OPS | Tony | LVEA | N | Sweep | 20:49 |
20:49 | ISS | Keita, Rahul | Optics lab | LOCAL | ISS array work | 22:55 |
20:58 | FAC | Chris | EX, MX | N | Air handler checks | 22:12 |
21:11 | PSL | Rick, 3IFO Delegation | PSL Anteroom | N | PSL Anteroom Tour | 22:06 |
21:21 | ISS | Jennie W | Optics lab | Local | Working on ISS system | 22:51 |
Trend of H1:IOP-SUS_ITMY_WD_OSEM1_RMSOUT shows increased motion during the 10 minutes post-RCG upgrade that OMC0, see alog 85120, was clobbering IPCs, including two peaks.
The attached screenshot has cursors at the approximate start and end of OMC0 clobbering IPCs. RMS remained high until guardian was started 30 minutes later, after which ITMY continued to ring until guardian was again restarted.
We will attempt to trace the clobbered IPCs to see if they plausibly could have driven ITMY.
The attach list shows the mapping from OMC0 IPCs to IPCs that were clobbered during the ten minutes OMC0 was running on the wrong IPC table.
ITMX, which received the same clobbered channel as ITMY, also showed a spike in movement during the same period, but was properly stilled by guardian.