TJ, Ibrahim, Betsy, Camilla, WPs 12428, 12414
We added guillotines to all VPs, removed the bellows and added yellow VP covers. IOT2 bellows were very tight so couldn't be removed until we moved the table an ~inch away from HAM2. The tables bellows adapters were covered with ameristat and the bellows were covered with foil and placed on a nearby rack. Photo.
We moved the small garbing cleanroom up against the TSCY / the HAM3 cleanroom. We moved ISCT1 and IOT2 next to it on the other side of the racks, leaving space and a pallet for the HAM1 door. Photo.
TJ and I removed and disassembled the HAM2 scaffolding and stored it with the other scaffolding in the High bay.
Tue Apr 01 10:12:47 2025 INFO: Fill completed in 12min 43secs
FAMIS 24833
pH of PSL chiller water was measured to be between 10.0 and 10.5 according to the color of the test strip.
Eric, Dave:
Bypass will expire:
Tue Apr 1 11:52:44 AM PDT 2025
For channel(s):
H0:FMC-CS_FIRE_PUMP_1
H0:FMC-CS_FIRE_PUMP_2
Alarms has been reconfigured to expect GV2 and GV5 to be in the hard-closed position and alarm if not.
Added PT114 (CP1)
Bypass will expire:
Tue Apr 1 12:40:00 PM PDT 2025
For channel(s):
H0:FMC-CS_FIRE_PUMP_1
H0:FMC-CS_FIRE_PUMP_2
H0:VAC-LY_Y3_PT114B_PRESS_TORR
Added GV5 position alarm to bypass
H0:VAC-LY_GV5_ZSM159A_VALVE_ANIM
We are getting multiple VACSTAT alarms as gatevalves are being closed, so for now I've bypassed those cell phone alarms.
H1:CDS-VAC_STAT_GLITCH_DETECTED
TITLE: 04/01 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 8mph Gusts, 4mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.22 μm/s
QUICK SUMMARY:
IFO is in NLN and OBSERVING, but not for long.
H1 was running PEM Mag injections when I walked in, which finished and went into OBSERVING thereafter. I will induce a lockloss and set IFO to PLANNED ENGINEERING shortly.
Today is the first day of our planned Vent Break! Here is a summary of today's planned activities, also found on Trello Coordination Page
Work safe everybody!
Workstations were updated. This was an OS packages update. Conda packages were not updated.
TITLE: 03/31 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY:
Tonight is the last in-person Operator shift (TJ is the last OWL) before the April-Jun2025 Maintenance+Commissioning Break which begins at 8am (Local Time) tomorrow morning.
H1 has been stellar. Rode through an Alaskan EQ and is going on almost 7.75hrs of lock. And the range has been higher than normal (just under 159Mpc)....but then it went back to the normal 150Mpc after the SQZ lost lock and relocked toward the end of the shift.
LOG:
Just had a ~3min drop from OBSERVING due to SQZ, but it cameback automatically.
Did notice the SQZ_OPO_LR node has the familiar User Message:
"pump fiber rej power in ham7 high, nominal 35e-3, align fiber pol on sqzt0"
It's been trending up the last 5 days when it was last touched up on 3/26 (alog83570). Looks like it moved above 0.35 counts at 10am (local time) this morning. See attached.
It's been a few minutes and one can see H1's range took a step down about 6Mpc after this SQZ drop.
Camilla, Sheila.
The drop was because the OPO PZT ran out of range, see t-cursor on attached plot. It's a known issue that the SQZ angle (and alignment) changes with different PZT1 voltage.
It seems like that the sqz angle was set for 60-70V and was bad once we relocked at 100V. This would have been improved by taking SQZ_MANAGER to SCAN_SQZANG_FDS so it can find the best sqz angle again. If we were running the SQZ_ANG_ADJUST servo, this may have improved itself as you can see the ADF reported SQZ angle change at the time.
With the higher (19 vs 11) NLG 83665, the range and 350Hz SQZ (yellow BLRMS) does seem to be improved, but the high frequency SQZ did seem to be less stable as we thermalized.
[M. Todd, C. Compton]
Camilla and I made several knife edge measurements of the L5 CO2 laser in the optics lab after she got back from her trip to Access. The beamwidth estimates are consistent with tests done by Gabriele and Camilla
Measurements:
Fits to both the numerical derivative and cumulative yield similar estimates of the beamwidth (1/e^2 radius) : around 1.3mm at 16cm from the aperature is consistent with the beam profiles done in Gabriele and Camilla's test, which estimated the beam waist to be around 1.2mm.
Code for analyzing this data
Closes FAMIS 26036. Last checked in alog 83560.
Overall much quieter traces across all plots from last week's. Namely, the 7.6Hz to 9Hz elevated signals and peaks that Oli found seem to be gone. Plot attached.
TITLE: 03/31 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 155Mpc
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 19mph Gusts, 12mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.17 μm/s
QUICK SUMMARY:
Ibrahim is handing over an H1 which has been at Nominal Low Noise for 2+hrs (and a nicer range just under 160Mpc---woo woo Sqz commissioning work this morning). Ibrahim also schooled me on when wind at EY can cause us grief if it hits EY at a pesky angle---like it was at 2000utc today).
Speaking of winds, it's continues to be generally below 25mph for the last 12hrs (but the forecast says it should drop after sunset. Secondary microseism had a small hump up between 10-22hrs ago and hovers just over the 50th percentile.
TITLE: 03/31 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY:
IFO is in NLN and OBSERVING as of 21:24 UTC
Overall calm final day of O4b with a successful comissioning session. Things of note:
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 15:17 | FAC | Nellie | MX | N | Technical Cleaning | 16:12 |
| 15:17 | FAC | Kim | MY | N | Technical Cleaning | 16:11 |
| 17:10 | FAC | Kim | H2 Building | N | Technical Cleaning | 17:18 |
| 17:43 | ISC | Mayank, Siva, Keita | OptLab | Yes | ISS Array work | 19:30 |
| 21:11 | ISC | Jennie, Mayank, Rahul, Keita, Sivananda | Optics Lab | Yes | ISS Array Work | 00:11 |