TITLE: 10/16 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 9mph Gusts, 7mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.36 μm/s
QUICK SUMMARY:
TITLE: 10/16 Eve Shift: 2330-0300 UTC (1630-2000 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: None
SHIFT SUMMARY: I've been picking up where commissioners left off this afternoon trying to engage more full IFO ASC loops.
When we reached PREP_ASC for the first time on my shift, I updated the green alignment references (SDF screenshots attached). My intention tonight was to get the references updated again once more ASC was on, but this proved slow-going as there have been many locklosses in PREP_ASC between 2 and 30 minutes spent in the state. By hand, I was enabling CHARD, INP1, and PRC2 (all P&Y) without any adjustment needed, then I moved PRM in pitch to bring the ADS PIT3 error signal to zero and close it as well. At 01:55 UTC (GPS 1476150918) is when I had all of these loops closed and close to converged. My plan after that was to start moving PRM in yaw to close YAW3, but we lost lock and haven't spent enough time in PREP_ASC on subsequent relocks since then for me to finish that process.
Relocking up to PREP_ASC continues to be smooth, and Sheila is taking over commissioning for the evening.
Louis, Sheila
I ran wfsreliefpast.py 1476150918 to go back to the alignment where Ryan had ADS P3 close to 0 and 8 ASC loops closed. This worked well, we relocked without an issue and indeed ADS P3 was close to zero. I ran the QPD scripts before trying to close any asc. We lost lock quickly, but the scripts were nearly done so Louis and I captured the green references and SDF'd them.
A large earth quake tripped ISI and HEPI ETMX, Louis reset the watchdogs (including the IOP DACKILL) after things had calmed down a bit.
Sheila, Louis, Elenna
We have been repeatedly locking fairly well to prep_asc_for_full_ifo. We have set some green references to a decent alignment. However, we have not been able to set the green references to the alignment that we think is best, which we got to after we walked dofs and closed some loops. However, the attached green references get us close enough.
We have successfully closed CHARD, INP1 and PRC2 P and Y. We tried closing MICH P without problems, but closing MICH Y seems to cause problems either by itself or with MICH P. We also starting walking the PRM to bring ADS3 to zero, but only got about a third of the way before a lockloss.
When we did successfully close MICH P, we did so with half gain, this gives about a 0.5 Hz UGF, based on this somewhat sketchy OLG. The design is for 2 Hz, but we think this is ok for now.
I disengaged PRC1 loop in DRMI ASC for now until we know what PRM alignment we will be happy with in full lock. The PRC1 error signal is set by arbitrary offsets on POP A, and we may prefer a different PRM alignment in full lock.
Sheila, Oli, and I took a look at some of our locklosses. We continue to lose lock while sitting in prep_asc, some we can attribute to alignment engagement going haywire, and others we have no reason for. The lockloss tool seems to be tagging many of these locklosses as "IMC" meaning that the IMC is dropping out within 50 ms of the power drop on AS_C. However, Oli notes that the L2 signals of all four test masses seem to be diverging even before the IMC drops out, so maybe this tag is misleading. The behavior of the coil drives suggests that maybe something is going wrong in DHARD P.
Sheila and I found that there are two DARM boosts we could be engaging, that are usually engaged around DARM offset or PREP DC readout. This might help suppress some low frequency DARM motion that DHARD could also be seeing. I moved both of these boosts to DRMI_TO_POP.
As a side note, we successfully used Stefan's "wfsreliefpast.py" script to revert to some good alignment we had when walking full IFO alignment!
TITLE: 10/15 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: Commissioners worked on ASC loops and CARM, the IFO can relock up to DRMI pretty quickly with its current alignment.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 16:35 | TCS | Camilla, Miriam | LVEA | Y | Move CHETA-Y barrier | 16:48 |
| 17:51 | CAL | Tony, Caroline | PCAL lab | LOCAL | TSK measurement setup | 18:20 |
| 20:21 | Mallika, Alex, Rachel | EndX | N | Walking | 20:44 | |
| 21:03 | TCS | Camilla | CER | Y | Grab headsets | 21:08 |
| 21:22 | TCS | Camilla, Sophie, Miriam | LVEA | Y | CHETA-Y laser measurements | Ongoing |
| 23:02 | CAL | Tony, Fil | EndX | N | Check on PCAL power supply and Chassis | Ongoing |
TITLE: 10/15 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 18mph Gusts, 11mph 3min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.25 μm/s
QUICK SUMMARY: Commissioning continuing, currently in PREP_ASC and setting green alignment references.
Closes FAMIS85193, last checked in alog92229
For the OUT building fans, EX_FAN2_570_2 (yellow) looks a bit noisier, on MY_FAN2_270_1 (pink), the noise seems more periodic than previously. They're all under 0.7.
For the CS building fans, everything looks fine.
Closes FAMIS85193, last checked in alog92117
Laser Status:
NPRO output power is 1.842W
AMP1 output power is 70.67W
AMP2 output power is 139.8W
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PDWD watchdog is GREEN
PMC:
It has been locked 23 days, 5 hr 24 minutes
Reflected power = 29.77W
Transmitted power = 104.9W
PowerSum = 134.7W
FSS:
It has been locked for 0 days 0 hr and 8 min
TPD[V] = 0.5066V
ISS:
The diffracted power is around 2.8%
Last saturation event was 0 days 0 hours and 9 minutes ago
Possible Issues:
PMC reflected power is high
Over the years, we've changed the order of guardian states, but choose not to renumber them during O4 so that trending would not be confusing. I've now renumbered several guardain states in ISC_LOCK, so that they now appear on the medm screen in the order that they happen. I also moved their locations in the ISC_LOCK file, so that file is more closely ordered in the way things happen.
I've deleted 4 states that were in use when we were changing our DARM loop but are no longer used.
Camilla, Miriam, Travis, Sophie
First attempt measuring the beam after a long propagation distance using the FLIR camera. Here are the measurement distances, laser power settings and corresponding images. Using the Fintrace model the beamsize at each point was modelled.
| Distance from QCL [m] | QCL power [W] | image range | Modelled Beamsize [x,y] [mm] |
| 5.732 | 0.2 | 280-284 | 7.087,7.233 |
| 8.5006 | 0.2 | 285-287 | 10.932,11.4911 |
| 15.871 | 0.2 | 288-289 | 21.219,22.868 |
| 23.618 | 0.4 | 290-291 | 32.047,34.840 |
| 32.216 | 0.6 | 292-297 | 44.069,48.129 |
note: Nominal distane to ITM is 36.735m but will be subject to exact table placement
Here is a drive with the pictures: https://drive.google.com/drive/folders/153uQSwYIMZdKYFz6KgaSdyBdOywcY-T0?usp=drive_link
A comment will be added with the procedure :)
[Sophie, Camilla, Travis, Miriam]
(This work was done yesterday, October 14, 2026)
The table layout that we used for the projections is this one. Where the distances from the QCL -> M1 -> M2 -> M3 -> M4 are the same distances as per the model that is stored in the cheta_modeling git repo.
The distances from M4 through D are not part of the original CHETA table setup and they were just used and labeled like that for the projections we were doing. The distances in between these mirrors is detailed in the image itself.
Now, before starting the projections we aligned the green laser to the irises on the table, this is to make sure the the green laser is co-aligned with the QCL CHETA laser. We started by projecting the green laser a short distance outside of the table onto a laser barrier to see where it landed, then turned the green laser flipper down to then project the CHETA laser (onto the same barrier) and checked they landed both as close to each other as possible. We moved the laser barrier back several times, each time checking where our green laser landed first. To see the CHETA beam we were using a FLIR camera (EXTECH i5). You can see our amazing pictures (taken at different distances) in the Google folder Sophie shared in this alog.
Camilla was pointing the FLIR camera to the beam (which was hitting the laser barrier) and I was holding a metal ruler which had very skinny pieces of tape taped every centimeter (I was warming up the ruler with my hands in between measurments), the ruler was hold either below or on top of the beam to gauge the beam size at the specific distances we were measuring it at. In this picture, you can see Camilla with the FLIR camera and me with the ruler, artistically framed by Sophie. Sophie was out laser operator. The QCL CHETA laser was always started at minimum power (0.5 A) and then slowly brought to full power until we could see the beam on the barrier/FLIR camera.
We use the minimum QCL power possible to still be able to see the beam, which meant we were chaging the power of the QCL with the rotaiton stage as we were moving away from the table. For the specific power that we used, see Sophie's table above.
We note that tha the laser barrier was flimsy and therefore it was challenging to keep the fabric straight while taking our pictures. Today we will go back to do more projectes and we will use a slightly less flimsy barrier to project the laser into.
This was done for CHETA Y, along the Y-arm inside the LVEA.
Last night, at 2W, we adjusted gains on the common mode board to achieve a carm UGF of about 15 kHz with 56 deg of phase margin, which we thought was close enough to our target (92306). I searched back in the alog and found a time when Sheila and Matt measured the CARM OLG at 2 W during O4 (May 2025), 84644. Matt reported a ugf of 11 kHz with 41 deg of phase margin.
Below is a table comparison of the common mode board gains between last night and this time in May 2025.
| Date | LSC REFL_SUM_A_IN2GAIN | LSC REFL_SERVO_IN1GAIN | LSC REFL_SERVO_FASTGAIN | IMC REFL_SERVO_IN2GAIN | IMC REFL_SERVO_IN1GAIN | IMC REFL_SERVO_FASTGAIN | LSC REFL_SERVO_COMCOMP | Overall CMB gain | UGF/Phase Margin |
| May 2025 | 12 | 0 | 16 | -22 | 3 | 5 | ON | 6 | 11 kHz, 41 deg |
| Now | 3 | 0 | 7 | 0 | 2 | 5 | OFF | 10 | 15 kHz, 56 deg |
This means that we have overall increased the common mode board gain by 4 dB, and maybe held on to more phase by not engaging the common comp boost. Perhaps we could drop the gain by 4 dB and have more room to turn on the comcomp.
Last night, we were worried that we might have lost some optical gain in CARM. However, this comparison indicates that actually we probably are the same as before.
Sophie, Miriam, Camilla
After Sophie and Miriam checked and adjusted the calibration of our thermal PD_C, we calibrated the CHETA ITMY Rotation stage using an updated veriosn of Ryan's Rotation Stage calibration code, now saved as /tcs/h1/scripts/RS_calibration/CHETA_CalibRotStage.py
TITLE: 10/15 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 4mph Gusts, 3mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.22 μm/s
QUICK SUMMARY:
Elenna, Sheila, Louis, Ryan Crouch, Tony
Summary- The IFO seems stable with ANALOG_CARM, and several ASC loops have been engaged.
I think this got missed in the details, Louis and I tried to engage the common comp boost, which is a 40 Hz/4 kHz. We think it caused a lockloss, so we commented it out of the guardian for now.
TITLE: 10/15 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: None
SHIFT SUMMARY:
NUC 30 never got re-imaged tonight as people were still actively using it.
Locking Notes:
Got up to PREP_ASC_FOR_FULL_IFO[429] @ 00:45 UTC for the first time tonight.
Duration: Stayed there for 14 minutes 48 seconds.
Violin Damping: Damping On RF actually started 11 minutes into Prep-ASC_4_F-IFO and Damping Lasted 3 minutes.
Delta PR_GAIN increased by ~0.6 once the damping started.
Initial mean:46.823
Final mean : 47.59
PopAIR_B_RF18: changed by -4.4 in the 14 minutes but it was a gradual change and the variabliliy in the signal may exceed this.
Initial: 101.9
Final: 97.51
PopAir_B_RF90 changed by +4.2 in the 14 minutes also gradually with variability in the signal.
Initial:15.3
Final: 19.4
Lockloss at 00:59 UTC
Next attempt reached Prep ASC @ 1:15 UTC & lasted 5 minutes.
Damping started but lost lock before VIOLIN_DAMPING guardian got out of DAMPING_SETTINGS[3].
PR_GAIN: mean increased by ~0.18 in that duration.
Initial Mean: 47.32
Final Mean: 47.53
PopAir_B_RF18: No change
PopAir_B_RF90 delta : 1.48
Initial: 19.15
Final: 20.64
Lockloss @ 1:20 UTC
Next attempt reached Prep ASC @ 1:40 UTC & lasted 6 minutes.
Damping started but lost lock before VIOLIN_DAMPING guardian got out of CLEAR_MONITORS[4].
delta PR_GAIN: mean increased by ~0.14 in that duration
Initial:47.25
Final:47.4
Delta PopAir_B_RF18: -3.2
Initial:101.27
Final:97.5
Delta PopAir_B_RF90: +2.1
Initial: ~15.91
final: ~18.08
Lockloss @ 1:46 UTC
Next Prep_ASC_For_FULL_IFO @ 158 UTC
Duration: 3 minutes.
No Violin damping.
PR_GAIN DELTA: 0.2
Initial:47.3
Final:47.5
PopAir_B_RF18 delta: no change
PopAir_B_RF90 delta: no change
Lockloss from Prep ASC @ 2:02 UTC
Lockloss from Start_TR_CARM @ 2:25 UTC
Arrived at Prep_ASC_For_FULL_IFO @2:51 UTC
Lockloss from Prep_ASC_For_FULL_IFO @ 2:52 UTC
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 22:09 | TCS | Camilla, Sophie, Miriam, Travis | LVEA | Y | Project CHETA beam onto barrier/wall, Travis Out at 23:46 | 00:00 |
| 23:10 | VAC | Gerardo, Jordan | MidY | N | CP3 line investigation | 23:47 |
TITLE: 10/14 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 10mph Gusts, 5mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.20 μm/s
QUICK SUMMARY:
H1 is currently Aquiring_DRMI_1F.
The commissioning team is back at it again sittign in RESONANCE [410] coming up with a game plan to get to CARM_to_Analog [420] without a lockloss.
VAC team went to investigate CP3 fill line.
NUC 30 will be down for a while so I can swap it's hard drive and re-image it.
Caroline C and I went down to EX... again.... (Sorry EY, I know it was your turn, but next time I promise I'll measure you... )
We took the PS4 Working Standard (WS) integrating sphere down to EX.
We found EX's PCAL system is covered in caution tape, like it was in the center of a foreboding crime scene!
Unfortunately the red Current Limit LED was Lit again, and I trended the channel H1:CAL-PCALX_LASERDIODECURRENT back to find it has been lit up since last Tuesday. Supisiously close to the beckhoff restart time. I'm not sure which channel is best to check for beckhoff restarts yet. I was able to just move the voltage down a little and back up to rectify this issue before starting the measurement.
We took some pictures of the beam spots before we started to prove our innocence.
Followed instructions on T1500062 and followed it without any deviations from our part. The SEI system was put in ISI Damped HEPI offline for this measurement for other work though.
Everything went as smooth as it can while dodging lifts, scaffolding, and caution tape.
Took some After measurement beam spot pics to prove our innocence again.
Overall I don't think the GV20 work had any real impact on PCAL pointing or performance. Shoutout to the GV20 team for doing such a great job!
Wanna see the Absolute Calibration details of this specific measurement and the commands input and output? :
@cdsws25: python3 generate_measurement_data.py --WS PS4 --date 2026-10-13
Reading in config file from python file in scripts
../../../Common/O4PSparams.yaml
PS4 rho, kappa, u_rel on 2026-10-13 corrected to ES temperature 299.8 K :
-4.700380443762894 -0.0002694340454223 0.0007505543347185126
Copying the scripts into tD directory...
Connected to h1daqnds1
martel run
reading data at start_time: 1475945650
reading data at start_time: 1475946100
reading data at start_time: 1475946460
reading data at start_time: 1475947100
reading data at start_time: 1475947444
reading data at start_time: 1475947820
reading data at start_time: 1475947998
reading data at start_time: 1475948640
reading data at start_time: 1475949030
Ratios: -0.45984106211593845 -0.46714267909102675
writing nds2 data to files
finishing writing
Background Values:
bg1 = 9.805339; Background of TX when WS is at TX
bg2 = 5.167711; Background of WS when WS is at TX
bg3 = 9.886270; Background of TX when WS is at RX
bg4 = 5.195956; Background of WS when WS is at RX
bg5 = 9.755134; Background of TX
bg6 = 0.367068; Background of RX
The uncertainty reported below are Relative Standard Deviation in percent
Intermediate Ratios
RatioWS_TX_it = -0.459841;
RatioWS_TX_ot = -0.467143;
RatioWS_TX_ir = -0.454541;
RatioWS_TX_or = -0.462195;
RatioWS_TX_it_unc = 0.068338;
RatioWS_TX_ot_unc = 0.070460;
RatioWS_TX_ir_unc = 0.074890;
RatioWS_TX_or_unc = 0.065120;
Optical Efficiency
OE_Inner_beam = 0.988231;
OE_Outer_beam = 0.989349;
Weighted_Optical_Efficiency = 0.988790;
OE_Inner_beam_unc = 0.046695;
OE_Outer_beam_unc = 0.045578;
Weighted_Optical_Efficiency_unc = 0.065252;
Martel Voltage fit:
Gradient = 1636.946737;
Intercept = 0.081815;
Power Imbalance = 0.984370;
Endstation Power sensors to WS ratios::
Ratio_WS_TX = -1.078768;
Ratio_WS_RX = -1.391922;
Ratio_WS_TX_unc = 0.042184;
Ratio_WS_RX_unc = 0.040097;
=============================================================
============= Values for Force Coefficients =================
=============================================================
Key Pcal Values :
GS = -5.135100; Gold Standard Value in (V/W)
WS = -4.700380; Working Standard Value
costheta = 0.988362; Angle of incidence
c = 299792458.000000; Speed of Light
End Station Values :
TXWS = -1.078768; Tx to WS Rel responsivity (V/V)
sigma_TXWS = 0.000455; Uncertainity of Tx to WS Rel responsivity (V/V)
RXWS = -1.391922; Rx to WS Rel responsivity (V/V)
sigma_RXWS = 0.000558; Uncertainity of Rx to WS Rel responsivity (V/V)
e = 0.988790; Optical Efficiency
sigma_e = 0.000645; Uncertainity in Optical Efficiency
Martel Voltage fit :
Martel_gradient = 1636.946737; Martel to output channel (C/V)
Martel_intercept = 0.081815; Intercept of fit of Martel to output (C/V)
Power Loss Apportion :
beta = 0.998895; Ratio between input and output (Beta)
E_T = 0.993829; TX Optical efficiency
sigma_E_T = 0.000324; Uncertainity in TX Optical efficiency
E_R = 0.994929; RX Optical Efficiency
sigma_E_R = 0.000325; Uncertainity in RX Optical efficiency
Force Coefficients :
FC_TxPD = 7.894807e-13; TxPD Force Coefficient
FC_RxPD = 6.188002e-13; RxPD Force Coefficient
sigma_FC_TxPD = 3.610367e-24; TxPD Force Coefficient
sigma_FC_RxPD = 2.777621e-24; RxPD Force Coefficient
data written to CDS: /ligo/gitcommon/Calibration/pcal/O4/ES/measurements/LHO_EndX/tD20261013
That's cool and all but perhaps you wanna see that data with relation to the End X's history, I gotchu:
You can see the trends here or go to the git page for this measurement.
The current limit issue came back again today after I powercycled the PCAL laser.
I left it in that state so Fil and I can go down to EX to check on the powersupply in the racks.
There are 3 potential failure points.
The powersupply in the racks.
The powersupply in the chassis.
Or the laser head it's self.
Fil suggests that since it's likely not the power supply in the racks, perhaps it's time to retire the decade old PCAL laser at EX.
I will start preparing for a laser swap at EX.