Displaying reports 221-240 of 89075.Go to page Start 8 9 10 11 12 13 14 15 16 End
Reports until 18:30, Wednesday 12 August 2026
H1 SPI
jennifer.wright@LIGO.ORG - posted 18:30, Wednesday 12 August 2026 (91504)
Updated SRC output filters

Jennie W, Jim W,

 

We swapped out the cdsOutput blocks SPI-H23_LO_SRC_CLKMON, SPI-H23_LO_SRC_SINMON, SPI-H23_LO_SRC_COSMON for cdsfilt clocks so we can put in some gains and readout fast channels in medm at this point in the model.

I made these changes in the HJK library part for SPI.

These filters banks are switched on with a gain of 1 but I still need to update the medm screen with the new channels and filter banks.

I also added the channels SPI-H23_LO_SRC_CLK_IN1, SPI-H23_LO_SRC_SIN_IN1, SPI-H23_LO_SRC_COS_IN1 to the DAQ channel list for the spi model.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 16:34, Wednesday 12 August 2026 (91491)
Wed DAY Ops Summary

TITLE: 08/12 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Ibrahim
SHIFT SUMMARY:

Today there was closeout work for HAM7 (with the plan of closing up HAM7 tomorrow).  Masayuki continued with overall detector work locking PRMI and working on JAC.  CDS team carried out a list of activities activiites in the afternoon (they were done in under an hour).  CRS work continued.  Jenne & Mike led a tour for small group from the Dept of Energy.

Smoke worsened rapidly around noon PDT with AQI dropping from GOOD to MODERATE  to UNHEALTHY by the end of the day. (could no longer see Rattlesnake)

LOG:

H1 ISC (ISC)
masayuki.nakano@LIGO.ORG - posted 14:45, Wednesday 12 August 2026 - last comment - 11:08, Thursday 13 August 2026(91501)
PRMI locked

Summary

PRMI locked!!
The MICH loop was reworked, the PRCL gain was raised, and the REFLAIR demodulation phases were tuned. The guardian has been updated to the new nominal.


Loop adjustment

After aligning BS and PRM using PRX and MICH, I first tried to lock with ISC_DRMI as it was, changing nothing. It never caught after about 20 minutes of waiting in total, split between yesterday and today.

So I went back to the MICH loop. With PRM misaligned and MICH locked, I measured the open loop gain. The UGF was at 5 Hz and the phase margin sat around 20 deg across 5–10 Hz. So, I decided to modify the MICH loop and push UGF up to 10 Hz with reasonable phase margine.

The largest phase eater was the ELP35 in FM2 of BS_M3_LOCK. I loaded an ELP200 into FM3, which was free, and used it in place of the ELP35 in FM2. That loosened the phase roll-off enough to give about 40 deg of margin at 10 Hz.

Back to PRMI. MICH1 and MICH2 also carried several low-pass filters, so I switched all of them off, and it locked within a few minutes. Once locked, all of the low-passes could be switched back on without losing lock.
Repeating this, it locked within a few minutes every time.

With the lock holding I measured the MICH and PRCL loop gains. MICH showed gain bump above 10 Hz, and the PRCL UGF turned out to be only 20 Hz. Doubling the PRCL loop gain brought its UGF up to 55 Hz, and the MICH gain bump went away. This was the most stable state I found, and the time to reacquire came down to 1–2 minutes, so I took it as the nominal and edited the guardian at this point.


Servo change summary

Filter changes

Filter bank Module Change
MICH1 FM5 (LP80) off for acquisition, on after lock
MICH2 FM2 (LP50) off for acquisition, on after lock
BS M3 LOCK FM2 (ELP35) → FM3 (ELP200) permanent; ELP200 newly loaded into the empty FM3
REFLAIR_A_RF9 input matrix set to 3.5, doubling the PRCL loop gain

Guardian edits

What File Line
MICH1 FM5 lscparams.py 530
MICH2 FM2 ISC_DRMI.py 219
BS M3 LOCK, ELP35 → ELP200 ISC_DRMI.py 298, 523, 585
REFLAIR_A_RF9 input matrix lscparams.py 718
Engage the low-passes after lock ISC_DRMI.py 628–630

REFLAIR demodulation phase

Last, I tuned the REFLAIR demodulation phases. A 50 Hz excitation of amplitude 3 was injected into PRCL1 ERR, and the phases were adjusted to minimise the peak in RF9_Q and RF45_Q. The I peak heights did not change much.

  demod phase [deg] Q peak height
RF45 -176 → -171 0.1 → barely visible
RF9 -29 → -34 0.1 → barely visible

OLG

A final open loop gain measurement gave:

Loop UGF Phase margin
MICH 10 Hz 50 deg
PRCL 50 Hz 50 deg

Both open loop TFs are attached.

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 11:08, Thursday 13 August 2026 (91517)

I do not understand why the PRCLK gain was low by a factor of 2, but Elenna noted a similar gain loss in March: 89567, this didn't go into the guardian at the time but is probably the same gain loss that Masayuki put into the PRMI input matrix yesterday.  

H1 SUS (SUS)
rahul.kumar@LIGO.ORG - posted 14:18, Wednesday 12 August 2026 - last comment - 14:59, Wednesday 12 August 2026(91500)
HAM7 close-out measurements - Suspensions look healthy!

Ryan C, Rahul

We have taken the pre-door close transfer function measurements on ZM1-5, FC1 and OPO and they all look healthy. I am attaching screenshots of ZM1-5 below (ZM4 results was posted by Ryan C yesterday - see alog 91486).

Ryan will post screenshots of FC1 and OPO in the comments section. 

HAM7 doors can close once seismic is happy as well.

Non-image files attached to this report
Comments related to this report
ryan.crouch@LIGO.ORG - 14:59, Wednesday 12 August 2026 (91502)

Adding screenshots of the OPO and FC1 suspensions.

Non-image files attached to this comment
H1 CDS
jonathan.hanks@LIGO.ORG - posted 12:20, Wednesday 12 August 2026 (91498)
WP 13472 - new frame writer software on h1daqfw1 + OS upgrade

Per WP 13472 the new frame writer software is deployed on h1daqfw1 and is writing frames.

We will need to do a daqd restart later to change the set of channels we are monitoring from the frame writers.  That will be scheduled with the control room.

It was done the same was as h1daqfw0.

 * Upgrade the OS in place to Debian 12

 * Apply the puppet policy

 * Restart to make sure everything loads

We will leave the nds1 redirect in place until the end of the day.

H1 ISC
masayuki.nakano@LIGO.ORG - posted 10:59, Wednesday 12 August 2026 (91495)
REFL AIR PD alignment check

I checked the REFL AIR PD centering at ISCT1. The centering was good from before I made move.

For the future reference, the PMC single bounce power is 2.64 at H1:LSC-REFLAIR_A_LF_OUT, and 5.5 at H1:LSC-REFLAIR_B_LF_OUT

H1 CDS
jonathan.hanks@LIGO.ORG - posted 10:40, Wednesday 12 August 2026 - last comment - 10:41, Wednesday 12 August 2026(91493)
WP 13472 - redirected queries to h1daqnds1 towards h1daqnds0

Per WP 13472 we will be upgrading the software on h1daqfw1.  In preparation for that we are redirecting all requests to h1daqnds1 onto h1daqnds0 (whose frame writer will be running through this).

 

Comments related to this report
jonathan.hanks@LIGO.ORG - 10:41, Wednesday 12 August 2026 (91494)

This should be transparent.  You should not have to do anything except maybe push the start button on your data viewer.

H1 SEI
shoshana.apple@LIGO.ORG - posted 10:06, Wednesday 12 August 2026 - last comment - 16:43, Wednesday 12 August 2026(91485)
CRS Commissioning Update Cont and Noise Hunting

8/11/26

[Huyen, Jim, Michael, Shoshana]

CRS Commissioning (from list in G2601523):

Noise Hunting:

Images attached to this report
Comments related to this report
shoshana.apple@LIGO.ORG - 12:13, Wednesday 12 August 2026 (91496)

Continued Noise Hunting

  • Changing temperature value on temporary TEC
    • Did math, to get a laser temp of 20 degree C, need to set R to 12.53kΩ
    • R=R0*eβ*(1/T - 1/T0) with R=set resistance (in Ω), R0= 10kΩ, T=desired temperature in K, T0 = 25oC = -248.15 K, β = 3950 K (information from E2600086 & TEC data sheet)
    • We have switched this back to 10.72, (i.e. 25 C), as that is where the laser is meant to operate  
  • Reducing Fiber Bend
    • in order to get rid of the bend in the fiber, we are just leaving the cover open, which we are allowed to do because there is a clasp on the connection point which cannot be opened by hand (picture 1)

Results: 

  • Neither adjusting the TEC or straightening out the fiber improved the noise (picutre 2)
  • It is unlikely that the excess noise is coming from the laser
  • Both HoQIs give around the same noise spectrum, so it's unlikely it's from the CRS drifting or being un-centered. 
  • There is very little coherence between the SUM and the HOQI_DIST which indicates that the SUM is working as a good estimate of the incoherent noise (i.e. the instrument noise)

Next Steps:

  • There is the possibility that the CRS is too rung up (i.e. not damped down enough) to get a good noise floor measurement
  • The constant low frequency drift/oscillation that we see in all the readouts from the ISI motion could also be a source of the excess noise, which we can test via putting the SUM data through a high pass filter and taking the spectra of that data. 
Images attached to this comment
shoshana.apple@LIGO.ORG - 15:20, Wednesday 12 August 2026 (91499)

Put the HoQI signals through a high pass in the front end, but this didn't fix the noise issue. (picture 1)

We grounded the damping pins to see if that would reduce some of the noise.

Additionally, the TEC should be set to 10.72, and stay there as that is ideal for the laser

 

Images attached to this comment
shoshana.apple@LIGO.ORG - 16:43, Wednesday 12 August 2026 (91503)

Damped down the CRS as much as it could go and took a spectra and left the damping on. When the damping is left on and soon after it is turned off, it looks like there is some slight improvement at the 1-3Hz range in the SUM measurement (picture 1). 

Additionally, we want to look at the drift that CRS sees, it's probably the CRS still settling, but it's something to keep an eye on

Images attached to this comment
LHO General
corey.gray@LIGO.ORG - posted 07:41, Wednesday 12 August 2026 (91492)
Wed DAY Ops Transition

TITLE: 08/12 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 2mph Gusts, 0mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.06 μm/s 
QUICK SUMMARY:

Went to EQ Mode twice overnight.  On the docket for today:  HAM7 close-out begins, Input Alignment work will continue, CDS w/ DAQ restarts in afternoon, HAM8 Annulus Ion Pump activity, & DOE tour in the afternoon.

H1 IOO (IOO)
masayuki.nakano@LIGO.ORG - posted 22:31, Tuesday 11 August 2026 - last comment - 13:02, Thursday 13 August 2026(91487)
Absolute angular calibration of the JAC steering actuators from the second harmonic of the cavity transmission.

Summary

We have calibrated the two JAC steering actuators the PZT (IO_MB_M4) and the JM1, in μrad per drive count at DC. The scale comes from the second harmonic of the cavity transmission under a dithered drive, which is insensitive to DC misalignment and so needs no external angle reference. 


Method

By expanding the injected field in the cavity's own eigenmode basis, we can describe the misaligned as,

Ein(t) = E0 + δ(t) E1

with E0 the cavity's TEM00 mode and E1 the TEM10 (pitch) or TEM01 (yaw) mode, orthonormal. As long as the misalignment is small enough comparing to the beam size, the single complex coefficient δ carries the whole misalignment on that axis: its real part is a transverse displacement in units of the waist size, its imaginary part an angle in units of the divergence angle. Only the TEM00 is resonant, so the transmitted power follows the fraction of the input that sits in E0, i.e. 1 − |δ|2 for |δ|2 « 1.

Dithering a steering actuator makes δ oscillate about whatever value it already had:

δ(t) = δofs + δa cos(2πft)

where δofs is the static misalignment already present, and δa is the dither we deliberately applied, which is exactly the quantity we want in order to calibrate the actuator. TRANS signal (1 − |δ|2) can devided into three components with its frequecies:

frequency value contains the unknown δofs?
DC ofs|2 + |δa|2/2 yes
f 2 Re(δofs*δa) yes — magnitude and relative phase
2f a|2/2 no

The static offset drops out of the second harmonic algebraically. 2f therefore delivers a| with no reference to the alignment state we happened to be sitting at, and with no external angle standard. The DC and f terms, the two one would reach for first, are both contaminated by it.

This is the whole point of the method, and it is directly visible in the plot. adding a static offset grows the 1f line by +528 % while the 2f line moves by +8 %, its own measurement noise.


Measurement

I proceeded 4+1 measurement in total with the JAC locked. For each measurement, one actuator axis was dithered at 11 Hz, with the excitation injected on the channels below and the drive read back on the corresponding _OUT. I excited JM1/PZT PIT/YAW per one measurement, and the other one is the PZT_PIT excitation with static offset (30 cnts) to demonstrate that the 2f peak is not affected by the offset. Transmission was read on H1:JAC-TRANS_A_LF_OUT.

record excitation channel drive read back on amplitude at 11 Hz [cnt] drive offset [cnt] TRANS DC [cnt]
PZT_PIT H1:JAC-PZT_PIT_EXC H1:JAC-PZT_PIT_OUT 20.0 0 6451.2
PZT_PIT_ofs H1:JAC-PZT_PIT_EXC H1:JAC-PZT_PIT_OUT 20.0 30 6442.5
PZT_YAW H1:JAC-PZT_YAW_EXC H1:JAC-PZT_YAW_OUT 20.0 0 6442.6
JM1_PIT H1:SUS-JM1_M1_TEST_P_EXC H1:SUS-JM1_M1_TEST_P_OUT 40.0 0 6445.5
JM1_YAW H1:SUS-JM1_M1_TEST_Y_EXC H1:SUS-JM1_M1_TEST_Y_OUT 40.0 0 6440.2

a| is calculated from peak heights of the transmission at 22 Hz, converted to a mirror tilt using the local beam radius at each actuator from the current JAC reflected-path layout model (alog91472 comment), and calibrated into DC responce using each actuator's frequency response as measured (described below).


Results

actuator axis excitation channel a|2 efficiency [μrad/cnt]
at 11 Hz (as measured) at DC
PZT PIT JAC-PZT_PIT_EXC 1.09e-5 0.0093 0.083
PZT YAW JAC-PZT_YAW_EXC 6.47e-6 0.0093 0.079
JM1 PIT SUS-JM1_M1_TEST_P_EXC 1.01e-5 0.0216 0.89
JM1 YAW SUS-JM1_M1_TEST_Y_EXC 1.67e-5 0.0254 0.92

The 11 Hz column is what the dither actually produced; the DC column is that value divided by the actuator's own response at 11 Hz, and is the number to use for a DC gain. 


Appendix

Actuator frequency response

The frequency response itself comes from a separate set of four broadband actuator-to-wavefront-sensor records (300 s each, one actuator per record, see atatched plots), from which the JM1 suspension resonance and the PZT drive pole are fitted. Only the shape of those transfer functions is used; their absolute scale plays no role in the calibration.

The fitted frequency responses are:

AOI compensation

Both actuators sit at a design AOI of 45°, and the rows above include the geometric correction that follows. A tilt whose rotation axis lies in the mirror surface and in the plane of incidence steers the beam by only 2θ cos(AOI), against the full for the axis perpendicular to that plane. At the PZT the suppressed axis is YAW in the cavity-referred channel naming (the HAM1 periscope exchanges the transverse planes downstream of it); JM1 sits after that periscope, so for it the suppressed axis is PIT. The assignments follow from each mirror's orientation, and the correction uses the design 45° rather than a value fitted to the measured ratio.

Cross-checks

Images attached to this report
Comments related to this report
masayuki.nakano@LIGO.ORG - 13:02, Thursday 13 August 2026 (91523)

Short note: a mirror rotated by θ, sitting where the beam radius is w(z), produces |δ| = k w(z) θ, and its phase relative to TEM00 is 90° plus the Gouy phase accumulated from the reference waist. This can be applied for the mirror which is transmitting the lens. This is because δ is the field amplitude of the first-order mode it is continuous across lenses, so a mirror separated from the reference space by lenses is handled by simply adding up the free-propagation Gouy phase to the reference waist. The table below therefore carries the beam radius and the accumulated Gouy phase at each actuator.

actuator axis excitation channel a|2 efficiency [μrad/cnt] beam radius
w [mm]
Gouy phase from
the JAC waist [deg]
at 11 Hz (as measured) at DC
PZT PIT JAC-PZT_PIT_EXC 1.09e-5 0.0093 0.083 3.020 -86.4
PZT YAW JAC-PZT_YAW_EXC 6.47e-6 0.0093 0.079 3.270 -73.5
JM1 PIT SUS-JM1_M1_TEST_P_EXC 1.01e-5 0.0216 0.89 0.620 -32.7
JM1 YAW SUS-JM1_M1_TEST_Y_EXC 1.67e-5 0.0254 0.92 0.681 -30.8

The beam radius (1/e2 intensity) and the Gouy phase are model values at the actuator, taken from the JAC REFL optical model.

H1 PSL
ryan.short@LIGO.ORG - posted 17:23, Tuesday 11 August 2026 (91489)
PSL 10-Day Trends

FAMIS 63911

PMC REFL has been rising very slightly, but otherwise, no major events of note.

Images attached to this report
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 17:20, Tuesday 11 August 2026 (91488)
X-Arm Peek, GV8 Open for the Day

(Travis S., Gerardo M.)
Around 11:00 am today we opened GV8 from soft close to allow for commissioners to peek down x-arm.  The gate annulus for GV8 was burped into the annulus ion pump, almost no response.  The 4 turbo pumps were isolated from the main vacuum envelope, the 4 large ion pumps are valved in, along with HAM6 ion pump (500 l/s), and we still have a filter cavity section valved into the main corner volume, the section from FCV-3 to FCV-4, and includes ion pump B-1 (150 l/s).
GV8 remained open for about 5 1/2 hours.
We closed GV8 around 16:30 local time.
Attached is a pressure response from gauges along the X-arm at the corner station.

Images attached to this report
H1 General
ryan.crouch@LIGO.ORG - posted 16:32, Tuesday 11 August 2026 (91479)
OPS Tuesday day shift summary

TITLE: 08/11 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: GV8 was opened and closed today for Xarm alignment commissioning, ZM4 PSAMs adjustment was finished up. We had a small power glitch in the afternoon that tripped off the end station HEPIs.
LOG:                            

Start Time System Name Location Lazer_Haz Task Time End
14:33 FAC Kim LVEA Y' Tech clean 15:11
14:59 FAC Chris LVEA Y FAMIS checks 15:26
15:26 FAC Chris All Out BLDs N FAMIS checks around site 17:44
16:09 SEI Carlos LVEA Y Seismometer checks 16:55
16:16 SEI Jim LVEA Y SPI checks 16:28
16:37 OPS RyanC LVEA Y -> N LASER hazard transition, hazard to safe 16:47
16:48 EE Fil LVEA N Check JAC shutter connections 16:52
16:48 EPO Jenne LVEA N Tour 17:30
16:52 EPO Camilla LVEA N Tour 17:25
16:54 SQZ Rahul, RyanS LVEA Y/N HAM7 work, bifurcated laser hazard area 18:15
17:21 EPO Corey LVEA N Tour, in @ 12:00 17:34
17:46 OPS RyanC LVEA N -> Y Laser hazard transition, safe bifurcated to hazard 17:58
17:48 VAC Gerardo, Travis LVEA YES Opening GV8 (XARM) 18:13
18:07 PEM Michael, Shoshana, Huyen LVEA Y NRS hardware under ITMY, Huyen out 18:21 19:45
18:22 ALS Jennie, Masayuki LVEA Y ISCT1 table checks 18:45
18:29 SEI Jim CER Y Quick check SPI, CER maybe LVEA 18:32
19:12 ALS Sheila, Masayuki LVEA Y ISCT1 alignment checks 19:26
19:15 ISC Betsy LVEA Y Checks 19:22
19:29 CDS Dave CER Y Accelerometer checks 00:28
19:43 CDS/SAF Patrick MSR N Beckhoff safety computer investigation 20:03
20:01 FAC Randy LVEA Y Clean room checks 20:58
20:02 EE Fil, Jackie EndX N Reset VFD and remove analog cameras 21:07
20:02 SEI Jim EndX N Reset VFD recover HEPI 20:33
20:03 SQZ RyanS LVEA Y Beam profiles at HAM7 21:50
20:23 SQZ Rahul LVEA Y HAM7 work, ZM4 21:23
20:59 FAC Randy EndY then X N Clean room checks 21:59
21:08 EE Fil, Jackie EndY N Remove analog cameras 21:39
21:25 ALS Sheila, Camilla LVEA Y ISCT1 beatnote adjustment 22:01
21:21 SEI Jim, Huyen FCES N CPS checks/tests 21:45
21:37 SAF Richard Mechanical N HEPI pump checks 21:50
21:39 EE Fil, Jackie CER Y Remove analog camera electronics 23:21
22:11 PEM Shoshana, Huyen LVEA Y CRS laser 22:24
22:19 ISC Sheila, Masayuki LVEA Y ISCT1 alignment checks 23:00
22:58 SEI Michael, Jim LVEA Y Wiggle SPI cable, look at other cabling at TCS rack 23:58
23:10 VAC Gerardo LVEA Y Close GV8 00:28
23:22 EE Fil, Jackie MSR N Remove analog camera electronics 00:22

The gate phone microphone doesn't seem to be working well, one instance I heard nothing after answering, the next was garbled and full of static.

Images attached to this report
H1 ISC
sheila.dwyer@LIGO.ORG - posted 16:06, Tuesday 11 August 2026 - last comment - 09:29, Monday 17 August 2026(91481)
arm peak today, COMM beatnote and PRMI flashes.

Camilla, Oli, Caroline, Masayuki, Sheila

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 09:29, Monday 17 August 2026 (91562)

During this realignment, SR3 was moved 65urad in Pitch, see attached.

Images attached to this comment
H1 SQZ (SUS)
ryan.short@LIGO.ORG - posted 15:57, Tuesday 11 August 2026 - last comment - 15:37, Friday 14 August 2026(91484)
ZM4 PSAMs Preload Adjusted (Again, Final)

R. Kumar, S. Dwyer, C. Compton, R. Short

Following the work done yesterday adjusting the preload on the ZM4 PSAMs (alog91471), Rahul and I set about adjusting it further today to get our calculated projected beam size on SRM close to where we want it. Using the same procedure as yesterday, I turned off the ZM4/5 PSAM drive chassis, Rahul went into HAM7, locked down ZM4, torqued the preload about 1/8" of a turn (it's hard to quantify a torque spec in this manner), then finally unlocked the suspension. I moved the ZM4 pitch alignment slider about -1400 counts to realign the beam on SQZT7 to our alignment irises as a result of this torque adjustment. I then proceeded to take a couple of beam profiles on the table with the M^2 device to see where we landed. This plot [initial] shows the difference between before and after this adjustment in terms of the projected beam at SRM with a few different PSAM settings on ZM4 and ZM5. The four points I took here informed us that we could stand to torque ZM4 a bit further to hopefully line up with the center of the plot.

Rahul went back into HAM7 and torqued another 1/8" and I took another couple of profiles after (I did not need to move ZM4's alignment sliders after this adjustment). I took a total of nine profile points here, all of which can be seen compared to other measurements today on this plot [full]. Since there are points in the bullseye, we decided to stop here and that this is where the ZM4 preloading will stay. This plot [final] shows just the beam profiles taken at our final preloading position.

Tomorrow we will move on to final closeout checks in HAM7.

Images attached to this report
Comments related to this report
ryan.crouch@LIGO.ORG - 16:26, Tuesday 11 August 2026 (91486)SUS

I ran a health check TF on ZM4 and it looks good.

2026-08-11_2200_H1SUSZM4_M1_WhiteNoise_L_0p02to50Hz.xml
2026-08-11_2200_H1SUSZM4_M1_WhiteNoise_P_0p02to50Hz.xml
2026-08-11_2200_H1SUSZM4_M1_WhiteNoise_Y_0p02to50Hz.xml

Non-image files attached to this comment
rahul.kumar@LIGO.ORG - 10:26, Thursday 13 August 2026 (91515)

The current pre-load value on the ZM4 is 60in-lb + 1/8th + 1/8th turn using a 0.5in size wrench.

sheila.dwyer@LIGO.ORG - 15:37, Friday 14 August 2026 (91551)

Here is a scatter plot for Ryan's final set of measurements, at the final ZM adjustment before the doors went on HAM7.  

It seems that in this position the values of M^2 are smaller than those in 91455 91385 and 90804, and the overlap between the vertical and horizontal q parameters is slighly better.  We can expect to get mode matching better than 99% between the squeezer and OMC for a pretty good amount of our psams range.  

Images attached to this comment
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