Displaying reports 2501-2520 of 85593.Go to page Start 122 123 124 125 126 127 128 129 130 End
Reports until 22:00, Thursday 03 July 2025
H1 General
ryan.crouch@LIGO.ORG - posted 22:00, Thursday 03 July 2025 (85544)
OPS Thursday EVE shift summary

TITLE: 07/04 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY: I did not see any PI ring ups during my shift. Ended the shift with a supervent!
LOG: No log

00:50 - 01:21 UTC I dropped Observing to run a calibration measurement

04:31 UTC Superevent S250704ab

05:00 UTC lockloss :(

 

Images attached to this report
H1 CAL (CAL)
ryan.crouch@LIGO.ORG - posted 18:25, Thursday 03 July 2025 - last comment - 12:37, Monday 07 July 2025(85543)
Thursday calibration measurement

We had been locked for just over 3 hours, the circulating power was ~378.5kW in each arm, a little under the usual 380kW.

Broadband:

Start: 2025-07-04 00:50:39

Stop: 2025-07-04 00:55:50

Data: /ligo/groups/cal/H1/measurements/PCALY2DARM_BB/PCALY2DARM_BB_20250704T005039Z.xml

Simulines:

Start: 2025-07-04 00:56:56.978617 UTC // GPS: 1435625834.978617

Stop: 2025-07-04 01:20:13.539672 UTC // GPS: 1435627231.539672

Data:

2025-07-04 01:20:13,381 | INFO | File written out to: /ligo/groups/cal/H1/measurements/DARMOLG_SS/DARMOLG_SS_20250704T005657Z.hdf5
2025-07-04 01:20:13,389 | INFO | File written out to: /ligo/groups/cal/H1/measurements/PCALY2DARM_SS/PCALY2DARM_SS_20250704T005657Z.hdf5
2025-07-04 01:20:13,394 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L1_SS/SUSETMX_L1_SS_20250704T005657Z.hdf5
2025-07-04 01:20:13,398 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L2_SS/SUSETMX_L2_SS_20250704T005657Z.hdf5
2025-07-04 01:20:13,403 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L3_SS/SUSETMX_L3_SS_20250704T005657Z.hdf5

 

Images attached to this report
Non-image files attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 12:37, Monday 07 July 2025 (85590)

PCAL broadband results attached.

Images attached to this comment
LHO General
corey.gray@LIGO.ORG - posted 16:29, Thursday 03 July 2025 (85519)
Thurs DAY Ops Summary

TITLE: 07/03 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY:

Today was Thursday Commissioning from 8am-1230pm, and had a locked H1 for 1hr45min of the commissioning time and had a few commissioning tasks squeezed in this time.  

H1 continues to be plagued by ringing up PI Modes that cause locklosses.  So, today different settings continued to be tried (latest & current ETMy Ring Heater setting is 1.5 W for the upper and lower).  But for some of these changes, we have had to try different violin mode settings (for ETMy Mode 20)---see this alog85527.

Also, the input pointing which was lost due to the HAM2 SEI Power supply swap on Maintenance Day, was reverted back by Elenna (alog85533).

Did not get to run the calibration suite today, so hope to do this after H1 gets to 3hrs during RyanC's shift tonight.
LOG:

H1 SQZ (OpsInfo)
sheila.dwyer@LIGO.ORG - posted 16:08, Thursday 03 July 2025 (85532)
new opo guardian state to adjust crystal temperature, SQZ ASC off and SQZ angle servo on

I started adding a state to the OPO guardian this morning while we were unlocked that scans the OPO temperature while the CLF is locked, and sets it to the temperature that maximizes CLF 6 Mz power in reflection off the OPO. 

The code is based on the SCAN_SQZ_ANG guardian state and it produces plots here: https://lhocds.ligo-wa.caltech.edu/exports/SQZ/GRD/OPOTEMP_SCAN/OPOTEMP_SCAN_250703142801.png

Screenshot shows that exmpale was a 1 minute scan with a 0.02 degree C range, this was a bit too fast for the TEC servo to keep up with so I've slowed it down to a 2 minute scan for the next time we try this out. 

Operators can use it to adjust the opo temp, by opening the SQZ_OPO_LR guardian and requesting SCAN_OPOTEMP.  I haven't tried this while squeezing was injected into the IFO, but it should work fine to do it then (not while in observing).   For future work we could add management that runs this each time the IFO relocks, but I haven't done that now.

Also note: This morning I set the sqz params to stop using SQZ ASC and start using the ADF servo for the squeezing angle.  These two can't run at the same time and I think that controlling the squeezing angle would be more beneficial right now.  However with various things we didn't get to test this and now we are observing with both ASC and the ADF servo off.  We momentarily dropped out of observing to engage the servo.  I also added to the SQZ_ANG_ADJUST guardian an if statement that updates the nominal state looking at sqzparams to check if the servo is supposed to be on or off in the guardian.   This will be compatible with the script that allows observing without squeezing for this weekend, but that script hard codes what the nominal state is, so in the long run we need to do something else.

Images attached to this report
H1 General
ryan.crouch@LIGO.ORG - posted 16:06, Thursday 03 July 2025 (85542)
OPS Thursday EVE shift start

TITLE: 07/03 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 146 Mpc
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 14mph Gusts, 8mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.06 μm/s
QUICK SUMMARY:

H1 PSL (PSL)
rahul.kumar@LIGO.ORG - posted 15:57, Thursday 03 July 2025 (85541)
ISS PD work in Optics lab - horizontal and vertical dither measurements for calibrating the beam motion on QPD

Jennie Wright, Rahul

Earlier, we have measured the QPD readout per mm to be around 44.1V (in X direction). This afternoon we dithered the input beam (spot size, radius = 200 microns, see LHO alog 85458) in horizontal and vertical direction at 100Hz using the signal generator (amplitude 2V peak to peak and offset 2.5V). This we did after centering the beam on the QPD (output was around 10,500 counts approx.). The output voltage applied on the dither was around 80V. Given below are the results,

Horizontal dithering:-

On the QPD the dither amplitude X (peak to peak) was estimated to be 2.2V, Mean 6.5V

Beam motion estimate X= 50microns

Dither amplitude Y (peak to peak) was estimated to be 1.2V, Mean -355mV

Vertical dithering:-

On the QPD the dither amplitude X (peak to peak) was estimated to be 1.0V, Mean 4.45V

Beam motion estimate X= 20microns

Dither amplitude Y (peak to peak) was estimated to be 1.62V, Mean -7.96V.

 

H1 CDS
jonathan.hanks@LIGO.ORG - posted 15:28, Thursday 03 July 2025 (85539)
Adjusting the runtime config of the daqd processes on h1daqnds*

During some ndscope testing Erik ran into a file descriptor limit on h1daqnds1 that required us to restart daqd.  The daqd stopped accepting requestions, giving a log message that the accept call had failed.  We bumped the file descriptor limit up and that solved the issue.  We have made runtime changes (no restart required) on h1daqnds[01].  We have put the new limits into the daqd puppet, but have not applied them yet.  We will reconcile the systems with puppet next week, after the long weekend.

 

H1 CAL
elenna.capote@LIGO.ORG - posted 13:01, Thursday 03 July 2025 (85529)
Attempted to Push new calibration from report 20250628T190643Z

with help online from Joe B

I revised this title to "attempted" because this push has failed and we reverted to the calibration from 20250610T224009Z.

Today I pushed a new calibration from calibration report 20250628T190643Z. We changed the SRCL offset on 6/26 which had a small effect on the sensing function, enough that Joe and I (with input from Sheila) decided to push a new calibration. With the change in the sensing function, I tagged a previous report on 6/26 with epoch-sensing and epoch-hfrl. When I regenerated the report, I set is_pro_spring to empty, since the previous iteration of the report showed that there was very little spring in the DARM sensing measurement, at least to 10 Hz. I confirmed with Joe that the resulting corner plots for the sensing that show very poor fits for F_spring and Q are ok- this is because the pipeline is unable to fit any appreciable spring in the sensing function.

I checked the GDS filter results by eye, and confirmed they all looked flat. I then went ahead to push this new calibration, following steps we took last time, specifically:

pydarm commit 20250628T190643Z --valid

pydarm export --push 20250628T190643Z

pydarm upload 20250628T190643Z

pydarm gds restart

Then, we waited ten minutes to begin the calibration measurement. This is where I made an error- I checked that the GDS calib strain channels all looked sensible, and I saw some lines updating on grafana, so I assumed we were good to go. Corey began a calibration suite, which starts with a broadband measurement. However, the broadband results were not very good. We lost lock right at the end of the measurement. This was my mistake- I never checked if kappaC and kappaTST had settled, which it looks like they hadn't. So, I think we need to relock and check the calibration again. If it still looks poor, we can revert to the previous calibration. This must be done before we go back to observing.

Follow up edit below here:

We relocked after the push above and remeasured and saw the calibration was even worse than before (orange trace). We think this may be a fit error to the L2 actuation function, but we're not sure. Joe helped me revert the calibration to the previous version, from 20250610T224009Z. Corey and I ran an early broadband and saw the error was better, red trace. Still not the best, but we were not thermalized yet. Hopefully we can try a new push next week with a better cal.

Images attached to this report
Non-image files attached to this report
H1 ISC
elenna.capote@LIGO.ORG - posted 11:45, Thursday 03 July 2025 - last comment - 12:49, Thursday 03 July 2025(85533)
Reverted IM2 and 3 position

Sheila, Matt, Corey, Elenna

I reverted the IM2 and IM3 osem positions in order to bring the beam on IM4 trans QPD back to its position before the mystery shift reported in alog 85486. I started by moving IM2 pitch, and noticed that bringing it back towards its previous position did help return the beam on IM4 trans to its previous spot. It was also very largely cross coupled with yaw, and shifted the yaw position slightly as well. I then moved IM3 pitch and further brought the pitch offset on IM4 trans back. I tried adjusting IM2 and 3 yaw slightly, but the adjustments to bring the yaw osems back did not correspond with returning the yaw IM4 trans position to the previous one. Overall, the shif tin yaw position is very small, so I chose to not make any more moves in yaw.

Corey reran input alignment, and I moved PR2 and IM4 by hand significantly in pitch (tens of microradians for both) to get the lock to catch.

While we locked, I reset the POP A offsets to well align PRM to the full lock alignment. This is SDFed in safe, but will be an observe diff too.

The attached ndscope shows the movement that I made. The y markers on the osem plots indicate where the suspensions were before the mystery shift. Note: IM1 also shows movement, but I chose not to adjust it.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 12:49, Thursday 03 July 2025 (85535)

Here's a screenshot of accepting the new POP Offsets.

Images attached to this comment
H1 ISC
sheila.dwyer@LIGO.ORG - posted 10:38, Thursday 03 July 2025 - last comment - 15:47, Thursday 03 July 2025(85527)
another ring heater step, changing PI 28 damping to ETMY

Kevin, Matt, Sheila, Elenna, Corey

After yesterday's ETMY RH change to avoid the 10kHz PI 85514, we lost lock 3 times overnight due to 80kHz PIs.

Apartently the RH change also changed a violin mode damping phase for ETMY 1 kHz mode (mode 20 1000.307 Hz), 85526, which did not cause the earlier locklosses but is growing to the point where it is dominating the DCPD RMS in this lock, but responded well the Elenna's sign flip.

Kevin took a look at the 10kHz higher order modes, second attachment.  The top panel shows how the higher order modes have been thermalizing before the ring heater change, the bottom panel shows three locks since the ring heater change which is a few minutes before 2 hours into the lock, so these can be compared to the green trace in the top panel. THe x arm higher order modes are sitting around 10.6kHz at this point in the self heating thermalization, the yarm modes were below the scale on this plot before the change and are now moving up to around 10480Hz.   If they gain another 20Hz as the self heating kept thermalizing similar to the x arm, this would have put them around 10500 Hz which doesn't have a lot of accoustic modes visible here. 

We don't want to revert the ring heater change from last night as that setting had the y arm sitting right below the forest of accoustic modes.  Matt estimates that we could move the y arm below this forest of accostic modes by going to 1.5 or 1.6W per segment, but that would mean that our two arm modes are more different from each other.  First we tried lowering the power a little more, to 0.9W per segment to see if that helps the 80 Hz modes.  Then Matt estiamted that we could put the Y arm 2nd order mode in a similar location to the x arm by using 0.6W per segment, so we've now set them to that.

Matt took a reference here before the PI rang up, it looks like the PI is 80297 Hz, I got a reference that includes the peak and the lockloss transient, which shows the frequency as 80298 Hz. The signal used for the PI damping is DCPDs downconverted at 80kHz, with a bandpass that goes from 294 to 298.5 Hz, so our peak is within the bandpass. The PLL set frequency is 299Hz, we lowered this 297.5Hz. It was being sent to ETMX for damping, which did appear to work once but not as the mode grew.  We think this is a y arm PI, since we have been changing the Y arm ring heaters, so I've changed the output matrix to send this to ETMY.

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 14:37, Thursday 03 July 2025 (85537)

I SDFed the ETMY ring heater change to 1.5 W in observe.

Images attached to this comment
corey.gray@LIGO.ORG - 15:47, Thursday 03 July 2025 (85540)SUS

For this new Ring Heater power (1.5), the ETMy Mode20 violin started to ring up again with default settings (+30deg + -1.0gain). 

Took the gain to +1.0, but this also rung up the violin.

It's been about an hour, but this seeting has been damping for this mode:

  • +60deg + +1.0gain

Have not updated lscparams since we are still figuring out a Ring Heater power which works for H1.  Once we find a good Ring Heater setting, we should update lscparams (if necessary).

LHO VE
david.barker@LIGO.ORG - posted 10:31, Thursday 03 July 2025 (85530)
Thu CP1 Fill

Thu Jul 03 10:11:40 2025 INFO: Fill completed in 11min 36secs

 

Images attached to this report
H1 SUS (OpsInfo)
elenna.capote@LIGO.ORG - posted 09:27, Thursday 03 July 2025 - last comment - 14:41, Thursday 03 July 2025(85526)
ETMY violin mode 20 ringing up, flipped gain sign

Sheila, Matt, Elenna

In the midst of trying to diagnose various PI issues, we noticed DCPD sum was slowly increasing, but not from PIs. We eventually figured out it was ETMY violin mode 20. The gain was set to -1. I flipped it to +1 and then mode started being damped down.

Comments related to this report
elenna.capote@LIGO.ORG - 14:41, Thursday 03 July 2025 (85538)

Sheila updated the ETMY ring heater again to 1.5 W, and it looks like ETMY mode 20 phase has flipped back, and a damping gain of -1 is working once again.

It appears that gains of both -1 and +1 are not damping the mode now. Corey is trying different phase filters.

H1 SEI
jim.warner@LIGO.ORG - posted 09:24, Thursday 03 July 2025 - last comment - 10:57, Tuesday 08 July 2025(85525)
HAM1 ISI tfs before and after adding Viton to ISC periscope

Thought I had posted this before, but couldn't find it, so here it is.  Attached plots compare L2L measurements of the HAM1 GS13s on May 21 during corner pumpdown before adding the periscope viton and June 6 the afternoon after we added viton. The Q and frequency of the 71.8hz mode is somewhat reduced, but the neighboring 69.9hz mode is sharper now, so I'm not sure we gained much. The June 6 measurement was collected in air, so I would still like to collect a set of in-vac measurements. This could probably be done on a Tuesday if there isn't too much activity around HAM1.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 10:57, Tuesday 08 July 2025 (85612)

I took 5-200hz matlab tfs this morning to compare to the  2 previous measurements above. It seems that the damping is quite effective now. I will try to look at the effect on the isolation filter design, maybe we can get some of the loop gain back. It would still be better to move these modes up above 100hz if possible.

Images attached to this comment
H1 PSL (ISC)
jennifer.wright@LIGO.ORG - posted 11:12, Wednesday 02 July 2025 - last comment - 15:17, Monday 21 July 2025(85458)
Calibrating ISS QPD

Jennie W, Rahul

Yesterday we made some measurements to calibrate the spot size on the QPD as we scan the beam position across it.

We used a connector Fil made us to plug in the OT301 QPD amplifier into a DC power supply after checking it contained voltage regulators that could cope with a voltage between 12 and 19 V ( as the unit says it expects DC supply but the previous one we were using was AC with a 100mA current rating and was getting too hot so we assume that was the incorrect one). We hooked it up at 16V (this draws about 150mA of current). The QPD readout looks normal and does not have any of the strange sawtooth we saw with the original power cable.

 

We moved the M2MS beam measurement system out of the way of the translation stage.

To calibrate the QPD we need to change the lateral position of the M1 mirror and lens to change the yaw positioning on the QPD and measure the X and Y voltages from the QPD.

We need to check we are centred first. The QPD bullseye readout shows the beam is off a tiny bit in yaw but this was as good as we could get at centering the beam when we moved the QPD. All 8 PDs are reading about 4.6 V so this means the beam is well centred in the array plane.

We measure 11000 counts on the bullseye qpd readout at this M1 position.

 

Translation Stage inch

QPD X (mV

)

QPD Y (V)
4.13 239e-3 -1.77
4.14 252e-3 -1.84
4.15 2.34 -1.60
4.16 4.46 -1.17
4.17 4.26 -1.11
4.18 5.62 -835e-3
4.19 7.80 -600e-3
4.20 7.81 -321e-3
4.21 8.45 -222e-3
4.22 8.82 +70.6e-3

4.23

9.19

771e-3

4.24 9.28 1.12
4.25 9.37 1.88
4.26 9.36 2.36
4.27 9.37 2.38
4.28 9.44 2.71
4.29 9.47 3.10
4.30 9.50 3.41
4.31 9.49 3.35
4.32 9.51 3.72
4.33 9.55 4.27
4.34 9.58 4.55
4.35 9.62 4.86
4.36 9.66 5.44
4.37 9.65 5.31
4.38 9.63 5.60
4.39 9.69 5.75
4.40 9.69 6.00
4.41 9.70 6.15
4.42 9.70 6.16
4.43 9.71 6.33
4.44 9.71 6.50
4.45 9.72 6.72
4.46 9.74 7.09
4.47 9.73 6.87
4.48 9.74 7.40
4.49 9.75 7.46
4.50 9.74 7.46
4.51 9.76 7.75
4.52 9.74 7.67
4.53 9.73 7.82
4.54 9.74 7.96
4.55 9.73 8.08
4.56 9.72 8.33
4.57 9.71 8.43
4.58 9.70 8.50
     
4.13 448e-3 -1.98
4.12 -1.02 -2.34
4,11 -1.17 -2.14
4.10 -2.92 -2.43
4.09 -4.63 -3.30
4.08 -5.91 -3.18
4.07 -6.97 -3.40
4.06 -8.17 -4.24
4.05 -8.13 -4.28
4.04 -8.52 -4.47
4.03 -8.76 -4.77
4.02 -8.89 -5.27
4.01 -9.01 -5.45
4.0 -9.08 -5.44
3.99 -9.10 -5.85
3.98 -9.11 -5.91
3.97 -9.11 -5.93
3.96 -9.12 -6.16
3.95 -9.12 -6.18
3.94 -9.13 -6.34
3.93 -9.13 -6.49
3.92 -9.12 -6.49
3.91 -9.13 -6.61
3.90 -9.11 -6.55
3.89 -9.11 -6.70
3.88 -9.10 -6.46
4.13    
     

 

I plotted the data from lowest reading on the translation stage to highest and fitted the linear region using Calibrate_QPD.m which is attached.

Data is shown in attached pdf.

The slop of the linear region in V/inch is 112 V/inch. Which means to if the beam moved 8.93 e-3 inches on the QPD in yaw, the yaw readout would change by 1 Volt.

Images attached to this report
Non-image files attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 15:35, Wednesday 02 July 2025 (85512)

I altered the code to plot in mm and the constant is 4.4 V/mm.

Images attached to this comment
jennifer.wright@LIGO.ORG - 11:05, Thursday 03 July 2025 (85531)

D'oh I read the scale on the translation stage wrong so the x readings are actually lower by a factor of 10.

This makes the slope 44.1 V/mm which is more in line with the 65.11 V/mm Mayank and Shiva found for the QPD calibration here.

Ours could be different because we have a slightly different beam size and we moved the QPD in its housing to centre it which could have changed X to Y coupling in the QPD readout.

This implies our beam diameter on the QPD is around 0.4mm which makes a lot more sense considering the diode is 3mm!

 

As a cross-check we used the QPD 'bullseye' readout unit and Rahul changed the translation stage in yaw and we measured the beam dropping from 10400 counts in the middle of the QPP to 100s of counts at the edges.

Translation Stage [inch] QPD Sum Counts
0.413 10400
0.365 500
0.413 10400
0.49 400

diode size ~ ((0.49-0.365)*0.0254*1000) = 3.175 mm.

Images attached to this comment
Non-image files attached to this comment
jennifer.wright@LIGO.ORG - 15:36, Monday 14 July 2025 (85749)

I redid the graphs for the horizontal motion of the input beam to X motion on the QPD with better labels (first attached graph) and did a fit for the Y data on the QPD collected at each horizontal position of the input beam (second attached graph). The third graph attached is comparing both fits on one graph.

Images attached to this comment
jennifer.wright@LIGO.ORG - 11:49, Thursday 17 July 2025 (85821)

If we take into account the input beam horizontal axis is not aligned with the QPD, we can work out the resultant calibration relative to the mirror displacement as:

V change along mirror displacement axis = sqrt((change V in X)^2 + (change V in Y)^2)

Calibration = V change along mirror displacemnt axis/change in mirror position

= 4.644 V/mm.

 

angle of QPD horizontal axis with mirror displacement axis = tan^-1(Voltage change V in Y/ Voltage change in X) = 38.8 degrees.

jennifer.wright@LIGO.ORG - 15:17, Monday 21 July 2025 (85897)

I got the above caluclation of the QPD calibration in the horizontal direction wrong as I use the total change in voltage we measured across the whole range of horizontal scan and not just the linear region where the beam is close to centred on the QPD.

The horizontal beam scan calibration is actually:

sqrt(11.8^2 + 44.1^2) = 10.6 V/mm

with an angle of tan^-1(11.8/44.1) = 14.9 degrees to the X direction on the QPD.

H1 AOS
robert.schofield@LIGO.ORG - posted 13:15, Friday 06 June 2025 - last comment - 09:00, Thursday 03 July 2025(84868)
Periscope damped on ISCT1

Jim, TJ, Robert

We damped the periscope on ISCT1 by removing the dog clamps one by one and inserting a strip of 1/16" viton between the dog clamp and the base of the periscope before retightening, making sure that the strips crossed the corner of the base. This is not the most effective way of damping the periscope but it was the fastest, safest and most simple damping we could do. Jim measured the Q to be around 1000, so we didn't have to do much to get an improvement. In Jim's first transfer functions after the damping, the peak looked a little wider.

Images attached to this report
Comments related to this report
robert.schofield@LIGO.ORG - 09:00, Thursday 03 July 2025 (85524)

This was HAM1 not ISCT1

H1 CAL (CAL)
richard.savage@LIGO.ORG - posted 14:17, Monday 15 April 2024 - last comment - 12:00, Thursday 03 July 2025(77181)
Pcal X/Y comparison excitation amplitudes and SNRs

FranciscoL, RickS

On April 4, 2024 we used DTT to measure the amplitudes of the Pcal lines used in the Pcal X/Y calibration comparison in both the Pcal end station Rx sensor outputs and the DARM_ERR signal.  The attached plots shows the peaks in the spectra measured with 0.001 Hz requested BW, 50% overlap, 10 averages during a long lock stretch.  The second image is a page from Francisco's lab book.

The SNRs for the lines from the Pcal Rx sensors is about 5e-5 and

the SNRs of the lines in the DARM_ERR signal are about 1350.

 

Non-image files attached to this report
Comments related to this report
dripta.bhattacharjee@LIGO.ORG - 12:00, Thursday 03 July 2025 (85534)

Typo: The SNRs for the lines from the Pcal Rx sensors is about 5e-5 --> 5e5 

Displaying reports 2501-2520 of 85593.Go to page Start 122 123 124 125 126 127 128 129 130 End