Displaying reports 1-20 of 85743.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 17:58, Wednesday 26 November 2025
LHO General
ryan.short@LIGO.ORG - posted 17:58, Wednesday 26 November 2025 (88263)
Ops Eve Shift Summary

TITLE: 11/27 Eve Shift 2030-0200 UTC (1230-1800 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: The last of the PEM measurements were done this evening when H1 was locked, but a couple of locklosses (both of which seemed to be caused by activity in sensitive areas in the LVEA) limited the amount of time at low noise. Following the most recent lockloss, I'm leaving H1 in 'IDLE' for the long weekend before the upgrade phase begins on Monday.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
20:49 PEM Rene CER N Moving magnetometers 20:56
21:05 PEM Robert LVEA N Running measurements 22:51
21:50 ISC Kar Meng Opt Lab Local OPO work 00:17
01:41 PEM Robert LVEA N Cleaning up 01:55
LHO General
ryan.short@LIGO.ORG - posted 12:45, Wednesday 26 November 2025 (88256)
Ops Eve Shift Start

TITLE: 11/26 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 8mph Gusts, 5mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.16 μm/s 
QUICK SUMMARY: H1 is relocking and currently up to LOWNOISE_ESD_ETMX. More PEM measurements ongoing today and into this evening.

H1 General
ryan.crouch@LIGO.ORG - posted 12:32, Wednesday 26 November 2025 (88249)
OPS Wednesday DAY shift summary

TITLE: 11/26 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: We've had two locklosses today, both while people where out on the floor. Relocking has been fairly automated, we had a TCS CO2Y laser issue that we resolved. We are relocking at MOVE_SPOTS as of 20:30 UTC. LVEA zone4G got a bit warm but its leveled out.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
16:47 PEM Robert LVEA N Set up measurements, check on zone4 17:05
17:31 PEM Robert LVEA N Setup shaker in *danger zone*, in and out 20:18
17:34 ISC Kar Meng Optics lab LOCAL OPO work 19:27
18:56 TCS Sheila LVEA N Reset CO2Y 19:11
19:38 FAC Tyler Mids N Find boom lift and inflate the tires 20:06
19:54 TCS Daniel, Sheila LVEA N Wiggle TCS CO2Y cable 20:03
H1 SQZ (SQZ)
karmeng.kwan@LIGO.ORG - posted 12:16, Wednesday 26 November 2025 - last comment - 13:30, Wednesday 26 November 2025(88254)
VOPO 532nm/1064nm into M1 alignment

Both the pump (532nm) and fundamental (1064nm) have now been alignment to the VOPO cavity based on the mode matching setup described in this log

From the mirror specification (C2500221), the theoretical escape efficiency is calculated to be 98.5% (derived from the decay rate of the mirror, k_in,r / k_in,tot).

The escape efficiency from the VOPO reflection is 97.9% (calculated from the photodiode reflection, trans/refl = (2nesc - 1)^2).

In short, input alignment done, rear seed injection is the next to go, escape efficiency checked, and the photons escaping the cavity with the enthusiasm of a PhD student during a conference lunch break.

Images attached to this report
Comments related to this report
karmeng.kwan@LIGO.ORG - 13:30, Wednesday 26 November 2025 (88258)

For the escape efficiency measurement, the transmission field refer to the light entering and exiting the cavity via M1 (shown as the "dip" on the reflection photodiode). Whereas the reflected field refer to the promptly reflected light from the photodiode (shown at the flat line on the reflection photodiode).

The measured escape efficiency is consisted with the measurement done at MIT (E2500270), where escape efficiency of 97.9% to 98.2% was reported for various crystal position.

H1 General (Lockloss)
ryan.crouch@LIGO.ORG - posted 12:01, Wednesday 26 November 2025 (88255)
19:58 UTC lockloss

19:58 UTC lockloss, there was a big fuzzy oscillation in PR_GAIN right before LL

LHO VE
david.barker@LIGO.ORG - posted 10:22, Wednesday 26 November 2025 (88252)
Wed CP1 Fill

Wed Nov 26 10:05:20 2025 INFO: Fill completed in 5min 16secs

 

Images attached to this report
H1 General
ryan.crouch@LIGO.ORG - posted 09:51, Wednesday 26 November 2025 - last comment - 11:37, Wednesday 26 November 2025(88251)
17:50 UTC lockloss

17:50 UTC lockloss, there was an ISI BS saturation a few seconds after the lockloss.

Comments related to this report
ryan.crouch@LIGO.ORG - 11:37, Wednesday 26 November 2025 (88253)

19:18 NLN but we've encountered a TCS CO2Y issue, the laser tripped off and doesn't want to come back.

H1 SQZ
sheila.dwyer@LIGO.ORG - posted 09:03, Wednesday 26 November 2025 - last comment - 18:19, Wednesday 26 November 2025(88250)
ADF sweeps and CO2 steps

Kevin, Sheila

Over the last few days we've run ADF sweeps a few times.  Here's a record of what happened and file names.  

The files are in /ligo/gitcommon/squeezing/sqzutils/data

 Nov 22 08:31 HF_10kHz_11_2025.h5 IFO had been powered up for 11:00, sweep started at about 14:50 UTC Nov 22.  NLG 24.3, measurement is in 88224.   Something seemed to go wrong towards the end of the sweep, we aren't sure what. 
 Nov 22 12:38 HF_10kHz_11_2025_2.h5  IFo had been powered up for 15:10, same lock as the previous measurement, same NLG measurement, sweep started at about 19 UTC.  

Nov 25 00:36 HF_10kHz_11_2025_b4_CO2_step.h5  IFO had been powered up for 4:20, in this sweep I didn't turn off the SQZ angle servo based on the ADF, so the demod phase was moved around during the sweep, making this data not useful.

Nov 26 01:56 HF_10kHz_11_2025_b4_CO2_step2.h5 last night's first scan, started only 38 minutes after power up at about 8:18 UTC Nov 26th.  The amplified seed was 7.8e-3, unamplified seed didn't happen correctly with the script but the waveplate hasn't moved since previous measurements of that level at 2.9e-4 (88223), giving an NLG of 26.9.  (Edit, I redid the unamplified seed measurement, it looks like 3.2e-4 now, making the NLG 24.4 for these last two measurements, which has been consistent (24.3 or 24.4) for the last week. 

Nov 26 08:15 HF_10kHz_11_2025_after_CO2_1hour.h5 this morning's sweep, IFO had been powered up for 7 hours, CO2s had been stepped from 1.7W each to 0.9W each for 1.5 hours when the sweep started at about 14:37 UTC Nov 26th. NLG should be the same as for above, 26.9.   24.4

Comments related to this report
kevin.kuns@LIGO.ORG - 18:19, Wednesday 26 November 2025 (88264)

The goal of these measurements is to use the ADF to measure the rotation of the squeezed state around higher order mode arm cavity resonances as described in section IV.B of LIGO-P2500132. Ultimately we would like to be able to use such measurements to diagnose the thermal state as a guide in how to tune TCS in order to improve mode matching.

While we are still digesting the results, the first plot shows the preliminary inferred squeezed state rotation for the three good data sets that we got. pre-step 1 and pre-step 2 are the two taken on Nov 22. (Everything turned out to be fine with the first sweep.) post-step is the last one taken this morning after the CO2s had been stepped and the IFO had been up for 7 hours. There is a small arbitrary constant offset in the SQZ angle of order a degree, so all angles have been shifted to be zero at 10.450 kHz. The second plot shows the OMC DCPD spectra 5 min before the start of each of these three sweeps.

Two rotation peaks are visible rather than the one shown in Fig 7 of P2500132. This is expected since the arms are astigmatic in reality, and our more detailed models show the same behavior. Each eigenmode is resonant at a slightly different frequency and is responsible for a rotation as in Fig 7 which are superimposed as observed in this data.

The post-step rotation is slightly smaller in magnitude and is shifted to slightly lower frequencies. Since the CO2 is mainly a higher order actuator, this is consistent with our expectations that this rotation is predominantly sensitive to quadratic mismatch with higher order aberrations altering the detailed behavior. However, seeing as how the pre-step was not taken just prior to the CO2 step in the same lock, I think it's just as likely that this is due to it being in a slightly different thermal state before the CO2 step. The peaks in the OMC DCPD spectra also appear slightly lower in frequency for the post-step.

I think the main takeaway from these measurements so far is showing that we can measure this rotation and resolve changes on the scale that our modeling suggests would be useful.

This analysis was done in the aligoNB environment by running
pytest /ligo/gitcommon/squeezing/sqzutils/analysis/T_10kHz_ADF.py --tb short -s -k T_Nov_CO2_step

Non-image files attached to this comment
H1 General
ryan.crouch@LIGO.ORG - posted 07:28, Wednesday 26 November 2025 - last comment - 07:36, Wednesday 26 November 2025(88247)
OPS Wednesday DAY shift start

TITLE: 11/26 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 146Mpc
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 7mph Gusts, 4mph 3min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.17 μm/s 
QUICK SUMMARY:

Comments related to this report
ryan.crouch@LIGO.ORG - 07:36, Wednesday 26 November 2025 (88248)

15:33 UTC GRB-Short E619679

H1 General
ryan.crouch@LIGO.ORG - posted 19:48, Tuesday 25 November 2025 - last comment - 20:32, Tuesday 25 November 2025(88239)
OPS Tuesday EVE shift summary

TITLE: 11/26 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: We had 2 locklosses, the first was easy to recover from, the second is still in progress. We're at MAX_POWER right now.
LOG:      

Start Time System Name Location Lazer_Haz Task Time End
00:16 PEM Rene, Alicia CER N Setup measurement, huddle test 00:33
00:20 ISC Kar Meng Optics lab LOCAL OPO work 01:13
00:21 ISC Marc Optics lab LOCAL Help with osciliscope issue 00:59
00:52 PEM Robert, Sam EndX N Setup measurement 01:20
Comments related to this report
ryan.crouch@LIGO.ORG - 20:32, Tuesday 25 November 2025 (88246)

04:10 UTC NLN

04:30 UTC We went into Obseving after I cleared a leftover EX PEM EXC

H1 PEM
ryan.short@LIGO.ORG - posted 08:44, Tuesday 25 November 2025 - last comment - 13:55, Wednesday 26 November 2025(88235)
Longer Magnetic Injection Suite Run

Last night I ran a longer version of the full magnetic injection suite starting at about 03:10 UTC, and it finished at 07:33 UTC. This used the same parameters as last week's run, except I doubled the injection time to 5 minutes each.

Exact times and injection parameters are in the usual log directory for the magnetic injections: /ligo/www/www/exports/pem/WeeklyMagneticInjection/logs/1448075483.txt

Comments related to this report
ryan.short@LIGO.ORG - 13:55, Wednesday 26 November 2025 (88260)

The last batch of injections (all 7 of the ones at EY E-bay) mistakenly overlapped with a scheduled SQZ script, so last night I re-ran these between 05:29 and 06:06 UTC.

Analysis results and plots can be found here: https://ldas-jobs.ligo.caltech.edu/~ryan.short/pem/Weekly_Mag_Inj/H1_Injection_Results/O4/20251125_1448075483/

H1 DetChar (DetChar)
joan-rene.merou@LIGO.ORG - posted 10:26, Thursday 13 November 2025 - last comment - 13:28, Wednesday 26 November 2025(88089)
With voltage set to 0, grounding of the ITMX ESD driver
[Joan-Rene Merou, Alicia Calafat, Sheila Dwyer, Jenne Driggers]

We have entered the LVEA and went to the Beer garden. There, we first turned off the Low Voltage ITM ESD Driver D1600092, first the 15V switch and then the medium voltage switch. In order to turn it on again, it should be reconnected in the opposite order. With the voltage request set to 0 and chassis powered off, we have unplugged the SHV cables going to the chamber and plugged into Robert's ground boxes, which we used to ground to the rack which is grounded to the chamber. This has been done at both drivers (See attached photos).

Afterwards, we have changed the code at /opt/rtcds/userapps/release/isc/h1/guardian/ISC_LOCK.py in order that the LOWNOISE_COIL_DRIVERS will go to LOWNOISE_ESD_ETMY instead of TRANSITION_FROM_ETMX. This has been done by changing lines 6670 and 6674, moving the ", 15" step from line 6670 to 6674. Finally, we communicated the change to the operator and loaded the guardian.
Images attached to this report
Comments related to this report
joan-rene.merou@LIGO.ORG - 13:28, Wednesday 26 November 2025 (88257)
It appears that the grounding did not decrease the amplitude of the combs. As seen in the attached figure, the relative amplitude of the first harmonics of the combs remains mostly the same before and after the change on November 13th.
Non-image files attached to this comment
H1 ISC
jennifer.wright@LIGO.ORG - posted 10:58, Monday 27 October 2025 - last comment - 17:13, Wednesday 26 November 2025(87766)
Change of reflected power from OMC during DARM offset step

I made plots of anti-symmetric power P_AS vs. power at reflected port of OMC P_OMC_REFL during the DARM offset step measurement on September 4th, (see LHO alog #86785 and 87629).

I had to use the Beckhoff reported power for this (H1:OMC-REFL_A_DC_POWER) as the front-end channel is calibrated wrongly (see LHO alog #87648).

I also plotted the P_OMC_REFL vs.  P_DCPD, ie. reflected vs. transmitted power for the OMC.

The plots for our two measurements taken at different times during IFO thermalisation are below, both were taken when OM2 was hot.

Non-image files attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 15:25, Wednesday 26 November 2025 (88259)

I reran these plots as the axis limits of the P_REFL vs. P_DCPD plot were wrong and were cutting off end point, plus removed line that explained what the y-intercept was for each plot as different dependent on whether we plot P_REFL vs P_AS or P_REFL vs. P_DCPD.

I also switched the P_REFL channel being used in my code to H1:OMC-REFL_A_DC_POWER from H1:OMC-REFL_A_DC_POWERMON as this latter channel has a factor of 100 relative to the former that I don't really undestand. The DC_POWER channel seems to give a realistic reading for the OMC reflected power that is much less than the power into HAM6.

First link contains two plots when we were half-way thermalised:

First plot is power at the OMC reflected PD vs. power at the antisymmetric port (calibrated into the power into HAM6) for the case where we were 1Hr 25 mins into lock.

Second plot is power at the OMC reflected PD vs. power transmitted to the DCPDs for the case where we were 1Hr 25 mins into lock.

 

The second link contains two plots also when we were thermalised:

First plot is power at the OMC reflected PD vs. power at the antisymmetric port (calibrated into the power into HAM6) for the case where we were 3 hrs 59 mins into lock.

Second plot is power at the OMC reflected PD vs. power transmitted to the DCPDs for the case where we were 2 hrs 59 mins into lock.

Non-image files attached to this comment
jennifer.wright@LIGO.ORG - 17:13, Wednesday 26 November 2025 (88262)

We can write down an equation for P_REFL from the OMC in terms of P_DCPD, using our linear fit.

P_REFL = ( c*P_DCPD + d ) mW

We know the nominal setting for P_DCPD is 40mA, and we can take the responsivity of the DCPDs at 100 % efficiency to be 

responsivity = e * lambda / (c * h)

From the squeezer budget (E2400269) we can get a number for the Q.E. of the PD that also includes OMC losses for the transmitted beam, transmissivity = 0.937

Therefore the power at the DCPDs at nominal DARM offset is 40mA/(responsivity*transmissivity) = 49.7 mW.

The reflectivity of the OMC breadboard is 2.75e-4 as calculated from parameters given in T1500060-v3.

The formula for the power measured at the reflected port of the OMC can also be expressed as:

P_REFL = R_cav [ P_00_arm + P_00_cd] + P_HOM_arm + P_sb + P_HOM_cd

where P_00_arm is the power in the fundamental carrier mode which changes with DARM offset, P_00_cd is the contrast defect light that is in the fundamental carrier mode, P_HOM_arm is light at higher order mode frequencies which also change with DARM offset, P_sb is power in the sidebands, P_HOM_cd is contrast defect light at higher order mode frequencies.

Whereas the formula for the power transmitted by the OMC can be described as:

P_DCPD = T_cav [ P_00_arm + P_00_cd]

As we assume that all HOM and sidebands are reflected by the OMC.

The mode-matching, MM, of the OMC to the differential arm mode is defined as:

P_00_arm / ( P_HOM_arm + P_00_arm )

This can be calculated using:

P_00_arm = (P_DCPD - d)/T_cav

P_HOM_arm = P_REFL - d - (R_cav*P_00_arm)

If we do this calculation for the half-way thermalised measurement we get 

MM = 0.9975

For the fully thermalised case we get:

MM = 0.9978

The code to calculate this is in: Calculate_refl_power.py located at /ligo/home/jennifer.wright/git/2025/DARM_OFFSET/

 

H1 ISC
jennifer.wright@LIGO.ORG - posted 10:37, Friday 17 October 2025 - last comment - 15:38, Wednesday 26 November 2025(86744)
Optical Gain and output loss checks with hot OM2 on 4th September

Jennie W, Sheila,

 

I took a long time to post this as have been working on other things...

We carried out a test (see LHO alog #86785) to look at the effect of DARM offset stepping on the power at OMC-DCPD_SUMS and OMC-REFL (transmitted through and reflected from the OMC). We did this with the heater on OM2 off as is nominal.

We then meant to redo these measurements once we heated up OM2 to change the mode-matching of the IFO to the OMC.

Unbfortunately we lost lock at about 15:06 UTC while Corey was taking out first measurement before heating up the OM2.

The meausrement is shown in this image, I have mislabelled it as 'third measurement' but it was the first. The optical gain is shown just before this measurment to be 0.994.

Then we waited as long as we could under out initial parameters of being finished cooling the OM2 again by 1:45pm.

We took another measurement at 1 hr 25 mins into lock after two false starts where I forgot to turn off the ASC. The optical gain was measured right before we started the measurements to be 0.978 but was still thermalising.

And then we took a third 2 hrs 59 minutes into lock, the IFO should be thermalised but the temperature of OM2 was still trending upwards a bit. Optical gain was 0.986.

We can use the slope of the power at the antisymmetric port (P_AS) vs. the power at the DCPDs (P_DCPD) as the DARM offset changes to estimate the throughput of carrier through the OMC which allows us one estimate of the loss.

The plots of this throughput are here for the cold state (minus the points taken after we lost lock), here for the partially thermalised state, and here for the thermalised state.

I am also in the middle of using the plot of P_AS varying with power at the OMC reflected port (P_REFL) to get a better estimate of the mode-mis match between the interferometer and the OMC.

 

Images attached to this report
Non-image files attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 12:33, Tuesday 21 October 2025 (87610)

I plotted the loss between the antisymmetric port (calibrated into the power entering HAM6) to the power on the DCPDs. This is the inverse of the slopes in the graphs above.

All three are poltted on one graph, using plot_AS_vs_DCPD_changes.py in my own cope of the labutils repository at /ligo/home/jennifer.wright/git/local_git_copies/labutils/darm_offset_step/ .

Sheila and Camilla both agreed the loss for the two bottom lines (purple and red) are too high. These imply that a hot OM2 gives us over 20 % output losses.

If we look at the increase in loss from cold OM2 to hot OM2 this is a factor of 2.1 (210 % increase).

Compared to the decrease in optical gain squared (which we expect to reflect the change in output losses, which was:

(0.986^2 - 0.994 ^2) / 0.994^2 = -0.016 (1.6 % decrease).

We might have to check the alignment of out optics was not changing while we changed the darm offset.

Non-image files attached to this comment
jennifer.wright@LIGO.ORG - 13:04, Tuesday 21 October 2025 (87614)

Looking at OM1, OM2 and SRM alignment it did change during the darm offset steps with the biggest change (in the third offsset step measurement) being in OM2 pitch and yaw, this is only a change around 6 microradians (Elenna and Jeff state this calibration in correct to within an order of magnitude). Not sure if this enough to invalidate the loss values we measure. OM3 and OMC sus did not change much but this is because IU purposely unlocked the OMC ASC while changing the darm offset.

Images attached to this comment
jennifer.wright@LIGO.ORG - 17:18, Tuesday 21 October 2025 (87629)

Jennie W, Matt T,

 

I plotted the antisymmetric power during the darm offset step vs. the power reflected by the OMC and am now very confused as the AS power looks to be smaller than the power reflected form the OMC. See the ndscope where I have zoomed in on the same time segment for both channels. The OMC-REFL channel is mean to be calibrated into mW and the ASC-AS_C channel is meant to be calibrated into W entering HAM 6 (even though the actual pick-off is the transmission through OM1).

The two plots attached show how the ratio between AS and OMC-REFL power changes during one of the DARM offset measurements we did right after I took this ndscope data.

Plot 1 hr 25 mins into lock.

Plot 2 hrs 59 mins into lock.

For each point the code returns the median of the time series at each step, this mioght be less valie for OMC-REFL as it is a lot noisier than ASC-AS_C.

I am still confused about the hogher power at OMC-REFL and wondering if:

a) I am confused about the calibration of one of these channels.

b) the calibration of one of these channels is wrong.

Images attached to this comment
Non-image files attached to this comment
jennifer.wright@LIGO.ORG - 15:38, Wednesday 26 November 2025 (88261)

I plotted the three measurements of P_AS vs. P_DCPD during thermalisation on the same plot to make them easier to compare.

The code for this is in /ligo/home/jennifer.wright/git/local_git_copies/labutils/darm_offset_step/plot_OMC_REFL_changes/P_as_vs_P_DCPD__comp_Sep_04.pdf

Non-image files attached to this comment
Displaying reports 1-20 of 85743.Go to page 1 2 3 4 5 6 7 8 9 10 End