Displaying reports 61-80 of 81333.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 08:39, Tuesday 01 April 2025
H1 PSL
ryan.short@LIGO.ORG - posted 08:39, Tuesday 01 April 2025 (83677)
PSL Cooling Water pH Test

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.

H1 CDS
david.barker@LIGO.ORG - posted 07:54, Tuesday 01 April 2025 - last comment - 15:46, Tuesday 01 April 2025(83675)
bypassed fire pump cell phone alarms during pump testing this morning

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
 

Comments related to this report
david.barker@LIGO.ORG - 15:46, Tuesday 01 April 2025 (83687)

Alarms has been reconfigured to expect GV2 and GV5 to be in the hard-closed position and alarm if not.

david.barker@LIGO.ORG - 08:40, Tuesday 01 April 2025 (83678)

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
 

david.barker@LIGO.ORG - 08:45, Tuesday 01 April 2025 (83679)

Added GV5 position alarm to bypass

    H0:VAC-LY_GV5_ZSM159A_VALVE_ANIM
 

david.barker@LIGO.ORG - 09:12, Tuesday 01 April 2025 (83680)

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

LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 07:43, Tuesday 01 April 2025 (83674)
OPS Day Shift Start

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!

H1 CDS
erik.vonreis@LIGO.ORG - posted 07:02, Tuesday 01 April 2025 (83673)
Workstations updated

Workstations were updated.  This was an OS packages update.  Conda packages were not updated.

LHO General
corey.gray@LIGO.ORG - posted 22:02, Monday 31 March 2025 (83670)
Mon EVE Ops Summary

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:

H1 SQZ (SQZ)
corey.gray@LIGO.ORG - posted 21:56, Monday 31 March 2025 - last comment - 08:29, Tuesday 01 April 2025(83672)
SQZ Drops H1 From OBSERVING & SQZ SHG Fiber Rejected Power High

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.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 08:29, Tuesday 01 April 2025 (83676)

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.

Images attached to this comment
H1 TCS
matthewrichard.todd@LIGO.ORG - posted 17:12, Monday 31 March 2025 - last comment - 11:33, Tuesday 01 April 2025(83669)
L5 Laser Beam Scan

[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:

  1.  20250327 - razorblade 16cm from laser aperature
  2.  20250328 - razorblade 16cm from laser aperature (moved laterally to have more range)
  3.  20250328v2 - razorblade 16cm from laser aperature

Results:

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.

Images attached to this report
Comments related to this report
matthewrichard.todd@LIGO.ORG - 11:33, Tuesday 01 April 2025 (83684)

Code for analyzing this data

Non-image files attached to this comment
H1 SEI (SEI)
ibrahim.abouelfettouh@LIGO.ORG - posted 16:41, Monday 31 March 2025 (83671)
H1 ISI CPS Sensor Noise Spectra Check - Weekly FAMIS

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.

Non-image files attached to this report
LHO General
corey.gray@LIGO.ORG - posted 16:31, Monday 31 March 2025 (83667)
Mon Eve Ops Transition

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.

LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 16:30, Monday 31 March 2025 (83668)
OPS Day Shift Summary

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
H1 SQZ
camilla.compton@LIGO.ORG - posted 14:33, Monday 31 March 2025 (83660)
SQZ with SRCL offset at -306, FC detuing at -28

Sheila, Camilla, Jennie

This morning we changed SRCL offset from -191 to -306 and FC de-tuning from -34 to -28, as discussed in  83570. Took some SQZ data here as we were interested if we could get FIS SQZ lower than No SQZ ~100Hz and below, Sheila's models (e.g. 83572) suggest we should but it looks like there's a low frequeceny noise source (in FIS not FDS) in our data sets preventing us from getting down to the modeled level of SQZ.

Sheila turned OPO trans setpoint up from 80uW to 95uW to increase NLG from 11 to 19 (similar to what we had earlier in O4). Measured NLG with 76542. OPO gain left at -8. Turned off  SQZ ASC.

opo_grTrans_ setpoint_uW Amplified Max Amplified Min UnAmp Dark NLG (usual) NLG (maxmin) OPO Gain
95  0.0176 0.000279 0.00002 0.00094 19.1 20.0 -8
110 0.03315 0.000269 0.000879 -0.00002 35   -8
 
Starting FC2 misaligned offsets in M1 TEST were 100 and 200, Sheila increased to 200 and 400. So that we know FC2 is really misaligned. Saw no difference at SQZ or ASQZ. So this low fruecny noise in FIS is not due to FC backscatter.
Data attached and saved at camilla.compton/Documents/sqz/templates/dtt/20250331_SRCL_neg306.xml
 
Type Time (UTC) Angle Notes DTT Ref
No SQZ 03/29 N/A   ref 0
FIS SQZ   171 Angle tuned for FDS (maybe thermalized since) ref1
FIS SQZ 17:05:00 154 Ang tuned for FIS ref2
FIS Mid(ish) 17:15:00 101 Little better than no SQZ at 60Hz ref3
FIS Mid(ish)   92   ref4
ASQZ FIS   68   ref5
ASQZ FIS -10deg 17:24:00 58   ref6
ASQZ FIS +10deg   78   ref7
FIS Mid(ish) 17:31:30 115   ref8
FIS Mid(ish) other side 17:43:00 27   ref9
FIS Mid(ish) 17:45:30 82 Check data doesn't include a glitch ref10
 
Then changed the SRCL de-tuning back to -191 (still in FIS so FC de-tuning doesn't matter). Comparison is attached.
This SRCL offset change didn't effect the level of low frequency noise.
 
Type Time (UTC) Angle Notes DTT Ref
FIS ASQZ +10deg 17:53:00 82 Plot seems similar with same ang, different SRCL offset ref 11
FIS ASQZ 17:56:00 72   ref12
FIS ASQZ -10deg   62   ref13
FIS Mid (ish)   104 Can see that rotation is a little different with SRCL de-tuning different but low freq noise level is the same. ref14
 
Kept SRCL de-tuning at -191 but increased NLG to 35. 
This was interesting for mid-SQZ values as the level of the low freq noise increased with the higher NLG but was the same at different SQZ angles (112 and 100deg). Plot attached. Compare grey and pink (NLG 35) to blue and brown (NLG19) <70Hz. So the low frequency FIS noise is NLG dependent.
 
Type Time (UTC) Angle Notes DTT Ref
Mid SQZ   112 Interesting data here. Low freq noise higher than with NLG 19. ref 15
ASQZ 18:20:00 70   ref16
MidSQZ 18:22:30 100   ref17

Sheila turned OPO trans back to 96uW so expect NLG to be 19 going into Observing, larger than normal but closer to the value uses before the last OPO crystal move. SQZ angle servo off and angle set back to 171. ADF left on.

Images attached to this report
H1 SQZ (DetChar)
camilla.compton@LIGO.ORG - posted 14:24, Monday 31 March 2025 (83665)
SQZ NLG increased from 11 to 19. ADF back on.

Today during commissioning we increased the SQZ NLG from 11 to 19, now the nominal OPO trans setpoint in sqzparams in 95uW. This was because before our last OPO crystal move 82134, the NLG was closer to 17-19.

We also turned the ADF (322Hz line) back on, it had been off since March 27th 83621, tagging DetChar.

H1 SQZ
sheila.dwyer@LIGO.ORG - posted 14:23, Monday 31 March 2025 (83658)
SQZ angle servo during thermalization

Sheila, Camilla

The IFO was just relocking at the start of commissioning time today, so we set the ADF back on and the sqz angle servo on.  This worked fine, with the phase shifter staying well within it's range (it stayed between 180 and 130 degrees, it's range is 0 -270 degrees). 

In the attached screenshot the vertical cursors are both at 25 minutes into the lock.  You can see that the SQZ BLRMS and the range behave differently with the servo on, but in both cases they start with a low range and move up slowly.  We think that the set point of the squeezing angle servo wasn't set ideally for this time.

In the second screenshot you can see that I changed the SRCL offset and the servo responded to it, taking about 3 minutes to settle.

Images attached to this report
H1 ISC (SUS)
camilla.compton@LIGO.ORG - posted 13:35, Monday 31 March 2025 (83664)
Future Beamdump placement behind HAM1 RM3/PM1 tip-tilt

Rahul, Betsy, Camilla

Attached are some photos of the proposed location of the beamdump that will be placed behind the HAM1 RM3 / PM1 tip-tilt with new D2500101 attached to existing Tip-Tilt DSUB Bracket Holder D1101430. In reality the beamdump will be placed at the mirror image of the photos as the HAM1 beam will be coming the opposite incoming angle.

The Beamdump is made from: 

Images attached to this report
H1 General (Lockloss)
ibrahim.abouelfettouh@LIGO.ORG - posted 12:35, Monday 31 March 2025 (83663)
Lockloss 19:29 UTC

Lockloss right after we got back to OBSERVING with good range.

First impression of cause is that it might be wind related since:

Relocking again now.

H1 SQZ
camilla.compton@LIGO.ORG - posted 13:42, Wednesday 26 March 2025 - last comment - 15:58, Monday 31 March 2025(83570)
SQZ Data set with high NLG, then adjusted SRCL offset and FC detuning.

Sheila, Camilla

Reduced HAM7 rejected pump power and increased SHG launch, turned OPO trans setpoint up to 120uW and measured NLG with 76542 to be 58 (this was a little lower than with 120uW in 83370). OPO gain turned down from -8  to -12. ADF was on for all apart from "Mean SQZ w/o ADF".

Type Time (UTC) Angle DTT Ref
No SQZ 16:01:00 - 16:15:00 N/A ref 0
SQZ 16:56:30 - 16:59:30 (CLF-) 174 ref1
SQZ +10deg 17:00:00 - 17:03:00 (CLF-) 184 ref2
SQZ -10deg 17:03:30 - 17:06:30 (CLF-) 164 ref3
Mean SQZ w/o ADF 17:07:30 - 17:10:30 N/A ref4
Mean SQZ w/ ADF 17:11:00 - 17:14:00 N/A ref5
Mid SQZ + 17:17:00 - 17:20:00 (CLF-) 209 ref6
Mid SQZ - 17:21:30 - 17:24:30 (CLF-) 152 ref7
ASQZ 17:27:30 - 17:30:30 (CLF-) 80 ref8
ASQZ +10deg 17:31:30 - 17:34:30 (CLF-) 90 ref9
ASQZ -10deg 17:35:00 -17:38:00 (CLF-) 70 ref10
Then went to FDS      
FDS SQZ, SRCL -191 17:46:00 - 17:49:00 (CLF-) 174 ref11
FDS SQZ +10deg, SRCL -191 17:49:30 - 17:51:30 (2mins) (CLF-) 184 ref12
FDS SQZ -10deg, SRCL -191 17:52:00 -17:54:00 (2mins) (CLF-) 164 ref13
FDS SQZ, SRCL -290 17:56:30 - 17:59:30 (CLF-) 146 ref14
FDS SQZ +10deg, SRCL -290 18:00:00 - 18:02:00 (2mins) (CLF-) 156 ref15
FDS SQZ -10deg, SRCL -290 18:02:30 - 18:04:30 (2mins) (CLF-) 136 ref16
Starting FC detuning -36Hz      
FDS SQZ, SRCL -290, FC detuning -40Hz 18:08:30 - 18:11:30 (CLF-) 146 ref17
FDS SQZ, SRCL -290, FC detuning -32Hz 18:12:00 - 18:15:00 (CLF-) 146 ref18
FDS SQZ, SRCL -290, FC detuning -32Hz 18:18:00 - 18:21:00 (CLF-) 149 ref19
FDS SQZ, SRCL -290, FC detuning -28Hz* 18:21:30 - 18:24:30 (CLF-) 149 ref20
FDS SQZ, SRCL -290, FC detuning -24Hz 18:225:30 - 18:28:30 (CLF-) 149 ref21
OPO trans back to nominal 80uW, NLG 12      
FDS SQZ, SRCL -290, FC detuning -28Hz 18:46:30 - 18:49:00 (2m30) (CLF-) 170 ref22
FDS SQZ, SRCL -191, FC detuning -36Hz 19:03:30 - 19:06:00 (2m30) (CLF-) 171 ref23

* For NLG of 58, SRCL -290, FC detuning -28Hz looked best.

Plots attached of FIS data showing SQZ, Mean SQZ, Mid SQZ and also SQZ and ASQZ, filename shown on screenshot.

Also did FDS SQZ, +/-10deg with nominal SRCL detuning (-191) and -290, plot attached. And adjusted the FC de-tuning with SRCL offset at -290, plot attached.

Finally we went back to the nominal NLG (NLG of 12 with 80uW OPO Trans setpoint) and checked FDS SQZ with the best found settings at high NLG: SRCL -290, FC de-tuning -28Hz and back to nominal settings, DARM plot attached.  We didn't have time to fully tune the angle in both settings so could repeat this to check at which settings the range is best. Sheila ran a SQZ angle scan at these settings (SRCL -290, FC de-tuning -28Hz), see attached, it is less frequency dependent than than the scans taken the day before at SRCL -191 (nominal) and -190, FC de-tuning -36Hz (nominal), plot attached.

opo_grTrans_ setpoint_uW Amplified Max Amplified Min UnAmp Dark NLG (usual) NLG (maxmin) OPO Gain
120 0.0540944 0.00026378 0.000913452 -0.0000233 57.75 58.68 -12
80 0.010857 0.0002927 0.000904305 -0.0000219 11.72 12.57 -8
Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 14:46, Wednesday 26 March 2025 (83572)

Here are some plots of Camilla's first dataset above, changing the SRC detuning while adjsuting the squeezing angle for high frequency squeezing, made with the same code used for 80318, which is available here

For the gwinc model, I've set the generated squeezing to 23 dB based on Camilla's measured NLG of 58.  Based on the loss estimates from 83457, I've set the Injection loss to 0.178 (17.8% loss) and the PD efficiency (readout efficiency) to 0.815, and the phase noise to 0.

The third attachment shows the model where I've manually adjusted the SRC detuning to roughly match the subtracted squeezing, and the second shows a linear fit of SRCL offset to these detunings.  This suggests that the SRCL offset should be at -306 counts to reduce the SRCL offset, and that we are currently running with a SRCL detuning of 0.013 radians. 

 

 

Images attached to this comment
camilla.compton@LIGO.ORG - 10:51, Thursday 27 March 2025 (83585)

This morning we put SRCL offset to -306, FC de-tuning -28Hz. I then ran SCAN_SQZANG which changed the angle form 171 to 161 and compare the before and after DARM, attached, SQZ looks alot better at higher frequencies, however the range, attached, is similar or a little worse, maybe the 300Hz (yellow BLRMs) squeezing is slightly worse.

Updated DTT legend as had typo.

Images attached to this comment
sheila.dwyer@LIGO.ORG - 15:58, Monday 31 March 2025 (83666)

Here are some preliminary plots from Camilla's data set of different squeezing angles taken at an NLG of 58 with the SRCL offset at it's nominal -191 counts setting, which we believe is about 13 mrad SRC detuning. 

The first plot shows some assumptions that go into making this model, we start with an assumption about arm power, use the noise budget estimate of non quantum noise at 2kHz (which may be out of date now), and set the readout losses to fit the no squeezing data at 2.1-2.3kHz.  Then subtract this quantum noise model without squeezing  from the no squeezing data, and use that as an estimate of the non-quantum noise, which can be added to all of the quantum noise models for different squeezing angles to compare to the measurement. (second plot is a somewhat overwhelming plot of all this added for completeness).

I've set the phase noise to 0 based on 83457.  Using the level of sqz and anti-squeeze at 2.1-2.3 kHz, we infer that the NLG was 63 and the total efficency was 66.5%.  Camilla measured the NLG to be 58, for 120uW circulating power, but in 83370 she measured 61-63 for 120uW.   The third plot here shows the data that Camilla took with the LO loop unlocked, so that the squeezing angle is averaging and rotating freely.  Using this and knowledge of the NLG, we should be able to infer the total squeezing efficiency as a function of frequency. Doing the subtraction of non quantum noise increases the infered efficiency, (compare thick lines to thin), the two different values of NLG suggest rather different efficiencies. There is evidence that the efficiency frequency dependent, which could be caused by a number of effects. Below 200 Hz there is some excess noise in the mean sqz trace, as you can see here, which causes the efficiency infered to be above 1.

The next two plots show the model broken into more readable plots, with the only thing I've adjusted by hand being the SRC detuning.  There is a discrepancy between the model + noise for the anti-squeezing and anti-squeezing +/-10 degrees traces without the filter cavity, which seems like it could be some excess noise that is similar for the different traces.  This is similar to the discrepancy seen in the last plot in 82097, but it is larger in this higher NLG dataset.

 

 

Images attached to this comment
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