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Reports until 16:35, Sunday 26 January 2025
LHO General
ryan.short@LIGO.ORG - posted 16:35, Sunday 26 January 2025 (82473)
Ops Day Shift Summary

TITLE: 01/27 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 154Mpc
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY: One lockloss this shift, but otherwise a quiet day. H1 has been locked and observing for almost 5 hours.

LOG:

Start Time System Name Location Lazer_Haz Task Time End
17:16 SAFETY LASER HAZ LVEA YES LVEA is Laser HAZARD Ongoing
19:09 PEM Robert LVEA - Viewport pictures 19:34
H1 General
ryan.crouch@LIGO.ORG - posted 16:09, Sunday 26 January 2025 - last comment - 16:53, Sunday 26 January 2025(82472)
OPS Sunday EVE shift start

TITLE: 01/27 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 154Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 4mph Gusts, 3mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.14 μm/s
QUICK SUMMARY:

Comments related to this report
ryan.crouch@LIGO.ORG - 16:53, Sunday 26 January 2025 (82474)

Dropped Observing from 00:46 to 00:52 UTC as the SQZer lost lock.

LHO VE
david.barker@LIGO.ORG - posted 10:18, Sunday 26 January 2025 (82470)
Sun CP1 Fill

Sun Jan 26 10:05:46 2025 INFO: Fill completed in 5min 43secs

TCmins [-87C, -51C] OAT (-1C, 30F) DeltaTempTime 10:05:55. Note TC-B didn't reach its minimum plateau.

 

Images attached to this report
H1 General (Lockloss)
ryan.short@LIGO.ORG - posted 10:13, Sunday 26 January 2025 - last comment - 11:43, Sunday 26 January 2025(82469)
Lockloss @ 17:57 UTC

Lockloss @ 17:57 UTC - link to lockloss tool

Usual signs of an ETMX glitch on this lockloss, otherwise cause not obvious. Ends lock stretch at just over 4 hours.

Images attached to this report
Comments related to this report
ryan.short@LIGO.ORG - 11:43, Sunday 26 January 2025 (82471)

H1 back to observing at 19:41 UTC. Helped PRM and SRM during DRMI locking, but otherwise the process was automatic.

I also loaded VIOLIN_DAMPING to take in the new ETMY mode 20 damping setting (gain of 0).

LHO General
ryan.short@LIGO.ORG - posted 07:49, Sunday 26 January 2025 (82468)
Ops Day Shift Start

TITLE: 01/26 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 153Mpc
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 7mph Gusts, 5mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.15 μm/s
QUICK SUMMARY: Two locklosses overnight, but H1 again relocked itself each time without issue. H1 has been locked and observing for 2 hours.

H1 General (OpsInfo, SEI, SUS)
ryan.crouch@LIGO.ORG - posted 22:00, Saturday 25 January 2025 (82467)
OPS Saturday eve shift summary

TITLE: 01/26 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 158Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY: The coherence checked yielded lots of CHARD_Y, MICH & SRCL. MC2 and ITMY cameras are blue from Roberts viewport work. We've been locked for ~4.5 hours.
LOG:                                                                                                                                                         

Start Time System Name Location Lazer_Haz Task Time End
17:16 SAFETY LASER HAZ  LVEA YES LVEA is Laser HAZARD 16:35
01:11 PEM Robert LVEA Y Viewport pictures 01:41

I was also getting a DIAG_MAIN message about "Noisy BSC CPS on: ITMY, ST1, V2" (SEI).

 

Images attached to this report
LHO General
ryan.short@LIGO.ORG - posted 16:30, Saturday 25 January 2025 - last comment - 16:46, Saturday 25 January 2025(82464)
Ops Day Shift Summary

TITLE: 01/26 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY: Mostly quiet shift aside from regular calibration sweeps and a lockloss this afternoon. H1 just finished initial alignment and is starting lock acquisition.

Comments related to this report
ryan.crouch@LIGO.ORG - 16:46, Saturday 25 January 2025 (82465)

ITMX_P was pretty far off, and as soon as it was FORCEd on the wfs loops brought it to a good spot.

Images attached to this comment
H1 General
ryan.crouch@LIGO.ORG - posted 16:05, Saturday 25 January 2025 (82463)
OPS Saturday eve shift start

TITLE: 01/26 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Aligning
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 17mph Gusts, 12mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.14 μm/s
QUICK SUMMARY:

H1 General (Lockloss)
ryan.short@LIGO.ORG - posted 15:40, Saturday 25 January 2025 - last comment - 17:23, Saturday 25 January 2025(82462)
Lockloss @ 23:11 UTC

Lockloss @ 23:11 UTC - link to lockloss tool

As usual, no obvious cause for this lockloss, but there's evidence of an ETMX glitch right before it. Ends lock stretch at almost 11 hours.

Images attached to this report
Comments related to this report
ryan.crouch@LIGO.ORG - 17:23, Saturday 25 January 2025 (82466)

01:23 UTC Observing

H1 CAL
ryan.short@LIGO.ORG - posted 12:02, Saturday 25 January 2025 (82461)
Broadband and Simulines Calibration Sweeps

Following instructions from the TakingCalibrationMeasurements wiki, this morning I ran the usual broadband PCal and Simulines sweeps.

Broadband PCal: 19:30:44 to 19:35:54 UTC

Simulines: 19:36:46 to 20:00:29 UTC

File written out to: /ligo/groups/cal/H1/measurements/DARMOLG_SS/DARMOLG_SS_20250125T193648Z.hdf5
File written out to: /ligo/groups/cal/H1/measurements/PCALY2DARM_SS/PCALY2DARM_SS_20250125T193648Z.hdf5
File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L1_SS/SUSETMX_L1_SS_20250125T193648Z.hdf5
File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L2_SS/SUSETMX_L2_SS_20250125T193648Z.hdf5
File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L3_SS/SUSETMX_L3_SS_20250125T193648Z.hdf5

H1 was out of observing from 19:30 to 20:01 UTC.

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:31, Saturday 25 January 2025 (82460)
Sat CP1 Fill

Sat Jan 25 10:10:10 2025 INFO: Fill completed in 10min 6secs

TCmins [-94C,-93C] OAT (1C,33F), deltaTempTime 10:10:12

Images attached to this report
LHO General
ryan.short@LIGO.ORG - posted 07:34, Saturday 25 January 2025 (82459)
Ops Day Shift Start

TITLE: 01/25 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 137Mpc
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 9mph Gusts, 6mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.18 μm/s
QUICK SUMMARY: Two locklosses overnight, but looks like H1 was able to recover well enough each time. H1 has now been locked for just over 3 hours, and calibration sweeps are scheduled for 19:30 UTC.

H1 General (SQZ)
ryan.crouch@LIGO.ORG - posted 22:01, Friday 24 January 2025 (82457)
OPS Friday EVE shift summary

TITLE: 01/25 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Tony
SHIFT SUMMARY: Over a few hours I've seen the range slowly degrade as the SQZ angle slowly increases and REFL_RF6_ABS_OUTPUT decreases. (Tagging SQZ) Lockloss at the end of the shift, currently relocking at DRMI
LOG: No log

00:56 Observing

05:15 UTC lockloss (6 hour lock)

We keep losing it at locking ALS, something makes the arm start oscillating and then the wfs start working hard to fix it and we lose lock. ALS_Y can survive it sometimes. The BS is wicked misaligned now, CHECK_MICH moved it 2 urads in pitch and 1 urad in yaw.

Images attached to this report
H1 General (Lockloss)
ryan.crouch@LIGO.ORG - posted 21:17, Friday 24 January 2025 (82458)
05:15 UTC lockloss

05:15 UTC lockloss

H1 TCS
matthewrichard.todd@LIGO.ORG - posted 17:31, Friday 24 January 2025 - last comment - 15:06, Tuesday 04 February 2025(82456)
CHETA RIN effect on ESD

[Matthew Camilla Louis Sheila]

There is concern that the CO2 laser proposed for the CHETA design has enough intensity noise to saturate the ESD preventing lock.

By calibrating the displacement noise projected from CHETA RIN data into counts at the L3_ADC, using the DARM loop OLG and transfer function between DeltaL_ctrl and L3_ADC, we can get a rough estimate of whether we expect the CHETA noise to saturate the ESDs. This is done by looking at the RMS of the cts/rtHz of CHETA noise at the ESD and comparing it to the 25% of saturation level (2^19 counts).

Figure 1 is the loop model for mapping the displament noise (CHETA RIN) to ESD counts, Figure 2 is a plot of the darm olg, Figure 3 is plot of the tf from deltaL_ctrl to L3_adc.
Figure 4 is the projection of CHETA RIN to the ADC counts, showing that we do not estimate CHETA is likely to saturate the ESDs.

Next steps are to see if we estimate CHETA nosie to saturate the DCPDs at different power up stages.

Non-image files attached to this report
Comments related to this report
matthewrichard.todd@LIGO.ORG - 15:22, Friday 31 January 2025 (82558)

[M. Todd, J. Kissel]

After measuring very low values for the coherence of the channels used to estimate the transfer function from H1:CAL-DELTAL_CTRL to H1:CAL-CS_DARM_FE_ETMX_L3_ESDOUTF_UL_OUT, it seemed better to go to the calibration model and use pydarm to do this calibration instead.

After making this change, the results are slightly more convincing, saying that we still do not expect CHETA to saturate the ESDs on the ETMX test-mass, however it is around 3% of the saturation level (2**19). The python code used to make this analysis as well as accompanying plots are listed below.

We do however worry about CHETA possibly saturating the coils on the L2 stage, as the noise is around 19% of the saturation level (2**19). This will require some more thought/testing. HOWEVER, this is during the Nominal Low Noise state (pydarm models NLN), and during lock-acquistion we expect that with the additional lowpass filters for the actuation stages we could have some more wiggle room with this.

Much of this code utilizes the pydarm model constructed from pydarm_report_H1.ini found at /ligo/groups/cal/H1/reports/20250123T211118Z/pydarm_H1.ini

The details about how to use the pydarm model and the transfer functions it contains can be found in Jeff's alog


Figures:

  1.  CHETA noise calibrated from m/rtHz to cts/rtHz and RMS to compare to saturation limit of ESDs (L3stage)
  2.  CHETA noise calibrated from m/rtHz to cts/rtHz and RMS to compare to saturation limit of L2 coils (L2stage)
  3.  CHETA noise calibrated from m/rtHz to cts/rtHz and RMS to compare to saturation limit of L1 coils (L1stage)
  4.  Transfer Function - deltaL_ctrl to L3_ESD_cts
  5.  Transfer Function - deltaL_ctrl to L2_coils_cts
  6.  Transfer Function - deltaL_ctrl to L1_coils_cts
  7.  Transfer Function - darm_err to darm_ctrl
  8.  Transfer Function - deltaL to darm_err
  9.  Open Loop Gain measurement of darm - pydar

Code:

Calibrating cheta darm to esd cts

Non-image files attached to this comment
matthewrichard.todd@LIGO.ORG - 15:06, Tuesday 04 February 2025 (82633)

[Edit!]

After noticing an error in the way that the RMS was calculated, I've fixed the code and updated the plots. Fortunately, this does not affect anything upstream (transfer functions and asd calibrations, etc.) but it does inform a better estimate of whether we expect CHETA to saturate the ESDs.

Updated plots:

    1) !cheta_in_esds.pdf
    2) !cheta_in_coilsL2.pdf
    3) !cheta_in_coilsL1.pdf

For more details/summary, refer to alog 82631

Non-image files attached to this comment
H1 DetChar (CAL, DetChar, ISC)
evan.goetz@LIGO.ORG - posted 17:19, Friday 24 January 2025 (82455)
Anti-aliasing filters doing a good job to remove high frequency artifacts
I reported in LHO aLOG 82376 that there were aliasing artifacts as well as a large number of line artifacts not predicted by the offline anti-aliasing analysis. Digging deeper into these unknown artifacts, these may instead be due to the fact that DTT normally holds data as single precision. The DCPD data has a large DC component, so if the data is processed with the "Remove mean" unchecked, then there may be artifacts owing to the large dynamic range. My hunch was confirmed when I tried two things:

1. re-check the "Remove mean" option. Many of the unknown additional line artifacts disappeared
2. using the diaggui_test program, which holds data as double precision.
 2a. Using "remove mean", the unknown additional line artifacts disappeared
 2b. Disabling "remove mean", the unknown additional line artifacts still were gone

Check out LHO aLOG 78559 for other experiences.

Attached is a plot comparing the 524 kHz data of H1:OMC-DCPD_A0_OUT (red) with the 16 kHz of H1:OMC-DCPD_A_OUT_DQ (blue). We don't see any significant differences now that the additional anti-aliasing filters have suppressed high frequency artifacts. The second figure is the now updated PSD comparison before the additional AA filtering in DTT using the "Remove mean" option for the 16k data. Additional artifacts consistent with the expected contribution from aliased artifacts are visible, but now the rest of the spectrum seems more-or-less in agreement.
Images attached to this report
H1 General
ryan.crouch@LIGO.ORG - posted 16:01, Friday 24 January 2025 - last comment - 16:59, Friday 24 January 2025(82450)
OPS Friday EVE shift start

TITLE: 01/25 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 153Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 16mph Gusts, 11mph 3min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.22 μm/s
QUICK SUMMARY:

Comments related to this report
ryan.crouch@LIGO.ORG - 16:59, Friday 24 January 2025 (82454)SQZ

I dropped Observing from 00:49 - 00:56 to adjust the SQZer, I brought H1:SQZ-ADF_OMC_TRANS_PHASE back to -136 alog82421 and then after the servo was done I adjusted the OPO temperature. I accepted the new phase in SDF.

Images attached to this comment
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