The noise reappeared after the unlock of yesterday 20/10 at 8:17 UTC (plot 1, RFC_8MHz has been band pass filter in the 10-40Hz band).

The noise appeared during the unlock of the 07/10, on the operator report it is said that the ITF unlocked because of the thunder around 18:51 UTC. 
I could not find anything that makes those two unlocks different from other unlocks in which the noise did not appear. (signals checked : IMC alignment, MC_Z, PMC_PZT, ML_TH, EOM_CORR_max...) 

This morning I tried to make a cycle of IMC unlock/lock but it did not make the noise disappear. 


EDIT : I added a channel to have an easy access to this addiotnal noise. The RMS of the RFC_8MHz signal betwenn 15Hz and 45Hz 
V1:DQ_BRMSMon_BRMS_INJ_RFC8MHZ_15Hz_45Hz_SIB2_RFC_8MHz_I 

As reported (here and there) few days ago, the LNFS installed on September 10th (SN: 06FS02-03), which at that time was the only fully working sample, appears to be too noisy for the low noise configuration of the ITF.

We thus decided to install the spare one that has been recently repaired (SN: EG-LNFS-002), yesterday afternoon between 12.30UTC anc 13.30UTC.

After setting the last modulation frequencies and amplitudes, I put back in remote control and check the noise level for the three output looking at the dfreq channels (see fig.1). It seems that noise is reduced everywhere.

We will keep tracking its behavior in the following days.

During this morning's maintenance, I installed the mask with a 20 mm diameter aperture. A new WI PAM measurement was then performed this afternoon with the mask in place (fig.1).

The main optics were aligned in the same configuration used for yesterday's measurement by Piernicola ( fig2- entry 69948). 

14.50 UTC: HWS-INJ START with a time sleep of 100 s (20261020T1650)

14.58: WI PAM ON  at 5 V with ramp of 15 min (WF 6)

At 15:58 UTC, I increased the voltage from 5 V to 6.5 V. Unfortunately, I then noticed that both MATLAB and the HWS-INJ acquisition had crashed.

The acquisition was restarted at 16:10 UTC (20261020T1810), using the reference images from the previous measurement (20261020T1650).

However, something seems to have gone wrong with the new acquisition. One of the correctly acquired wavefronts is shown in Fig. 3.

The measurement will probably need to be repeated tomorrow.

The actuator was switched off at 18:30 UTC.

AIm : replace NEN and NWN rotors, survey all rotor position from North End Building

Situation on arrival :

• NEN: box 2024-12 (led "away" from the mirror)
• NWN: box 2024-10 (led "away")
• NSN: box 2021-08 (led "Away")
• NNN: box 2021-04 (led "close" to the mirror) 

Situation after replacement:

• NEN: box 2026-16, R4-11 (led "close")
• NWN: box 2026-15, R4-15 (led "close")
• NSN: box 2021-08 (led "Away")
• NNN: box 2021-04 (led "close") 

Remark: Some tests and changes in the electronic (see logbook...). Tests on LV supply do affect position measurements ( observed between 10 :18 :44 and 10 :29 :02). Pause these tests to finalize survey in stable conditions

Survey

• 11:55 UTC : Place jigs under NSN and NEN to prepare for survey measurement 
• Measurement from survey group from 12:00 UTC to 13:05 UTC (with 2cm spacer between rotors and sphere)
• Measure horizontality of NSN and NWN plates (see pictures "HORIZ*" by pairs: first is global view, second is a zoom on the bubble )
• ~13:15 move jig and bars to NNN and NWN setups to prepare for Survey
• Measure horizontality of NNN and NEN plates (see pictures "HORIZ*" by pairs: first is global view, second is a zoom on the bubble)
• Measurement from survey group @ 13:51 UTC  with first station and 14:09 with second station on this side.
• Remove jigs and test vertical direction of sensor between 14:22 and 14:29 UTC
• Values of NCal position sensors are saved in attached excell file

Tuning

• Correct merchanically for too low position for NNN and NSN (was -1.48 for NSN, -0.8 for NNN). Done at 16:15 UTC. New sensorpositions are in same  excell file. together with the corresponding displacement.
• Correct for phase asymmetry in NEN done at 16:48 in NEB_NCal.cfg

Today we carried out the survey for measuring the position of the NCal benches @NE. We measured the point on top of the calibrators (Fig.1, 2, 3 and 4) for the two sides of the tower (Staz01, Staz02 for the East side, Staz03, Staz04 for the West side).

Tab1 reports the result of the survey in VRS coordinates, while the scheme of the survey is shown in Fig.5

Following the completion of the electrical work in the TCS chiller room and the filter cleaning carried out by Cecilia, all CO₂ lasers were switched back ON.

The main lasers were restarted at around 13.40 UTC (see fig.1).

Some issues were then identified with the auxiliary cooling system, which were successfully solved by Nicola and Cecilia.

The auxiliary lasers were restarted at around 15.35 UTC (see fig.2).

Note that the WI CO₂ beams are currently blocked on the bench to allow the ongoing WI PAM measurements.

ITF found in UPGRADING mode and DOWN state with arms locked on the IR via ARMS_LOCK Metatron node.
All times are UTC.

06:00 MAINTENANCE mode set and ITF unlocked (ARMS_LOCK set to DOWN state).
07:00 Begin of NEB power supply check (Letendre, Frappez, Lafrasse) and Ncal installation (Mours).
07:07 PAM/TCS Room activity (Nardecchia).
07:26 - 09:32 Laser Lab checks (Spinicelli, Craighero).
07:47 CEB Clean Room Level 1 PC retrivial (Margarita, Fede).
08:10 IP noise injections (Ruggi).
08:38 UTA INJ Lab set to full speed (Portata Nominale). 
09:39 UTA INJ Lab se to normal speed (Portata Ridotta).
10:01 End of Maintenance.
10:18 End of Switch-off of TCS chillers room.
13:07 TCS chilles cleaning completed (Zaza).
Restart of the TCS laser is in progress..

ITF left in UPGRADING mode and DOWN state, with arms locked on the IR via ARMS_LOCK node.

Activity during maintenance:
- Cleaning with external company at WEB and SWEB.
- HYMO maintenance at CEB.

The aim of this shift, and the subsequent ones, is to perform the fine alignment of the WI PAM and characterize it using HWS-INJ.

Last Friday, I noticed that both TCS_PAM_WI_PowerSupply and TCS_PAM_WI_pico processes were grey in the VPM. I attempted to restart them, but without success. I then asked Giulio to check the devices, and he confirmed that neither the pico driver (picocltcs2) nor the power supply (rstcs3) was responding to ping requests.

This morning, Giulio restarted the WI pico driver and pico server, restoring communication with the devices (see 69946).

After lunch, we went to the TCS room to restart the WI PAM power supply process. 

Since the WI mirror will be repeatedly heated during the PAM tests, the etalon control loop was switched off at 12:34 UTC by Madda and Francesco.

For the HWS-INJ measurement, I retrieved the positions of the optical components along the beam path used during the CO₂ actuator centering on the West CP (see 69694). The goal is to reproduce the same optical configuration, for which the position of the WI mirror center on the HWS-INJ wavefront maps has already been determined. The corresponding reference measurement was performed on September 4, 2026, between 17:19 and 17:35 UTC. The data are stored in folder 20260904T1919 (see Fig. 1).However, Francesco noticed that the current alignment differed significantly from that of September 4. Therefore, I decided to repeat the HWS-INJ measurement by switching on the CH to determine the current position of the WI mirror center on the HWS-INJ map.

% CH switching ON
I switched ON the HWS-INJ SLED at 1.42 V
ITF in WI SINGLE BOUNCE +PR aligned 
13.29 UTC: HWS-INJ START (20261019T1529)
13.35 UTC: CH ON at high power (WF 8)
13.48 UTC: CH OFF (WF 33 ) and HWS acquisition stopped

The CH appeared clearly in the HWS map (see fig.2).
%%%%%%%%%%
Then, I took advantage of the thermal transient to go to the TCS room and switch off the lasers (69955). 
%%%%%%%%%%

% WI PAM switching ON

The first measurement with the WI PAM was performed with the beam in free propagation, without any mask installed.
The voltage applied to the source was gradually increased using voltage ramps lasting several hundred seconds.

Data acquisition started at 14:57 UTC (20261019T1657). At approximately 5 V (T ≈ 430 °C), the OPL induced by the PAM became visible in the HWS maps only after piston and tilt removal (Fig. 3).

At 6.5 V (T ≈ 620 °C), the PAM-induced OPL was clearly visible in the HWS maps even without removing piston and tilt (Fig. 4).

At the end of the shift (20:00 LT), I switched off the actuator. Tomorrow, we will proceed with further characterization measurements.
I left the ITF in WI single bounce+ PR aligned.

This afternoon, between 14:00 and 14:30 UTC, all CO₂ lasers (Main and CH) and their chillers were switched off in preparation for the electrical work scheduled for tomorrow morning in the TCS chiller room (Fig. 2).

The chillers and the microphone were also covered with protective sheets to prevent dust accumulation.

This morning we did some tests to try to understand the excess of noise
Here are the GPS :

09:38 UTC - INJ AA loop open (from DSP card)
09: 59 UTC - IMC unlock (from VPM)
13:18 UTC - PSTAB open

Surprisingly the cycle IMC unlocked / locked arounf 10 am made the noise as seen on RFC_8MHz disappear. This might go in favour of some saturation in the frequency loop actuators. 
However, I checked some IMC unlocks of the previous days and the noise was present both before and after the unlock. 
I checked if there was other changes in the INJ parameters but could not spot anything obvious. 

ITF found in locked arms IR.

Below the activities communicated in control room:

• SR electrical check (Fabio);
• HYMO maintenace at WEB/MCB;
• from 8:30 UTC noise injections on the suspesions with ITF unlocked (Manuel and Paolo);
• from 12:00 UTC PAM pre-commissioning (Ilaria) with the ITF in WI single bounce with PR aligned. Activity in progress at the end of the shift.

SBE

SIB2 and SPRB vertical position recovered with stepper motors; loops properly closed.

LSC

at 12:34 UTC WI etalon disabled under request of Maddalena.

Since the access to SR tower is over, today at 10:15 UTC I removed the beam dumps from EQB1.

To prevent any unintentional change to the CO2 configuration, I put in PAUSE the TCS_MAIN node; ITF_LOCK is already paused and should not be revived before we start relocking on Thursday afternoon.

Laser frequency noise has been a major limitations during these measurements, making any conclusions on the effect on the BNS range in general, or on the HOM noise (mystery noise) difficult to make. The higher laser frequency noise is due to something that happened on Oct 7 around 19:00 UTC and above 300Hz due to the more noisy LNFS: https://logbook.virgo-gw.eu/virgo/?r=69929.

Figure 1 shows a noise budget in the starting tuned SR configuration. The fitted HOM noise level is comparable to the case of January, when the first stage of SR diaphragm was already installed, for the times when the etalon effect was making the B1p higher. It is unclear in what position the etalon effect was on Oct 14. The estimated frequency noise contribution is comparable to the HOM noise, so the fitted level of HOM noise depends strongly on whether that frequency noise estimation is correct or not.

Figure 2 shows the SR detuned configuration. The frequency noise estimation decreases, because the coupling was lower by a factor ~2 in detuned SR. The estimated HOM noise also decreases by about 20%, which is less of decrease than what was measured in March with the SR diaphragm. It is hard to draw a conclusion from that, as it may be due to many reasons. A tentative conclusion is that the SR detuning is not dramatically better at reducing the HOM noise without the SR diaphragm. At low frequency the sensitivity is much worse, because this data is in LN2 (with many dither lines on), unlike the figure 1 in LN3. 

The 2026-10-18 I found  some SBE SPRB DMS flags red with the follozing comment : SBE_SPRB_ACT_F0H0_raw loops ringing . The SBE SPRB controls was in this state  since the 2026-10-17-08h00-UTC 

I made some actions trying to recover the correct running conditions but without success : 

• actions performed between  the 2026-10-18-06h25m05-UTC and 2026-10-18-06h35m33-UTC

At the end the SBE SPRB loops were left open 

In preparation for the HWS-INJ measurements with the WI PAM, I blocked all CO₂ beams (DAS and CH) on the bench.

• 2026-10-19 08h06m03 UTC    ilaria 'WI_Bench:OUT UP [byte=2]' sent to TTL_co2
• 2026-10-19 08h06m04 UTC    ilaria 'WI_Bench:CH UP [byte=3]' sent to TTL_co2

This morning at 9.45 LC, I restarted the Pico driver (picocltcs2), which was running but was not responding to ping...
I then successfully restarted the TCS_PAM_WI_Pico server via VPM.

14:00 ITF found in DOWN state UPGRADING mode

15:30 UTC SR tower baffle installation completed (#69941), start of vacuum pumping

ITF left in DOWN state and UPGRADING mode

here the BruCo using as target LSC_PRCL: https://scientists.virgo-gw.eu/DataAnalysis/DetCharDev/users/fiori/bruco/LSC_PRCL_1475998223/bruco.html

ITF found in UPGRADING mode and DOWN state.
All times are UTC.
07:40 Permit to work inside SR tower open (Galimberti, #69937). Flange open shortly after (VAC, #69938).
08:35 SR diaphragm installation begin (Majorana, Pinto). Still ongoing at 14:35.

ITF left in UPGRADING mode and LOCKED_ARMS_IR_ALS requested by ARMS_LOCK metatron node.

We run a BruCo, coherences are computed up to 1kHz:
https://scientists.virgo-gw.eu/DataAnalysis/DetCharDev/users/fiori/bruco/Hrec_hoft_1475998223/bruco.html

The pole at 500Hz noise that appeared on Oct 7 around 19:00 UTC is also visible in other channels earlier in the INJ chain.

Figure 1 and 2 compare the time before the issue started (purple) with a time after (blue) respectively on Oct 8 and Oct 14. All the times are with the interferometer in LN2 or LN3. The additional noise is visible clearly also on the Audio band monitoring of the EOM transmission, on the EOM correction, and much less clearly on the PMC transmission.

If the extra noise is visible on the EOM transmission (INJ_EAB_EOM_TRA_AUDIO) both with the IMC locked and unlocked, then it should make it easier to find. As the IMC can be excluded from the investigation, but most likely the problem becomes invisible in that case, as the laser amplitude noise will dominate everything with the PSTAB loop open.