To measure the sensing and driving matrix of BPL, a sinusoidal signal at 2 Hz, with 0.2 V amplitude was injected on channels:

• PZT_EIB_M1BH_CORR
• PZT_EIB_M1BV_CORR
• PZT_LB_M14H_CORR
• PZT_LB_M14V_CORR

Directly on the piezo correction signal. The BPL loop was open while injecting noise.

The signals were injected respectively at GPS times [1464363022, 1464363121, 1464363296, 1464363397] , each injection lasted for 60 s.

The channels QF_h_norm, QF_v_norm, QN_h_norm and QN_v_norm were monitored to see the effect of each piezo on each quadrant.

Piernicola's matlab script "Sensing_matrix_BPL.m" was used to compute the matrices:

sensing_matrix =

   -0.6230   -0.0278    0.0033    0.0012
    0.0233   -0.3838    0.0010   -0.0059
   -0.5035    0.0063    0.4332    0.0151
    0.0154    0.3421    0.0166    0.2886

driving_matrix =

   -1.6099   -0.1078   -1.8808    0.3216
    0.1242   -2.6459    0.0738    3.1261
    0.0118    0.0090    2.3271   -0.1449
    0.0085   -0.0545   -0.1126    3.5359

However, the loop does not close. We tried to adjust the setpoint of the piezo (TILT/SHIFT_X/Y_CORR_SET) so as the norm signal of the QPDs come close to 0, and tried several values of the DRIFT_FILTER gain but we did not succeed.

Paolo got a similar driving matrix, the values of the set point has to be studied more deeply.

One of the performed tests consisted in closing the air valves of the inlet and outlet ducts while the HVAC was off. Acoustic modes of the ducts themself,  associated to air pressure waves resonating inside the ducts, would be affected changing their frequency or reducing. A similar test has been done for DET: https://logbook.virgo-gw.eu/virgo/?r=69058

The plots compare microphones inside the inj lab (and the horizontal accelerometer on LB) at two times with HVAC off: ducts open (blue) and ducts closed (purple). No significant change is observed.

The purple curve shows extra noise due to the fact that on May 19 the Tower HVAC was on (NI open). The blue line in Figures 2 and 3 was taken on April 14 2025 when the ambient noise outside the lab was much quieter (also the CR HVAC responsible a 18.5 Hz line was turned off at that time). 

Figure 3 zooms in the bumps region. Acoustic bumps peaks at 12.07 Hz and 18.20 Hz. The seismic bump present in the laser bench peaks at 18.06 Hz.

In 2021we did tests of mechanically stimulating the LB and measured a mechanical mode of the bench around 17Hz: https://logbook.virgo-gw.eu/virgo/?r=50496. This seems not present now... did it move to 18.06? Could be tested by tapping the bench.

Data sheets of the Quantum gravimeters are now available in the Environmental Monitoring Sys > Sensors and Tools > Documentation: https://scientists.virgo-gw.eu/EnvMon/List/Gravimeter/

ITF DOWN in UPGRADING mode.

Activities communicated to the control room:
- 07:00 UTC - NI CP mount assembly (Travasso)
- 08.40 UTC - STAC site visit (Zaza)
- 12:40 UTC - sniffing for 1Hz magnetic noise in CEB area (Tringali , Fiori)
- TCS Chiller assembly & test at 1500W (Zaza, Ciardelli) in progress.
- NI cleaning (Clean Op team) postponed.

Activities communicated to the control room:

• Confined space safety training

• NI CP mount assembly (Travasso)

• TCS Chiller assembly & test (Zaza)

I confirm that NI tower is still safe wrt laser hazard

This morning from 10:30h to 11h LT we went to the laser lab to realign the beam onto the PMC. We slightly improved the power transmitted by the PMC (Fig. 1) looking at the reflection of the cavity and trying to minimize the 01 mode on the oscilloscope. Afterwards, we flipped down the mirror at the end of the Laser Bench to allow to beam to reach the BPL loop so we can work on it in the next days.

Since May 17 the gravimeter was not reachable from remote. This has been fixed today. Attached are two pictures of the gravimeter (Fig.1) and the laser box (Fig.2).

The issue was with the USB-to-RJ45 adapter, which for some reason was not working properly (the network communication LEDs were off, and the network interface was also disconnected from the console). After unplugging and reconnecting it, the connection was restored, but it went down again a few minutes later. The procedure was repeated, and the connection was re-established. Now, after returning, the machine appears to still be up and running.

Measurement continued through the Cascina holiday, and approximately 48 hours of data was stored.

I evaluated the ASD peak heights for the 1 Hz comb and 50 Hz power line hourly, and plotted their median, max, and min values.

To eliminate calibration uncertainty, the values are expressed in counts.

The median value of the 1 Hz peak was highly stable, whereas other metrics showed temporal variation.

Graphs show data of the accelerometer installed (vertical) on the floor next to the Gravimeter. Fig.1 shows that the noise conditions is more or less stable over 24 hours. Figure 2 compares the spectral noise with one accelerometer sensor (vertical) on the CEB floor (near Guralp). The Fiber lab floor is noisier above 10Hz and below 1Hz.  

related logbook: https://logbook.virgo-gw.eu/virgo/?r=69040

We measured magnetic field at WT 900m, where less instrumental noise is expected. 
We used a portable setup with Bartington Mag-03 MC100 + Nanometrics Centaur.
These data; time series, ASDs, and spectrogram are plotted here. We can see the 1, 2, 3, ... Hz comb noise stationally. 

(NOTE: Calibration should be confirmed)

The slave laser remained stable over the weekend, so this morning we continued working on the alignment.
We seeded the Neovan with the SL and everything was as we let it on Friday afternoon.

We first attempted to optimize the alignment using the mirror in front of the Neovan while monitoring both the transmitted power and the beam profile on AMP_cam.

Since the improvement remained limited and the AMP NF was still significantly away from what it was before, we decided to realign the SL beam towards the Neovan using LB_M04 (the second mirror after the SL) hoping for both effect on the shift and the tilt of the beam inside the neovan. This proved to be very beneficial for both the output power and the beam profile. We managed to recover 0.38 V on AMP_DC.

We then adjusted the Neovan pumping diodes to investigate whether the situation could be further improved. We decreased the current of all four pumping diodes by 0.1 A and obtained a better output beam shape together with a lower temperature of the Neovan head, while maintaining good output power (Figure 1).
New pumping diode current values: 4.8 A.

Overall, we now measure 0.37 V on AMP_DC, compared to 0.34 V previously, and the low-frequency noise is reduced (Figure 2).

The beam shape also looks improved (Figures 3 before and figure 4 after).

Having recovered both good output power and a good beam shape, we proceeded to work on the PMC alignment.
We realigned it and now measure 0.52 V at the output, compared to 0.49 V previously (Figure 5).

While normalizing PMC_TRA and PMC_REFL with AMP_DC, the throughput initially appeared lower. However, after further inspection, it seems that about 3.7% is still coupled into the TEM01 mode. This should recover once the system is fully thermalized. The mismatch is instead around 1%.

We also computed the throughput using PMC_REFL in the unlocked and locked states. We now estimate throughput losses of 20%, whereas they used to be around 22%.

It should be noted that, since the IMC transmission signal is currently unavailable, we could neither work on the PSTAB nor easily verify the alignment in the AOM. These checks will need to be performed later. However, only minor adjustments were required for the alignment towards the PMC.

We let everything locked for the coming days for thermalization. Fine alignment of the PMC as well as check of the order 1 in the AOM will be done on wednesday. 

YAG beam is blocked into LaserLab, with IMC unlocked and SIB1 valve closed. There is  no main laser beam in the interferometer.

CO2 lasers are switched off as well as the green ones. 

Confirm that there is no laser hazard to enter the NI tower.