Reports of 63832
Detector Operation (Operations Report)
berni - 15:28 Tuesday 22 September 2026 (69792) Print this report
Operator Report - Morning shift

ITF found in locked arms.

At 6:00 UTC started the planned maintenance, below the list of the activities communicated in control room:

  • cleaning of the experimental areas;
  • TCS chiller refill;
  • TCS thermo camera reference (operator);
  • LNFS 22MHz replacement with a DDS
  • tuning of the TCS CH (Ilaria from remote)

All the maintenance activities completed around 11:00 UTC; then started the planned commissioning activity of ISC.

 

 

AdV-INJ (General opto-mechanical layout, common parts construction, Installation and pre-commissioning)
nocera - 15:02 Tuesday 22 September 2026 (69793) Print this report
IR1 Sideband Generation

R. Cavalieri, F. Nocera, P. Spinicelli

This is to detail the RF Modulation configuration we are likely to use for IR1.

Starting today, the 22 MHz sideband is generated with a single-output DDS, as per AdV baseline design.

In an attempt to have a fallback plan for the remaining interferometer RF sidebands generation heading towards IR1, we have tried to verify the phase noise of the LNFS referred to an Synth4 in https://logbook.virgo-gw.eu/virgo/?r=69715, i.e. the one which did not turn on, after hacking our way around the power-on issue (we've tracked down the problem to a failure of one of the two AC-DC converter, the one for the +5Vdc, that we bypassed using a bench power supply in its place).
We verified its phase noise performance are not in spec but they are comparable or better than the one currently in use for 6, 8, and 56 MHz. In addition channel three seems to be working as well, contrary to what has been observed in the last few days in the Lab.

The serial communication works ok.


We have left it on but, at this time, not connected to the modulation chain.

The situation therefore is shaky (the "spare" relies on an external power supply, channel 3 reliability is uncertain) but not as bad as it looked yesterday.
 

Injection system (General activities)
gosselin, nocera, cavalieri - 12:09 Tuesday 22 September 2026 (69791) Print this report
LNFS 22MHz replacement with a DDS

This morning we swapped the LNFS that generates the 22.3 MHz used for IMC longitudinal and angular controls with a DDS. 
This LNFS is the one with the communication problem. It will be sent for repair. 

When resetting the output frequency and amplitude of the DDS to nominal values the IMC relocked and so did the RFC. 

We checked some INJ signals : IMC and RFC error signals, 22 dfreq, IMC OLTF... and everything seems to be ok (figures attached)

Images attached to this report
AdV-ISC (Commissioning up to first full interferometer lock)
mwas - 9:22 Tuesday 22 September 2026 (69790) Print this report
Comment to Recovery after DAS step (69783)

To attempt to help with COMMp, yesterday at 14h53 UTC I have increased the SNEB drift control loop gain by a factor 2. The loop error signal is power normalized, so this is not intended to compensate a loss of loop gain due to low power, but to actually increase the loop gain.

AdV-ISC (Commissioning up to first full interferometer lock)
mwas - 9:20 Tuesday 22 September 2026 (69789) Print this report
Comment to Locking difficulties around CARM Null (69787)

Another direction to explore is what is happening with PRCL.

Figure 1 shows an example of an unlock of yesterday evening, B2 6MHz I is in loop for PRCL, but the out of loop signals B2 18MHz I and B2 8MHz I start to diverge at the same time as the power in the arm drops. B2 18MHz is independent of the carrier, so the drop in carrier power is not sufficient to explain the change in B2 18MHz I. There is also a sharp drop in B4 12MHz mag that starts at the same time, which is also independent from the carrier.

Figure 2 shows an example of a longer lock from last Friday, which shows that the offset on B2 6MHz I  is comparable to what it used to be, and that the change in sign of the offset is just due to the adjustment of the demodulation phase of  B2 6MHz before the signal is used. B2 18MHz and B2 8MHz have large fluctuation that start at that time, which makes the running away of these signals on Figure 1 less convincing. However, there is no simulataneous decrease in B4 12MHz mag in that case.

Images attached to this comment
Detector Operation (Operations Report)
zaza - 22:56 Monday 21 September 2026 (69788) Print this report
Operator Report - Afternoon shift

During the afternoon two activities went on: #69785 TCS tuning and #69787 CARM_NULL locking

Activities ended at 20:00 UTC

ITF left in LOCKED_ARMS_IR

AdV-ISC (Commissioning up to first full interferometer lock)
bersanetti, mantovani - 21:37 Monday 21 September 2026 (69787) Print this report
Locking difficulties around CARM Null

In the afternoon shift we noticed a difficulty in locking the DRMI; once we could lock we checked the different steps, and yet again the MICH/SRCL demodulation phase had changed, especially for the 56MHz (and less so for the 169MHz); we checked a few things along the following steps:

  • gains were mostly ok, we increased ASC_PR given the sidebands were lower today; both DARM and MICH had also to be increased (the former especially);
  • the demodulation phase for DARM was also retuned, although to a lesser extent;
  • a first check of the calibration between PD2 and PD1 for B7 was attempted, as we could see that during the swap the level of B7_DC changes; it doesn't look a lot when the change happens (CARM offset 150Hz), but it clearly escalates with the intracavity power; this was done by heart as I couldn't compute the ratio with dataDisplay (it returned a plain zero) nor did I dare to open Matlab during the shift; this will be checked again offline;
  • when we managed to get to CARM Null, the PR vertical resonance at 11.6 Hz killed the lock after a while;
  • later on, the acquisition up to STEP3 was quite reproducible, but we then faced issues going to CARM Null; a general lack of gains (PR, DARM, DIFFp) that we increased, but the gain of SSFS was quite high and we reduced it (again, to be better checked offline);
  • what killed the lock consistently was a quick drift of the carrrier, that we could not explain so far; it happened most of the time in CARM_NULL_3F or while doing the transition to 1F. Sometime we could link it to DIFFp/WE, but not all times so this is not conclusive.
Images attached to this report
Comments to this report:
mwas - 9:20 Tuesday 22 September 2026 (69789) Print this report

Another direction to explore is what is happening with PRCL.

Figure 1 shows an example of an unlock of yesterday evening, B2 6MHz I is in loop for PRCL, but the out of loop signals B2 18MHz I and B2 8MHz I start to diverge at the same time as the power in the arm drops. B2 18MHz is independent of the carrier, so the drop in carrier power is not sufficient to explain the change in B2 18MHz I. There is also a sharp drop in B4 12MHz mag that starts at the same time, which is also independent from the carrier.

Figure 2 shows an example of a longer lock from last Friday, which shows that the offset on B2 6MHz I  is comparable to what it used to be, and that the change in sign of the offset is just due to the adjustment of the demodulation phase of  B2 6MHz before the signal is used. B2 18MHz and B2 8MHz have large fluctuation that start at that time, which makes the running away of these signals on Figure 1 less convincing. However, there is no simulataneous decrease in B4 12MHz mag in that case.

Images attached to this comment
AdV-TCS (CO2 laser projector)
bersanetti, corubolo, lumaca, mantovani, menzione, nardecchia, spinicelli, zaza - 21:03 Monday 21 September 2026 (69786) Print this report
TCS tuning part.4

At around 13:30 UTC, we prepared the DET HWS measurement to sense the NI mirror: the INJ HWS beam was turned OFF and the DET HWS beam was set to 1.4V.

After various attempts of lock acquisition up to CARM NULL 1F, we agreed with the ISC team to perform a CH common step. Specifically, at 14:11 UTC both the CH powers have been increased by 20% (STEP 10), as detailed in the table below.

 

STEP 10

CH [W]

INNER DAS [W]

OUTER DAS [W]

 W 

 on the ITF

 0.044 → 0.053 

 0.120

 1.296

 on the pickoff 

 0.272 → 0.326 

 0.019

 0.216

 N

 on the ITF

 0.040 → 0.048 

 0.216

 0.864

 on the pickoff 

 0.247 → 0.296 

 0.035

 0.142

No sufficiently long locks have occurred to allow a measurement with the HWS DET, so the activity will be postponed to the upcoming shifts.

AdV-TCS (CO2 laser projector)
melo - 18:06 Monday 21 September 2026 (69785) Print this report
Comment to TCS tuning part.3 and HWS-INJ measurements (69775)

Today, an analysis of the WI point absorber was performed using thermocamera images.

  • Fig. 1 shows the reference thermal image selected for the analysis.

  • Fig. 2 displays the MATLAB analysis output, highlighting a differential temperature of approximately 0.65 degrees for the point absorber (calculated by subtracting the mirror image in CARM_NULL from the image taken with the ITF in DOWN status).

  • Fig. 3 illustrates the reconstructed mirror geometry, featuring the identified mirror center and the point absorber location based on pixel-to-distance mapping.

Geometric Mapping:

  • X-Axis (Columns): The mirror center is located at column 388, whereas the point absorber is at column 384. This places the point absorber slightly to the left of the center (a offset of 3.5 pixels in the image, corresponding to approximately 0.5 cm in physical space).

  • Y-Axis (Rows): The mirror center is located at row 241, whereas the point absorber is at row 221. This places the point absorber above the center (an offset of 19.5 pixels in the image, corresponding to approximately 3.0 cm in physical space).

  • Radial Distance: The total estimated physical distance of the point absorber from the mirror center is approximately 3.1 cm.

Note that because this spatial mapping is reconstructed manually from off-axis thermocamera images, it is subject to geometric projection and pixel-resolution uncertainties. Consequently, this estimate should be considered less precise than the HWS measurement and serves primarily as a qualitative/cross-checking reference.

I will soon perform a similar analysis of the NI PAs.

 

Images attached to this comment
AdV-ISC (Commissioning up to first full interferometer lock)
boldrini, bossilkov, ruggi, bersanetti, mantovani - 16:08 Monday 21 September 2026 (69783) Print this report
Recovery after DAS step

Today we attempted to recover the lock acquisition after this Sunday's DAS step.

We noticed that sidebands power has decreased at the DRMI step (Fig.1), but despite this the lock acquisition is somewhat workable without the need of any major change, although it tends to fail in STEP_3_OF_3 for reasons unclear.

The lock in CARM_NULL_1F is achievable, but not particularly stable. We noticed that a frequent cause of unlock is COMMp, who attempts to engage far away from its working point, possibly due to a slight misalignment of the SNEB that introduces a large DC offset in the error signal. For the moment, COMMp and the soft loops have been commented in ITF_LOCK.py (lines 4544-4545 for COMMp and 4458-4461 for soft modes)

Images attached to this report
Comments to this report:
mwas - 9:22 Tuesday 22 September 2026 (69790) Print this report

To attempt to help with COMMp, yesterday at 14h53 UTC I have increased the SNEB drift control loop gain by a factor 2. The loop error signal is power normalized, so this is not intended to compensate a loss of loop gain due to low power, but to actually increase the loop gain.

Detector Operation (Operations Report)
menzione - 15:54 Monday 21 September 2026 (69779) Print this report
Operator Report - Morning shift

ITF found in LOCKED_ARMS_IR in COMMISSIONING mode.
Locking in progress up to CARM_NULL_1F after the usual cross-alignment in ACQUIRE_DRMI.

Planned activity:
CARM NULL locking / DAS adjustment (Boldrini)

Sub-system reports

DET
Both SDB2_B1p_QD1 and SDB2_B1p_QD2 VBias' rearmed and shutter opened several times during the locking attempts.

Images attached to this report
On-call intervention (General)
Oncall-system - 9:34 Monday 21 September 2026 (69782) Print this report
On-call intervention

The following report has been submitted to the On-call interface.

On-call events -> Air Conditioning

Title: Compressore d'aria n. 2 TB in blocco

Author(s): soldani, Pezzimenti

Called at: , , by: Alarm or monitoring system
Remote intervention: Started: ; Ended:
On-site intervention: Started: 07:41, 20-09-2026; Ended: 07:56, 20-09-2026
Status: Resolved
Operator when issue resolved: None

Details:

Allarme ricevuto sabato ore 21, sia da me che dal Reperibile HVAC in turno Marco Tacchi. Telefonicamente e con l'ausilio del DMS e' stato verificato che il compressore n. 2 in TB era in blocco ("mancata ripartenza") ma il n. 1 era correttamente funzionante e l'impianto non ha subito cali di pressione. E' stato deciso che un intervento immediato sul sito non era necessario.
Ho provveduto a ripristinare il funzionamento del compressore n. 2 alle 7:45 circa del mattino successivo (domenica 20/09).

* Note that any files attached to this report are available in the On-call interface.

On-call intervention (General)
Oncall-system - 8:38 Monday 21 September 2026 (69781) Print this report
On-call intervention

The following report has been submitted to the On-call interface.

On-call events -> Air Conditioning

Title: Compressore d'aria n. 2 TB in blocco

Author(s): soldani, Pezzimenti

Called at: , , by: Alarm or monitoring system
Remote intervention: Started: ; Ended:
On-site intervention: Started: 07:41, 20-09-2026; Ended: 07:56, 20-09-2026
Status: Resolved
Operator when issue resolved: None

Details:

Allarme ricevuto sabato ore 21, sia da me che dal Reperibile HVAC in turno F. Pezzimenti. Telefonicamente e con l'ausilio del DMS e' stato verificato che il compressore n. 2 in TB era in blocco ("mancata ripartenza") ma il n. 1 era correttamente funzionante e l'impianto non ha subito cali di pressione. E' stato deciso che un intervento immediato sul sito non era necessario.
Ho provveduto a ripristinare il funzionamento del compressore n. 2 alle 7:45 circa del mattino successivo (domenica 20/09).

* Note that any files attached to this report are available in the On-call interface.

On-call intervention (General)
Oncall-system - 8:38 Monday 21 September 2026 (69780) Print this report
On-call intervention

The following report has been submitted to the On-call interface.

On-call events -> Air Conditioning

Title: Compressore d'aria n. 2 TB in blocco

Author(s): soldani, Pezzimenti

Called at: , , by: Alarm or monitoring system
Remote intervention: Started: ; Ended:
On-site intervention: Started: 07:41, 20-09-2026; Ended: 07:56, 20-09-2026
Status: Resolved
Operator when issue resolved: None

Details:

Allarme ricevuto sabato ore 21, sia da me che dal Reperibile HVAC in turno F. Pezzimenti. Telefonicamente e con l'ausilio del DMS e' stato verificato che il compressore n. 2 in TB era in blocco ("mancata ripartenza") ma il n. 1 era correttamente funzionante e l'impianto non ha subito cali di pressione. E' stato deciso che un intervento immediato sul sito non era necessario.
Ho provveduto a ripristinare il funzionamento del compressore n. 2 alle 7:45 circa del mattino successivo (domenica 20/09).

* Note that any files attached to this report are available in the On-call interface.

AdV-TCS (CO2 laser projector)
nardecchia - 11:53 Sunday 20 September 2026 (69778) Print this report
DAS COMMON STEP

As agreed during Friday's Daily Meeting, we increased the power of all DAS actuators by 20%.

I also switched ON the WI inner ring, which had remained OFF so far, setting it to the minimum power of 120 mW.

The powers corresponding to this new configuration (STEP 10) are summarized in the table below:


 

STEP 10

CH [W]

INNER DAS [W]

OUTER DAS [W]

W

on the ITF

0.044

0.120

1.296

on the pickoff 

0.272 

0.019

0.180*(1+20%)=0.216

N

on the ITF

0.040 

0.216

0.864

on the pickoff 

0.247 

0.029*(1+20%)=0.035

0.118*(1+20%)=0.142

The activity was completed at 09:11 UTC. In order to follow the transient, I asked to keep the CITF locked. Then, just as a test, we attempted a lock acquisition up to CARM NULL. The interferometer remained in CARM NULL for a few minutes before unlocking. I left the ITF locked in CITF. Later in the afternoon, I will request Locked Arms on IR.

AdV-TCS (CO2 laser projector)
mwas - 8:28 Saturday 19 September 2026 (69777) Print this report
Comment to TCS tuning part.3 and HWS-INJ measurements (69775)

These results are so far qualitevely similar to the point absorbers measurements done at LMA VIR-0406A-26

For WI the LMA measurements had shown one strong point absorber close to the center (-10mm, +24mm) with an expected absorbtion of 7-8mW for 100kW of power in the arms. It was point 5012 of the input mirror scan. 

Analyzing the HWS image from yesterday with the same type of code as the LMA measurements I find that to make a comparable effect to what is on the HWS image, an absorption of 11mW is needed. The power in the arms is currentlny around 80kW, so scaling it to 100kW it correspond to an absorption of 14mW, almost double what was expected. 

Figure 1 shows the HWS image after 10 wavefronts, roughly 5 minutes. 

Figure 2 shows the model of the HWS image after 5 minutes for one point absorber and uniform absorption of 20mW.

Figure 3 shows the difference between the HWS image and the model

Figure 4 and 5 shows vertical and horizontal cuts through the HWS image and the model

/users/mwas/TCS/HWS_image_convolution/image_convolution_WI_IM01_transient.m

For NI several point absorbers with lower absorption are expected from the LMA measurement. Which qualitely is what is seen on the NI thermal camera image, where the points look much less bright than on the WI thermal camera image. A HWS image of NI would be needed to confirm that indeed the NI point absorbers have a lower absorption than the WI point.

 

Images attached to this comment
AdV-TCS (CO2 laser projector)
bersanetti, nardecchia, spinicelli - 19:36 Friday 18 September 2026 (69776) Print this report
Comment to TCS tuning part.3 and HWS-INJ measurements (69775)

In the afternoon, the lock acquisition worked smoothly. Thus, I took some time to check the focus of the NI and WI thermocamera. In addition I also tried to focus the PAY NI Cam.

I could look at the camera images during several lock acquisitions, and those seem to confirm the presence of the WI PA (Fig. 1 and the down in fig 2, tiff and csv data on demand). Unfortunately, also the NI mirror seems to have some points (a clear one on the left part of the image and a fainter one on its right) that shine up with the lock acquisition (fig. 3 and the donw in fig. 4, tiff and csv data on demand).
To be confirmed with further HWS absorption measurements.

In both cases, they start to shine already at step 3/3 (250mW).

I left the ITF locked on the arms for the weekend.

 

Images attached to this comment
AdV-TCS (CO2 laser projector)
bersanetti, corubolo, lumaca, mantovani, menzione, nardecchia, ruggi, spinicelli - 17:55 Friday 18 September 2026 (69775) Print this report
TCS tuning part.3 and HWS-INJ measurements

Yesterday evening we raised the WI CH power (STEP 5, around +40%) in an attempt to set the SBs level in CITF back to their maximum values, i.e. around 0.054 mW for the 6 MHz and 0.032 mW for the 56MHz. So the starting point of this morning is summarised in the table below:

Starting Point

CH [W]

INNER DAS [W]

OUTER DAS [W]

on the ITF

0.044

0

1.08

on the pickoff 

0.272 

0

0.180

on the ITF

0.031

0.18

0.72

on the pickoff 

0.192

0.029

0.118

Also this morning we made a further action, this time on the NI CH; we performed two steps:

  • STEP 6, NI CH power +18%, at 7.23 UTC

  • STEP 7, NI CH power +18%, at 7.42 UTC

Since STEP 7 decreased the 12 MHz signal, we partially reverted the change by 9% with respect to STEP 7.

After these two steps, we resumed the lock acquisition attempts up to CARM NULL. After several attempts, which consistently unlocked at the same stage of the lock acquisition, the ISC team solved the issue by adjusting some lock acquisition parameters.

At 08:31 UTC, CARM_NULL_1F was reached and the lock lasted for about 30 minutes.

Figure 1 shows a comparison between this CARM_NULL_1F lock (08:31 UTC, lasting about 30 min, blue and orange lines) and the one obtained yesterday (17/09 at 14:14 UTC, lasting about 25 min, purple lines). The DAS STEP3 improved the sideband level, as can be seen from the comparison.

After the 08:31 UTC lock, we were not able to lock again due to a vertical oscillation of the PR mirror at around 11 Hz, similar to the one observed yesterday (69770). We therefore called Paolo for support.

At 10:38 UTC, following Paolo's indications, Diego managed to reach CARM_NULL_1F again.

From this point on, the CARM_NULL_1F lock became reasonably reproducible. Thanks to Diego, we also recovered the automation for the gentle unlock. After a few trials, we were able to perform the planned HWS-INJ measurements, manually unlocking the interferometer when needed.

A PA signature is visible in the HWS-INJ maps in two different measurements: during the lock acquisition (heating phase) and after the unlock from CARM NULL (cooling phase), as shown in Fig. 2. In the same figure, the CH measurement reported in entry 69694 is shown as a reference for the mirror center. From this preliminary comparison, the PA appears to be reasonably close to the center of the mirror. A more detailed analysis of the acquired data will follow.

We left the following TCS settings:

 

 

CH [W]

INNER DAS [W]

OUTER DAS [W]

W

on the ITF

0.044

0

1.08

on the pickoff 

0.272 

0

0.180

N

on the ITF

0.040 

0.18

0.72

on the pickoff 

 0.247 

0.029

0.118

 

Images attached to this report
Comments to this report:
bersanetti, nardecchia, spinicelli - 19:36 Friday 18 September 2026 (69776) Print this report

In the afternoon, the lock acquisition worked smoothly. Thus, I took some time to check the focus of the NI and WI thermocamera. In addition I also tried to focus the PAY NI Cam.

I could look at the camera images during several lock acquisitions, and those seem to confirm the presence of the WI PA (Fig. 1 and the down in fig 2, tiff and csv data on demand). Unfortunately, also the NI mirror seems to have some points (a clear one on the left part of the image and a fainter one on its right) that shine up with the lock acquisition (fig. 3 and the donw in fig. 4, tiff and csv data on demand).
To be confirmed with further HWS absorption measurements.

In both cases, they start to shine already at step 3/3 (250mW).

I left the ITF locked on the arms for the weekend.

 

Images attached to this comment
mwas - 8:28 Saturday 19 September 2026 (69777) Print this report

These results are so far qualitevely similar to the point absorbers measurements done at LMA VIR-0406A-26

For WI the LMA measurements had shown one strong point absorber close to the center (-10mm, +24mm) with an expected absorbtion of 7-8mW for 100kW of power in the arms. It was point 5012 of the input mirror scan. 

Analyzing the HWS image from yesterday with the same type of code as the LMA measurements I find that to make a comparable effect to what is on the HWS image, an absorption of 11mW is needed. The power in the arms is currentlny around 80kW, so scaling it to 100kW it correspond to an absorption of 14mW, almost double what was expected. 

Figure 1 shows the HWS image after 10 wavefronts, roughly 5 minutes. 

Figure 2 shows the model of the HWS image after 5 minutes for one point absorber and uniform absorption of 20mW.

Figure 3 shows the difference between the HWS image and the model

Figure 4 and 5 shows vertical and horizontal cuts through the HWS image and the model

/users/mwas/TCS/HWS_image_convolution/image_convolution_WI_IM01_transient.m

For NI several point absorbers with lower absorption are expected from the LMA measurement. Which qualitely is what is seen on the NI thermal camera image, where the points look much less bright than on the WI thermal camera image. A HWS image of NI would be needed to confirm that indeed the NI point absorbers have a lower absorption than the WI point.

 

Images attached to this comment
melo - 18:06 Monday 21 September 2026 (69785) Print this report

Today, an analysis of the WI point absorber was performed using thermocamera images.

  • Fig. 1 shows the reference thermal image selected for the analysis.

  • Fig. 2 displays the MATLAB analysis output, highlighting a differential temperature of approximately 0.65 degrees for the point absorber (calculated by subtracting the mirror image in CARM_NULL from the image taken with the ITF in DOWN status).

  • Fig. 3 illustrates the reconstructed mirror geometry, featuring the identified mirror center and the point absorber location based on pixel-to-distance mapping.

Geometric Mapping:

  • X-Axis (Columns): The mirror center is located at column 388, whereas the point absorber is at column 384. This places the point absorber slightly to the left of the center (a offset of 3.5 pixels in the image, corresponding to approximately 0.5 cm in physical space).

  • Y-Axis (Rows): The mirror center is located at row 241, whereas the point absorber is at row 221. This places the point absorber above the center (an offset of 19.5 pixels in the image, corresponding to approximately 3.0 cm in physical space).

  • Radial Distance: The total estimated physical distance of the point absorber from the mirror center is approximately 3.1 cm.

Note that because this spatial mapping is reconstructed manually from off-axis thermocamera images, it is subject to geometric projection and pixel-resolution uncertainties. Consequently, this estimate should be considered less precise than the HWS measurement and serves primarily as a qualitative/cross-checking reference.

I will soon perform a similar analysis of the NI PAs.

 

Images attached to this comment
AdV-ISC (Commissioning up to first full interferometer lock)
bersanetti, mantovani - 17:16 Friday 18 September 2026 (69774) Print this report
Change of etalon setpoint

Today around 15:12 UTC we changed the etalon setpoints:

  • NI: 20.207 degC in 172800 s (48 h)
  • WI: 19.60 degC in 172800 s (48 h)
Detector Operation (Operations Report)
menzione - 15:59 Friday 18 September 2026 (69773) Print this report
Operator Report - Morning shift

ITF found in LOCKED_ARMS_IR and in COMMISSIONING mode.

Planned activity:
CARM NULL locking / DAS adjustment (Mantovani, Bersanetti, Spinicelli, TCS crew).

- ITF relocked up to CARM_NULL_1F after the usual cross-alignment in ACQUIRE_DRMI.
At the end of the morning TCS tuning, I set "False" at line 17 in the ITF_LOCK.ini and restarted the lock acquisition. ITF acheived easily CARM_NULL_1F.
DAS adjustment in progress...

Sub-system reports

DET
06:05 UTC - Both SDB2_B1p_QD1 and SDB2_B1p_QD2 VBias' rearmed several times during the locking attempts.

Images attached to this report
Detector Operation (Operations Report)
lunghini - 23:01 Thursday 17 September 2026 (69768) Print this report
Operator Report - Afternoon shift

ITF found in COMMISSIONING Mode and LOCKING_CARM_NULL_1F State with activity on CARM NULL locking / DAS adjustment ongoing.
The activity went on up to 19:38 UTC (#69770).
ITF left in COMMISSIONING Mode and LOCKED_ARMS_IR State.

 

Images attached to this report
AdV-TCS (CO2 laser projector)
bersanetti, boldrini, bossilkov, corubolo, lumaca, mantovani, nardecchia, pinto, spinicelli, ruggi - 21:18 Thursday 17 September 2026 (69770) Print this report
TCS tuning part.2

This morning, we continued the tuning activity started yesterday (69761). 
The initial TCS settings are summarized in the table below.

 

STARTING POINT

After STEP 2 (logbook entry 69761)

CH [W]

INNER DAS [W]

OUTER DAS [W]

W

on the ITF

0.026 

0

0.90

on the pickoff 

0.160 

0

0.150

N

on the ITF

0.026

0.15 

0.60

on the pickoff 

0.160

0.024

0.098

The CARM NULL locks were limited by a vertical oscillation of the PR at around 11 Hz, which was causing the ITF to unlock. Paolo and Manuel took care of the issue and managed to solve it.

At some point, we also experienced a few unlocks due to the green losing lock. This issue was investigated and solved by Piernicola.

At this point, since the B1p fringe was already quite dark (~0.016 mW), we decided to try a common step on both DASes in an attempt to increase the sideband power. We therefore decided to increase both the WI and NI DAS powers by 20% at 14:42 UTC (STEP 3)

Unfortunately, shortly afterwards, the ITF unlocked due to an earthquake, which prevented further lock acquisition attempts for some time (earthquake at 14:19 UTC).

Once the earthquake transient had approximately settled, we noticed that the sideband powers in CITF had decreased by about 10%.

ISC then attempted two lock acquisitions, but both failed at the same step (CARM offset, step 3/3).

Therefore, before retuning the lock acquisition, we decided to also increase both the WI and NI CH powers by 20% (STEP 4, at 16:25 UTC).

The sideband increased but not recovering the level before the STEP 3. Some attempts were made to reach CARM NULL, but we did not manage to reach it. The ITF always unlocked at the same step (CARM offset, between step 2 and 3).

The final CO₂ laser configuration is summarized in the table below.

 

FINAL POINT 

After STEP 4

CH [W]

INNER DAS [W]

OUTER DAS [W]

W

on the ITF

0.031 

0

1.08

on the pickoff 

0.192 

0

0.18

N

on the ITF

0.031 

0.18

0.72

on the pickoff 

0.192 

0.029

0.118

 

 

AdV-TCS (Point Absorbers Mitigation)
boldrini, bossilkov, mantovani, bersanetti - 20:46 Thursday 17 September 2026 (69772) Print this report
Comment to NI and WI thermal camera videos of a CARM_NULL (69766)

We could not recover CARM_NULL_1F after the TCS steps: the lock parameters need a more careful tuning after these changes.

Presently, the lock breaks at step 2/3 of the CARM offset reduction.

 

We also undid the change in the /virgoDev/Automation/PyALP/PyUGF/algo.py, resetting the UGF servos step to ±\pm5%

AdV-TCS (Point Absorbers Mitigation)
mwas - 18:53 Thursday 17 September 2026 (69771) Print this report
Comment to NI and WI thermal camera videos of a CARM_NULL (69766)

Figure 1 and 2 shows two screenshots from the video of WI. One towards the end of the CARM NULL lock and well before. Jumping back and forth between the two pictures there is a faint absorber visible in the middle of the image. And that point disappears shortly after the unlock. 

Figure 3 shows that faint point circled.

Figure 4 and 5 shows the same type of analysis for the NI video. There I cannot notice any points, but it might be harder to notice on the color videos than on the black and white one.

Images attached to this comment
AdV-TCS (Point Absorbers Mitigation)
corubolo, kraja, lumaca, nardecchia, spinicelli - 16:47 Thursday 17 September 2026 (69766) Print this report
NI and WI thermal camera videos of a CARM_NULL

In the following, the link to NI and WI thermal cameras videos of yesterday's lock acquisition starting around 14:39 UTC, CARM NULL (of around 40 seconds) and a brief time after, together with main ITF signals.

https://owncloud.ego-gw.it/s/NDrWctmKC5ebyb4 

As already observed (69742), there is no clear evidence of PAs.

Comments to this report:
mwas - 18:53 Thursday 17 September 2026 (69771) Print this report

Figure 1 and 2 shows two screenshots from the video of WI. One towards the end of the CARM NULL lock and well before. Jumping back and forth between the two pictures there is a faint absorber visible in the middle of the image. And that point disappears shortly after the unlock. 

Figure 3 shows that faint point circled.

Figure 4 and 5 shows the same type of analysis for the NI video. There I cannot notice any points, but it might be harder to notice on the color videos than on the black and white one.

Images attached to this comment
boldrini, bossilkov, mantovani, bersanetti - 20:46 Thursday 17 September 2026 (69772) Print this report

We could not recover CARM_NULL_1F after the TCS steps: the lock parameters need a more careful tuning after these changes.

Presently, the lock breaks at step 2/3 of the CARM offset reduction.

 

We also undid the change in the /virgoDev/Automation/PyALP/PyUGF/algo.py, resetting the UGF servos step to ±\pm5%

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