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Daily Reports (2026/01/06-13, NIKA2 run 78, Cryo run 90)

Observers on-site: Beth Jones, Michael Logue, Remi Adam, Tuan-Anh Duong

Astronomer on Duty: Stefano Berta (SB)
Pool Manager: Angel Bongiovanni

Operators: Kike (day), Frederic (night)

Organization of shifts:
21:00-03:00 UT: Tuan-Anh
03:00-09:00-10:00 UT: Remi
09:00:15:00 UT: Beth
15:00-21:00 UT: Michael

Important

Focus offsets shall be measured on Ar1
Pointing offsets shall be measured on Ar2

Pool-Account usage: Accounting of observing times

Focus and Beam maps accounting

Please fill the Table with the Ar1,2,3 focus values as follows. At best, make one table per day.

Similarly, if any beam maps (total power or polarimetry) are taken:

Tuesday 6th January 2026

@9:30 UT: the team arrived safely to the telescope. Blue skies, low tau, strong winds.
Short briefing to share important mountain information and recommendations. We re-organize the shifts (see top of this page).

@13:30 UT: system checks finished, Dave goes back to Granada. Starting the rotation of the HWP required to reboot the DAQ few times and also the mppsync server.
NIKA2 system setup completed: DAQ running, HWP rotating, NIKA2 window open, PaKo running, QL monitors x6 running, make-imbf new/old running. We wait only for the wind to calm down.

@14:00 UT Alessandro and Martino ask for some time to remotely check the amplifier of the noisy Box C (Ar2). They think that this enhanced noise might be due to the polarization of the Box C amplifier, that needs to be re-set from time to time. Alessandro and Martino check the amplifier. In Alessandro's words: "The gain of the amplifier C is too low. (...) I could fix it by playing with the parameters of the amplifier C but now with the parameters that worked in June 2025 it is not working anymore (...) it seems that the third stage of the amplifier C (YL026, the one that we have installed in June) is not working. The gain must thus be much lower, and adding noise. Just the less gain doesn't explain what we observe", though.

@15:00-21:00 UT Michael + all. Taumeter tau < 0.1. The telescope is parked because of the high wind. We take the chance to have a long explanation about NIKA2 operations. In the next days we hopefully will be able to put in practice what we learned.

Brrrrrrr!

@21:00-03:00 UT Tuan-Anh + Stefano. We start observing at 22:30 UT. It takes some time to set everything. We need to reboot crates 3 and 1, the DAQ and the HWP rotation. All good now. Lost KIDs: 18/7/12 in Ar1/2/3. The first pointing scan is at 23:05 UT: 20260106s17.

The secondary mirror (M2, subreflector) is a capricious tonight and sends errors at every scan, including tracks:

Now the observations can start. But the DAQ has lost part of Ar3. We tune again. After 4 tuning with Boxes P and Q completely lost, we stop the HWP rotation and reboot the DAQ. KIDs lost: 15/7/12. We finally start the observations at 1:09 UT

Obviously the new make-imbf ain't working. I try to produce by hand the imbf of scan 26 and it tells "LD_LIBRARY_PATH unbound variable". Same for some old_ldpath. This was with Stefano's account. We try with the operator's account. It gives the same message. We have to work with the old one for now. We're in polarimetry and we should focus on Ar1 -> very slow. Perfect weather!

Not bad this NIKA2 2026 start! We had every possible hic-hup in one night. The next 6 weeks can only be smooth :D

Pointing, focus, calib_1scan on Uranus (although now at low elevation). 1 rep on NGC2264d and one calib_1scan on 3C286

Wednesday 7th January 2026

03:00-09:00 UT Remi

Good morning!

09:00-15:00 UT Beth + Stefano

15:00-21:00 UT Michael + Stefano + Beth

21:00-03:00 UT Tuan-Anh: The tau value ~ 0.23 at the beginning of the shift and it is increasing. So we continue with total power.

Thursday 8th January 2026

03:00-9:00 UT Remi: The opacity was showing large variations so far, but is stabilizing and decreases during the shift (about 0.2), the wind is about 5-7m/s. Box A2-C is still as yesterday. IMBFITS are made with both versions smoothly.

09:00-15:00 UT Beth (+ Stefano)

Observng our favorite source

15:00-21:00 UT Michael + Beth (+ Stefano)

21:00-03:00 UT Tuan-Anh:

Friday 9th January 2026

03:00-09:00 UT Remi: The opacity was stable/slowly decreasing so far (< 0.2), the wind is about 5-7m/s. We start in polarization mode.

09:00-15:00 UT Beth. I take over with the telescope parked.

A supernumerary fog bow! A supernumerary fog bow!

15:00-21:00 UT Michael

21:00-03:00 UT Tuan-Anh

Saturday 10th January 2026

03:00-10:30 UT Remi: The opacity show large jumps but the sky is clear and the NIKA2 data are very good (about +/- 2 Jy/beam over the last pointing), the wind is about 5m/s. We are in total power.

10:30-15:00 UT Beth:

15:00-21:00 UT Michael + Beth + Stefano

Meaow After so much blue, a bit of yellow... ...and red!

21:00-03:00 UT Tuan-Anh

Sunday 11th January 2026

03:00-09:00 UT Remi

...and red! ...and red!

08:30-15:00 UT Beth + Stefano

15:00-21:00 Michael + Stefano

Africa and Gibraltar

...and red!

21:00-03:00 Tuan-Anh

Monday 12th January 2026

03:00/09:00 Remi Very stable condition, low wind (2m/s), and the opacity is dropping (0.16 at the start). The plan is to do total power beam maps under such conditions.

...and red! ...and red!

SB about the scans with weird (corrupted) timelines: Some scans show a very weird behavior of the timelines, with the signal jumping and many records being rejected by the PIIC QL-monitor data processing. The problem affects all three NIKA2 arrays simultaneously. And it seems to be happening throughout the whole scan (not just a fraction of it). It happens only on one scan: the previous and next scans are just fine. Therefore one suspect we had was whether there might be some incorrect tuning at the beginning (remember that during the scan no re-tuning is performed). But would it be incorrect for all KIDs? Remi tried to reduce one of them offline with PIIC and the whole scan was rejected. As of 2026/01/12 @8:00 UT we have seen at least 4 cases. Two of them are in 197-25 science scans 20260111s56 (06:49 a.m. UT) and 20260112s68 (06:27 a.m. UT). Other two examples I am aware of: 20260111s49 (05:53 a.m. UT, pointing scan), 20260111s24 (02:53 a.m. UT, focus). Note that the QL does not process big scans (e.g., beam maps or long polarimetry scans), therefore there might be (many) more scans affected by this issue. We don't know what is the cause of this behavior. It does not seem to be related to the sky conditions, because on 20260112 the sky was great, but during the night of 20260111 it was less good. Magnetic fields induced by the telescope motors? Problems in the tuning at the start of the scan? Satellites? Geomagnetic storm due to solar activity? Cosmic rays? Other ideas? -- EMIR Local oscillators ? <CK> SB: Frederic says it's a good idea but they're off since the XPOL session.

@12:00 UT checks in the cabin by SB: a) there is no active WiFi; b) one of the two ladders on top of the NIKA2 cryostat (the one closer to the mirrors and to the NIKA2 window) was touching the cryostat. I moved it enough to allow a 5-7-10 cm gap.

On 2026/01/13 Alessandro suggested that it looks like tuning during the scans. SB notes that this is not a feature of the NIKA2 DAQ, unless someone modified or intervened remotely while we were observing.

On 2026/01/13 also Xavier and Nicolas have quickly analysed the data: their conclusion is that the problem was caused by vibrations. I copy here their message: "Our conclusions are that all electronic boxes are affected. There are no unwanted tuning during the scan except at the beginning as expected. Looking at individual detector raw data: for some Kids, they look perfect. For some others, it is terrible: see in the I,Q plane the large deviations from the circle. This is not possible with photons. Therefore, vibrations are the main culprits. Some kids are more sensitive than others to that. The vibrations are stronger at the beginning of the scan for this scan. We let Alessandro and Martino say whether the PT heads can be guilty or not, otherwise something is shaking the cryostat. The end result is that up to half the kids will be killed in the processing."

SB: Thank you all for your ideas and analysis! Could the culprit really have been the ladder touching the cryostat? Why did it affect only few (random) scans?

09:00-15:00 UT Beth

15:00-21:00 UT Michael and Beth

Last evening of this pool week

21:00-03:00 UT Tuan-Anh

03:00-09:00 UT Remi

Thank you all for your presence at the telescope, the support in the observations and the wonderful time together during this past week. See you next Time. Stefano.

DailyReportsNika2Pool060126 (last edited 2026-01-13 18:32:20 by NikaBolometer)