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Daily Reports (2025/10/21-28, NIKA2 run 75, Cryo run 87)

Observers on-site: Monica Rodriguez, Samuel Leclercq, Raphaël Maris, Stefano Berta and Stergios Amarantidis (AoD).

Operators: Sergio and Mario.

Shifts: 10-16 Raphaël; 16-22 Samuel; 22-4 Stefano; 4-10 Monica.

All times reported are in UTC (if not mentioned otherwise).

Preparatory notes

Please, remember to use the focus value of Ar1 (roughly Ar2 + 0.65 mm, but use directly the focus Ar1 monitor if possible). Please use the custom modified focus script focusOTF-Z_2025.pako.

Therefore, importantly, when checking the quality of the beam on a pointing map to decide if a new focus is needed, it is better to do it on the Ar1 map, because that's the one focused at best.

Project D01-25 (M51) requires DAQ restarting with the run87_newSweep_M51_tp.ini file. Come back to run87_neSweep_tp.ini after observing this project.

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 are taken:

October 21st, 2025, Tuesday

15:00-22:00 [All]: Maintenance finished with no issues. DAQ started at 14:10 with 21/3/47 bad KIDS for arrays 1,2 and 3, respectively. Repeating the DAQ at 14:24 with 28/3/89. Trying to point at NGC7027 and MWC349 but the weather is too unstable (p2p~10-20Jy/beam), moving to K3-50A for pointing and focus (using the modified 2025 script). Moving for calib_1scan to MWC349, etc. Switching to project 053-25 (source 1803+784 is better for pointing/focus). One repetition of L1157B. Around 17:12 we moved to a skydip and then to the normal flux calibrators. After pointing/focus on 1803+784 we move to project 022-25. Two repetitions of Ceph-4.

22:00-04:00 [Stefano]: here follows the evolution of the night:

October 22nd, 2025, Wednesday

04:00-10:00 [Monica]: Pointing, Focus and calib_1 scan in Uranus. Then project 066-25 (Source M31_inner) for 1 hr (1 round), weather started to became very unstable in the last scan peak to peak variations > 50 Jy/beam (Ar2). Then pointing and focus in Uranus, then the opacity rise to 1.0, so we stopped ~ 50 minutes. Continue with pointing, focus, pointing and calib_1scan in Uranus and Alfori. Then observe project 082-25 (Source PSz2G107) 2 rounds (~ 2hr).

10:00-16:00 [Raphaël]: Pointing Focus on f source 1418+546. Then observe project 082-25 (Source PSZ2G107) 2 rounds (2 hr). Making Skydip. Starting D01-M51 source. Changed to 47 Hz sampling rate: 15/4/37 lost KIDs. Nothing so bright around our science target so we move to 1633+382 to focus. Then back to 1418+546 and then to the science target (observed 6 repetitions of M51).
- @11:15 UT, Jean fixes a problem in the make-imbf. Yesterday the new make-imbf did not produce the imbf files of scan 20251021s171. we ran it manually, but the result was flawed. Jean fixed the manual version of the new make-imbf, that was looking for the Antenna traces in the wrong location. Thank you! The initial issue (that the automatic version did not produce the s171 files) is under investigation.

16:00-22:00 [Samuel]: Tau values have increased above the threshold of the project D01-M51 (0.4) thus we move to calib_1scan observations with the higher sampling rate of project D01-25 and monitor the weather. Pointing on MWC349 with p2p~10Jy/b, repeating + focus. Weather seems to go better in fact: calib_1scan on MWC349 gives now p2p ~ +-5Jy/b and tau=0.37... same for CRL2688 and for NGC7027 --> weather stabilized below D01-25 limits, so we iterate more on it after all. Alas, the time to point on nearby point source and run the script weather evolved just above limits. Switch back to 23 Hz acquisition. After reloading frequencies and tune: bad pix = 30/5/123 for Arr 1/2/3. Lots of lost kid on Arr3 probably due to relatively high sky fluctuations now. But conditions still good enough for project 053-25, though with a little doubt regarding the stability, p2p still < +-10 Jy/b in pointing scans preceding the series of scans on L1157.
- Below, screenshot showing the difference of response to sky fluctuation between Arr1 and Arr3: Arr3 gets x3 higher p2p response than Arr1 besides identical calibrated value for the source! (see today's regular NIKA2 meeting for the discussion about this topic).
Hello!

22:00-04:00 [Stefano]: ...

October 23rd, 2025, Thursday

04:00-10:00 [Monica]: ...

10:00-16:00 [Raphaël]: ...

16:00-22:00 [Samuel]: ...

22:00-04:00 [Stefano]: ...

October 24th, 2025, Friday

04:00-10:00 [Monica]: ...

10:00-16:00 [Raphaël]: ...

16:00-22:00 [Samuel]: ...

22:00-04:00 [Stefano]: ...

October 25th, 2025, Saturday

04:00-10:00 [Stergios]: ...

10:00-16:00 [Raphaël]: ...

16:00-22:00 [Samuel]: ...

22:00-04:00 [Stefano]: ...

October 26th, 2025, Sunday

04:00-10:00 [Stergios]: ...

10:00-16:00 [Raphaël]: ...

16:00-22:00 [Samuel]: ...

22:00-04:00 [Stefano]: ...

October 27th, 2025, Monday

04:00-10:00 [Stergios]: ...

10:00-16:00 [Raphaël]: ...

16:00-22:00 [Samuel]: ...

22:00-04:00 [Stefano]: ...

October 28th, 2025, Tuesday

04:00-10:30 [Stergios]: ...