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Run80 data processing

Contributions by: Stefano Berta, Kaiyi Du.

Here we include the preliminary data reduction results of the re-commissioning NIKA2 run 80, as obtained at the telescope during this week (2026/03/24-31).

Focus difference between the three arrays

As of 2026/03/25 @01:25 UT.
The focus difference Ar1-Ar2 is roughly +1.00 mm.
The focus difference Ar3-Ar1 is roughly -0.05 mm.

Ar2 focus, scans 153-157 Ar1 focus, scans 153-157 Ar3 focus, scans 153-157

Ar2 focus, scans 163-167 Ar1 focus, scans 158-162 Ar3 focus, scans 158-162

Ar1 focus, scans 206-210 Ar3 focus, scans 206-210

Beam maps analysis

We have a new Ar3 and we need to characterize its geometry and its flat field. To this aim, on 2026/03/24 we took two beam maps focused on Ar1 (scans 20260324s169 and 177). The idea and hope is that the focus of Ar3 is roughly the same of that of Ar1, thanks to the March 10 intervention, and these beam maps will be good for our purpose.

We reduce the beam maps during the night between 2026/03/24 and 25.
Ar2 is out of focus and in order to be able to reduce it, we need to relax completely the constraints on its beam size and shape.
Ar1 is well on focus. The best beam map is 177. The other (169) has some problems at the lower edge for unknown reasons.
The Ar3 focus is decent. The array is missing Box S, as already known, and also several KIDs in Boxes M, N O (supposedly).

Below here you can see the geometry of the three Arrays as derived from the average of these two beam maps.

Ar2 beam maps 169 and 177 Ar1 beam maps 169 and 177 Ar3 beam maps 169 and 177

Study of the Ar1 and Ar2 beams at different focus values

On 2026/03/25, we carried out a series of calib_1scan with different focus values, starting from the Ar1 optimal focus to the Ar2 optimal focus, in steps of 0.2 mm. The aim was to study the change of MB flux (because the CAL is based on main beams), % of flux in the side lobes of the beam, and FWHM of the minor/major axes of the beam, as a function of focus (distance from the optimal position). Below here you find a table that summarizes our measurements and a series of plots produced by the PIIC monitors for Ar1 and Ar2.

Note, however that polarimetry observations would at best be carried out at the Ar1+3 optimal focus (rather than at a compromise focus) because of the criticality of the IP correction.

Studying this table, we have the suspicion that we need to perform a new lateral focus (XY). We are considering to postpone it to Sep-Oct, after a possible new NIKA2 hardware intervention.

Beam analysis, scan 243, Ar1 Beam analysis, scan 243, Ar2

Beam analysis, scan 245, Ar1 Beam analysis, scan 245, Ar2

Beam analysis, scan 247, Ar1 Beam analysis, scan 247, Ar2

Beam analysis, scan 249, Ar1 Beam analysis, scan 249, Ar2

Beam analysis, scan 251, Ar1 Beam analysis, scan 251, Ar2

Beam analysis, scan 253, Ar1 Beam analysis, scan 253, Ar2

New Study of the Ar1, Ar3 and Ar2 beams at different Z focus values

2026/03/28-29 Following the request by Carsten, we repeat the experiment. Carsten noted that the best Ar2 beam is not at the best Ar2 focus, but a bit far from it. Several factors might be causing this:

Check the table below: the Ar1 and Ar3 MB fluxes increase when they should be decreasing! Are we seeing the QSO that is bursting? Or is it the wind? Or the change of Elevation (I hope not!)

Third (and last attempt to study of the Ar1, Ar3 and Ar2 beams at different Z focus values

2026/03/30 I try again. The wind has decreased significantly. This time I use 3C273 (much more stable than 3C279). I do it close to culmination, such that the change of Elevation is minimized. I also monitor the P100 information, i.e. the behaviour of the main dish / back structure temperature sensors. In fact, it is known that these sensors suffer humidity and condensation of the water that accumulates into the back structure. When they "get wet", the temperature difference in the back structure has some peaks and the temperature compensation of the focus goes bananas.

The procedure is as in the two previous attempts:

Test of focus difference between the three arrays after cryostat total warm-up and cool-down cycle (April 24, 2026)

AoD: Ioannis

Outline of test slot T21-25:

As of 2026/04/25 @22:00 UT.
The focus difference Ar1-Ar2 is roughly +1.20 mm.
The focus difference Ar3-Ar1 is roughly -0.05 mm.

Ar2 focus, scans 56-60 Ar1 focus, scans 61-65 Ar3 focus, scans 61-65

Ar2 DAQ traces Ar1 DAQ traces Ar3 DAQ traces

Testing focus difference between the arrays: May 19, 2026

Ar2 DAQ traces, closed Ar1 DAQ traces, closed Ar3 DAQ traces, closed

Ar2 DAQ traces, open Ar1 DAQ traces, open Ar3 DAQ traces, open

Ar2 focus, scans 244-248 Ar1 focus, scans 239-243 Ar3 focus, scans 239-243

Ar2 focus, scans 255-259 Ar1 focus, scans 250-254 Ar3 focus, scans 250-254

Testing focus difference between the arrays: May 20, 2026

Ar2 focus, scans 196-200 Ar1 focus, scans 201-205 Ar3 focus, scans 201-205

Ar2 focus, scans 206-210 Ar1 focus, scans 211-215 Ar3 focus, scans 211-215

Testing focus difference between the arrays: May 21, 2026

Ar2 DAQ traces, closed Ar1 DAQ traces, closed Ar3 DAQ traces, closed

Ar2 DAQ traces, open Ar1 DAQ traces, open Ar3 DAQ traces, open

Ar2 focus, scans 306-310 Ar1 focus, scans 306-310 Ar3 focus, scans 306-310

Ar2 focus, scans 316-320 Ar1 focus, scans 311-315 Ar3 focus, scans 311-315

Cross-talking of Ar3

2026/05 Kaiyi started the cross-talk analysis of run 80. It seems that the new Ar3 has quite a number of cross-talking KIDs. Here follows an example of 42 KIDs, showing that several are affected (at least 16/42 in this case). The analysis is ongoing and the list of cross-talking KIDs will be updated in the PIIC DAFs as soon as we have converged on the final identification.

New Ar3 cross-talk analysis New Ar3 cross-talk analysis

Testing focus difference between the arrays: June 5, 2026

Testing focus difference between the arrays: June 9, 2026

Ar2 DAQ traces, closed Ar1 DAQ traces, closed Ar3 DAQ traces, closed

Ar2 DAQ traces, open Ar1 DAQ traces, open Ar3 DAQ traces, open

Testing focus difference between the arrays: July 8, 2026

Ar2 focus, scans 284-288 Ar1 focus, scans 279-283 Ar3 focus, scans 279-283

Ar2 noise traces, window closed Ar1 noise traces, window closed Ar3 noise traces, window closed

Ar2 noise traces, window open Ar1 noise traces, window open Ar3 noise traces, window open

Testing focus difference between the arrays: July 9, 2026

Ar2 focus, scans 292-296 Ar1 focus, scans 287-291 Ar3 focus, scans 287-291

Ar2 noise traces, window closed Ar1 noise traces, window closed Ar3 noise traces, window closed

Ar2 noise traces, window open Ar1 noise traces, window open Ar3 noise traces, window open

Testing focus difference between the arrays: July 28, 2026

* First focus tests after the NIKA2 DAQ problem.

* Starting at 16h30 LT, under very poor weather conditions. Opacity ~ 1 (~ 0.8 towards the end of the session). However, not very unstable: +/- 5 to 7 Jy/beam peak-to-peak at 2 mm.

* Low wind (~ 2.5 m/s); ambient temperature ~ 20 C.

* 3C279: El. ~ 45 deg; 3C273: El. ~ 50 deg.

* Given the very high opacity, today's focus tests should be taken with a pinch of salt. Note also the large number of bad KIDs.

* Bad KIDs Ar1/Ar2/Ar3: 74/8/154

* We try to recover more KIDs with a new tuning. Bad KIDs Ar1/Ar2/Ar3: 71/9/38.

* Focus offsets: Ar1-Ar2 = 1.16 mm, Ar3-Ar1 = -0.07 mm.

* Window open and low wind speed (~2.5 m/s), tau_225GHz ~ 1. Noise traces:

Ar1 noise traces, window open Ar2 noise traces, window open Ar3 noise traces, window open

Testing focus difference between the arrays: July 29, 2026

* Starting at 15 LT, under very poor weather conditions. Opacity ~ 1 most of the time, but ~ 0.6 towards the end of the session. Ambient temperature 19.9 C.

* Again: given the very high opacity, today's focus tests should be taken with a pinch of salt. Note also the large number of bad KIDs when NIKA2 window is open (tried retuning several times, but getting always similar results).

* Not able to get a calib_1scan on Mars (bad pointing and focus + low elevation) and similar situation at the end of the session on MWC349.

* Checking noise traces.

NIKA2 windows closed, vertex closed, mirrors pointing EMIR. Antenna at 70 deg in elevation. DAQ started at 15h16LT. Bad KIDS Ar1/Ar2/Ar3: 15/4/8.

Ar1 noise traces, window open Ar2 noise traces, window open Ar3 noise traces, window open

NIKA2 windows open, vertex open. Antenna at 70 deg in elevation. DAQ started at 16LT. Bad KIDS Ar1/Ar2/Ar3: 53/13/27.

Ar1 noise traces, window open Ar2 noise traces, window open Ar3 noise traces, window open

* Stopped for an hour waiting for the weather to improve and resumed observations at 18 LT. Bad KIDs Ar1/Ar2/Ar3: 56/8/30.

* Focus offsets: Ar1-Ar2 = 1.16 mm, Ar3-Ar1 = -0.04 mm.

Testing focus difference between the arrays: July 30, 2026

* Starting with opacity ~ 0.8 and finishing with opacity ~ 0.5.

* Wind ~ 3 m/s; ambient temperature 19 C.

* Checking noise traces.

NIKA2 windows closed, vertex closed, mirrors pointing EMIR. Antenna at 70 deg in elevation. DAQ started at 15h08 LT. Bad KIDS Ar1/Ar2/Ar3: 24/6/9.

Ar1 noise traces, window open Ar2 noise traces, window open Ar3 noise traces, window open

NIKA2 windows open, vertex open. Antenna at 70 deg in elevation. DAQ started at 15h30 LT. Bad KIDS Ar1/Ar2/Ar3: 34/10/20.

Ar1 noise traces, window open Ar2 noise traces, window open Ar3 noise traces, window open

* Two calib_1scan on Mars (20260730s202 and 20260730s203), under pretty bad conditions; with focus correction from Ar1 and pointing correction from Ar2.

* Finished the slot with a few test scans for the NIKA2 high-frequency noise analysis, but only for the 60”/sec version, but only checking the vertex status (open/closed). Test scan range: 20260730s257 and 20260730s265.

* Focus offsets: Ar1-Ar2 = 1.28 mm, Ar3-Ar1 = -0.06 mm.

Testing focus difference between the arrays: July 31, 2026

* Opacity at the beginning: ~0.7; increasing up to ~1 at the end of the shift along with atmosphere instabilities. Peak-to-peak variations of the timelines > 10 Jy/beam (2 mm).

* Max. wind speed between 6 and 9 m/s; ambient temperature up to 21C. Enhanced 2mm-beam shape: 20.2" x 20.9" from a pointing scan after the first best focus on Ar2.

Ar2 focus, scans 195-199 Ar1 focus, scans 190-194 Ar3 focus, scans 190-194

Ar2 focus, scans 212-216 Ar1 focus, scans 217-221 Ar3 focus, scans 217-221

* After the last focus correction, a series of scans on Arp220 for testing high-frequency noise was launched: (i) on-sky (opacity/instabilities increased substantially in the middle): scans 20260731s231-233 (120 arcsec/s), s234-236 (60 arcsec/s) and (ii) window closed: scans s237-239 (120 arcsec/s), s240-242 (60 arcsec/s). Scans with vertex closed + window open omitted by mistake (AB). Scans s243-248 should not be used.

* Checking noise traces:

NIKA2 window closed, vertex close, mirrors pointing EMIR. Antenna at 70 deg in elevation. DAQ started at 15:05 LT. Bad KIDS Ar1/Ar2/Ar3: 13/6/11.

Ar2 noise traces, window open Ar1 noise traces, window open Ar3 noise traces, window open

NIKA2 window open, vertex open. Antenna at 70 deg in elevation. DAQ re-started at ~15:50 LT. Bad KIDS Ar1/Ar2/Ar3: 49/9/25.

Ar2 noise traces, window open Ar1 noise traces, window open Ar3 noise traces, window open

Testing focus difference between the arrays: August 4, 2026

Ar2 focus, scans 187-191 Ar1 focus, scans 192-196 Ar3 focus, scans 192-196

/!\ /!\ DRAFT TEXT BELOW, TO BE EDITED LATER /!\ /!\

NIKA2 test time: August 5, 2026

Ar2 focus, scans 187-191 Ar1 focus, scans 192-196 Ar3 focus, scans 192-196

Summary of focus offset tests (mean values) - Run 80

Please update this table after a new session and keep it at the bottom of the page. FWHM-only individual focus corrections were not taken into account: