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Contents
NIKA2 Re-Commissioning: NIKA2 run 80, Cryo run 92
Observers on-site: Miren Muñoz, Mairi Nonhebel, Kaiyi Du, Stefano Berta, Ioannis Myserlis (remote), Angel Bongiovanni
Operators: Mario Cervera (day), Sergio Amaya (night)
Organization of shifts:
22:00-04:00 LT:
04:00-10:00 LT:
10:00:16:00 LT:
16:00-22:00 LT:
Initialization files:
run91*.ini (previous sweep)
run92*.ini (new sweep)
Tables (from 2026/03/24 ~15:00 LT to 2025/03/31 ~10:30:00 LT)
Focus sequences
Scan nr
Target
Ar2
Ar1
Ar3
Polarized?
Notes
20260324s153-157
Uranus
0.27
1.25
n/a
no
Started at 1.0 mm; tadadada; Ar3 not available for now because of new sweep; Ar2 good fit; Ar1 fit is marginal
158-162
Uranus
out
1.3
n/a
no
Started at 1.5 mm; Ar1 perfect fit; Ar2 out of range
163-167
Uranus
0.28
out
n/a
no
Started at 0.5 mm; Ar2 perfect fit; Ar1 out of range
171-175
Uranus
n/a
no
started at 1.5 mm;
Beam maps (99 sub-scans)
Scan Nr
Target
Focus
Notes
Polarization beam maps (95 sub-scans)
Scan Nr
Target
Focus
Notes
Calibrators (calib_1scan)
Scan Nr
Target
Focus
Notes
Preliminary plan
We wish to do the following:
- OK start in total power: point, focus (!), point
- OK analyze focus difference between Ar1 and Ar2
calib_1scan, beam maps (at least 2)
analyze beam maps and produce DAFs RPPs for the new Ar3. Install the new RPPs for Ar3
analyze the focus difference between Ar1 and Ar3
- perform many focus sequences to have some statistics
- polarimetry beam maps
- more total power beam maps
- out of focus total power beam maps
total power deep field (HLS 091828), to derive the new, final NEFD of NIKA2 TP
polarimetry deep field (3C286, M87, 3C353, ...?) to derive the new IQU NEFD of NIKA2-Pol
- 084-25 polarimetry
- 140-25, 146-25 polarimetry
- 196-25 total power
- test long subscans with our favorite, total power, 100 arcsec/s
- C/2025 R3 Panstarrs, polarimetry
- deep field 03h32m31.75s −27d46m51.5s, total power, 14x14 arcmin2, 100 arcsec/s
- test Sgr A* polarimetry scan strategy
- ... other wishes ...
Tuesday, 24th March 2026
The team arrives safely to the observatory
we are all thrilled and super excited to test and use the new NIKA2++!
During maintenance, the new make-imbf is transformed into the default one. From now on we will use only the new make-imbf and the old one will be kept inactive. We verify that the directory where the make-imbf wrote is now the "production" directory and that users can read its content. We also run the PIIC QL manually on a couple of old scans, of which William newly produces the files using the new make-imbf and writing them here. The QL reads and processes these scans regurlarly. Well done!
We take over after maintenance at 14:45 UT. All is ready. We start with total power (TP). And we stop at scan nr zero, because we are in the clouds and the humidity is at 100%. The rain alarm rings loud!
Progress of the day:
- @17:45 UT we start!!! Total power, KIDs lost 17/8/14 (Ar3 without counting Box S)
- Uranus... the moment of reckoning... pointing... both Ar2 and Ar1 are out of focus, which is promising! ... focus ... the difference between Ar2 and Ar1 tonight is 1.0 mm.
