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NIKA2 Re-Commissioning (2nd. part)

June 10th-12th + 16th-18th, 2025

NIKA2 run 73
Cryo run 85

Infos about the PIIC DAFs for the PIIC monitor

SB has produced some temporary DAFs to be used for run 73 Ar2. They are already copied at Pico.

The idea is to use two different sets of DAFs for Ar1+3 and for Ar2:

• for Ar1 and Ar3, use the DAFs that were produced with the run 72 data. These DAFs work with the new Arrays 1 and 3, but their reference KID is not the central one (because of the bix C issue), and therefore they's a bit of an offset.
• for Ar2, use the older DAFs (run 68). The SWEEP has not changed since then. These DAFs do include the correct (central) reference KID. Use these for pointing, such that the data will all be properly centered.

I cannot mix the two sets of DAFs, because Ar1 and Ar3 use Ar2 as reference and were built with the non-centra reference KID.

As soon as we have beam maps, I will build (temporary) DAFs for all three arrays, referred to the central KID, and we'll be fine.

Ho to proceed in practice:

• Ar2
  • open a terminal, go to the QL directory
  • gagpiic
  • export MOPSIC_DAFS=/local/users/flexible/reduce/dafs_bck/dafs_local_tmp_run73_ar2
  • start the Ar2 monitor (pf)
  • repeat in another terminal for the Ar2 monitor (m)
• Ar1 and Ar3
  • open a new terminal, go to the QL directory
  • gagpiic

  • echo $MOPSIC_DAFS -> check that it says /sw/gildas/mopsic/dafs

  • if not, then set it to that directory
  • proceed normally with the Ar1 and Ar3 monitors
• if Ar2 does not work, please let SB know, and meanwhile use the standard DAFs (i.e. the same as for Ar1 and Ar3)

At this point, use Ar2 for pointing, such that all data are well centered. As soon as there's a decent beam map available, SB will produce new (maybe temporary) DAFs for all three Arrays, referred to the good old (central) reference KID and will install them at Pico, to be used with the next observations.

Tuesday, June 10th, 2025

Mónica, Ioannis, Dave, Angel at the telescope. Starting DAQ at the beginning of the maintenance slot.

11:00: All amplifiers are switched on. T_MC = 0.173 K. Noise traces at this time (ar2, ar1, ar3) are given below.

Traces of ar2 look qualitatively better than those in force during the campaign of March (for a comparison, see the Daily Report of Sunday, March 23rd, 2025 at https://publicwiki.iram.es/DailyReportsNika2Run72).

15:30: Dave, Mónica, Angel. Cloudy. Rain intervals. Trying to catch a sky hole for a decent resonance work. Configuring NIKA2 at Rx cabin. Restarting DAQ. Impossible to have a reasonably good tuning with the current weather conditions. Waiting for a while.

17:00: Still being unstable. Taking advantage for testing mppsync/server & HWP. It was necessary to restart the Arduino server. Check: OK.

18:30: We tried our best for getting good resonances under (very) poor conditions. With 17/6/110 bad KIDS in a1/a2/a3, we tried a quick & dirty (specially the latter) pointing on Mars when wind speed dropped a bit. The good news: the QL-reduction indicates that the amplifier replacement has been successful. Congratulations!:

20:28 Weather still unstable. We did a pointing and see a big offset between a2 and a1/a3 so we changed to the latest DAF's for all arrays. After that there is not offset anymore. We continued with pointing and focus.

21:00 Stopped. light rain.

SB @22:55 LT: the offset between Ar2 (special DAFS, run 68, see above) and Ar13 (run 72 DAFs) is normal because the Ar2 are referred to the central KID while the Ar13 are not. So basically this offset is on purpose. It will disappear once I produce the new DAFs with new beam maps. Please keep using the run 68 DAFs for Ar2 (special instructions above), so that all data are referred to the central KID and I can produce the new DAFs for Ar13 with the proper reference KID. Thanks.