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December 8, (Thursday)
The cryostat recovery operation by AM MC AB seems to have worked, and we foreseen to reach base temperature in the early afternoon. Carsten agreed to give back to NIKA2 a bit of the time we let to EMIR last night by allowing us to start as soon as the cryostat cold.
The cryostat still show a non optimal behaviour. Nothing too serious hopefully. We added some 4He gas in the dilution mixture, to improve the cooling and calm down the strange temperature behaviours.
The plan for today once we have the telescope and till tomorrow morning is:
- Check the alignment of the pupil.
- Adjust mirrors and cryostat position to have the best alignment. Use possibly the laser of the telescope, removing the M3 mirror.
- Optimize detectors parameters if needed.
- Go on a strong source to do pointing-focus, then a series of few pointings to check the offsets.
- Install the external calibrator and characterize it, by doing several types of scans (pointing, focus, beam maps).
- Find the best XYZ focus.
- Make a pointing session.
- Do beam maps.
- Auxiliary but important scans: dark test, skydip, to be inserted anywhere between items 3 and 8.
December 7, (Wednesday)
Alain fixed a few issues during the night. I'll let him explain in details, I think he already did it by emails to the relevant people. He also performed an alignment test by moving a sheet of ecosorb in front of the entrance window and found that there indeed was a problem of alignment. by a few millimeters. This will probably be the first thing we address this afternoon when we take the antenna.
Short summary of Alain's mail about the events of the night (Tuesday to Wednesday):
Cryostat cooling too slow: we miss He mixture, this can be deduced from the fact that the still got liquid when the pressure dropped below 2 bars.
NIKEL boards didn't accept to do tuning while the external calibrator is running. → We found out latter during the day that it was due to a "funnel" in the network structure: the 3 crates were plugged to a small switch with a too low bit rate, plugging them directly on the big switch which has the optical link to the computer room solved the issue.
One of the 3 crates crashed, only a power reboot allowed to recover it.
The new synthesizer for the 2mm band showed the same problems as the previous one. → It turned out that the problem was not the synthesizer but the board which allow controlling it.
Quick test on the pupil at the entrance of the cryostat show indication of a misalignment. To be repeated more properly next day.
Around 16h the cryostat had a new blockage, most probably a follow up from the blockage wee had the day before: the dirt that did the 1st blockage must have migrated a bit and blocked again the circuitry yesterday. Alessandro, Martino, and Alain warmed up and cooled down again the cryostat in a special way to trap the dirt in a harmless section of the circuitry.
We had a number of other events. In particular a loss of network that nearly killed the run, because it put the "automate" (electronic box which contain the devices controlling the cryostat) in a wrong state with bad consequences on the cooling. Hopefully we recovered from this. More info probably a bit latter.
December 6, (Tuesday)
Alain, Johannes, Nicolas, Frédéric, Jean-François, Andrew, and Samuel arrived at the telescope.
Alain, Johannes Samuel with the help of Dave and Gregorio spent most of the day in the cabin, installing and testing the new external calibrator. Installation on a horizontal bar fixed in the vertex cabin (between M2 and M3 after passing the M1 vertex). We tested it using the EMIR receiver, plugged on a spectrum analyser. After solving some minor problem it worked. We also changed the synthesizer of the 2mm band (a new generation with an option that caused us some trouble in the previous run) with an older one that Alain brought in his baggages. Nico worked on the Pipeline. Alessandro and Martino took care of the cryostat remotely (need to warm up a bit to take care of a blockage in the dilution unit, then cool down again). We foresee to reach the base temperature near 2am. In the mean time we make a better characterization of the calibrator using the EMIR receiver with its FTS backend: we take the spectra for each of the line emitted by the calibrator (139.5 GHz, 155 GHz, 170.5 GHz, etc.).
