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January 22nd, Monday
We take the telescope at 14:50 UT. It was pointing very close to the Sun for a while, because of Sun avoidance tests, therefore it will take at least 2h before it relaxes. Nevertheless, we lauch several scans to study how the tracking behaves.
NIKA2 is tuned. The PIIC monitor tells us that the the data of the pointing pixel (Ar2) are corrupted. We tune again (lost KIDs: 58, 8, 68), but we don;'t recover the pointing pixel.
We study the tracking. Lots of overshooting at the turns between subscans.
Experiments with Uranus (starting at 30 deg elevation):
pointing scans (20240122s135 to 138)
standard OTF (139)
OTF with tTune changed from 3 to 5 seconds (140)
OTF with no zig zag (141)
When scanning only in Azimuth, the overshoot follows a repeating pattern.
Without zigzag we avoid the big positive overshoot.
The temperature inside NIKA2 oscillates by 0.2 mK (0.1 mK amplitude) every ~7 minutes.
Dave reduces the pressure of the pump. We wait a bit for a new equilibrium.
Note that the EMIR pointing model is installed. We have no updated NIKA2 pointing model. We should make a pointing session, as soon as the telescope relaxes. For now we apply the big offsets given by the PIIC monitor (-16 arcsec, -54 arcsec) and the pointing pixel is recovered. Pointing scans: 142 to 144. We now focus properly (16 UT forward).
Then we test different scan speeds, to study the tracking, on Uranus, 12x3 arcmin scans (Equatorial), step 30 arcsec, 0 and 90 deg direction (Eq). Scan speeds 20, 40, 60, ...
Summary (Uranus):
20240122s134 track
20240122s135 to 138 pointing
20240122s139 OTF
140 OTF tTune 5 instead of 3
141 OTF no zigzag
142-144 pointing
145-154 two focus sequences 155 pointing -> 2mm beam ~18,7x19.5 arcsec (best we can do at the moment); but 1mm beam still terrible
156-157 OTF 20 arcsec/s
158-159 OTF 40 arcsec/s
160-161 OTF 60 arcsec/s