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1) one repetition of source G75.78 for project 043-24.<<BR>> 2) pointing, focus, pointing, beammap (95 sub-scans, 20241105s111), calib_1scan (20241105s112) on Uranus.<<BR>> |
- one repetition of source G75.78 for project 043-24.<<BR>> - pointing, focus, pointing, beammap (95 sub-scans, 20241105s111), calib_1scan (20241105s112) on Uranus.<<BR>> |
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3) calib_1scan (20241105s114) and beammap (99 sub-scans, 20241105s115) on Uranus in total power<<BR>> 4) skydip (20241105s116)<<BR>> 5) 011-24, orion-b-4 (w/ homology problems); orion-b-5; orion-b-6 (w/ other problems); one repetition each. |
- calib_1scan (20241105s114) and beammap (99 sub-scans, 20241105s115) on Uranus in total power<<BR>> - skydip (20241105s116)<<BR>> - 011-24, orion-b-4 (w/ homology problems); orion-b-5; orion-b-6 (w/ other problems); one repetition each. |
Daily Reports
Nov 5th, Tuesday
Rémi, Léo, Simon, Ste B., Léa, Ioannis and maaaaaany others arrived at the observatory.
We start the week in the best possible way...
15:30 - 17:00; Ioannis: System check.
17:00 - 21:00; Rémi, Léo, Simon, Stefano, Lea & Ioannis: NIKA2 training + observations. Note that scans 20241105s57 to 20241105s69 that we did during the training were done with the polarization .ini file, where the DAQ frequency is 46.12 Hz but the HWP was stopped. Starting from scan 20241105s70, the HWP is also in use properly. After training we did polarimetry observations: one repetition of project 043-24, source G75.78.
21:00 - 03:00. Léa & Stefano. We take over and continue with polarimetry:
- one repetition of source G75.78 for project 043-24.
- pointing, focus, pointing, beammap (95 sub-scans, 20241105s111), calib_1scan (20241105s112) on Uranus.
Then we switch to total power and we proceed with:
- calib_1scan (20241105s114) and beammap (99 sub-scans, 20241105s115) on Uranus in total power
- skydip (20241105s116)
- 011-24, orion-b-4 (w/ homology problems); orion-b-5; orion-b-6 (w/ other problems); one repetition each.
Nov 6th, Wednesday
03:00 - 09:00; Rémi: NIKA2 observations continue in total power with good weather conditions, tau225 ~ 0.2-0.3.
- pointing, focus and calib_1scan (20241106s18) on Uranus.
- 1.5 repetitions of source A520 for project 089-24.
- pointing and calib_1scan (20241106s31) on Mars.
- skydip (20241106s33)
- very good beam size on bright pointing targets (17.5x17.5" for Ar2)
- 3 repetitions of source PSZG201 for project 091-24.
- 1 repetition of source PSZG186 for project 090-24.
09:00 - 13:45; Léo: NIKA2 observations continue in total power with good weather conditions, tau225 ~ 0.3.
13:45 - ...; Ioannis: Change to EMIR. WSw tests with EMIR after OHB intervention to solve the blanking signal phases problem.