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- Use the upgraded PIMP to characterize in situ NIKA2 instrumental band passes, with possible dependence on polarization angle. |
NIKA2 technical run 32 / 17-24 September 2019
Back to the NIKA2 Run 32 main page
Goals
- Continue commissioning of the new acquisition software (DAQ v3), after June's fix on tuning and few other "minor" things.
- New sweep to define new tones comb parameter (closed window + open on good sky if possible).
- Use the external calibrator: tests scans on/off, then rest of the run on (if no deterioration of data: from now on always use it).
- Continue polarization commissioning (help of calibrator for leakage and so on / synchronization / calibration).
- Scans - mainly beam maps - in total power & polar to acquire statistics for DAQ v3 commissioning.
- Use the upgraded PIMP to characterize in situ NIKA2 instrumental band passes, with possible dependence on polarization angle.
- Possible tests on tuning parameters.
Observers and Schedule
All the people who will participate to the pool run must appear in the table below; each one must inform Samuel and contact Laura to reserve rooms in Granada and at the telescope. For those who travel on IRAM funds, contact Samuel; see also the NIKA2 travel rules.
Staff of the run in September 2019: table of the nights spent at the observatory for the NIKA2 collaboration members participating to the run (T = Tuesday, S = Saturday, 1 = night scheduled at the telescope, g = night in Granada office).
People\Date |
13 |
14 |
15 |
16 |
T17 |
18 |
19 |
20 |
21 |
22 |
23 |
T24 |
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Samuel Leclercq |
0 |
0 |
0 |
g |
1 |
1 |
1 |
1 |
1 |
1 |
1 |
0 |
People |
0 |
0 |
0 |
0 |
|
|
|
|
|
|
|
0 |
Rooms at obs. |
0 |
0 |
0 |
0 |
|
|
|
|
|
|
|
0 |
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Alessia Ritacco |
|
|
|
|
1 |
1 |
|
|
|
|
|
0 |
(*) For the rooms, count persons from the NIKA collaboration and Grenoble, but not from IRAM Granada.
IRAM's http://www.iram.es/IRAMES/mainWiki/AstronomersOnDutySchedule.