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| * If beam maps statistics sufficient: test deep integration. * If beam maps statistics sufficient: map extended features, and at least 1 showcase. * If beam maps statistics sufficient: start polarization commissioning. |
* In parallel to beam maps, test deep integration on well known sources: the goal should be to show reproducibility in reaching the rms expected after one hour of integration. * If beam maps statistics sufficient: map extended features (already done with complex secondary calibrators), and at least 1 showcase : can be a nearby galaxy NGC 3938 or NGC6946 (left/right 10 arcmin diameter circle) J2000 coordinates for NGC6946 are: 20:34:52.3 +60:09:14 {{attachment:NGC6946FaceOns.png||height=370}}. * If beam maps statistics sufficient: start polarization commissioning [that should be postponed to next run]. |
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| ||<rowbgcolor="#ddccff"> N. Ponthieu || g || 1 || 1 || 1 || 1 || 1 || 1 || g || || ||<rowbgcolor="#ddccff"> F. Mayet || g || 1 || 1 || 1 || 1 || 1 || 1 || 1 || || ||<rowbgcolor="#ddccff"> J-F. Lestrade || g || 1 || 1 || 1 || 1 || 1 || 1 || 1 || || ||<rowbgcolor="#ddccff"> A. Rigby || g || 1 || 1 || 1 || 1 || 1 || 1 || 1 || || |
NIKA2 run #7 December 2016
Goals of the run
Continue the commissioning started in run 5 and continued in run 6:
Perform test observations and any hardware configuration change possible outside the cryostat (since it's sealed and cold) which could allow investigating the problems we see from the data analysis of the previous runs: WE NEED TO THINK ABOUT AND DEFINE THESE POSSIBLE TESTS ASAP.
Still stack more beam maps at various focus (Z,Y,X), various elevation and various scan orientations (standard az-el, but also el-az) to increase the statistics on what we already have.
- Test the external calibrator mounted on a bar in front of the vertex window.
- Continue to monitor regularly secondary calibrators to check stability of the instrument gains.
- Continue any necessary work on detectors working point, electronics, acquisition, synchronizations, data files...
- In parallel to beam maps, test deep integration on well known sources: the goal should be to show reproducibility in reaching the rms expected after one hour of integration.
- If beam maps statistics sufficient: map extended features (already done with complex secondary calibrators), and at least 1 showcase : can be a nearby galaxy NGC 3938 or NGC6946 (left/right 10 arcmin diameter circle) J2000 coordinates for NGC6946 are: 20:34:52.3 +60:09:14
.
- If beam maps statistics sufficient: start polarization commissioning [that should be postponed to next run].
See all the goals listed and described in run 5 and related links for more details.
Schedule of the run
Telescope Schedule ~14h/day Observations.
All the persons who will participate to the run must appear in the table below; each one must have informed at least Samuel, Esther (for the rooms in Granada and at the telescope), Beatrice (for the ones who fly on IRAM funds, see NIKA2 travel rules).
Staff of the run: 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.
First day at the telescope: Tuesday, October 25, 2016.
People\Date |
5 |
T6 |
7 |
8 |
9 |
S10 |
11 |
12 |
T13 |
Confirmed travels: |
|||||||||
S. Leclercq |
g |
1 |
1 |
1 |
1 |
1 |
1 |
1 |
|
N. Ponthieu |
g |
1 |
1 |
1 |
1 |
1 |
1 |
g |
|
F. Mayet |
g |
1 |
1 |
1 |
1 |
1 |
1 |
1 |
|
J-F. Lestrade |
g |
1 |
1 |
1 |
1 |
1 |
1 |
1 |
|
A. Rigby |
g |
1 |
1 |
1 |
1 |
1 |
1 |
1 |
|
A. Benoit |
g |
1 |
1 |
1 |
|
|
|
|
|
J. Goupy |
g |
1 |
1 |
1 |
|
|
|
|
|
Sleep at obs. (*) |
0 |
3 |
3 |
3 |
1 |
1 |
1 |
1 |
0 |
(*) Count persons from the NIKA collaboration not from IRAM Granada.
IRAM's Astronomer on Duty.