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| '''14 November 2013''': OTF geometries on Mars and Uranus. Check of the focal plane geometry. First light of NIKA prototype with polarisation facilities. | '''14 November 2013''': OTF geometries on Mars and Uranus. Check of the focal plane geometry. First light of NIKA prototype with polarisation facilities. In the afternoon tests on the power on the pixels check its uniformity on the 2 arrays. |
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| 129 pixels 2mm - about 1Hz/sqrtHz noise (sky with tau about 0); 185 pixels 1mm about 10Hz/sqrtHz noise (sky with tau about 0) |
130 (129 good) pixels 2mm - about 1Hz/sqrtHz noise (sky with tau about 0); 201 (about 185 good) pixels 1mm - about 5Hz/sqrtHz noise (sky with tau about 0); The tests for the optimal power where conducted with the window closed with some alu foil -> not great in term of stability, could add some 1/f. Touching the foil made a clear signal (at least on the 1mm). The final values for the different DAC gains can be seen in this image: |
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| '''Modulation frequency''': 8kHz 1mm, 4kHz 2mm | {{attachment:DACgains.png||width=600}} ''Figures: Reglages of the 2 arrays. In red, NIKEL1 = 1mm, in blue NIKEL2 = 2mm.'' '''Modulation frequency''': 8kHz 1mm, 5kHz 2mm |
November 11th 2013, Alain Benoit, Martino Calvo and Andrea Catalano come to the 30m to install, cool down and testing the NIKA prototype.
12-13 November 2013: cryostat and Read-Out positioning in the cabin, cooling down, HWP Modulator installation at the pupil (120mm from the entrance lens of the cryostat).
14 November 2013: OTF geometries on Mars and Uranus. Check of the focal plane geometry. First light of NIKA prototype with polarisation facilities. In the afternoon tests on the power on the pixels check its uniformity on the 2 arrays.
15 November 2013: Cryostat back to 300K: 3He-4He mix recovery, heating trap. Polarisation facilities dismantling. Back to Granada.
STATUS
Cryostat Temperature: 150mK (set by temperature control).
Arrays: 130 (129 good) pixels 2mm - about 1Hz/sqrtHz noise (sky with tau about 0); 201 (about 185 good) pixels 1mm - about 5Hz/sqrtHz noise (sky with tau about 0); The tests for the optimal power where conducted with the window closed with some alu foil -> not great in term of stability, could add some 1/f. Touching the foil made a clear signal (at least on the 1mm). The final values for the different DAC gains can be seen in this image:
Figures: Reglages of the 2 arrays. In red, NIKEL1 = 1mm, in blue NIKEL2 = 2mm.
Modulation frequency: 8kHz 1mm, 5kHz 2mm
OBSERVATIONS Log
Opacity is measured with the taumeter at 225 GHz
p2cor : 0
p7cor : 0
initial Focus : -2.40 mm
Scan |
UT |
Source |
Command |
Az |
El |
Pointing X, Y, Focus |
Tau225 |
Comment |
15 |
04h39 |
Mars |
Track |
|
|
0 , 0 , -2.4 |
0.15 |
|
16 |
04h45 |
Mars |
OTF_Geometry |
|
|
0 , 0 , -2.4 |
0.15 |
First map for choosing the reference pixels |
17-21 |
04h58-05h04 |
Mars |
Focus_Liss |
|
|
0, 0, -2.4 |
0.15 |
|
22 |
05h05 |
Mars |
Focus |
|
|
0, 0, -2.4 |
0.15 |
|
23 |
05h47 |
Mars |
OTF_Geometry |
|
|
0, 0, -2.4 |
0.15 |
Tuning working during the map |
211-218 |
21h34-21h57 |
Uranus |
Track 300 300 |
55 |
190 |
0, 0, -2.4 |
0.00001 |
|
220-224 |
22h01-22h08 |
Uranus |
Focus_Liss |
|
|
0, 0, -2.4 |
0.00001 |
optimal focus probably over the range |
225 |
22h10 |
Uranus |
Cross |
|
|
0, 0, -2.4 |
0.00001 |
|
226-230 |
22h12-22h18 |
Uranus |
Focus_Liss |
|
|
0, 0, -1 |
0.00001 |
set pointing Az=-12.8 El=3.8 set focus = -1.5 |
231 |
22h24 |
Uranus |
OTF_Geometry |
|
|
-12.8, 3.8, -1.5 |
0.00001 |
|
232 |
22h49 |
Uranus |
OTF_Geometry |
|
|
-12.8, 3.8, -1.5 |
0.00001 |
HWP+Pol |
241-245 |
23h34-23h47 |
others observing |
various |
|
|
|
|
HWP+Pol+Cryostat in the cabin environment |
FIRST RESULTS
Figures: Focal Plane Geometry derived using scan 16: we chose the following reference pixels: 491 for 2mm array, 5 for 1mm array.
Figures: 1mm array from scan 231.
Figures: 2mm array from scan 231.
Figures: Entire (top) and zoomed (bottom) Timeline of the scan 232 on Uranus in configuration NIKA + HWP-Pol
Further results on polarisation measurements will come soon.......