|
Size: 1781
Comment:
|
Size: 1921
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 32: | Line 32: |
| ||120 || 12h21m || 3C273 || otf 240X240 arcsec || 200 || 42 || 0,0,-1.3 || 0.2-0.3 |||| | ||121 || 12h21m || 3C273 || otf 240X240 arcsec || 200 || 42 || 0,0,-1.3 || 0.2-0.3 |||| ||122 || 12h21m || 3C273 || otf 240X240 arcsec || 200 || 42 || 0,0,-2 || 0.2-0.3 ||changing focus|| |
NIKA October 7th, 2015 / S1
Back to list of day to day logbook of observations
2015-10-07
Following not updated
.Cryostat Temperature: 170mK cooling down slowly Modulation frequency: 10kHz 1mm, 5kHz 2mm Opacity is measured with the new taumeter at 225 GHz Nasmyth offsets : 0, 0 Set Focus : -1.3 mm (not at all optimised) Quick description of the session: Test the Pako sequences and data flows.
Data Repository: /home/nika2/NIKA/Data/run13_mirror_1m_X/
Scan |
UT |
Source |
Command |
Az |
El |
Pointing X, Y, Focus |
Tau225 |
Comment |
112 |
12h10m |
Mars |
otf 400X220 arcsec |
200 |
45 |
0,0,-1.3 |
0.2-0.3 |
All the scan are not reconized from Elvin. It appears as _I_ |
113 |
12h21m |
Mars |
otf 400X400 arcsec |
200 |
40 |
0,0,-1.3 |
0.2-0.3 |
|
114 |
12h21m |
Mars |
beam-map1 otf 300X300 arcsec |
200 |
35 |
0,0,-1.3 |
0.2-0.3 |
|
115 |
12h21m |
Mars |
beam-map2 otf 300X300 arcsec |
200 |
35 |
0,0,-1.3 |
0.2-0.3 |
|
116 |
12h21m |
Mars |
beam-map3 otf 300X300 arcsec |
200 |
35 |
0,0,-1.3 |
0.2-0.3 |
|
119 |
12h21m |
Mercury |
otf 400X400 arcsec |
200 |
43 |
0,0,-1.3 |
0.2-0.3 |
|
121 |
12h21m |
3C273 |
otf 240X240 arcsec |
200 |
42 |
0,0,-1.3 |
0.2-0.3 |
|
122 |
12h21m |
3C273 |
otf 240X240 arcsec |
200 |
42 |
0,0,-2 |
0.2-0.3 |
changing focus |