NIKA October 31, 2015 / S10
Back to list of day to day logbook of observations
2015-10-31
IMPORTANT NOTES ON OBSERVING INFO
- TAPAS is not working anymore: we resume here from scan 87
Comments: configuration of the acquisition soft 2mm and 1mm:run13.ini
Source |
scan number |
Az |
El |
Pointing type |
focus x |
focus y |
focus z |
pointing x y |
comment |
Mars |
87 |
? |
? |
@beammap: scan 1/3 |
0.3 |
0 |
0 |
5.2 -0.6 |
|
Mars |
88 |
? |
? |
scan2/3 |
0.3 |
0 |
0 |
5.2 -0.6 |
|
Mars |
89 |
? |
? |
scan3/3 |
0.3 |
0 |
0 |
5.2 -0.6 |
|
Mars |
90 |
? |
? |
@beammap: scan 1/3 |
0.3 |
-1 |
0 |
5.2 -0.6 |
|
Mars |
91 |
? |
? |
scan2/3 |
0.3 |
-1 |
0 |
5.2 -0.6 |
|
Mars |
92 |
? |
? |
scan3/3 |
0.3 |
-1 |
0 |
5.2 -0.6 |
not analysed in RT because merged with 91 |
Mars |
93 |
? |
? |
@beammap: scan 1/3 |
0.3 |
+1 |
0 |
5.2 -0.6 |
|
Mars |
94 |
? |
? |
scan2/3 |
0.3 |
+1 |
0 |
5.2 -0.6 |
|
Mars |
95 |
? |
? |
scan3/3 |
0.3 |
+1 |
0 |
5.2 -0.6 |
|
IRC10216 |
96 |
250 |
44 |
track |
0.3 |
+1 |
0 |
5.2 -0.6 |
|
IRC10216 |
97 |
250 |
44 |
@nkotf 5 5 0 0 15 30 azel |
0.3 |
+1 |
0 |
5.2 -0.6 |
forgot to get back to focus y = 0 |
IRC10216 |
98 |
251 |
43 |
@nkotf 5 5 0 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
repeat with good focus |
IRC10216 |
99 |
252 |
42 |
@nkotf 5 5 90 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
|
IRC10216 |
100 |
252 |
42 |
@nkotf 5 5 45 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
|
IRC10216 |
101 |
252 |
42 |
@nkotf 5 5 135 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
|
IRC10216 |
102 |
251 |
43 |
@nkotf 5 5 0 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
|
IRC10216 |
103 |
252 |
42 |
@nkotf 5 5 90 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
|
IRC10216 |
104 |
252 |
42 |
@nkotf 5 5 45 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
|
IRC10216 |
105 |
252 |
42 |
@nkotf 5 5 135 0 15 30 azel |
0.3 |
0 |
0 |
5.2 -0.6 |
|
1156+295 |
106 |
253 |
69 |
track |
0.3 |
0 |
0 |
5.2 -0.6 |
pointing source to observe CLJ1227 |
1156+295 |
106 |
253 |
69 |
@nkpoint l |
0.3 |
0 |
0 |
5.2 -0.6 |
set pointing 1.2 -1.3 |
CLJ1227 |
108 |
261 |
74 |
track |
0.3 |
0 |
0 |
1.2 -1.3 |
telescope error we change source |
1144+402 |
109 |
285 |
66 |
track |
0.3 |
0 |
0 |
1.2 -1.3 |
CLJ1227 was too high in elevation |
1144+402 |
110 |
285 |
66 |
@nkpoint l |
0.3 |
0 |
0 |
1.2 -1.3 |
set pointing 2.8 -0.4 |
CLJ1227 |
111 |
265 |
71 |
track |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
112 |
265 |
71 |
@nkotf 10 5 0 0 15 30 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
scan speed of 30 until El < 70 |
CLJ1227 |
113 |
267 |
68 |
@nkotf 10 5 90 0 15 30 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
114 |
267 |
68 |
@nkotf 10 5 0 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
115 |
268 |
67 |
@nkotf 10 5 90 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
116 |
268 |
67 |
@nkotf 10 5 45 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
117 |
268 |
67 |
@nkotf 10 5 135 0 15 60azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
118 |
271 |
63 |
@nkotf 10 5 0 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
119 |
271 |
63 |
@nkotf 10 5 90 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
120 |
268 |
67 |
@nkotf 10 5 45 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
121 |
268 |
67 |
@nkotf 10 5 135 0 15 60azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
118 |
271 |
63 |
@nkotf 10 5 0 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
119 |
271 |
63 |
@nkotf 10 5 90 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
120 |
273 |
60 |
@nkotf 10 5 45 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
121 |
273 |
60 |
@nkotf 10 5 135 0 15 60azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
122 |
273 |
60 |
@nkotf 10 5 0 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
123 |
274 |
57 |
@nkotf 10 5 90 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
124 |
274 |
57 |
@nkotf 10 5 45 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
125 |
275 |
56 |
@nkotf 10 5 135 0 15 60azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
CLJ1227 |
126 |
276 |
54 |
@nkotf 10 5 0 0 15 60 azel |
0.3 |
0 |
0 |
2.8 -0.4 |
|
19:00 Starting of the observations. We try the two 1mm arrays configuration but we did not see so much pixels on the array 3 so we came back to the configuration with the 1 and 2 arrays.
Comments : Tapas came back. Go to TAPAS page for more details about the observations.
Goal of the session:
Observing some secondary calibrator and some extended sources to test the performance of the arrays.