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Size: 600
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Size: 1232
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| Deletions are marked like this. | Additions are marked like this. |
| Line 3: | Line 3: |
| '''''Coordinates:''''' .R.A. = 09h18m28.6s .Dec. = 51d42'23.3" |
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| Line 4: | Line 7: |
| '''''Coordinates:''''' R.A. = 09h18m28.6s Dec. = 51d42'23.3" |
'''''Expected luxes (Combes et al. 2012): ''''' .F1.3sma= 55+-7mJy .F0.88mm= 125+-8mJy .F2mm= 15+-7mJy |
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| '''''Fluxes (Combes et al. 2012): ''''' F1.3sma= 55+-7mJy F0.88mm= 125+-8mJy F2mm= 15+-7mJy |
'''''NIKA obsevations:''''' .''Day:'' 13/06/2013 .''Scans'': 9 Lissajous of 5 min (<=> 45 min) each with followed by tracks (for tuning), 180 to 197 .''Size of the map'':90"x90" .We detect the source at both wavelenghts, shown on the maps given bellow. || {{attachment:1mm_map.png}} || {{attachment:2mm_map.png||width=550,height=400}} || || [[attachment:1mm_map.pdf]] || [[attachment:2mm_map.pdf]] || |
| Line 17: | Line 21: |
| '''''NIKA obsevations:''''' | .The profiles are computed by averaging the map in concentric annuli, and we check that the measured flux is, a priori, consistent with what we expect. |
| Line 19: | Line 23: |
| Day: 13/06/2013 | || {{attachment:1mm_profile.png}} || {{attachment:2mm_profile.png}} || || [[attachment:1mm_profile.pdf]] || [[attachment:2mm_profile.pdf]] || |
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| Scans: 9 Lissajous of 5 min each with followed by tracks (for tunning), 180 to 197 | .The time per pixel maps are also shown || {{attachment:1mm_time.png}} || {{attachment:2mm_time.png}} || || [[attachment:1mm_time.pdf]] || [[attachment:2mm_time.pdf]] || |
| Line 23: | Line 30: |
| Size of the map:90"x90" We detect the source at both wavelenght, shown on the maps given bellow {{attachment:1mm_map.pdf||width=600}} {{attachment:2mm_map.pdf||width=600}} |
.Using Jack-Knives maps, we are able to estimate the noise level in the data. |
Brief analysis of the faint source HLS091828 (z=5.243)
Coordinates:
- R.A. = 09h18m28.6s
- Dec. = 51d42'23.3"
Expected luxes (Combes et al. 2012):
- F1.3sma= 55+-7mJy
- F0.88mm= 125+-8mJy
- F2mm= 15+-7mJy
NIKA obsevations:
Day: 13/06/2013
Scans: 9 Lissajous of 5 min (<=> 45 min) each with followed by tracks (for tuning), 180 to 197
Size of the map:90"x90"
- We detect the source at both wavelenghts, shown on the maps given bellow.
- The profiles are computed by averaging the map in concentric annuli, and we check that the measured flux is, a priori, consistent with what we expect.
- The time per pixel maps are also shown
- Using Jack-Knives maps, we are able to estimate the noise level in the data.
