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| .We detect the source at both wavelenghts, shown on the maps given bellow .{{attachment:1mm_map.pdf||width=700,height=400}} {{attachment:2mm_map.pdf||width=700,height=400}} . . . .The profiles are computed by averaging the map in concentric annuli .{{attachment:1mm_profile.pdf||width=500,height=400}} {{attachment:2mm_profile.pdf||width=500,height=400}} |
.We detect the source at both wavelenghts, shown on the maps given bellow. {{attachment:1mm_map.pdf||width=700,height=400}} {{attachment:2mm_map.pdf||width=700,height=400}} . . .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 {{attachment:1mm_profile.pdf||width=700,height=400}} {{attachment:2mm_profile.pdf||width=700,height=400}} {{attachment:1mm_time.pdf||width=700,height=400}} {{attachment:2mm_time.pdf||width=700,height=400}} |
Brief analysis of the faint source HLS091828 (z=5.243)
Coordinates:
- R.A. = 09h18m28.6s
- Dec. = 51d42'23.3"
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 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