Diff for "HLS091828" - www.iram.es Main Wiki

Differences between revisions 9 and 30 (spanning 21 versions)

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

-  ⇤ ← Revision 9 as of 2013-06-14 14:05:24 → 
  Size: 584
  Editor: NikaBolometer
  Comment:
+   ← Revision 30 as of 2013-06-14 14:30:34 → ⇥
  Size: 1004
  Editor: NikaBolometer
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
 Line 1:
-Brief analysis of the faint source HLS091828 (z=5.243).
+'''Brief analysis of the faint source HLS091828 (z=5.243)'''
 Line 3:
+'''''Coordinates:'''''
 .R.A. = 09h18m28.6s  
 .Dec. = 51d42'23.3"
-Line 4:
+Line 7:
+'''''Fluxes (Combes et al. 2012): '''''
 .F1.3sma= 55+-7mJy
 .F0.88mm= 125+-8mJy
 .F2mm= 15+-7mJy
-Line 5:
+Line 12:
-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 tunning), 180 to 197
     Size of the map:90"x90"

     We detect the source at both wavelenght, shown on the maps given bellow
     {{attachment:1mm_map.pdf||widht=3000,height=300}}
     {{attachment:2mm_map.pdf||widht=3000,height=300}}
+'''''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
 .{{attachment:1mm_map.pdf||width=700,height=400}}  {{attachment:2mm_map.pdf||width=700,height=400}}
 .{{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}}