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lbaops:lbajun2017:v547c

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lbaops:lbajun2017:v547c [2017/06/08 17:04]
vasaant [Comments:]
lbaops:lbajun2017:v547c [2017/06/08 17:06] (current)
vasaant [Comments:]
Line 39: Line 39:
 ==== Comments: ==== ==== Comments: ====
  
-Break down of the schedule:+Breakdown ​of the schedule:
  
-07:00 - 08:00   ​Fringe check +07:00 - 08:00   ​Fringe check\\  
- +08:00 - 08:05   Delay calibrator scan (3C273)\\  
-08:00 - 08:05   Delay calibrator scan (3C273) +08:05 - 10:20   ​G339.884-1.2\\  
- +10:20 - 10:31   Delay calibrator scan (3C273)\\  
-08:05 - 10:20   ​G339.884-1.2 +10:31 - 12:50   ​G339.884-1.2\\  
- +12:50 - 13:13   Delay calibrator scan (1921-293) & D-terms\\  
-10:20 - 10:31   Delay calibrator scan (3C273) +13:13 - 16:26   ​G339.884-1.2\\  
- +16:26 - 16:58   Delay calibrator scan (1921-293) & D-terms\\  
-10:31 - 12:50   ​G339.884-1.2 +16:58 - 18:08   ​G339.884-1.2\\  
- +18:38 - 18:30   Delay calibrator scan (1921-293) & D-terms\\  
-12:50 - 13:13   Delay calibrator scan (1921-293) & D-terms +18:30 - 19:38   ​G339.884-1.2\\  
- +19:38 - 20:00   Delay calibrator scan (1921-293) & D-terms\\ 
-13:13 - 16:26   ​G339.884-1.2 +
- +
-16:26 - 16:58   Delay calibrator scan (1921-293) & D-terms +
- +
-16:58 - 18:08   ​G339.884-1.2 +
- +
-18:38 - 18:30   Delay calibrator scan (1921-293) & D-terms +
- +
-18:30 - 19:38   ​G339.884-1.2 +
- +
-19:38 - 20:00   Delay calibrator scan (1921-293) & D-terms+
  
 The aim of our project is to conduct astrometric observations of the 22 GHz water masers in G339.884-1.259 to sub-milliarcsecond accuracy. We will be phase referencing this source with respect to J1706-4600 to determine the absolute proper motions of the maser features to probe the 3D gas dynamics at scales of 10 to 1000 AU to understand the outflow structure of this source. The aim of our project is to conduct astrometric observations of the 22 GHz water masers in G339.884-1.259 to sub-milliarcsecond accuracy. We will be phase referencing this source with respect to J1706-4600 to determine the absolute proper motions of the maser features to probe the 3D gas dynamics at scales of 10 to 1000 AU to understand the outflow structure of this source.
lbaops/lbajun2017/v547c.txt · Last modified: 2017/06/08 17:06 by vasaant