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lbaops:lbanov2013:v255u [2013/11/15 01:06]
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lbaops:lbanov2013:v255u [2015/12/18 16:38] (current)
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 The purpose of these observations is to obtain the subsequent epoch for proper motion/​parallax for G263.250+0.514,​ G305.202+0.208,​ G305.208+0.206 and G305.200+0.019,​ G339.884-1.259,​ G339.681-1.208 and G339.682-1.207. The purpose of these observations is to obtain the subsequent epoch for proper motion/​parallax for G263.250+0.514,​ G305.202+0.208,​ G305.208+0.206 and G305.200+0.019,​ G339.884-1.259,​ G339.681-1.208 and G339.682-1.207.
  
-The G263.250 observations should show a modest peak at a sky frequency of 6669.37 MHz. The G305.21 observations should show a modest peak at a sky frequency around 6669.MHz and the 339.88-1.26 should show a strong peak at a sky frequency of around 6669.27 MHz during these observations.+The G263.250 observations should show a modest peak at a sky frequency of 6668.23 MHz. The G305.21 observations should show a modest peak at a sky frequency around 6669.36 MHz and the 339.88-1.26 should show a strong peak at a sky frequency of around 6669.27 MHz during these observations.
  
 During the ICRF runs we have sometimes had to exclude certain antennas from observations of some sources in order to get a good spread of azimuths and elevations. During the ICRF runs we have sometimes had to exclude certain antennas from observations of some sources in order to get a good spread of azimuths and elevations.
lbaops/lbanov2013/v255u.txt · Last modified: 2015/12/18 16:38 (external edit)