• Listing of the solution. WRMS of the solution is 32 psec, it is not bad, but VLBA experiments usually have better fit. I deselected GGAO, since it doesn't seem to improve geometry. Adjustments of positions of 12 sources: 0201_113, NGC1052, NGC1218, 0422_004, 0919-260. 0920-397, 1104+728, 1156+295 1416+067, 2149+056, VR422201, 2337+264 were significant and I left them in the final solution. I deselected a source 1910-293 -- it showed unusual problems.
  
  Performance of the VLBA stations in the experiment were rather better than European stations.
• UPWEI table when positions of 12 sources were estimated. Values at the last column has meaning of the ratio of partial sum of squares of weighted residuals over the certain baseline or source to its mathematical expectation.
• UPWEI table when no source positions were estimated.
• Plot of residual phases at the X-band for baseline NYALES20/ONSALA60 for the first 10 hours. Units are radians. Residual phases for 4 different channels are shown by different colors.
• Plot of residual phases at the S-band for baseline NYALES20/ONSALA60 for the first 10 hours. Units are radians. Residual phases for 4 different channels are shown by different colors.
• Plot of formal error of group delay at X-band (hollow green circles) based on SNR and formal error of determination of group delay based on phase residuals (filled blue circles) for the baseline NYALES20/ONSALA60.
• Plot of residual phases at the X-band for baseline KP-VLBA/LA-VLBA for the first 10 hours. Units are radians. Residual phases for 4 different channels are shown by different colors.
• Plot of residual phases at the S-band for baseline KP-VLBA/LA-VLBA for the first 10 hours. Units are radians. Residual phases for 4 different channels are shown by different colors.
• Plot of formal error of group delay at X-band (hollow green circles) based on SNR and formal error of determination of group delay based on phase residuals (filled blue circles) for the baseline KP-VLBA/LA-VLBA.

Last update: 04-AUG-98 11:53:57