IVS Analysis Report for I19192 ($19JUL11XU) 
       This report is the official IVS analysis report that corresponds to 
       the database maintained by the IVS Data Centers for this session.  
   (Analyzed by Karen Baver, Goddard Space Flight Center VLBI Analysis Center.
    Spoolfile source: interactive solve/nuSolve analysis.) 

Problems: None. 

Number of observations rejected during correlation:    2 

    observation of 3C418 at 19:15:24 by SESHAN25:SVETLOE 
    observation of 3C418 at 19:15:24 by SESHAN25:WETTZELL 

Number of observations not usable by the software:     2 

    observation    5, SESHAN25:SVETLOE , 1639-062, 18:35:26, quality code X-band: 9 S-band: 9, H fringe error code in X band
    observation    6, SESHAN25:WETTZELL, 1639-062, 18:35:26, quality code X-band: 9 S-band: 9, H fringe error code in X band

Number of observations rejected during analysis:       0 

Other comments: None. 

Parameterization: 
   10 parameters: 
     UT1 offset 
     atmosphere offset for:
         SESHAN25 SVETLOE WETTZELL
     clock offset, first order term, and second order term for:
         SVETLOE WETTZELL

Clock breaks: None

Session Statistics 

  Observations:       61 scheduled 
                      59 correlated (included in the database) 
                      57 recoverable (usable in Solve/nuSolve) 
                      57 used
  Session fit:        15.954 ps
  UT1 formal error:    6.59 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  1726+455              1           1        1
  1749+096              9           9        9
  1803+784              7           7        7
  3C418                 9           7        7
  2209+236             12          12       12
  1639-062              3           3        1
  0016+731              5           5        5
  1751+288             15          15       15
  ------------  ---------  ----------   ------
  Source Total         61          59       57

 * Correlated means included in the database. 
   Please note that the number of recoverable (usable) observations 
   cannot be broken down by source for Intensive solutions.