IVS Analysis Report for I19296 ($19OCT23XU) 
       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:    0 

Number of observations not usable by the software:     2 

    observation   20, ISHIOKA :NYALES20, 1418+546, 18:56:11, quality code X-band: 9 S-band: 0 
    observation   29, ISHIOKA :NYALES20, 1418+546, 19:07:52, quality code X-band: 9 S-band: 0 

Number of observations rejected during analysis:       0 

Other comments: None. 

Parameterization: 
   6 parameters: 
     UT1 offset 
     atmosphere offset for:
         ISHIOKA NYALES20
     clock offset, first order term, and second order term for:
         NYALES20

Clock breaks: None

Session Statistics 

  Observations:       45 scheduled 
                      45 correlated (included in the database) 
                      43 recoverable (usable in Solve/nuSolve) 
                      43 used
  Session fit:        41.706 ps
  UT1 formal error:    9.40 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0017+200              1           1        1
  0059+581              2           2        2
  0119+115              4           4        4
  0202+319              3           3        3
  0552+398              5           5        5
  0642+449              5           5        5
  OJ287                 5           5        5
  1030+415              5           5        5
  1128+385              5           5        5
  1418+546              5           5        3
  1803+784              5           5        5
  ------------  ---------  ----------   ------
  Source Total         45          45       43

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