NASA Analysis Report for Q18154 ($18JUN03XK) 
       This report is a contributed analysis report that does not correspond to 
       the database maintained by the IVS Data Centers for this session.  
   (Analyzed by Sergei Bolotin, Goddard Space Flight Center NASA.
    Spoolfile source: interactive solve/nuSolve analysis.) 

Problems: None. 

Number of observations rejected during correlation:    0 

Number of observations not usable by the software:     0 

Number of observations rejected during analysis:       1 

    observation   24, ISHIOKA :WETTZELL, OJ287   , 08:13:54, which fits at      174.5 +/-      40.9 ps 

Other comments: None. 

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

Clock breaks: None

Session Statistics 

  Observations:       32 scheduled 
                      32 correlated (included in the database) 
                      32 recoverable (usable in Solve/nuSolve) 
                      31 used
  Session fit:        38.360 ps
  UT1 formal error:   10.03 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0059+581              1           1        1
  0458-020              2           2        2
  0552+398              4           4        4
  0805+410              4           4        4
  OJ287                 2           2        1
  0955+476              3           3        3
  1418+546              3           3        3
  1803+784              1           1        1
  3C371                 1           1        1
  0420+022              1           1        1
  0529+483              3           3        3
  0716+714              2           2        2
  0748+126              4           4        4
  0016+731              1           1        1
  ------------  ---------  ----------   ------
  Source Total         32          32       31

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