NASA Analysis Report for Q18084 ($18MAR25XK) 
       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 Karen Baver, Goddard Space Flight Center VLBI Analysis Center.
    Spoolfile source: interactive solve/nuSolve analysis.) 

Problems: None. 

Number of observations rejected during correlation:   22 

  The ISHIOKA-KASHIM34 baseline was not correlated because it is too short to
  be useful for UT1-TAI estimation.

Number of observations not usable by the software:     0 

Number of observations rejected during analysis:       0 

Other comments: None. 

Parameterization: 
   10 parameters: 
     UT1 offset 
     atmosphere offset for:
         ISHIOKA KASHIM34 WETTZELL
     clock offset, first order term, and second order term for:
         KASHIM34 WETTZELL

Clock breaks: None

Session Statistics 

  Observations:       66 scheduled 
                      44 correlated (included in the database) 
                      44 recoverable (usable in Solve/nuSolve) 
                      44 used
  Session fit:        92.767 ps
  UT1 formal error:   21.39 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0059+581              9           6        6
  0119+115              6           4        4
  0133+476              3           2        2
  0552+398              6           4        4
  0955+476              6           4        4
  1300+580              6           4        4
  1803+784              3           2        2
  3C371                 6           4        4
  3C418                 3           2        2
  2229+695              3           2        2
  0529+483              3           2        2
  1144+402              6           4        4
  0016+731              6           4        4
  ------------  ---------  ----------   ------
  Source Total         66          44       44

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