USNO Analysis Report for I22150 ($22MAY30XU) 
       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 David Gordon, US Naval Observatory.
    Spoolfile source: interactive nuSolve analysis.) 

Problems: None. 

Number of observations rejected during correlation:    0 

Number of observations not usable by the software:     1 

    observation    2, MK-VLBA :WETTZELL, 0738+491, 18:33:17, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' 

Number of observations rejected during analysis:       1 

    observation    1, MK-VLBA :WETTZELL, 0133+476, 18:30:20, which fits at     -136.4 +/-      24.6 ps 

Other comments: None. 

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

Clock breaks: None

Session Statistics 

  Observations:       30 scheduled 
                      30 correlated (included in the database) 
                      29 recoverable (usable in Solve/nuSolve) 
                      28 used
  Session fit:        19.294 ps
  UT1 formal error:    6.65 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0133+476              1           1        0
  0529+483              3           3        3
  0552+398              4           4        4
  0602+673              3           3        3
  0613+570              3           3        3
  0716+714              4           4        4
  0738+491              4           4        3
  NGC6251               3           3        3
  1803+784              4           4        4
  3C371                 1           1        1
  ------------  ---------  ----------   ------
  Source Total         30          30       28

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