IVS Analysis Report for I19060 ($19MAR01XU) 
       This report is the official IVS analysis report that corresponds to 
       the database maintained by the IVS Data Centers for this session.  
   (Analyzed by Sergei Bolotin, NVI, Inc. / NASA Goddard Space Flight 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    3, KOKEE   :WETTZELL, 2000+472, 18:53:03, quality code X-band: 9 S-band: 0 
    observation   12, KOKEE   :WETTZELL, 0017+200, 19:23:42, quality code X-band: 0 S-band: 9 

Number of observations rejected during analysis:       1 

    observation   18, KOKEE   :WETTZELL, 1504+377, 19:43:03, which fits at      266.1 +/-      58.3 ps 

Other comments: None. 

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

Clock breaks: None

Session Statistics 

  Observations:       18 scheduled 
                      18 correlated (included in the database) 
                      16 recoverable (usable in Solve/nuSolve) 
                      15 used
  Session fit:        30.213 ps
  UT1 formal error:   11.94 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0017+200              2           2        1
  0059+581              2           2        2
  1053+704              1           1        1
  1324+224              1           1        1
  1504+377              3           3        2
  1803+784              2           2        2
  1849+670              2           2        2
  2000+472              1           1        0
  2229+695              1           1        1
  2309+454              3           3        3
  ------------  ---------  ----------   ------
  Source Total         18          18       15

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