IVS Analysis Report for I19206 ($19JUL25XU) 
       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:   24 

  The final six ISHIOKA:SVETLOE observations and the final 18 ISHIOKA:WETTZELL observations 
  were not included in the correlated data set:

      observation of 1751+288 at 19:12:12 by ISHIOKA:SVETLOE
      observation of 0059+581 at 19:16:42 by ISHIOKA:SVETLOE
      observation of 1803+784 at 19:20:08 by ISHIOKA:SVETLOE
      observation of 0016+731 at 19:22:03 by ISHIOKA:SVETLOE
      observation of 1803+784 at 19:26:47 by ISHIOKA:SVETLOE
      observation of 0016+731 at 19:28:41 by ISHIOKA:SVETLOE

      observation of 0642+449 at 19:09:55 by ISHIOKA:WETTZELL
      observation of 1726+455 at 19:11:16 by ISHIOKA:WETTZELL
      observation of 1751+288 at 19:12:12 by ISHIOKA:WETTZELL
      observation of 1803+784 at 19:13:31 by ISHIOKA:WETTZELL
      observation of 3C418    at 19:14:31 by ISHIOKA:WETTZELL
      observation of 0016+731 at 19:15:27 by ISHIOKA:WETTZELL
      observation of 0059+581 at 19:16:42 by ISHIOKA:WETTZELL
      observation of 0642+449 at 19:17:38 by ISHIOKA:WETTZELL
      observation of 1726+455 at 19:19:01 by ISHIOKA:WETTZELL
      observation of 1803+784 at 19:20:08 by ISHIOKA:WETTZELL
      observation of 3C418    at 19:21:07 by ISHIOKA:WETTZELL
      observation of 0016+731 at 19:22:03 by ISHIOKA:WETTZELL
      observation of 0059+581 at 19:23:18 by ISHIOKA:WETTZELL
      observation of 0642+449 at 19:24:14 by ISHIOKA:WETTZELL
      observation of 1726+455 at 19:25:38 by ISHIOKA:WETTZELL
      observation of 1803+784 at 19:26:47 by ISHIOKA:WETTZELL
      observation of 3C418    at 19:27:45 by ISHIOKA:WETTZELL
      observation of 0016+731 at 19:28:41 by ISHIOKA:WETTZELL

Number of observations not usable by the software:     6 

    observation    9, ISHIOKA :WETTZELL, 0642+449, 18:34:44, quality code X-band: 0 S-band: 9 
    observation   24, ISHIOKA :WETTZELL, 0642+449, 18:46:03, quality code X-band: 0 S-band: 9 
    observation   30, ISHIOKA :WETTZELL, 1751+288, 18:50:13, quality code X-band: 9 S-band: 0 
    observation   39, ISHIOKA :WETTZELL, 0642+449, 18:55:38, quality code X-band: 0 S-band: 9 
    observation   49, ISHIOKA :WETTZELL, 0642+449, 19:02:23, quality code X-band: 0 S-band: 9 
    observation   51, ISHIOKA :WETTZELL, 1751+288, 19:04:40, quality code X-band: 8 S-band: 0 

Number of observations rejected during analysis:       1 

    observation   50, ISHIOKA :WETTZELL, 1726+455, 19:03:43, which fits at      296.5 +/-      88.7 ps 

Other comments: 

  The correlator removed channel SR4U from SVETLOE's fringe fitting and applied manual phase cal for SVETLOE.

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

Clock breaks: None

Session Statistics 

  Observations:       89 scheduled 
                      65 correlated (included in the database) 
                      59 recoverable (usable in Solve/nuSolve) 
                      58 used
  Session fit:        26.262 ps
  UT1 formal error:   23.77 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0016+731             16          11       11
  0059+581             13          10       10
  0642+449              7           4        0
  NRAO512               4           4        4
  1726+455             12           9        8
  1751+288             10           8        6
  1803+784             16          11       11
  3C418                11           8        8
  ------------  ---------  ----------   ------
  Source Total         89          65       58

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