IVS Analysis Report for W19189 ($19JUL08XW) 
       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:    0 

Number of observations not usable by the software:    15 

    observation   30, PIETOWN :WETTZELL, 1053+815, 08:49:32, quality code X-band: 0 S-band: 8 
    observation   32, MK-VLBA :WETTZELL, 1418+546, 08:51:29, quality code X-band: 9 S-band: 0 
    observation   42, PIETOWN :WETTZELL, 2214+350, 08:58:13, quality code X-band: 0 S-band: 9 
    observation   44, MK-VLBA :WETTZELL, 2307+106, 09:00:25, quality code X-band: 0 S-band: 9 
    observation   45, PIETOWN :WETTZELL, 2307+106, 09:00:25, quality code X-band: 0 S-band: 9 
    observation   50, MK-VLBA :WETTZELL, 1520+437, 09:06:42, quality code X-band: 0 S-band: 9 
    observation   69, PIETOWN :WETTZELL, 2214+350, 09:22:08, quality code X-band: 0 S-band: 9 
    observation   98, MK-VLBA :WETTZELL, 2214+350, 09:45:25, quality code X-band: 0 S-band: 8 
    observation   99, PIETOWN :WETTZELL, 2214+350, 09:45:25, quality code X-band: 0 S-band: 9 
    observation  101, MK-VLBA :WETTZELL, NGC6251 , 09:48:00, quality code X-band: 9 S-band: 0 
    observation  102, PIETOWN :WETTZELL, NGC6251 , 09:48:00, quality code X-band: 9 S-band: 0 
    observation  134, MK-VLBA :WETTZELL, 2214+350, 10:13:20, quality code X-band: 0 S-band: 8 
    observation  135, PIETOWN :WETTZELL, 2214+350, 10:13:20, quality code X-band: 0 S-band: 9 
    observation  148, MK-VLBA :PIETOWN , 1418+546, 10:28:23, quality code X-band: 0 S-band: 9 
    observation  150, PIETOWN :WETTZELL, 1418+546, 10:28:23, quality code X-band: 0 S-band: 9 

Number of observations rejected during analysis:       2 

    observation   64, MK-VLBA :PIETOWN , 1823+689, 09:19:15, which fits at   -12037.1 +/-      96.0 ps 
    observation   95, MK-VLBA :WETTZELL, 3C371   , 09:43:15, which fits at      437.5 +/-      68.5 ps 

Other comments: None. 

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

Clock breaks: None

Session Statistics 

  Observations:      150 scheduled 
                     150 correlated (included in the database) 
                     135 recoverable (usable in Solve/nuSolve) 
                     133 used
  Session fit:        77.433 ps
  UT1 formal error:    8.69 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0016+731              3           3        3
  0059+581             15          15       15
  0133+476              3           3        3
  0718+793              9           9        9
  1053+815              3           3        2
  1300+580             12          12       12
  1342+662              9           9        9
  1418+546              6           6        3
  1520+437             12          12       11
  NGC6251               3           3        1
  1636+473             12          12       12
  1746+470              3           3        3
  1803+784              3           3        3
  3C371                 6           6        5
  1823+689              3           3        2
  2113+293              6           6        6
  2209+236              3           3        3
  2214+350             12          12        6
  2215+150              3           3        3
  2229+695              9           9        9
  2307+106              3           3        1
  2319+317              9           9        9
  2356+385              3           3        3
  ------------  ---------  ----------   ------
  Source Total        150         150      133

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