BKG Analysis Report for v23164 (20230613-v23164)
       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 Gerald Engelhardt, Federal Agency for Cartography and Geodesy (BKG),
    Spoolfile source: interactive nuSolve analysis.) 

Problems: None.

Number of observations rejected during correlation:    0

Number of observations not usable by the software:     1

    observation   71,          0529+483, ISHIOKA :WETTZ13S, 19:29:17, quality codes - S:-, X:9

Number of observations rejected during analysis:       1

    observation   65, ISHIOKA :WETTZ13S, 2113+293, 19:22:53, which fits at -165.7 +/- 36.3 ps

Other comments: 
    The vgosDb BKG analysis output is available at
    ftp://ivs.bkg.bund.de/pub/vlbi/ivsdata/vgosdb_bkg/20230613-v23164.tgz

Parameterization: 
    6 parameters:
     UT1 offset
     atmosphere offset for:
         ISHIOKA WETTZ13S
     clock offset (0), first order term (1), and/or second order term (2) for:
         WETTZ13S (0,1,2)

Clock breaks: None.

-----------------------------------------

Session Statistics 

  Observations:       72 scheduled (included in correlation report)
                      71 correlated (included in database) 
                      70 recoverable (usable in Solve/nuSolve) 
                      69 used 
  Session fit:        34.793 ps
  UT1 formal error:    4.710 microsec

-----------------------------------------


Source Performance 

                    Number of Observations

             Scheduled(*)  Correlated*    Used    


  0059+581              3           1        1
  0345+460              2           3        3
  0529+483              1           3        2
  0602+673              1           1        1
  0613+570              2           2        2
  0716+714          source not found in scheduling.
  0800+618              1           1        1
  1053+704              1           1        1
  1417+385          source not found in scheduling.
  1418+546              2           2        2
  1504+377              4           2        2
  1514+197          source not found in scheduling.
  1520+319              3           2        2
  1520+437          source not found in scheduling.
  1606+106          source not found in scheduling.
  1616+063          source not found in scheduling.
  1617+229              1           1        1
  1636+473              2           3        3
  1639+230          source not found in scheduling.
  1639-062          source not found in scheduling.
  1705+018              3           2        2
  1722+330          source not found in scheduling.
  1741-038              3           2        2
  1746+470          source not found in scheduling.
  1749+096              3           4        4
  1751+288              3           4        4
  1758+388              1           1        1
  1803+784              1           1        1
  1806+456              1           1        1
  1842+681          source not found in scheduling.
  1846+322              2           2        2
  1849+670              1           1        1
  1909+161              3           3        3
  1929+226              5           1        1
  2000+472              3           3        3
  2113+293              3           1        0
  2229+695              3           1        1
  2309+454              2           3        3
   NRAO512              4           3        3
  1726+455              1           0        0
  2013+163              1           0        0
  0552+398              1           0        0
  1656-075              1           0        0
  0016+731              1           0        0
  1732+389              2           0        0
  1538+149              1           0        0
  ------------  ---------  ----------   ------
  Source Total         72          71       69

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