IVS Analysis Report for W19185 ($19JUL04XW) 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: 5 observation 11, MK-VLBA :WETTZELL, 1758+388, 07:23:51, quality code X-band: 9 S-band: 0 observation 78, PIETOWN :WETTZELL, NGC6251 , 08:11:15, quality code X-band: 9 S-band: 0 observation 98, MK-VLBA :WETTZELL, 1800+440, 08:28:02, quality code X-band: 0 S-band: 0 observation 99, PIETOWN :WETTZELL, 1800+440, 08:28:02, quality code X-band: 0 S-band: 9 observation 153, PIETOWN :WETTZELL, 2214+350, 09:11:39, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 2 observation 8, MK-VLBA :WETTZELL, 2013+163, 07:20:42, which fits at -675.0 +/- 78.9 ps observation 18, PIETOWN :WETTZELL, 1418+546, 07:27:10, which fits at -324.7 +/- 107.5 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: 159 scheduled 159 correlated (included in the database) 154 recoverable (usable in Solve/nuSolve) 152 used Session fit: 68.141 ps UT1 formal error: 6.65 microsec Source Performance Number of Observations Scheduled Correlated* Used 0059+581 3 3 3 0718+793 3 3 3 1053+815 3 3 3 1128+385 3 3 3 1300+580 12 12 12 1342+662 9 9 9 1418+546 9 9 8 NGC6251 3 3 2 1636+473 12 12 12 1746+470 3 3 3 1758+388 3 3 2 1803+784 6 6 6 1800+440 6 6 4 3C371 15 15 15 2013+163 3 3 2 2113+293 12 12 12 2141+175 3 3 3 2144+092 6 6 6 2209+236 9 9 9 2214+350 15 15 14 2215+150 9 9 9 2229+695 9 9 9 2319+317 3 3 3 ------------ --------- ---------- ------ Source Total 159 159 152 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.