IVS Analysis Report for W19154 ($19JUN03XW) 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: 6 observation 5, MK-VLBA :WETTZELL, 1929+226, 08:32:29, quality code X-band: 0 S-band: 8 observation 66, PIETOWN :WETTZELL, 1732+389, 09:15:01, quality code X-band: 0 S-band: 9 observation 69, PIETOWN :WETTZELL, 1418+546, 09:17:06, quality code X-band: 0 S-band: 9 observation 74, MK-VLBA :WETTZELL, 2141+175, 09:21:40, quality code X-band: 0 S-band: 9 observation 104, MK-VLBA :WETTZELL, 2141+175, 09:45:53, quality code X-band: 0 S-band: 9 observation 140, MK-VLBA :WETTZELL, 2141+175, 10:13:32, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 0 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: 162 scheduled 162 correlated (included in the database) 156 recoverable (usable in Solve/nuSolve) 156 used Session fit: 70.724 ps UT1 formal error: 7.63 microsec Source Performance Number of Observations Scheduled Correlated* Used 0955+476 3 3 3 1053+815 6 6 6 1128+385 6 6 6 1144+402 12 12 12 1226+373 3 3 3 1300+580 12 12 12 1342+662 3 3 3 1418+546 6 6 5 NGC6251 3 3 3 1636+473 12 12 12 1732+389 6 6 5 1746+470 3 3 3 1803+784 3 3 3 1800+440 3 3 3 3C371 15 15 15 1823+689 3 3 3 1929+226 3 3 2 2113+293 12 12 12 2141+175 9 9 6 2144+092 9 9 9 2209+236 6 6 6 2214+350 9 9 9 2215+150 6 6 6 2229+695 9 9 9 ------------ --------- ---------- ------ Source Total 162 162 156 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.