IVS Analysis Report for W19178 ($19JUN27XW) 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: 3 observation 8, MK-VLBA :WETTZELL, 1929+226, 07:20:29, quality code X-band: 0 S-band: 9 observation 17, MK-VLBA :WETTZELL, 1636+473, 07:27:23, quality code X-band: 9 S-band: 0 observation 113, MK-VLBA :WETTZELL, 2141+175, 08:38:47, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 4 observation 72, PIETOWN :WETTZELL, 1418+546, 08:08:07, which fits at 11680.6 +/- 131.0 ps observation 77, MK-VLBA :WETTZELL, 2141+175, 08:12:41, which fits at -320.3 +/- 118.2 ps observation 111, PIETOWN :WETTZELL, 1418+546, 08:36:07, which fits at -11923.3 +/- 125.0 ps observation 140, MK-VLBA :WETTZELL, 2319+317, 08:58:52, which fits at 294.3 +/- 105.0 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: 162 scheduled 162 correlated (included in the database) 159 recoverable (usable in Solve/nuSolve) 155 used Session fit: 72.391 ps UT1 formal error: 7.59 microsec Source Performance Number of Observations Scheduled Correlated* Used 1053+815 3 3 3 1128+385 3 3 3 1144+402 3 3 3 1300+580 12 12 12 1342+662 9 9 9 1418+546 9 9 7 NGC6251 3 3 3 1636+473 15 15 14 1732+389 3 3 3 1746+470 3 3 3 1803+784 3 3 3 1800+440 3 3 3 3C371 15 15 15 1929+226 3 3 2 2013+163 3 3 3 2113+293 15 15 15 2141+175 9 9 7 2144+092 6 6 6 2209+236 9 9 9 2214+350 12 12 12 2215+150 9 9 9 2229+695 9 9 9 2319+317 3 3 2 ------------ --------- ---------- ------ Source Total 162 162 155 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.