IVS Analysis Report for W19030 ($19JAN30XW) This report is the official IVS analysis report that corresponds to the database maintained by the IVS Data Centers for this session. (Analyzed by Sergei Bolotin, NVI, Inc. / NASA Goddard Space Flight Center. Spoolfile source: interactive solve/nuSolve analysis.) Problems: None. Number of observations rejected during correlation: 1 MK-VLBA :PIETOWN , 0804+499, 08:43:14 --- not in data base: probable G- or H- code in one or both bands Number of observations not usable by the software: 4 observation 38, MK-VLBA :WETTZELL, 0016+731, 07:42:58, quality code X-band: 9 S-band: 0 observation 77, MK-VLBA :WETTZELL, 0345+460, 08:16:58, quality code X-band: 0 S-band: 9 observation 89, MK-VLBA :WETTZELL, 3C274 , 08:25:48, quality code X-band: 9 S-band: 0 observation 153, PIETOWN :WETTZELL, NGC6251 , 09:13:45, quality code X-band: 9 S-band: 0 Number of observations rejected during analysis: 1 observation 11, MK-VLBA :WETTZELL, 0133+476, 07:22:21, which fits at 192.0 +/- 58.9 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: 153 scheduled 152 correlated (included in the database) 148 recoverable (usable in Solve/nuSolve) 147 used Session fit: 50.432 ps UT1 formal error: 5.06 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 6 6 5 0059+581 12 12 12 0133+476 9 9 8 0345+460 6 6 5 0529+483 6 6 6 0613+570 6 6 6 0716+714 6 6 6 0718+793 3 3 3 0738+491 6 6 6 0800+618 6 6 6 0804+499 3 2 2 0805+410 6 6 6 0920+390 3 3 3 0955+476 12 12 12 1015+359 3 3 3 1040+244 9 9 9 1053+815 3 3 3 1101+384 3 3 3 1111+149 3 3 3 1144+402 3 3 3 1156+295 3 3 3 1212+171 3 3 3 1226+373 3 3 3 3C274 6 6 5 1300+580 9 9 9 1308+328 3 3 3 1324+224 3 3 3 1342+662 3 3 3 NGC6251 3 3 2 1803+784 3 3 3 ------------ --------- ---------- ------ Source Total 153 152 147 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.