IVS Analysis Report for W19343 ($19DEC09XW) 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: 2 observation 14, MK-VLBA :WETTZ13N, 1015+359, 09:02:28, quality code X-band: 0 S-band: 0 observation 31, MK-VLBA :WETTZ13N, 1040+244, 09:44:03, quality code X-band: 0 S-band: 0 Number of observations rejected during analysis: 2 observation 5, MK-VLBA :WETTZ13N, 0345+460, 08:40:09, which fits at -234.2 +/- 47.9 ps observation 21, MK-VLBA :WETTZ13N, 0345+460, 09:19:58, which fits at 1692.3 +/- 56.1 ps Other comments: The data for PIETOWN were not included. The correlator report was not available, so it is not currently known whether or not this is the final correlated version and whether or not PIETOWN observed. Parameterization: 6 parameters: UT1 offset atmosphere offset for: MK-VLBA WETTZ13N clock offset, first order term, and second order term for: WETTZ13N Clock breaks: None Session Statistics Observations: 153 scheduled (from all stations---includes PIETOWN) 51 scheduled (from available stations---does not include PIETOWN) 51 correlated (included in the database) 49 recoverable (usable in Solve/nuSolve) 47 used Session fit: 34.088 ps UT1 formal error: 5.14 microsec Source Performance Number of Observations Scheduled Correlated* Used 0059+581 12 4 4 0133+476 12 4 4 0345+460 12 4 2 0529+483 6 2 2 0552+398 3 1 1 0613+570 12 4 4 0641+392 3 1 1 0714+457 3 1 1 0716+714 9 3 3 0738+491 9 3 3 0759+183 3 1 1 0804+499 3 1 1 0805+410 12 4 4 0920+390 6 2 2 0955+476 12 4 4 1015+359 12 4 3 1040+244 6 2 1 1053+815 3 1 1 NGC6251 3 1 1 1803+784 3 1 1 2229+695 6 2 2 2356+385 3 1 1 ------------ --------- ---------- ------ Source Total 153 51 47 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.