IVS Analysis Report for I19039 ($19FEB08XU) 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: WETTZ13N started late because the MK5 system crashed at the session's beginning. Number of observations rejected during correlation: 8 The first four KOKEE-WETTZ13N and WETTZ13N-WETTZELL observations were lost due to the WETTZ13N system crash: observations of 1156+295 at 18:45:00 observations of 2209+236 at 18:47:22 observations of 0016+731 at 18:51:40 observations of 3C371 at 18:53:23 Number of observations not usable by the software: 5 observation 2, KOKEE :WETTZELL, 2209+236, 18:49:02, quality code X-band: 0 S-band: 9 observation 3, KOKEE :WETTZELL, 0016+731, 18:52:12, quality code X-band: 9 S-band: 0 observation 5, KOKEE :WETTZELL, 2356+385, 18:57:18, quality code X-band: 0 S-band: 9 observation 15, KOKEE :WETTZELL, NGC6251 , 19:11:49, quality code X-band: 9 S-band: 0 observation 42, KOKEE :WETTZELL, 3C371 , 19:43:17, quality code X-band: 4 S-band: 6 Number of observations rejected during analysis: 13 The WETTZ13N:WETTZELL baseline was deselected. Other comments: None. Parameterization: 10 parameters: UT1 offset atmosphere offset for: KOKEE WETTZ13N WETTZELL clock offset, first order term, and second order term for: WETTZ13N WETTZELL Clock breaks: None Session Statistics Observations: 54 scheduled 46 correlated (included in the database) 41 recoverable (usable in Solve/nuSolve) 28 used Session fit: 84.029 ps UT1 formal error: 18.42 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 3 1 0 0059+581 9 9 6 0718+793 1 1 1 1144+402 3 3 2 1156+295 3 1 1 1300+580 6 6 4 1418+546 3 3 2 NGC6251 1 1 0 1803+784 6 6 4 3C371 6 4 2 2209+236 3 1 0 2229+695 3 3 2 2319+317 6 6 4 2356+385 1 1 0 ------------ --------- ---------- ------ Source Total 54 46 28 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.