IVS Analysis Report for I19035 ($19FEB04XU) 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: 8 observation 7, KOKEE :WETTZ13N, 0016+731, 18:37:14, quality code X-band: 9 S-band: 0 observation 8, KOKEE :WETTZELL, 0016+731, 18:37:14, quality code X-band: 9 S-band: 0 observation 16, KOKEE :WETTZ13N, 2209+236, 18:46:11, quality code X-band: 0 S-band: 9 observation 17, KOKEE :WETTZELL, 2209+236, 18:46:11, quality code X-band: 0 S-band: 9 observation 19, KOKEE :WETTZ13N, 2319+317, 18:50:07, quality code X-band: 0 S-band: 9 observation 20, KOKEE :WETTZELL, 2319+317, 18:50:07, quality code X-band: 0 S-band: 9 observation 22, KOKEE :WETTZELL, NGC6251 , 18:54:28, quality code X-band: 9 S-band: 0 observation 38, KOKEE :WETTZELL, NGC6251 , 19:15:01, quality code X-band: 9 S-band: 0 Number of observations rejected during analysis: 17 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: 53 scheduled 53 correlated (included in the database) 45 recoverable (usable in Solve/nuSolve) 28 used Session fit: 40.444 ps UT1 formal error: 9.44 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 3 3 0 0059+581 3 3 2 1144+402 6 6 4 1156+295 3 3 2 1300+580 6 6 4 1418+546 6 6 4 NGC6251 2 2 0 1803+784 3 3 2 3C371 6 6 4 2113+293 3 3 2 2209+236 3 3 0 2229+695 3 3 2 2319+317 6 6 2 ------------ --------- ---------- ------ Source Total 53 53 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.