IVS Analysis Report for I18031 ($18JAN31XU) 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 4, KOKEE :WETTZELL, 1823+689, 18:37:24, quality code X-band: 0 S-band: 9 observation 14, KOKEE :WETTZELL, 2209+236, 19:07:15, quality code X-band: 0 S-band: 9 observation 18, KOKEE :WETTZELL, 2209+236, 19:21:23, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 0 Other comments: This session has been re-analyzed because the correlator recorrelated it to apply multi-tone phase cal to KOKEE. Parameterization: 6 parameters: UT1 offset atmosphere offset for: KOKEE WETTZELL clock offset, first order term, and second order term for: WETTZELL Clock breaks: None Session Statistics Observations: 20 scheduled 20 correlated (included in the database) 17 recoverable (usable in Solve/nuSolve) 17 used Session fit: 60.784 ps UT1 formal error: 17.70 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 1 1 1 0718+793 2 2 2 1101+384 1 1 1 1144+402 1 1 1 1156+295 1 1 1 1300+580 1 1 1 1418+546 1 1 1 NGC6251 1 1 1 1803+784 1 1 1 3C371 1 1 1 1823+689 1 1 0 2113+293 1 1 1 2209+236 2 2 0 2214+350 1 1 1 2215+150 2 2 2 2229+695 1 1 1 2319+317 1 1 1 ------------ --------- ---------- ------ Source Total 20 20 17 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.