IVS Analysis Report for I17271 ($17SEP28XU) 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: 1 The following observation was not correlated in S-band: observation 28, SVETLOE :WETTZELL, 0718+793, 19:08:49 Number of observations not usable by the software: 0 Number of observations rejected during analysis: 6 The following observations were rejected: observation 5, KOKEE :SVETLOE , 0529+483, 18:34:41, which fits at 2381.83 +/- 456.82 ps observation 7, SVETLOE :WETTZELL, 0529+483, 18:34:41, which fits at -2360.81 +/- 236.29 ps observation 14, KOKEE :SVETLOE , 0955+476, 18:50:50, which fits at 5955.62 +/- 457.27 ps observation 16, SVETLOE :WETTZELL, 0955+476, 18:50:50, which fits at -5899.63 +/- 236.71 ps observation 20, SVETLOE :WETTZELL, 1520+437, 18:58:12, which fits at -5441.41 +/- 236.76 ps observation 31, SVETLOE :WETTZELL, 0307+380, 19:13:27, which fits at 824.69 +/- 236.39 ps Other comments: None. Parameterization: 10 parameters: UT1 offset atmosphere offset for: KOKEE SVETLOE WETTZELL clock offset, first order term, and second order term for: SVETLOE WETTZELL Clock breaks: None Session Statistics Observations: 39 scheduled 38 correlated (included in the database) 38 recoverable (usable in Solve/nuSolve) 32 used Session fit: 30.851 ps UT1 formal error: 5.96 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 2 2 2 0307+380 3 3 2 0340+362 1 1 1 0529+483 3 3 1 0716+714 3 3 3 0718+793 3 2 2 0738+491 1 1 1 0800+618 1 1 1 0955+476 3 3 1 1128+385 1 1 1 1300+580 1 1 1 1324+224 1 1 1 1418+546 3 3 3 1441+252 4 4 4 1520+437 6 6 5 1803+784 3 3 3 ------------ --------- ---------- ------ Source Total 39 38 32 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.