IVS Analysis Report for Q22136 ($22MAY16XK) 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 and WETTZELL did not observe due to maintenance. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 1 observation 9, NYALES20:SESHAN25, 0229+131, 07:03:07, quality code X: 0 S: 8, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 2 observation 73, NYALE13S:NYALES20, 0718+793, 07:44:45, which fits at 2149.7 +/- 34.6 ps observation 94, NYALE13S:NYALES20, 0016+731, 07:57:05, which fits at -2885.8 +/- 31.1 ps Other comments: None. Parameterization: 13 parameters: UT1 offset atmosphere offset for: NYALE13S NYALES20 SESHAN25 clock offset, first order term, and second order term for: NYALES20 SESHAN25 station coordinates for: NYALE13S Clock breaks: None Session statistics Observations: 330 scheduled 99 correlated (included in the database) 98 recoverable (usable in Solve/nuSolve) 96 used Session fit: 40.069 ps UT1 formal error: 16.12 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 20 6 5 0119+115 20 6 6 0133+476 20 6 6 0202+319 20 6 6 0229+131 30 9 8 0235+164 30 9 9 0552+398 10 3 3 0716+714 10 3 3 0718+793 20 6 5 0805+410 10 3 3 0814+425 10 3 3 0955+476 20 6 6 1039+811 20 6 6 1803+784 30 9 9 3C371 30 9 9 2229+695 30 9 9 ------------ --------- ---------- ------ Source Total 330 99 96 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.