IVS Analysis Report for Q19259 ($19SEP16XK) This report is the official IVS analysis report that corresponds to the database maintained by the IVS Data Centers for this session. (Analyzed by Sergei Bolotin, NVI, Inc. / NASA Goddard Space Flight Center. Spoolfile source: interactive solve/nuSolve analysis.) Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 0 Number of observations rejected during analysis: 5 observation 18, NYALES20:WETTZELL, NRAO512 , 07:05:30, which fits at -173.3 +/- 30.5 ps observation 34, ISHIOKA :NYALES20, 0613+570, 07:12:09, which fits at 252.4 +/- 50.1 ps observation 35, ISHIOKA :WETTZELL, 0613+570, 07:12:09, which fits at 323.7 +/- 51.6 ps observation 94, ISHIOKA :NYALES20, 0613+570, 07:35:48, which fits at 316.6 +/- 52.9 ps observation 95, ISHIOKA :WETTZELL, 0613+570, 07:35:48, which fits at 350.0 +/- 51.6 ps Other comments: Preliminary solution; the data for WETTZ13N have not arrived yet. Parameterization: 10 parameters: UT1 offset atmosphere offset for: ISHIOKA NYALES20 WETTZELL clock offset, first order term, and second order term for: NYALES20 WETTZELL Clock breaks: None Session Statistics Observations: 312 scheduled (from all stations---includes WETTZ13N) 156 scheduled (from available stations---does not include WETTZ13N) 156 correlated (included in the database) 156 recoverable (usable in Solve/nuSolve) 151 used Session fit: 37.836 ps UT1 formal error: 6.17 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 12 6 6 0059+581 18 9 9 0133+476 6 3 3 0613+570 12 6 2 0716+714 12 6 6 0718+793 12 6 6 0955+476 12 6 6 1030+415 6 3 3 1040+244 12 6 6 1053+704 6 3 3 1059+282 6 3 3 1128+385 12 6 6 1144+402 12 6 6 1156+295 18 9 9 1324+224 12 6 6 1417+385 6 3 3 NRAO512 18 9 8 1726+455 18 9 9 1803+784 18 9 9 1806+456 6 3 3 3C371 18 9 9 1849+670 12 6 6 3C418 18 9 9 2229+695 12 6 6 2309+454 18 9 9 ------------ --------- ---------- ------ Source Total 312 156 151 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.