IVS Analysis Report for Q17254 ($17SEP11XK) 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: 6 The following observations were not correlated: the three observations of 1040+244 at 07:40:33 by the NYALES20 baselines the three observations of 1800+440 at 07:42:54 by the NYALES20 baselines Number of observations not usable by the software: 2 The following observation had a quality code of 0 in X-band: observation 93, ISHIOKA :NYALES20, 2229+695, 07:28:16 The following observation had a quality code of 0 in S-band: observation 147, ISHIOKA :NYALES20, 2000+472, 07:45:03 Number of observations rejected during analysis: 34 The WETTZ13N-WETTZELL baseline was deselected to follow current procedures at the GSFC VLBI Analysis Center. Other comments: None. Parameterization: 14 parameters: UT1 offset atmosphere offset for: ISHIOKA NYALES20 WETTZ13N WETTZELL clock offset, first order term, and second order term for: NYALES20 WETTZ13N WETTZELL Clock breaks: None Session Statistics Observations: 204 scheduled 198 correlated (included in the database) 196 recoverable (usable in Solve/nuSolve) 162 used Session fit: 39.687 ps UT1 formal error: 6.10 microsec Source Performance Number of Observations Scheduled Correlated* Used 0059+581 6 6 5 0718+793 6 6 5 0804+499 12 12 10 0805+410 6 6 5 0955+476 12 12 10 1128+385 12 12 10 1156+295 6 6 5 1300+580 12 12 10 1418+546 6 6 5 NRAO512 18 18 15 DA426 6 6 5 1726+455 6 6 5 1803+784 6 6 5 1800+440 12 9 7 2000+472 12 12 9 2229+695 6 6 4 0716+714 6 6 5 1040+244 18 15 12 1144+402 6 6 5 0016+731 6 6 5 1030+415 12 12 10 1039+811 6 6 5 1849+670 6 6 5 ------------ --------- ---------- ------ Source Total 204 198 162 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.