NASA Analysis Report for Q18223 ($18AUG11XK) This report is a contributed analysis report that does not correspond 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: 8 observation 3, KOKEE :WETTZ13N, 2214+350, 07:33:42, quality code X-band: 0 S-band: 9 observation 10, KOKEE :WETTZ13N, NGC6251 , 07:51:14, quality code X-band: 0 S-band: 0 observation 11, KOKEE :WETTZ13N, 0016+731, 07:53:05, quality code X-band: 0 S-band: 9 observation 13, KOKEE :WETTZ13N, 1418+546, 07:57:12, quality code X-band: 9 S-band: 0 observation 16, KOKEE :WETTZ13N, 1520+437, 08:04:27, quality code X-band: 0 S-band: 9 observation 19, KOKEE :WETTZ13N, 1418+546, 08:10:38, quality code X-band: 9 S-band: 0 observation 24, KOKEE :WETTZ13N, 2214+350, 08:22:04, quality code X-band: 0 S-band: 9 observation 26, KOKEE :WETTZ13N, 1520+437, 08:27:39, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 0 Other comments: None. Parameterization: 6 parameters: UT1 offset atmosphere offset for: KOKEE WETTZ13N clock offset, first order term, and second order term for: WETTZ13N Clock breaks: None Session Statistics Observations: 26 scheduled 26 correlated (included in the database) 18 recoverable (usable in Solve/nuSolve) 18 used Session fit: 67.132 ps UT1 formal error: 16.38 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 1 1 0 0059+581 1 1 1 0133+476 2 2 2 0718+793 1 1 1 1053+815 1 1 1 1156+295 1 1 1 1300+580 2 2 2 1324+224 1 1 1 1418+546 2 2 0 1520+437 2 2 0 NGC6251 1 1 0 1636+473 2 2 2 1803+784 1 1 1 3C371 1 1 1 2214+350 2 2 0 2229+695 2 2 2 2319+317 3 3 3 ------------ --------- ---------- ------ Source Total 26 26 18 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.