IVS Analysis Report for I18257 ($18SEP14XU) 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: 8 observation 5, KOKEE :WETTZELL, 0307+380, 18:53:43, quality code X-band: 0 S-band: 0 observation 7, KOKEE :WETTZELL, 1418+546, 18:59:00, quality code X-band: 0 S-band: 0 observation 8, KOKEE :WETTZELL, 0716+714, 19:00:54, quality code X-band: 9 S-band: 0 observation 10, KOKEE :WETTZELL, 1300+580, 19:07:33, quality code X-band: 0 S-band: 9 observation 13, KOKEE :WETTZELL, 0016+731, 19:15:34, quality code X-band: 0 S-band: 9 observation 19, KOKEE :WETTZELL, 0749+540, 19:31:26, quality code X-band: 0 S-band: 9 observation 21, KOKEE :WETTZELL, 1300+580, 19:37:30, quality code X-band: 0 S-band: 9 observation 23, KOKEE :WETTZELL, 1418+546, 19:42:07, 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 WETTZELL clock offset, first order term, and second order term for: WETTZELL Clock breaks: None Session Statistics Observations: 24 scheduled 24 correlated (included in the database) 16 recoverable (usable in Solve/nuSolve) 16 used Session fit: 38.904 ps UT1 formal error: 12.18 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 1 1 0 0059+581 1 1 1 0133+476 1 1 1 0307+380 1 1 0 0529+483 2 2 2 0716+714 1 1 0 0738+491 1 1 1 0749+540 1 1 0 0800+618 1 1 1 0955+476 3 3 3 1053+815 1 1 1 1128+385 2 2 2 1144+402 1 1 1 1156+295 1 1 1 1300+580 2 2 0 1324+224 1 1 1 1418+546 2 2 0 1803+784 1 1 1 ------------ --------- ---------- ------ Source Total 24 24 16 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.