IVS Analysis Report for S22158 ($22JUN07VJ) 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: 1 observation 82, MACGO12M:WETTZ13S, 0552+398, 20:40:00, quality code X: 4 S: -, fringe code X: ' ' S: '-' Number of observations rejected during analysis: 3 observation 32, MACGO12M:WETTZ13S, 1642+690, 20:06:40, which fits at -185.1 +/- 43.8 ps observation 34, MACGO12M:WETTZ13S, 4C67.05 , 20:07:44, which fits at -165.5 +/- 44.2 ps observation 44, MACGO12M:WETTZ13S, 1059+282, 20:13:05, which fits at -143.4 +/- 44.4 ps Other comments: None. Parameterization: 6 parameters: UT1 offset atmosphere offset for: MACGO12M WETTZ13S clock offset, first order term, and second order term for: WETTZ13S Clock breaks: None Session statistics Observations: 88 scheduled 88 correlated (included in the database) 87 recoverable (usable in Solve/nuSolve) 84 used Session fit: 42.348 ps UT1 formal error: 6.26 microsec Source Performance Number of Observations Scheduled Correlated* Used 0110+495 2 2 2 4C67.05 1 1 0 0300+470 2 2 2 0529+483 6 6 6 0552+398 7 7 6 0602+405 5 5 5 0602+673 1 1 1 0642+449 2 2 2 0716+714 1 1 1 0748+126 1 1 1 0754+100 1 1 1 0759+183 2 2 2 0808+019 1 1 1 0812+367 1 1 1 0823+033 1 1 1 0827+243 2 2 2 OJ287 2 2 2 0912+029 2 2 2 0917+624 1 1 1 4C39.25 1 1 1 0954+658 1 1 1 1030+415 1 1 1 1038+064 3 3 3 1040+244 1 1 1 1045-188 2 2 2 1059+282 1 1 0 1124-186 1 1 1 1128+385 5 5 5 1144+402 5 5 5 1149-084 1 1 1 1156+295 1 1 1 3C274 1 1 1 1300+580 5 5 5 1418+546 6 6 6 NGC6251 1 1 1 1642+690 2 2 1 1803+784 2 2 2 3C371 2 2 2 1849+670 2 2 2 2007+777 3 3 3 ------------ --------- ---------- ------ Source Total 88 88 84 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.