IVS Analysis Report for S22312 ($22NOV08VJ) 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 3, MACGO12M:WETTZ13S, 1936-155, 19:46:26, which fits at 550.5 +/- 91.8 ps observation 18, MACGO12M:WETTZ13S, 1639+230, 19:56:03, which fits at -446.1 +/- 91.1 ps observation 21, MACGO12M:WETTZ13S, 0917+624, 19:57:58, which fits at 417.4 +/- 91.1 ps observation 62, MACGO12M:WETTZ13S, 2126-158, 20:25:55, which fits at -1111.1 +/- 91.2 ps observation 69, MACGO12M:WETTZ13S, 4C67.05 , 20:30:20, which fits at 362.3 +/- 91.4 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: 90 scheduled 90 correlated (included in the database) 90 recoverable (usable in Solve/nuSolve) 85 used Session fit: 87.699 ps UT1 formal error: 10.95 microsec Source Performance Number of Observations Scheduled Correlated* Used 4C67.05 6 6 5 0602+673 2 2 2 0716+714 2 2 2 0917+449 2 2 2 0917+624 2 2 1 0920+390 1 1 1 4C39.25 1 1 1 0954+658 2 2 2 0955+476 2 2 2 1053+704 1 1 1 1504+377 1 1 1 1633+38 6 6 6 NRAO512 6 6 6 1639+230 2 2 1 DA426 5 5 5 1732+389 4 4 4 1739+522 1 1 1 1746+470 2 2 2 1749+096 1 1 1 1751+288 5 5 5 1803+784 1 1 1 3C371 1 1 1 1821+107 2 2 2 1846+322 1 1 1 1936-155 1 1 0 1958-179 1 1 1 2000+472 1 1 1 2008-159 2 2 2 2029+121 2 2 2 3C418 1 1 1 2059+034 2 2 2 2113+293 1 1 1 2126-158 1 1 0 2144+092 3 3 3 2201+171 2 2 2 2214+241 3 3 3 2214+350 6 6 6 2215+150 2 2 2 2319+317 3 3 3 ------------ --------- ---------- ------ Source Total 90 90 85 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.