IVS Analysis Report for V21025 ($21JAN25VI) 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: - Extremely noise data. Number of observations rejected during correlation: 1 Number of observations not usable by the software: 1 observation 15, KOKEE12M:WETTZ13S, 1803+784, 18:49:39, quality code X: 0 S: -, fringe code X: ' ' S: '-' Number of observations rejected during analysis: 7 observation 5, KOKEE12M:WETTZ13S, 0016+731, 18:35:37, which fits at 278.4 +/- 76.9 ps observation 12, KOKEE12M:WETTZ13S, 1806+456, 18:46:26, which fits at -317.1 +/- 77.1 ps observation 20, KOKEE12M:WETTZ13S, 2215+150, 18:57:12, which fits at -271.1 +/- 77.5 ps observation 27, KOKEE12M:WETTZ13S, 2215+150, 19:07:05, which fits at -443.4 +/- 77.1 ps observation 35, KOKEE12M:WETTZ13S, 2215+150, 19:16:50, which fits at -795.3 +/- 77.1 ps observation 40, KOKEE12M:WETTZ13S, 1156+295, 19:24:29, which fits at -256.5 +/- 76.8 ps observation 41, KOKEE12M:WETTZ13S, 2215+150, 19:26:22, which fits at -778.0 +/- 77.0 ps Other comments: None. Parameterization: 6 parameters: UT1 offset atmosphere offset for: KOKEE12M WETTZ13S clock offset, first order term, and second order term for: WETTZ13S Clock breaks: None Session Statistics Observations: 45 scheduled 44 correlated (included in the database) 43 recoverable (usable in Solve/nuSolve) 36 used Session fit: 70.230 ps UT1 formal error: 11.18 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 3 3 2 1039+811 2 2 2 1040+244 2 2 2 1156+295 1 1 0 1418+546 4 4 4 NGC6251 2 2 2 1746+470 3 3 3 1803+784 3 3 2 1806+456 2 2 1 1849+670 2 1 1 2000+472 5 5 5 2113+293 5 5 5 2155+312 1 1 1 2214+350 3 3 3 2215+150 4 4 0 2309+454 3 3 3 ------------ --------- ---------- ------ Source Total 45 44 36 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.