IVS Analysis Report for V21344 ($21DEC10VI) 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: 7 observation 29, KOKEE12M:WETTZ13S, 1030+415, 18:40:25, which fits at -448.7 +/- 91.2 ps observation 46, KOKEE12M:WETTZ13S, 1030+415, 18:51:12, which fits at -293.7 +/- 91.1 ps observation 62, KOKEE12M:WETTZ13S, 0529+483, 18:59:07, which fits at -323.7 +/- 90.7 ps observation 69, KOKEE12M:WETTZ13S, 1030+415, 19:04:43, which fits at -361.5 +/- 91.0 ps observation 92, KOKEE12M:WETTZ13S, 0529+483, 19:16:42, which fits at -423.7 +/- 90.7 ps observation 93, WESTFORD:WETTZ13S, 0529+483, 19:16:42, which fits at -445.9 +/- 76.2 ps observation 101, KOKEE12M:WETTZ13S, 1030+415, 19:21:26, which fits at -390.9 +/- 91.0 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: 43 scheduled 43 correlated (included in the database) 43 recoverable (usable in Solve/nuSolve) 41 used Session fit: 54.947 ps UT1 formal error: 8.75 microsec Source Performance Number of Observations Scheduled Correlated* Used 0716+714 2 2 2 0743+277 1 1 1 0920+390 1 1 1 1030+415 2 2 2 1039+811 2 2 2 1053+704 1 1 1 1308+554 3 3 3 1418+546 2 2 2 1636+473 4 4 4 NGC6251 1 1 1 NRAO512 2 2 2 DA426 2 2 2 1746+470 3 3 3 1751+288 2 2 2 1758+388 2 2 2 1803+784 1 1 1 1806+456 1 1 1 1823+689 2 2 2 1849+670 2 2 2 1909+161 2 2 2 1929+226 2 2 0 2000+472 3 3 3 ------------ --------- ---------- ------ Source Total 43 43 41 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.