BKG Analysis Report for V22286 (22OCT13VI) This report is a contributed analysis report that does not correspond to the database maintained by the IVS Data Centers for this session. (Analyzed by Anastasiia Girdiuk, Federal Agency for Cartography and Geodesy (BKG), Spoolfile source: interactive 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: 4 observation 12, KOKEE12M:WETTZ13S, 0718+793, 18:39:15, which fits at -164.8 +/- 33.0 ps observation 15, KOKEE12M:WETTZ13S, NGC6251, 18:42:17, which fits at -189.2 +/- 34.7 ps observation 22, KOKEE12M:WETTZ13S, 0718+793, 18:49:38, which fits at -175.6 +/- 33.2 ps observation 33, KOKEE12M:WETTZ13S, 0718+793, 18:59:59, which fits at -198.5 +/- 32.7 ps Other comments: The vgosDb BKG analysis output is available at https://ivs.bkg.bund.de/data_dir/vlbi/ivsdata/vgosdb_bkg/22OCT13VI.tgz Parameterization: 6 parameters: UT1 offset atmosphere offset for: KOKEE12M WETTZ13S clock offset (0), first order term (1), and/or second order term (2) for: KOKEE12M (0,1,2) Clock breaks: None. ----------------------------------------- Session Statistics Observations: 62 scheduled (included in correlation report) 62 correlated (included in database) 62 recoverable (usable in Solve/nuSolve) 58 used Session fit: 30.688 ps UT1 formal error: 3.730 microsec ----------------------------------------- Source Performance Number of Observations Scheduled(*) Correlated* Used 0016+731 2 2 2 0552+398 4 4 4 0602+673 4 4 4 0613+570 2 2 2 0716+714 4 4 4 0718+793 3 3 0 0738+491 5 5 5 0749+540 5 5 5 1053+704 2 2 2 1306+360 2 2 2 1308+328 1 1 1 1417+385 4 4 4 1418+546 5 5 5 1504+377 4 4 4 1520+319 5 5 5 1538+149 2 2 2 1636+473 2 2 2 1803+784 4 4 4 NGC6251 2 2 1 ------------ --------- ---------- ------ Source Total 62 62 58 * Correlated means included in the database. (*) All possible observations on scheduled network. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.