BKG Analysis Report for q23161 (20230610-q23161) 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 Gerald Engelhardt, 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: 2 observation 3, 2013+163, WETTZELL:MK-VLBA , 07:35:00, quality codes - S:0, X:9 observation 20, 2013+163, WETTZELL:MK-VLBA , 08:01:06, quality codes - S:9, X:0 Number of observations rejected during analysis: 2 observation 1, WETTZELL:MK-VLBA , 0821+394, 07:30:38, which fits at 468.9 +/- 46.7 ps observation 27, WETTZELL:MK-VLBA , 1732+389, 08:14:33, which fits at 204.3 +/- 37.8 ps Other comments: The vgosDb BKG analysis output is available at ftp://ivs.bkg.bund.de/pub/vlbi/ivsdata/vgosdb_bkg/20230610-q23161.tgz Parameterization: 6 parameters: UT1 offset atmosphere offset for: MK-VLBA WETTZELL clock offset (0), first order term (1), and/or second order term (2) for: MK-VLBA (0,1,2) Clock breaks: None. ----------------------------------------- Session Statistics Observations: 34 scheduled (included in correlation report) 34 correlated (included in database) 32 recoverable (usable in Solve/nuSolve) 30 used Session fit: 40.991 ps UT1 formal error: 6.160 microsec ----------------------------------------- Source Performance Number of Observations Scheduled(*) Correlated* Used 0016+731 1 1 1 0814+425 1 1 1 0821+394 1 1 0 0920+390 1 1 1 0955+476 2 2 2 1015+359 1 1 1 1030+415 2 2 2 1039+811 1 1 1 1053+704 1 1 1 1732+389 2 2 1 1758+388 2 2 2 1800+440 2 2 2 1803+784 1 1 1 1806+456 2 2 2 1846+322 1 1 1 1851+488 2 2 2 1929+226 2 2 2 2000+472 2 2 2 2013+163 3 3 1 2106+143 1 1 1 2113+293 1 1 1 2229+695 1 1 1 3C418 1 1 1 ------------ --------- ---------- ------ Source Total 34 34 30 * 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.