BKG Analysis Report for Q22003 (22JAN03XK) 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 Dieter Ullrich, 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: 1 observation 188, 2229+695, ISHIOKA :NYALES20, 07:42:21, quality codes - S:9, X:0 Number of observations rejected during analysis: 3 observation 145, ISHIOKA :NYALE13S, 3C371, 07:33:05, which fits at -155.4 +/- 46.4 ps observation 220, NYALE13S:NYALES20, 0529+483, 07:50:11, which fits at -1285.1 +/- 52.8 ps observation 242, ISHIOKA :NYALES20, 2113+293, 07:56:34, which fits at -183.8 +/- 61.6 ps Other comments: Ny cabledata suspicious, not applied The vgosDb BKG analysis output is available at ftp://ivs.bkg.bund.de/pub/vlbi/ivsdata/vgosdb_bkg/22JAN03XK.tgz Parameterization: 14 parameters: UT1 offset atmosphere offset for: ISHIOKA NYALE13S NYALES20 WETTZELL clock offset (0), first order term (1), and/or second order term (2) for: ISHIOKA(0,1,2) NYALE13S(0,1,2) NYALES20 (0,1,2) Clock breaks: None. ----------------------------------------- Session Statistics Observations: 430 scheduled (included in correlation report) 258 correlated (included in database) 257 recoverable (usable in Solve/nuSolve) 254 used Session fit: 40.002 ps UT1 formal error: 4.360 microsec ----------------------------------------- Source Performance Number of Observations Scheduled(*) Correlated* Used 0016+731 30 18 18 0059+581 30 18 18 0133+476 20 12 12 0529+483 10 6 5 0552+398 20 12 12 0613+570 30 18 18 0642+449 30 18 18 1039+811 20 12 12 1749+096 20 12 12 1751+288 30 18 18 1803+784 40 24 24 2000+472 30 18 18 2113+293 30 18 17 2229+695 20 12 11 3C371 30 18 17 3C418 40 24 24 ------------ --------- ---------- ------ Source Total 430 258 254 * 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.