BKG Analysis Report for V21350 (21DEC16VI) 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: 0 Number of observations rejected during analysis: 4 observation 10, KOKEE12M:WETTZ13S, 1909+161, 18:40:17, which fits at 246.1 +/- 46.5 ps observation 18, KOKEE12M:WETTZ13S, 1308+554, 18:51:42, which fits at -209.5 +/- 45.8 ps observation 24, KOKEE12M:WETTZ13S, 1909+161, 18:59:53, which fits at 182.2 +/- 45.8 ps observation 43, KOKEE12M:WETTZ13S, 1929+226, 19:28:30, which fits at -327.1 +/- 46.4 ps Other comments: The vgosDb BKG analysis output is available at ftp://ivs.bkg.bund.de/pub/vlbi/ivsdata/vgosdb_bkg/21DEC16VI.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: 44 scheduled (included in correlation report) 44 correlated (included in database) 44 recoverable (usable in Solve/nuSolve) 40 used Session fit: 41.509 ps UT1 formal error: 6.190 microsec ----------------------------------------- Source Performance Number of Observations Scheduled(*) Correlated* Used 0716+714 1 1 1 0827+243 3 3 3 1030+415 2 2 2 1039+811 2 2 2 1053+704 1 1 1 1308+554 3 3 2 1418+546 3 3 3 1636+473 4 4 4 1726+455 1 1 1 1746+470 3 3 3 1751+288 2 2 2 1758+388 2 2 2 1803+784 1 1 1 1823+689 1 1 1 1849+670 2 2 2 1909+161 2 2 0 1929+226 3 3 2 2000+472 4 4 4 DA426 1 1 1 NGC6251 1 1 1 NRAO512 2 2 2 ------------ --------- ---------- ------ Source Total 44 44 40 * 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.