BKG Analysis Report for C22162 (22JUN11VC) 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: 2 observation 95, ISHIOKA :ONSA13SW, 1015+359, 09:36:26, which fits at 263.5 +/- 50.0 ps observation 107, ISHIOKA :ONSA13SW, 1823+568, 09:42:39, which fits at 349.1 +/- 48.9 ps Other comments: The vgosDb BKG analysis output is available at ftp://ivs.bkg.bund.de/pub/vlbi/ivsdata/vgosdb_bkg/22JUN11VC.tgz Parameterization: 6 parameters: UT1 offset atmosphere offset for: ISHIOKA ONSA13SW clock offset (0), first order term (1), and/or second order term (2) for: ONSA13SW (0,1,2) Clock breaks: None. ----------------------------------------- Session Statistics Observations: 222 scheduled (included in correlation report) 111 correlated (included in database) 111 recoverable (usable in Solve/nuSolve) 109 used Session fit: 47.222 ps UT1 formal error: 4.480 microsec ----------------------------------------- Source Performance Number of Observations Scheduled(*) Correlated* Used 0059+581 9 3 3 0300+470 3 1 1 0528+134 3 1 1 0529+483 9 3 3 0536+145 3 1 1 0556+238 6 2 2 0602+405 12 4 4 0602+673 12 4 4 0657+172 9 3 3 0716+714 12 4 4 0749+540 6 2 2 0754+100 12 4 4 0800+618 3 1 1 0805+410 12 4 4 0805-077 3 1 1 0808+019 12 4 4 0812+367 12 4 4 0823+033 12 4 4 0917+449 12 4 4 1015+359 6 2 1 1030+415 12 4 4 1040+244 6 2 2 1053+704 12 4 4 1128+385 9 3 3 1417+385 6 2 2 1418+546 12 4 4 1732+389 15 5 5 1823+568 12 4 3 1846+322 9 3 3 1849+670 12 4 4 2000+472 3 1 1 2229+695 12 4 4 3C418 12 4 4 DA426 12 4 4 NGC6251 9 3 3 NRAO512 12 4 4 ------------ --------- ---------- ------ Source Total 222 111 109 * 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.