USNO Analysis Report for I19346 ($19DEC12XU) 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 Christopher Dieck, US Naval Observatory. Spoolfile source: interactive nuSolve analysis.) Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 7 observation 1, MK-VLBA :WETTZELL, 2229+695, 18:30:20, quality codes - S:0, X:0 observation 4, MK-VLBA :WETTZELL, 1300+580, 18:36:05, quality codes - S:9, X:0 observation 5, MK-VLBA :WETTZELL, 1520+437, 18:38:35, quality codes - S:9, X:0 observation 7, MK-VLBA :WETTZELL, 1053+815, 18:42:45, quality codes - S:9, X:0 observation 19, MK-VLBA :WETTZELL, 1300+580, 19:06:53, quality codes - S:9, X:0 observation 25, MK-VLBA :WETTZELL, 2013+163, 19:18:05, quality codes - S:0, X:0 observation 30, MK-VLBA :WETTZELL, 1300+580, 19:29:33, quality codes - S:9, X:0 Number of observations rejected during analysis: 1 observation 16, MK-VLBA :WETTZELL, 1342+662, 19:00:37, which fits at 1232.9 +/- 55.7 ps Other comments: None. Parameterization: 5 parameters: UT1 offset atmosphere offset for: MK-VLBA WETTZELL clock offset (0), first order term (1), and/or second order term (2) for: WETTZELL (0,1) Clock breaks: None Session Statistics Observations: 30 scheduled 30 correlated (included in the database) 23 recoverable (usable in Solve/nuSolve) 22 used Session fit: 30.121 ps UT1 formal error: 6.15 microsec Source Performance Number of Observations Scheduled Correlated* Used 0800+618 1 1 1 0805+410 1 1 1 0955+476 2 2 2 1015+359 1 1 1 1053+815 1 1 0 1300+580 3 3 0 1342+662 1 1 0 1418+546 2 2 2 1520+437 1 1 0 NGC6251 1 1 1 1636+473 2 2 2 NRAO512 2 2 2 DA426 1 1 1 1746+470 2 2 2 1758+388 2 2 2 1803+784 1 1 1 3C371 2 2 2 1929+226 2 2 2 2013+163 1 1 0 2229+695 1 1 0 ------------ --------- ---------- ------ Source Total 30 30 22 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.