USNO Analysis Report for I20331 ($20NOV26XU) 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 Andrew Sargent, 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 2, MK-VLBA :WETTZELL, 0714+457, 18:33:15, quality codes - S:0, X:9 observation 13, MK-VLBA :WETTZELL, 1300+580, 18:51:52, quality codes - S:9, X:0 observation 18, MK-VLBA :WETTZELL, 1342+662, 19:03:32, quality codes - S:0, X:9 observation 23, MK-VLBA :WETTZELL, 1520+437, 19:14:02, quality codes - S:9, X:0 observation 24, MK-VLBA :WETTZELL, 1300+580, 19:16:32, quality codes - S:9, X:0 observation 27, MK-VLBA :WETTZELL, 1929+226, 19:23:48, quality codes - S:0, X:0 observation 29, MK-VLBA :WETTZELL, 2229+695, 19:29:45, quality codes - S:0, X:0 Number of observations rejected during analysis: 1 observation 7, MK-VLBA :WETTZELL, 3C371 , 18:41:30, which fits at -228.0 +/- 55.5 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: 29 scheduled 29 correlated (included in the database) 22 recoverable (usable in Solve/nuSolve) 21 used Session fit: 36.873 ps UT1 formal error: 8.52 microsec Source Performance Number of Observations Scheduled Correlated* Used 0714+457 1 1 0 0716+714 1 1 1 0749+540 1 1 1 0800+618 1 1 1 0805+410 1 1 1 0920+390 2 2 2 0955+476 2 2 2 1053+815 1 1 1 1300+580 2 2 0 1342+662 1 1 0 1418+546 1 1 1 1520+437 1 1 0 NGC6251 1 1 1 1636+473 2 2 2 NRAO512 2 2 2 1651+391 1 1 1 1732+389 1 1 1 1746+470 1 1 1 1758+388 1 1 1 1803+784 1 1 1 1800+440 1 1 1 3C371 1 1 0 1929+226 1 1 0 2229+695 1 1 0 ------------ --------- ---------- ------ Source Total 29 29 21 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.