USNO Analysis Report for W19063 ($19MAR04XW) 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: 1 MK-VLBA :WETTZ13N, 0955+476, 09:40:08 --- not in data base: probable G- or H- code in one or both bands Number of observations not usable by the software: 3 observation 65, MK-VLBA :WETTZELL, 1342+662, 09:02:38, quality codes - S:0, X:9 observation 71, MK-VLBA :WETTZELL, 0714+457, 09:08:07, quality codes - S:0, X:9 observation 215, MK-VLBA :WETTZELL, NGC6251 , 10:24:25, quality codes - S:0, X:9 Number of observations rejected during analysis: 24 The WETTZ13N:WETTZELL baseline was deselected, accounting for 23 observations. observation 190, PIETOWN :WETTZ13N, 0749+540, 10:12:33, which fits at 197.7 +/- 68.6 ps Other comments: None. Parameterization: 11 parameters: UT1 offset atmosphere offset for: MK-VLBA PIETOWN WETTZ13N WETTZELL clock offset (0), first order term (1), and/or second order term (2) for: PIETOWN (0,1) WETTZ13N (0,1) WETTZELL (0,1) Clock breaks: None Session Statistics Observations: 225 scheduled 224 correlated (included in the database) 220 recoverable (usable in Solve/nuSolve) 197 used Session fit: 44.456 ps UT1 formal error: 3.69 microsec Source Performance Number of Observations Scheduled Correlated* Used 0529+483 24 24 20 0552+398 12 12 11 0613+570 18 18 15 0714+457 3 3 2 0716+714 12 12 10 0718+793 3 3 3 0738+491 6 6 6 0749+540 9 9 7 0800+618 9 9 9 0955+476 18 17 14 1053+815 3 3 3 1128+385 6 6 5 1144+402 6 6 5 1226+373 3 3 3 1300+580 12 12 12 1324+224 3 3 3 1342+662 3 3 2 1418+546 18 18 15 1520+437 9 9 9 1606+106 12 12 10 NGC6251 3 3 2 1636+473 6 6 6 NRAO512 3 3 3 1639+230 3 3 3 1651+391 3 3 3 DA426 3 3 3 1803+784 6 6 5 3C371 6 6 5 1823+689 3 3 3 ------------ --------- ---------- ------ Source Total 225 224 197 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.