USNO Analysis Report for W19346 ($19DEC12XW) 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 24, PIETOWN :WETTZ13N, 0641+392, 07:31:44, quality codes - S:8, X:0 observation 46, MK-VLBA :PIETOWN , OJ287 , 07:52:41, quality codes - S:0, X:0 observation 47, MK-VLBA :WETTZ13N, OJ287 , 07:52:41, quality codes - S:0, X:0 observation 49, MK-VLBA :PIETOWN , 0920+390, 07:54:24, quality codes - S:0, X:0 observation 50, MK-VLBA :WETTZ13N, 0920+390, 07:54:24, quality codes - S:0, X:0 observation 61, MK-VLBA :PIETOWN , 0955+476, 08:03:12, quality codes - S:0, X:0 observation 62, MK-VLBA :WETTZ13N, 0955+476, 08:03:12, quality codes - S:0, X:0 Number of observations rejected during analysis: 1 observation 112, MK-VLBA :PIETOWN , 2356+385, 08:42:42, which fits at 216.1 +/- 43.7 ps Other comments: None. Parameterization: 8 parameters: UT1 offset atmosphere offset for: MK-VLBA PIETOWN WETTZ13N clock offset (0), first order term (1), and/or second order term (2) for: PIETOWN (0,1) WETTZ13N (0,1) Clock breaks: None Session Statistics Observations: 159 scheduled 159 correlated (included in the database) 152 recoverable (usable in Solve/nuSolve) 151 used Session fit: 37.434 ps UT1 formal error: 4.49 microsec Source Performance Number of Observations Scheduled Correlated* Used 0059+581 9 9 9 0133+476 12 12 12 0345+460 12 12 12 0415+398 3 3 3 0529+483 12 12 12 0552+398 6 6 6 0613+570 12 12 12 0641+392 3 3 2 0714+457 3 3 3 0716+714 9 9 9 0738+491 9 9 9 0748+126 6 6 6 0759+183 6 6 6 0804+499 6 6 6 0805+410 9 9 9 OJ287 9 9 7 0920+390 3 3 1 0955+476 9 9 7 1053+815 3 3 3 NGC6251 3 3 3 1803+784 6 6 6 2229+695 6 6 6 2356+385 3 3 2 ------------ --------- ---------- ------ Source Total 159 159 151 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.