USNO Analysis Report for Q21031 ($21JAN31XK) 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 Nicole Geiger, 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: 1 observation 14, WETTZELL:MK-VLBA , NGC6251 , 07:44:29, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 6 observation 2, WETTZELL:MK-VLBA , 1059+282, 07:31:10, which fits at -1737.3 +/- 115.2 ps observation 7, WETTZELL:MK-VLBA , 2353+816, 07:36:09, which fits at -541.2 +/- 63.6 ps observation 24, WETTZELL:MK-VLBA , 1040+244, 07:58:51, which fits at -207.3 +/- 58.3 ps observation 25, WETTZELL:MK-VLBA , 1059+282, 07:59:47, which fits at 11727.3 +/- 111.5 ps observation 37, WETTZELL:MK-VLBA , 1030+415, 08:14:10, which fits at -3624.5 +/- 71.8 ps observation 46, WETTZELL:MK-VLBA , 1053+704, 08:24:40, which fits at -3566.7 +/- 61.8 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: MK-VLBA (0,1) Clock breaks: None Session Statistics Observations: 51 scheduled 51 correlated (included in the database) 50 recoverable (usable in Solve/nuSolve) 44 used Session fit: 49.062 ps UT1 formal error: 6.95 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 3 3 3 0059+581 3 3 3 0133+476 3 3 3 0418+532 1 1 1 0529+483 2 2 2 0613+570 2 2 2 0642+449 1 1 1 0716+714 2 2 2 0738+491 2 2 2 0805+410 1 1 1 0814+425 2 2 2 0821+394 1 1 1 0955+476 2 2 2 1030+415 2 2 1 1039+811 3 3 3 1040+244 3 3 2 1053+704 3 3 2 1059+282 3 3 1 1128+385 3 3 3 1144+402 3 3 3 1145+268 1 1 1 NGC6251 1 1 0 1803+784 1 1 1 2353+816 3 3 2 ------------ --------- ---------- ------ Source Total 51 51 44 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.