USNO Analysis Report for Q21024 ($21JAN24XK) 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: 4 observation 2, WETTZELL:MK-VLBA , 1059+282, 07:31:10, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 20, WETTZELL:MK-VLBA , 0418+532, 07:52:37, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 35, WETTZELL:MK-VLBA , NGC6251 , 08:10:29, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 38, WETTZELL:MK-VLBA , 1059+282, 08:17:08, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 2 observation 22, WETTZELL:MK-VLBA , 1059+282, 07:55:44, which fits at 11745.1 +/- 106.7 ps observation 27, WETTZELL:MK-VLBA , 2353+816, 08:00:42, which fits at 3489.7 +/- 64.4 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: 49 scheduled 49 correlated (included in the database) 45 recoverable (usable in Solve/nuSolve) 43 used Session fit: 40.645 ps UT1 formal error: 5.96 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 0 0529+483 1 1 1 0613+570 2 2 2 0642+449 1 1 1 0716+714 3 3 3 0738+491 1 1 1 0805+410 1 1 1 0814+425 1 1 1 0821+394 1 1 1 0955+476 3 3 3 1030+415 1 1 1 1039+811 3 3 3 1040+244 3 3 3 1053+704 3 3 3 1059+282 3 3 0 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 49 49 43 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.