NASA Analysis Report for Q23021 ($23JAN21XK) 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 Karen Baver, Goddard Space Flight Center VLBI Analysis Center. Spoolfile source: interactive solve/nuSolve analysis.) Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 7 observation 3, MK-VLBA :WETTZELL, 0059+581, 07:30:14, quality code X: 9 S: 0, fringe code X: '.' S: '.' observation 35, ISHIOKA :WETTZELL, 0059+581, 07:50:13, quality code X: 9 S: 0, fringe code X: '.' S: '.' observation 36, MK-VLBA :WETTZELL, 0059+581, 07:50:13, quality code X: S: -, fringe code X: ' ' S: ' ' observation 68, ISHIOKA :WETTZELL, 0059+581, 08:10:02, quality code X: 9 S: 0, fringe code X: '.' S: '.' observation 69, MK-VLBA :WETTZELL, 0059+581, 08:10:02, quality code X: 9 S: 0, fringe code X: '.' S: '.' observation 101, ISHIOKA :WETTZELL, 0059+581, 08:29:45, quality code X: 9 S: 0, fringe code X: '.' S: '.' observation 102, MK-VLBA :WETTZELL, 0059+581, 08:29:45, quality code X: 9 S: 0, fringe code X: '.' S: '.' Number of observations rejected during analysis: 0 Other comments: None. Parameterization: 10 parameters: UT1 offset atmosphere offset for: ISHIOKA MK-VLBA WETTZELL clock offset, first order term, and second order term for: ISHIOKA MK-VLBA Clock breaks: None Session statistics Observations: 102 scheduled 102 correlated (included in the database) 95 recoverable (usable in Solve/nuSolve) 95 used Session fit: 34.860 ps UT1 formal error: 5.95 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 9 9 9 0059+581 12 12 5 0133+476 9 9 9 0602+673 3 3 3 0613+570 6 6 6 0642+449 9 9 9 0738+491 9 9 9 0805+410 9 9 9 0814+425 9 9 9 0955+476 6 6 6 1039+811 9 9 9 1053+704 6 6 6 1803+784 6 6 6 ------------ --------- ---------- ------ Source Total 102 102 95 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.