NASA Analysis Report for Q21094 ($21APR04XK) 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: 5 observation 16, WETTZELL:MK-VLBA 1849+670, 07:48:29, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' observation 18, WETTZELL:MK-VLBA NGC6251 , 07:51:10, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 19, WETTZELL:MK-VLBA 0418+532, 07:53:11, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 34, WETTZELL:MK-VLBA 1616+063, 08:12:41, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' observation 39, WETTZELL:MK-VLBA 1849+670, 08:19:20, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 1 observation 1, WETTZELL:MK-VLBA 1514+197, 07:30:27, which fits at 459.3 +/- 38.8 ps Other comments: None. Parameterization: 6 parameters: UT1 offset atmosphere offset for: MK-VLBA WETTZELL clock offset, first order term, and second order term for: WETTZELL Clock breaks: None Session Statistics Observations: 48 scheduled 48 correlated (included in the database) 43 recoverable (usable in Solve/nuSolve) 42 used Session fit: 23.663 ps UT1 formal error: 3.88 microsec Source Performance Number of Observations Scheduled Correlated* Used 0418+532 1 1 0 0529+483 3 3 3 0552+398 2 2 2 0613+570 3 3 3 0642+449 3 3 3 0716+714 3 3 3 0738+491 3 3 3 0955+476 2 2 2 1039+811 3 3 3 1053+704 2 2 2 1417+385 3 3 3 1418+546 3 3 3 1504+377 2 2 2 1514+197 1 1 0 1606+106 1 1 1 1616+063 1 1 0 1617+229 1 1 1 NGC6251 1 1 0 1639+230 1 1 1 DA426 1 1 1 1803+784 2 2 2 3C371 2 2 2 1849+670 2 2 0 2353+816 2 2 2 ------------ --------- ---------- ------ Source Total 48 48 42 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.