NASA Analysis Report for Q20242 ($20AUG29XK) 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: 6 observation 1, WETTZELL:MK-VLBA , 0017+200, 07:30:15, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 5, WETTZELL:MK-VLBA , 1418+546, 07:34:52, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 10, WETTZELL:MK-VLBA , 0202+319, 07:41:01, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' observation 20, WETTZELL:MK-VLBA , 0017+200, 07:54:54, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 25, WETTZELL:MK-VLBA , 1418+546, 08:00:42, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 42, WETTZELL:MK-VLBA , 1418+546, 08:22:20, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 1 observation 32, WETTZELL:MK-VLBA , 2000+472, 08:10:52, which fits at 232.9 +/- 51.8 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: 47 scheduled 47 correlated (included in the database) 41 recoverable (usable in Solve/nuSolve) 40 used Session fit: 46.217 ps UT1 formal error: 8.05 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 3 3 3 0017+200 2 2 0 0059+581 3 3 3 0133+476 3 3 3 0202+319 3 3 2 0718+793 2 2 2 1039+811 3 3 3 1417+385 2 2 2 1418+546 3 3 0 1504+377 3 3 3 NRAO512 1 1 1 1726+455 2 2 2 1803+784 3 3 3 3C371 2 2 2 1842+681 1 1 1 1849+670 2 2 2 2000+472 2 2 1 3C418 1 1 1 2229+695 2 2 2 2309+454 2 2 2 2353+816 2 2 2 ------------ --------- ---------- ------ Source Total 47 47 40 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.