NASA Analysis Report for Z24099 (20240408-z24099) 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 autoINT.js script, NVI inc, NASA Goddard Space Flight Center VLBI Analysis Center. Spoolfile source: automated nuSolve solutions.) Session scheduled at DACH, correlated at UTAS and analyzed at NASA Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 6 observation 22, HART15M :YARRA12M, 0332-403, 06:42:25, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 24, HOBART12:YARRA12M, 0332-403, 06:42:25, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 58, HART15M :YARRA12M, 0332-403, 07:02:40, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 60, HOBART12:YARRA12M, 0332-403, 07:02:40, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 67, HART15M :YARRA12M, 0405-385, 07:09:08, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 70, HART15M :YARRA12M, 0346-279, 07:10:39, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 0 Other comments: None. Parameterization: 10 parameters: UT1 offset atmosphere offset for: HART15M HOBART12 YARRA12M clock offset, first order term, and second order term for: HOBART12 YARRA12M Clock breaks: None Session statistics Observations: 99 scheduled 99 correlated (included in the database) 93 recoverable (usable in Solve/nuSolve) 93 used Session fit: 66.423 ps UT1 formal error: 13.65 microsec Source Performance Number of Observations Scheduled Correlated* Used 0003-066 6 6 6 0035-252 3 3 3 0048-427 3 3 3 0104-408 6 6 6 0119+115 6 6 6 0229+131 3 3 3 0235+164 6 6 6 0308-611 9 9 9 0332-403 9 9 5 0346-279 6 6 5 0402-362 9 9 9 0405-385 9 9 8 0437-454 3 3 3 0530-727 3 3 3 0537-441 3 3 3 1057-797 9 9 9 2255-282 6 6 6 ------------ --------- ---------- ------ Source Total 99 99 93 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.