NASA Analysis Report for Q20256 ($20SEP12XK) 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 Sergei Bolotin, NVI, Inc. / NASA Goddard Space Flight Center. Spoolfile source: interactive solve/nuSolve analysis.) Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 3 observation 2, ZELL:MK-VLBA 141, +546 , 07:31:51, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 16, ZELL:MK-VLBA 184, +681 , 07:47:56, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 33, ZELL:MK-VLBA 184, +681 , 08:09:35, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 4 observation 1, ZELL:MK-VLBA 150, +377 , 07:30:32, which fits at 3581.4 +/- 58.3 ps observation 13, ZELL:MK-VLBA 230, +454 , 07:44:30, which fits at 3489.9 +/- 49.3 ps observation 28, ZELL:MK-VLBA 173, +389 , 08:02:48, which fits at 3512.6 +/- 73.6 ps observation 38, ZELL:MK-VLBA 235, +816 , 08:16:54, which fits at 3491.0 +/- 46.1 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) 45 recoverable (usable in Solve/nuSolve) 41 used Session fit: 36.771 ps UT1 formal error: 6.01 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 3 3 3 0059+581 3 3 3 0133+476 3 3 3 0202+319 2 2 2 0235+164 2 2 2 0322+222 1 1 1 0718+793 2 2 2 1039+811 3 3 3 1418+546 1 1 0 1504+377 1 1 0 NRAO512 1 1 1 1726+455 3 3 3 1732+389 1 1 0 1746+470 1 1 1 1803+784 3 3 3 1806+456 2 2 2 3C371 3 3 3 1842+681 2 2 0 1849+670 2 2 2 2000+472 1 1 1 3C418 2 2 2 2229+695 2 2 2 2309+454 2 2 1 2353+816 2 2 1 ------------ --------- ---------- ------ Source Total 48 48 41 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.