NASA Analysis Report for Q20306 ($20NOV01XK) 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: 4 observation 19, KOKEE :WETTZELL, 3C371 , 07:53:26, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 20, KOKEE :WETTZELL, 1758+388, 07:55:04, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 26, KOKEE :WETTZELL, 0642+449, 08:02:50, quality code X: 0 S: 8, fringe code X: ' ' S: ' ' observation 33, KOKEE :WETTZELL, 2000+472, 08:12:46, quality code X: 0 S: 8, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 2 observation 10, KOKEE :WETTZELL, 0642+449, 07:40:53, which fits at -226.2 +/- 77.0 ps observation 14, KOKEE :WETTZELL, 2229+695, 07:46:57, which fits at -234.2 +/- 68.1 ps Other comments: The MK-VLBA logs were not applied during correlation or analysis. Parameterization: 6 parameters: UT1 offset atmosphere offset for: KOKEE WETTZELL clock offset, first order term, and second order term for: WETTZELL Clock breaks: None Session Statistics Observations: 45 scheduled 45 correlated (included in the database) 41 recoverable (usable in Solve/nuSolve) 39 used Session fit: 48.035 ps UT1 formal error: 7.68 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 3 3 3 0059+581 3 3 3 0133+476 3 3 3 0529+483 3 3 3 0552+398 3 3 3 0613+570 2 2 2 0642+449 3 3 1 0716+714 2 2 2 1039+811 3 3 3 1746+470 1 1 1 1751+288 2 2 2 1758+388 1 1 0 1803+784 3 3 3 3C371 3 3 2 1846+322 1 1 1 1849+670 2 2 2 2000+472 2 2 1 3C418 3 3 3 2229+695 2 2 1 ------------ --------- ---------- ------ Source Total 45 45 39 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.