NASA Analysis Report for Q18077 ($18MAR18XK) 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: 25 The ISHIOKA-KASHIM34 baseline was not correlated because it is too short to provide a good UT1 estimation. Number of observations not usable by the software: 0 Number of observations rejected during analysis: 0 Other comments: WETTZELL was scheduled, but WETTZ13N replaced it because of equipment problems at WETTZELL. Parameterization: 10 parameters: UT1 offset atmosphere offset for: ISHIOKA KASHIM34 WETTZ13N clock offset, first order term, and second order term for: KASHIM34 WETTZ13N Clock breaks: None Session Statistics Observations: 75 scheduled 50 correlated (included in the database) 50 recoverable (usable in Solve/nuSolve) 50 used Session fit: 114.910 ps UT1 formal error: 25.65 microsec Source Performance Number of Observations Scheduled Correlated* Used 0059+581 9 6 6 0119+115 9 6 6 0552+398 3 2 2 0955+476 6 4 4 1128+385 3 2 2 1803+784 6 4 4 3C371 9 6 6 3C418 9 6 6 2229+695 3 2 2 0529+483 6 4 4 1144+402 3 2 2 0016+731 9 6 6 ------------ --------- ---------- ------ Source Total 75 50 50 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.