IVS Analysis Report for I19018 ($19JAN18XU) This report is the official IVS analysis report that corresponds 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: 2 observation of 1803+784 by KOKEE:WETTZ13N at 19:01:05 was not in the database --- possible G code observation of 2000+472 by KOKEE:WETTZ13N at 19:25:19 was not in the database --- possible G code Number of observations not usable by the software: 7 observation 1, KOKEE :WETTZ13N, 1128+385, 18:30:40, quality code X-band: 0 S-band: 0 observation 2, KOKEE :WETTZELL, 1128+385, 18:30:40, quality code X-band: 0 S-band: 0 observation 4, KOKEE :WETTZ13N, 2000+472, 18:34:23, quality code X-band: 9 S-band: 0 observation 5, KOKEE :WETTZELL, 2000+472, 18:34:23, quality code X-band: 9 S-band: 0 observation 47, KOKEE :WETTZELL, 2000+472, 19:26:57, quality code X-band: 9 S-band: 0 observation 56, KOKEE :WETTZ13N, 2000+472, 19:42:33, quality code X-band: 9 S-band: 0 observation 57, KOKEE :WETTZELL, 2000+472, 19:42:33, quality code X-band: 9 S-band: 0 Number of observations rejected during analysis: 19 The WETTZ13N:WETTZELL baseline was deselected. Other comments: None. Parameterization: 10 parameters: UT1 offset atmosphere offset for: KOKEE WETTZ13N WETTZELL clock offset, first order term, and second order term for: WETTZ13N WETTZELL Clock breaks: None Session Statistics Observations: 60 scheduled 58 correlated (included in the database) 51 recoverable (usable in Solve/nuSolve) 32 used Session fit: 57.531 ps UT1 formal error: 10.36 microsec Source Performance Number of Observations Scheduled Correlated* Used 0716+714 3 3 2 1030+415 6 6 4 1053+704 3 3 2 1128+385 6 6 2 1803+784 6 5 3 1849+670 6 6 4 2000+472 9 8 0 2113+293 3 3 3 2141+175 6 6 4 2229+695 6 6 4 2309+454 6 6 4 ------------ --------- ---------- ------ Source Total 60 58 32 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.