IVS Analysis Report for Q18225 ($18AUG13XK) 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: 1 SESHAN25:WETTZELL, 1504+377, 07:49:54 --- not correlated in S-band Number of observations not usable by the software: 3 observation 4, SESHAN25:WETTZ13N, 2000+472, 07:02:59, quality code X-band: 9 S-band: 0 observation 34, SESHAN25:WETTZ13N, 0657+172, 07:34:48, quality code X-band: 0 S-band: 9 observation 35, SESHAN25:WETTZELL, 0657+172, 07:34:48, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 20 The WETTZ13N:WETTZELL baseline was deselected according to standard procedures at the GSFC VLBI Analysis Center. But the correlator also noted that the baseline was not usable. Other comments: NYALES20 did not observe. Parameterization: 10 parameters: UT1 offset atmosphere offset for: SESHAN25 WETTZ13N WETTZELL clock offset, first order term, and second order term for: WETTZ13N WETTZELL Clock breaks: None Session Statistics Observations: 120 scheduled (from all stations---includes NYALES20) 60 scheduled (from available stations---does not include NYALES20) 59 correlated (included in the database) 56 recoverable (usable in Solve/nuSolve) 36 used Session fit: 96.973 ps UT1 formal error: 22.57 microsec Source Performance Number of Observations Scheduled Correlated* Used OJ287 6 3 2 1053+815 6 3 2 3C274 6 3 2 1418+546 6 3 2 1726+455 6 3 2 3C371 6 3 2 0657+172 6 3 0 0912+029 6 3 2 1145+268 6 3 2 2000+472 6 3 1 2229+695 6 3 2 0529+483 6 3 2 0716+714 6 3 2 1040+244 6 3 2 1053+704 6 3 2 0016+731 6 3 2 1806+456 6 3 2 0736+017 6 3 2 0814+425 6 3 2 1504+377 6 2 1 ------------ --------- ---------- ------ Source Total 120 59 36 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.