IVS Analysis Report for W19023 ($19JAN23XW) 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: 0 Number of observations not usable by the software: 3 observation 98, MK-VLBA :WETTZELL, NGC6251 , 08:28:08, quality code X-band: 9 S-band: 0 observation 99, PIETOWN :WETTZELL, NGC6251 , 08:28:08, quality code X-band: 9 S-band: 0 observation 143, MK-VLBA :WETTZELL, NGC6251 , 09:07:02, quality code X-band: 9 S-band: 0 Number of observations rejected during analysis: 1 observation 71, MK-VLBA :WETTZELL, 0920+390, 08:09:57, which fits at 2708.2 +/- 52.5 ps Other comments: WETTZ13N was included in the schedule but was not supposed to be, according to the correlator report. MK-VLBA (Mk/m): Removed channel(s) from fringe fitting: SR3U Parameterization: 10 parameters: UT1 offset atmosphere offset for: MK-VLBA PIETOWN WETTZELL clock offset, first order term, and second order term for: PIETOWN WETTZELL Clock breaks: None Session Statistics Observations: 231 scheduled (from all stations---includes WETTZ13N) 153 scheduled (from available stations---does not include WETTZ13N) 153 correlated (included in the database) 150 recoverable (usable in Solve/nuSolve) 149 used Session fit: 49.232 ps UT1 formal error: 5.33 microsec Source Performance Number of Observations Scheduled Correlated* Used 0059+581 12 6 6 0133+476 24 12 12 0345+460 12 12 12 0529+483 12 6 6 0613+570 18 9 9 0714+457 3 3 3 0716+714 18 9 9 0718+793 3 3 3 0738+491 6 6 6 0800+618 6 6 6 0805+410 12 6 6 0920+390 6 6 5 0955+476 12 6 6 1015+359 6 6 6 1040+244 18 9 9 1053+815 3 3 3 1111+149 6 6 6 1128+385 6 3 3 1144+402 6 3 3 1156+295 6 3 3 1300+580 12 12 12 1342+662 6 6 6 NGC6251 6 6 3 1803+784 6 3 3 2229+695 6 3 3 ------------ --------- ---------- ------ Source Total 231 153 149 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.