IVS Analysis Report for W19028 ($19JAN28XW) This report is the official IVS analysis report that corresponds to the database maintained by the IVS Data Centers for this session. (Analyzed by Sergei Bolotin, NVI, Inc. / NASA Goddard Space Flight Center. Spoolfile source: interactive solve/nuSolve analysis.) The session has been reanalyzed including cable calibration and meteo parameters from VLBA stations. Problems: WETTZELL and WETTZ13N did not observe. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 0 Number of observations rejected during analysis: 3 observation 1, MK-VLBA :PIETOWN , 1803+784, 08:30:20, which fits at -91.8 +/- 21.7 ps observation 13, MK-VLBA :PIETOWN , 1418+546, 08:57:46, which fits at 309.1 +/- 32.5 ps observation 50, MK-VLBA :PIETOWN , 1520+437, 10:28:11, which fits at 369.5 +/- 36.7 ps Other comments: Preliminary solution; the data for WETTZ13N and WETTZELL have not arrived yet. Parameterization: 6 parameters: UT1 offset atmosphere offset for: MK-VLBA PIETOWN clock offset, first order term, and second order term for: PIETOWN Clock breaks: None Session Statistics Observations: 219 scheduled (from all stations---includes WETTZ13N and WETTZELL) 50 scheduled (from available stations---does not include WETTZ13N and WETTZELL) 50 correlated (included in the database) 50 recoverable (usable in Solve/nuSolve) 47 used Session fit: 23.068 ps UT1 formal error: 17.13 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 6 1 1 0059+581 12 2 2 0133+476 6 1 1 0345+460 12 4 4 0415+398 6 2 2 0529+483 12 2 2 0613+570 12 2 2 0716+714 12 2 2 0718+793 3 1 1 0738+491 6 2 2 0749+540 3 1 1 0800+618 6 2 2 0920+390 3 1 1 0955+476 18 3 3 1053+815 3 1 1 1128+385 12 2 2 1144+402 12 2 2 1156+295 24 4 4 1212+171 3 1 1 1226+373 6 2 2 3C274 9 2 2 1300+580 9 3 3 1308+328 3 1 1 1324+224 6 2 2 1342+662 3 1 1 1418+546 3 1 0 1520+437 3 1 0 1803+784 6 1 0 ------------ --------- ---------- ------ Source Total 219 50 47 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.