IVS Analysis Report for Q20062 ($20MAR02XK) 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: 9 observation 42, WETTZ13N:WETTZELL, 0059+581, 07:07:22, quality code X-band: 9 S-band: 4 observation 92, ISHIOKA :WETTZ13N, 0017+200, 07:19:20, quality code X-band: 0 S-band: 9 observation 104, ISHIOKA :WETTZ13N, 2309+454, 07:21:37, quality code X-band: 0 S-band: 9 observation 110, ISHIOKA :WETTZ13N, 2229+695, 07:22:49, quality code X-band: 0 S-band: 9 observation 128, ISHIOKA :WETTZ13N, 1842+681, 07:26:25, quality code X-band: 0 S-band: 9 observation 152, ISHIOKA :WETTZ13N, 1030+415, 07:32:42, quality code X-band: 0 S-band: 9 observation 230, ISHIOKA :WETTZ13N, 0017+200, 07:49:50, quality code X-band: 0 S-band: 9 observation 248, ISHIOKA :WETTZ13N, 2309+454, 07:53:21, quality code X-band: 0 S-band: 9 observation 254, ISHIOKA :WETTZ13N, 2229+695, 07:54:33, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 13 observation 66, WETTZ13N:WETTZELL, 1053+704, 07:12:33, which fits at 2692.4 +/- 66.2 ps observation 96, WETTZ13N:WETTZELL, 0017+200, 07:19:20, which fits at -3911.4 +/- 66.8 ps observation 102, WETTZ13N:WETTZELL, 0025+197, 07:20:21, which fits at 3189.6 +/- 67.6 ps observation 108, WETTZ13N:WETTZELL, 2309+454, 07:21:37, which fits at -607.7 +/- 67.0 ps observation 132, WETTZ13N:WETTZELL, 1842+681, 07:26:25, which fits at -13458.8 +/- 68.6 ps observation 144, WETTZ13N:WETTZELL, 2215+150, 07:29:19, which fits at 1418.9 +/- 66.9 ps observation 174, WETTZ13N:WETTZELL, 0613+570, 07:36:10, which fits at -2612.0 +/- 66.6 ps observation 216, WETTZ13N:WETTZELL, 1053+704, 07:44:37, which fits at 1754.2 +/- 66.6 ps observation 228, WETTZ13N:WETTZELL, 0019+058, 07:48:34, which fits at -554.8 +/- 65.9 ps observation 234, WETTZ13N:WETTZELL, 0017+200, 07:49:50, which fits at -1072.8 +/- 66.8 ps observation 246, WETTZ13N:WETTZELL, 0025+197, 07:52:05, which fits at -1504.0 +/- 66.7 ps observation 252, WETTZ13N:WETTZELL, 2309+454, 07:53:21, which fits at -9196.3 +/- 66.9 ps observation 258, WETTZ13N:WETTZELL, 2229+695, 07:54:33, which fits at -652.3 +/- 65.8 ps Other comments: The correlator provided the following station notes: ISHIOKA (Is/Q): Eight non-detections in X-band on baseline Is-Wn (low SNR). NYALES20 (Ny/N): OK. WETTZ13N (Wn/W): Eight non-detections in X-band on baseline Is-Wn (low SNR). RFI in both bands on baseline Wn-Wz leading to one G code in X-band; channel SR1U particularly affected and removed from frine fitting. Applied notch filters on baseline Wn-Wz. WETTZELL (Wz/V): RFI in both bands on baseline Wn-Wz leading to one G code in X-band; channel SR1U particularly affected and removed from frine fitting. Applied notch filters on baseline Wn-Wz. Parameterization: 14 parameters: UT1 offset atmosphere offset for: ISHIOKA NYALES20 WETTZ13N WETTZELL clock offset, first order term, and second order term for: NYALES20 WETTZ13N WETTZELL Clock breaks: None Session Statistics Observations: 282 scheduled 282 correlated (included in the database) 273 recoverable (usable in Solve/nuSolve) 260 used Session fit: 45.589 ps UT1 formal error: 5.03 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 12 12 12 0017+200 12 12 8 0019+058 6 6 5 0025+197 12 12 10 0059+581 12 12 11 0133+476 12 12 12 0202+319 12 12 12 0529+483 12 12 12 0613+570 12 12 11 0716+714 12 12 12 0955+476 12 12 12 1030+415 12 12 11 1039+811 12 12 12 1053+704 12 12 10 1128+385 6 6 6 1803+784 6 6 6 3C371 6 6 6 1842+681 6 6 4 1849+670 6 6 6 2000+472 12 12 12 3C418 12 12 12 2113+293 12 12 12 2144+092 6 6 6 2215+150 12 12 11 2229+695 12 12 9 2309+454 12 12 8 2318+049 12 12 12 ------------ --------- ---------- ------ Source Total 282 282 260 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.