IVS Analysis Report for Q20195 ($20JUL13XK) 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.) This report is being Updated to add the station notes from the correlator report. Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 7 observation 17, SESHAN25:WETTZELL, 1746+470, 07:02:32, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 61, NYALES20:SESHAN25, 1745+624, 07:12:56, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 64, SESHAN25:WETTZ13N, 1745+624, 07:12:56, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 144, WETTZ13N:WETTZELL, 1746+470, 07:35:09, quality code X: 9 S: 1, fringe code X: ' ' S: 'G' observation 175, NYALES20:SESHAN25, 1842+681, 07:42:53, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 187, NYALES20:SESHAN25, 1053+815, 07:45:38, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 190, SESHAN25:WETTZ13N, 1053+815, 07:45:38, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 15 observation 5, SESHAN25:WETTZELL, 1806+456, 07:00:15, which fits at 169.4 +/- 50.8 ps observation 18, WETTZ13N:WETTZELL, 1746+470, 07:02:32, which fits at 1610.4 +/- 62.5 ps observation 36, WETTZ13N:WETTZELL, 1842+681, 07:06:09, which fits at -2050.3 +/- 61.6 ps observation 48, WETTZ13N:WETTZELL, 2353+816, 07:08:43, which fits at -14768.4 +/- 61.0 ps observation 84, WETTZ13N:WETTZELL, 0808+019, 07:20:53, which fits at -2316.3 +/- 61.0 ps observation 114, WETTZ13N:WETTZELL, 0759+183, 07:27:19, which fits at 390.9 +/- 60.4 ps observation 163, NYALES20:SESHAN25, 2353+816, 07:40:08, which fits at -3341.4 +/- 68.1 ps observation 168, WETTZ13N:WETTZELL, 2353+816, 07:40:08, which fits at 651.9 +/- 60.9 ps observation 192, WETTZ13N:WETTZELL, 1053+815, 07:45:38, which fits at 3314.6 +/- 60.5 ps observation 193, NYALES20:SESHAN25, 0536+145, 07:48:39, which fits at 247.3 +/- 67.4 ps observation 196, SESHAN25:WETTZ13N, 0536+145, 07:48:39, which fits at -383.8 +/- 80.8 ps observation 197, SESHAN25:WETTZELL, 0536+145, 07:48:39, which fits at -260.3 +/- 41.7 ps observation 198, WETTZ13N:WETTZELL, 0536+145, 07:48:39, which fits at 16029.4 +/- 60.1 ps observation 216, WETTZ13N:WETTZELL, 0613+570, 07:52:59, which fits at -3689.8 +/- 60.4 ps observation 228, WETTZ13N:WETTZELL, 0738+491, 07:55:30, which fits at -2514.0 +/- 60.9 ps Other comments: The correlator report provided the following station notes: NYALES20 (Ny/N): Ok. SESHAN25 (Sh/C): Some non-detections in X-band. WETTZ13N (Wn/W): RFI in S-band channels SR1U and SR2U on baseline Wn-Wz; channels removed from fringe fitting on this baseline. WETTZELL (Wz/V): RFI in S-band channels SR1U and SR2U on baseline Wn-Wz; channels removed from fringe fitting on this baseline. Parameterization: 14 parameters: UT1 offset atmosphere offset for: NYALES20 SESHAN25 WETTZ13N WETTZELL clock offset, first order term, and second order term for: SESHAN25 WETTZ13N WETTZELL Clock breaks: None Session Statistics Observations: 246 scheduled 246 correlated (included in the database) 239 recoverable (usable in Solve/nuSolve) 224 used Session fit: 50.130 ps UT1 formal error: 7.16 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 6 6 6 0529+483 6 6 6 0536+145 6 6 2 0552+398 6 6 6 0613+570 6 6 5 0642+449 6 6 6 0738+491 6 6 5 0748+126 6 6 6 0759+183 6 6 5 0805+410 12 12 12 0808+019 6 6 5 0814+425 12 12 12 0821+394 6 6 6 0823+033 6 6 6 0827+243 6 6 6 OJ287 6 6 6 1039+811 6 6 6 1053+815 6 6 3 1418+546 6 6 6 1636+473 6 6 6 1726+455 12 12 12 1745+624 6 6 4 1746+470 12 12 9 1803+784 12 12 12 1806+456 12 12 11 3C371 12 12 12 1842+681 12 12 10 1849+670 12 12 12 2229+695 12 12 12 2353+816 12 12 9 ------------ --------- ---------- ------ Source Total 246 246 224 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.