IVS Analysis Report for Q21011 ($21JAN11XK) 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: 1 observation 24, WETTZ13N:WETTZELL, 1636+473, 07:09:14, quality code X: 8 S: 4, fringe code X: ' ' S: 'G' Number of observations rejected during analysis: 24 observation 15, WETTZ13N:WETTZELL, 1053+815, 07:04:55, which fits at -7304.9 +/- 43.0 ps observation 20, SESHAN25:WETTZELL, 1418+546, 07:07:46, which fits at 122.1 +/- 27.8 ps observation 27, WETTZ13N:WETTZELL, 1732+389, 07:10:27, which fits at -20158.4 +/- 42.4 ps observation 33, WETTZ13N:WETTZELL, 1746+470, 07:12:38, which fits at -12058.5 +/- 41.9 ps observation 36, WETTZ13N:WETTZELL, 1806+456, 07:13:42, which fits at -7319.5 +/- 42.0 ps observation 39, WETTZ13N:WETTZELL, 1758+388, 07:14:48, which fits at -11371.0 +/- 41.9 ps observation 42, WETTZ13N:WETTZELL, 1849+670, 07:16:23, which fits at -3030.9 +/- 41.8 ps observation 51, WETTZ13N:WETTZELL, 2353+816, 07:19:53, which fits at -22181.7 +/- 41.5 ps observation 57, WETTZ13N:WETTZELL, 1936-155, 07:26:12, which fits at -3865.6 +/- 41.9 ps observation 69, WETTZ13N:WETTZELL, 1732+389, 07:31:24, which fits at -27230.6 +/- 42.1 ps observation 75, WETTZ13N:WETTZELL, 1746+470, 07:33:35, which fits at -14525.1 +/- 42.0 ps observation 78, WETTZ13N:WETTZELL, 1806+456, 07:34:39, which fits at -16277.7 +/- 42.0 ps observation 81, WETTZ13N:WETTZELL, 1758+388, 07:35:44, which fits at -20566.7 +/- 41.8 ps observation 84, WETTZ13N:WETTZELL, 1846+322, 07:36:56, which fits at -779.9 +/- 42.0 ps observation 87, WETTZ13N:WETTZELL, 1929+226, 07:38:11, which fits at 1092.5 +/- 42.6 ps observation 88, SESHAN25:WETTZ13N, 2000+472, 07:39:47, which fits at 112.6 +/- 31.3 ps observation 92, SESHAN25:WETTZELL, 0642+449, 07:42:23, which fits at 157.0 +/- 31.0 ps observation 108, WETTZ13N:WETTZELL, 1053+815, 07:48:35, which fits at 10174.0 +/- 43.5 ps observation 117, WETTZ13N:WETTZELL, 1849+670, 07:52:13, which fits at -2143.4 +/- 42.1 ps observation 120, WETTZ13N:WETTZELL, 1842+681, 07:53:17, which fits at -16089.8 +/- 41.8 ps observation 123, WETTZ13N:WETTZELL, 1746+470, 07:54:45, which fits at -19997.4 +/- 41.8 ps observation 126, WETTZ13N:WETTZELL, 1806+456, 07:55:49, which fits at 30284.1 +/- 42.3 ps observation 129, WETTZ13N:WETTZELL, 1758+388, 07:56:54, which fits at 25978.7 +/- 41.8 ps observation 132, WETTZ13N:WETTZELL, 1732+389, 07:58:01, which fits at 20386.3 +/- 42.0 ps Other comments: Cable values were not available for SESHAN25 or WETTZ13N. The correlator report noted the following: WETTZ13N (Wn/W): RFI in S-band channel SR1U on baseline Wn-Wz; channel removed from fringe fitting on this baseline. WETTZELL (Wz/V): RFI in S-band channel SR1U on baseline Wn-Wz; channel removed from fringe fitting on this baseline. 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: 135 scheduled 135 correlated (included in the database) 134 recoverable (usable in Solve/nuSolve) 110 used Session fit: 30.896 ps UT1 formal error: 4.22 microsec Source Performance Number of Observations Scheduled Correlated* Used 0529+483 6 6 6 0613+570 6 6 6 0642+449 3 3 2 0716+714 6 6 6 1039+811 6 6 6 1053+704 3 3 3 1053+815 6 6 4 1418+546 3 3 2 1636+473 3 3 2 1726+455 9 9 9 1732+389 9 9 6 1741-038 3 3 3 1746+470 9 9 6 1749+096 3 3 3 1751+288 3 3 3 1758+388 9 9 6 1803+784 6 6 6 1806+456 9 9 6 3C371 6 6 6 1842+681 3 3 2 1846+322 3 3 2 1849+670 6 6 4 1908-201 3 3 3 1929+226 3 3 2 1936-155 3 3 2 2000+472 3 3 2 2353+816 3 3 2 ------------ --------- ---------- ------ Source Total 135 135 110 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.