IVS Analysis Report for C23253 (20230910-c23253) This report is the official IVS analysis report that corresponds to the database maintained by the IVS Data Centers for this session. (Analyzed by autoINT.js script, NVI inc, NASA Goddard Space Flight Center VLBI Analysis Center. Spoolfile source: automated nuSolve solutions.) Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 11 observation 33, ONSA13NE:ONSA13SW, 4C67.05 , 08:50:10, quality code X: 4 S: -, fringe code X: ' ' S: '-' observation 99, ONSA13NE:ONSA13SW, 4C67.05 , 09:02:25, quality code X: 4 S: -, fringe code X: ' ' S: '-' observation 108, ONSA13NE:ONSA13SW, 0955+476, 09:03:49, quality code X: 3 S: -, fringe code X: ' ' S: '-' observation 120, ONSA13NE:ONSA13SW, 1039+811, 09:05:39, quality code X: 3 S: -, fringe code X: ' ' S: '-' observation 123, ONSA13NE:ONSA13SW, 2007+777, 09:06:08, quality code X: 4 S: -, fringe code X: ' ' S: '-' observation 135, ONSA13NE:ONSA13SW, 1739+522, 09:07:57, quality code X: 4 S: -, fringe code X: ' ' S: '-' observation 195, ONSA13NE:ONSA13SW, 0917+624, 09:18:45, quality code X: 3 S: -, fringe code X: 'G' S: '-' observation 258, ONSA13NE:ONSA13SW, 2007+777, 09:29:20, quality code X: 4 S: -, fringe code X: ' ' S: '-' observation 267, ONSA13NE:ONSA13SW, 1726+455, 09:30:44, quality code X: 4 S: -, fringe code X: ' ' S: '-' observation 288, ONSA13NE:ONSA13SW, 0917+624, 09:34:06, quality code X: 4 S: -, fringe code X: ' ' S: '-' observation 318, ONSA13NE:ONSA13SW, 0954+658, 09:40:07, quality code X: 4 S: -, fringe code X: ' ' S: '-' Number of observations rejected during analysis: 15 observation 1, ISHIOKA :ONSA13NE, 1351-018, 08:45:04, which fits at -255.6 +/- 42.2 ps observation 2, ISHIOKA :ONSA13SW, 1351-018, 08:45:04, which fits at -218.1 +/- 43.8 ps observation 28, ISHIOKA :ONSA13NE, 0917+449, 08:49:37, which fits at 517.4 +/- 42.0 ps observation 29, ISHIOKA :ONSA13SW, 0917+449, 08:49:37, which fits at 530.5 +/- 43.2 ps observation 45, ONSA13NE:ONSA13SW, 1746+470, 08:52:02, which fits at 448.3 +/- 54.5 ps observation 94, ISHIOKA :ONSA13NE, 0133+476, 09:01:57, which fits at -295.0 +/- 41.8 ps observation 95, ISHIOKA :ONSA13SW, 0133+476, 09:01:57, which fits at -281.4 +/- 43.0 ps observation 132, ONSA13NE:ONSA13SW, 1746+470, 09:07:30, which fits at 12571.7 +/- 52.7 ps observation 142, ISHIOKA :ONSA13NE, 1015+359, 09:09:33, which fits at 317.6 +/- 42.8 ps observation 143, ISHIOKA :ONSA13SW, 1015+359, 09:09:33, which fits at 316.9 +/- 44.0 ps observation 168, ONSA13NE:ONSA13SW, 1726+455, 09:13:48, which fits at -124.8 +/- 43.1 ps observation 181, ISHIOKA :ONSA13NE, 0955+476, 09:16:47, which fits at 184.6 +/- 41.9 ps observation 182, ISHIOKA :ONSA13SW, 0955+476, 09:16:47, which fits at 191.5 +/- 43.0 ps observation 223, ISHIOKA :ONSA13NE, 1219+044, 09:23:34, which fits at 151.4 +/- 42.0 ps observation 224, ISHIOKA :ONSA13SW, 1219+044, 09:23:34, which fits at 156.6 +/- 43.1 ps Other comments: None. Parameterization: 10 parameters: UT1 offset atmosphere offset for: ISHIOKA ONSA13NE ONSA13SW clock offset, first order term, and second order term for: ONSA13NE ONSA13SW Clock breaks: None Session statistics Observations: 345 scheduled 345 correlated (included in the database) 334 recoverable (usable in Solve/nuSolve) 319 used Session fit: 26.858 ps UT1 formal error: 3.61 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 15 15 15 0133+476 12 12 10 4C67.05 15 15 13 0718+793 12 12 12 0917+449 3 3 1 0917+624 12 12 10 0954+658 12 12 11 0955+476 12 12 9 1015+359 3 3 1 1030+415 12 12 12 1039+811 12 12 11 1044+719 15 15 15 1128+385 12 12 12 1144+402 12 12 12 1156+295 15 15 15 1219+044 12 12 10 1324+224 18 18 18 1334-127 3 3 3 1351-018 15 15 13 1504+377 12 12 12 1514+197 3 3 3 1520+319 12 12 12 1637+574 12 12 12 1642+690 12 12 12 1726+455 9 9 7 1739+522 12 12 11 1746+470 12 12 10 1803+784 12 12 12 3C371 12 12 12 2007+777 15 15 13 ------------ --------- ---------- ------ Source Total 345 345 319 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.