NASA Analysis Report for P23190 (20230709-p23190) This report is a contributed analysis report that does not correspond 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: nuSolve solutions.) Session scheduled at USNO, correlated at WASH and analyzed at NASA Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 6 observation 6, HN-VLBA :MK-VLBA , 0434-188, 18:20:03, quality code X: 0 S: 8, fringe code X: ' ' S: ' ' observation 17, HN-VLBA :MK-VLBA , 1842+681, 18:33:07, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' observation 27, HN-VLBA :MK-VLBA , 1053+704, 18:43:33, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' observation 30, HN-VLBA :MK-VLBA , 0834-201, 18:49:48, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 36, HN-VLBA :MK-VLBA , 0743+259, 18:55:51, quality code X: 9 S: 4, fringe code X: ' ' S: ' ' observation 80, HN-VLBA :MK-VLBA , 0418+532, 19:44:38, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 3 observation 1, HN-VLBA :MK-VLBA , 0646-306, 18:15:08, which fits at 321.9 +/- 61.4 ps observation 2, HN-VLBA :MK-VLBA , 0632-235, 18:16:07, which fits at 257.2 +/- 76.5 ps observation 3, HN-VLBA :MK-VLBA , 0630-261, 18:16:57, which fits at 331.6 +/- 88.0 ps Other comments: None. Parameterization: 6 parameters: UT1 offset atmosphere offset for: HN-VLBA MK-VLBA clock offset, first order term, and second order term for: MK-VLBA Clock breaks: None Session statistics Observations: 80 scheduled 80 correlated (included in the database) 74 recoverable (usable in Solve/nuSolve) 71 used Session fit: 63.157 ps UT1 formal error: 12.43 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 1 1 1 0059+581 1 1 1 0133+476 1 1 1 0151+474 1 1 1 0307+380 1 1 1 0322+222 1 1 1 0332+078 1 1 1 CTA26 1 1 1 0340+362 1 1 1 0345+460 1 1 1 0354+231 1 1 1 0358+210 1 1 1 0403-132 1 1 1 0415+398 1 1 1 0418+532 1 1 0 0420+022 1 1 1 0420-014 1 1 1 0422+004 1 1 1 0434-188 1 1 0 0436-129 1 1 1 0442+389 1 1 1 0454+844 2 2 2 0454-234 1 1 1 0458-020 1 1 1 0515+208 1 1 1 0524+034 1 1 1 0529+483 1 1 1 0537-286 1 1 1 0548+378 1 1 1 0552+398 1 1 1 0556+238 1 1 1 0601-172 1 1 1 0602+673 2 2 2 0606-223 1 1 1 0613+570 2 2 2 0627-199 1 1 1 0630-261 2 2 1 0632-235 2 2 1 0641+392 1 1 1 0642+449 1 1 1 0646-306 2 2 1 0648-165 1 1 1 0656+082 1 1 1 0657+172 1 1 1 0700-197 1 1 1 0716+714 1 1 1 0718+793 1 1 1 0727-115 1 1 1 0729+259 1 1 1 0738+491 1 1 1 0743+259 2 2 1 0743+277 2 2 2 0747+185 2 2 2 0759+183 2 2 2 0823+033 1 1 1 0834-201 1 1 0 0847-120 1 1 1 0854-108 1 1 1 0955+476 1 1 1 1039+811 1 1 1 1053+704 1 1 0 1053+815 1 1 1 NGC6251 1 1 1 1803+784 2 2 2 1842+681 1 1 0 2017+743 2 2 2 2229+695 1 1 1 2353+816 1 1 1 ------------ --------- ---------- ------ Source Total 80 80 71 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.