NASA Analysis Report for P23280 (20231007-p23280) 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: 5 observation 30, HN-VLBA :MK-VLBA , 1406-267, 19:02:35, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 43, HN-VLBA :MK-VLBA , 0016+731, 19:17:37, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' observation 56, HN-VLBA :MK-VLBA , 1418-192, 19:32:35, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 69, HN-VLBA :MK-VLBA , 0418+532, 19:48:09, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' observation 70, HN-VLBA :MK-VLBA , 0016+731, 19:49:52, quality code X: 0 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 5 observation 5, HN-VLBA :MK-VLBA , 1124-186, 18:34:06, which fits at 141.7 +/- 38.8 ps observation 35, HN-VLBA :MK-VLBA , 1124-186, 19:07:41, which fits at 215.6 +/- 42.0 ps observation 48, HN-VLBA :MK-VLBA , 0718+793, 19:22:56, which fits at 139.0 +/- 44.8 ps observation 52, HN-VLBA :MK-VLBA , 0642+449, 19:27:01, which fits at -184.0 +/- 39.6 ps observation 53, HN-VLBA :MK-VLBA , 0738+491, 19:28:05, which fits at -141.0 +/- 42.0 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) 75 recoverable (usable in Solve/nuSolve) 70 used Session fit: 46.543 ps UT1 formal error: 8.72 microsec Source Performance Number of Observations Scheduled Correlated* Used 0016+731 2 2 0 0418+532 2 2 1 0454+844 2 2 2 0529+483 1 1 1 0602+673 2 2 2 0613+570 2 2 2 0642+449 1 1 0 0716+714 1 1 1 0718+793 1 1 0 0738+491 2 2 1 0749+540 2 2 2 0804+499 2 2 2 0933+503 1 1 1 0955+476 1 1 1 1030+415 1 1 1 1039+811 2 2 2 1040+244 1 1 1 1053+704 1 1 1 1053+815 2 2 2 1059+282 1 1 1 1101+384 1 1 1 1111+149 1 1 1 1124-186 2 2 0 1133-032 2 2 2 1144+402 1 1 1 1145+268 1 1 1 1149-084 1 1 1 1204+399 1 1 1 1212+171 1 1 1 1213-172 2 2 2 1219+044 1 1 1 1243-160 2 2 2 1244-255 2 2 2 1255-316 2 2 2 1300+580 2 2 2 1306+360 2 2 2 1308+328 1 1 1 1318+225 1 1 1 1324+224 1 1 1 1327+504 2 2 2 1330+476 1 1 1 1334-127 1 1 1 1351-018 1 1 1 1354-152 1 1 1 1406-076 1 1 1 1406-267 1 1 0 1417+273 1 1 1 1418-192 1 1 0 1456+044 1 1 1 1502+036 1 1 1 1508-055 1 1 1 1546+027 1 1 1 1555+001 1 1 1 1601+112 1 1 1 1606+106 1 1 1 NGC6251 1 1 1 1803+784 1 1 1 3C371 1 1 1 1823+689 1 1 1 2353+816 2 2 2 ------------ --------- ---------- ------ Source Total 80 80 70 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.