IVS Analysis Report for S22081 ($22MAR22VJ) This report is the official IVS analysis report that corresponds 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: interactive solve/nuSolve analysis.) Problems: None. Number of observations rejected during correlation: 0 Number of observations not usable by the software: 0 Number of observations rejected during analysis: 5 observation 13, MACGO12M:WETTZ13S, 0642+449, 19:54:51, which fits at 99.6 +/- 20.8 ps observation 20, MACGO12M:WETTZ13S, 1642+690, 19:58:58, which fits at -94.3 +/- 20.8 ps observation 61, MACGO12M:WETTZ13S, 0642+449, 20:25:10, which fits at 95.9 +/- 20.8 ps observation 66, MACGO12M:WETTZ13S, 1642+690, 20:28:10, which fits at -112.5 +/- 20.7 ps observation 86, MACGO12M:WETTZ13S, 0642+449, 20:42:41, which fits at 132.3 +/- 20.8 ps Other comments: None. Parameterization: 6 parameters: UT1 offset atmosphere offset for: MACGO12M WETTZ13S clock offset, first order term, and second order term for: WETTZ13S Clock breaks: None Session statistics Observations: 90 scheduled 90 correlated (included in the database) 90 recoverable (usable in Solve/nuSolve) 85 used Session fit: 20.237 ps UT1 formal error: 2.38 microsec Source Performance Number of Observations Scheduled Correlated* Used 0110+495 2 2 2 0123+257 2 2 2 0149+218 3 3 3 0202+319 4 4 4 0234+285 4 4 4 0300+470 1 1 1 CTA26 1 1 1 0420+022 2 2 2 0420-014 2 2 2 0446+112 2 2 2 0458-020 2 2 2 0528+134 2 2 2 0529+483 1 1 1 0556+238 2 2 2 0607-157 1 1 1 0642+449 4 4 1 0656+082 1 1 1 0657+172 2 2 2 0714+457 3 3 3 0749+540 4 4 4 0800+618 3 3 3 0804+499 3 3 3 0805+410 4 4 4 0812+367 1 1 1 0814+425 2 2 2 0821+394 1 1 1 0917+624 2 2 2 0954+658 2 2 2 1039+811 2 2 2 1053+704 2 2 2 NGC6251 1 1 1 1642+690 2 2 0 1739+522 3 3 3 1803+784 2 2 2 3C371 2 2 2 1823+568 2 2 2 1849+670 2 2 2 2000+472 2 2 2 2007+777 3 3 3 3C418 4 4 4 ------------ --------- ---------- ------ Source Total 90 90 85 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.