NASA Analysis Report for Q19012 ($19JAN12XK) 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 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 27, ISHIOKA :WETTZELL, 1726+455, 08:22:24, quality code X-band: 0 S-band: 9 Number of observations rejected during analysis: 1 observation 9, ISHIOKA :WETTZELL, 0016+731, 07:45:48, which fits at 3572.3 +/- 66.0 ps Other comments: The correlator report's correlator notes said: The fringe amplitude of X-band were weak. The observed SNRs were only about 50 % of the predicted SNRs. Scan 012-0821: FQ = 0 on X-band, source 1726+455 There was good integration time but low SNR. The correlator report's station notes said: ISHIOKA (I-Is): The pcal amplitude of the X-band were weak than usual. observed pcal amplitude : about 2 % usual pcal amplitude : about 3 % WETTZELL(V-Wz): The pcal amplitude of the X-band were weak than usual. observed pcal amplitude : about 4 % usual pcal amplitude : about 5 % Parameterization: 6 parameters: UT1 offset atmosphere offset for: ISHIOKA WETTZELL clock offset, first order term, and second order term for: WETTZELL Clock breaks: None Session Statistics Observations: 30 scheduled 30 correlated (included in the database) 29 recoverable (usable in Solve/nuSolve) 28 used Session fit: 47.992 ps UT1 formal error: 16.04 microsec Source Performance Number of Observations Scheduled Correlated* Used 0059+581 2 2 2 0133+476 2 2 2 NRAO512 1 1 1 1726+455 3 3 2 1803+784 4 4 4 3C371 4 4 4 3C418 1 1 1 2000+472 4 4 4 0716+714 1 1 1 1053+704 4 4 4 0016+731 1 1 0 1751+288 3 3 3 ------------ --------- ---------- ------ Source Total 30 30 28 * Correlated means included in the database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.