GENERAL C-band VLBI observed on 23 Feb 2016. 14 stations scheduled, 12 observed. Participating telescopes were Effelsberg, Jodrell Bank (Mk2), Medicina, Noto, Onsala (25m), Tianma64, Yebes, Torun, Westerbork (single dish), Svetloe, Badari, Zelenchk, Urumqi, Irbene.

IR antab is nominal.
/// ERIVAL 0.81 /// ERISTAR 0.68 /// ERICOMM The ERI* value takes into account that:
-JB clock search failed.
Note that only EVN stations contribute to the ERI statistics. In this case IR is not included in the ERI.
The ERI value also takes into account losses that are outside the station's control.
- EF didn't observe due to snow.
/// POSSM_AUTOCORR Each scan plotted separately, all stations. /// VPLOT_UNCAL Full-experiment for Ys-* baselines, no calibration applied. A 1.5-minute plot-averaging was used. /// POSSM_UNCAL Scalar averaged Ys-* baselines, each scan plotted separately. No calibration applied yet. /// POSSM_CPOL Scalar averaged Ys-* baselines showing LR, each scan plotted separately. No calibration applied yet. /// TSYS TY1 table, each IF/pol on a separate plot. ANTAB edited for KVASARS and UR to add time point at FF/BP scan. /// GAIN Gain amplitude from CL2 table. /// FRING_PHAS CL3 station phase solutions -- CL3 = CL2+SN2, thus also includes the initial amplitude/parallactic angle calibration from CL2 and the fringe solutions from SN2. /// FRING_DELAY SN2 station delay solutions for the fringed sources, each IF/pol on a separate plot. /// FRING_RATE SN2 station rate solutions. /// BANDPASS Bandpass table 1. OQ208 used for bandpass calibration. /// VPLOT_CAL Full-experiment for Ys-* baselines, calibrated with CL3. A 1.5-min plot-averaging was used. /// POSSM_CAL Ys-* baselines calibrated with CL3 and BP1. The amp and phase plots self-scale, not necessarily going down to 0 in the case of the amps. /// IMAPN Naturally-weighted dirty maps of the phase-referenced-to sources. /// IMAPU Uniformly-weighted dirty maps of the phase-referenced-to sources. /// CALIB_PHAS1 Plots of post-SPLIT tables SN1 for the sources that have been individually fringed. /// CALIB_AMP2 As above, but for the post-SPLIT table SN2. /// SENS CL4 gain-amp. /// CLPHS Separate files per (fringed) source, showing closure phase plots for all the triangles. Only stokes=I shown. /// VPLOT_MODEL For each (fringed) source, plots of amp/phase on Ys-* baselines, calibrated with (post-SPLIT) table CL3, with a model-line overplotted. /// UVCOV For each source, a plot of the u-v coverage. /// UVPLT For each source, a plot of amp vs. |uv| distance. /// ICLN For each source, a CLEAN map resulting from the automated fringing and self-cal iterations (or phase-referencing) in the pipeline script. The target is clearly detected. ///