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.
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ERIVAL
0.81
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ERISTAR
0.68
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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.
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POSSM_AUTOCORR
Each scan plotted separately, all stations.
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VPLOT_UNCAL
Full-experiment for Ys-* baselines, no calibration
applied. A 1.5-minute plot-averaging was used.
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POSSM_UNCAL
Scalar averaged Ys-* baselines, each scan plotted separately.
No calibration applied yet.
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POSSM_CPOL
Scalar averaged Ys-* baselines showing LR, each scan plotted separately.
No calibration applied yet.
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TSYS
TY1 table, each IF/pol on a separate plot. ANTAB edited for KVASARS and UR to
add time point at FF/BP scan.
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GAIN
Gain amplitude from CL2 table.
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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.
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FRING_DELAY
SN2 station delay solutions for the fringed sources, each IF/pol on
a separate plot.
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FRING_RATE
SN2 station rate solutions.
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BANDPASS
Bandpass table 1.
OQ208 used for bandpass calibration.
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VPLOT_CAL
Full-experiment for Ys-* baselines, calibrated with
CL3. A 1.5-min plot-averaging was used.
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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.
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IMAPN
Naturally-weighted dirty maps of the phase-referenced-to sources.
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IMAPU
Uniformly-weighted dirty maps of the phase-referenced-to sources.
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CALIB_PHAS1
Plots of post-SPLIT tables SN1 for the sources that have been individually
fringed.
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CALIB_AMP2
As above, but for the post-SPLIT table SN2.
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SENS
CL4 gain-amp.
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CLPHS
Separate files per (fringed) source, showing closure phase
plots for all the triangles. Only stokes=I shown.
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VPLOT_MODEL
For each (fringed) source, plots of amp/phase on Ys-*
baselines, calibrated with (post-SPLIT) table CL3, with a model-line
overplotted.
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UVCOV
For each source, a plot of the u-v coverage.
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UVPLT
For each source, a plot of amp vs. |uv| distance.
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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.
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