EVN User Experiment Pipeline Feedback
Last updated: Fri Jun 5 15:57:05 CEST 2015
surcis@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
N15M1 had 11 stations (+ DBBC from JB that is listed as JD), 16 x 2 MHz IFs, 4 polarizations, and used 64 frequency points per IF/pol, with 1s integrations. The SOLINT was set at 1.0 min. Ef was used as the reference station. The fringe-finder and bandpass calibrator were '3C84', '0528+134', and 'DA193'. The continuum target sources 'J0313+4120' and 'J0552+3754' were calibrated using the phase-reference sources '3C84' and 'DA193', respectively.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.95 . ERI* = 0.95 .
(EF=1, WB=1, JB=1, ON=1, MC=0.75, NT=1, TR=1, YS=1, SH=1, HH=1, SR=1)
Plots of the autocorrelations
Comments.
Each scan plotted separately, all stations.
plots of the uncalibrated amplitude and phase
against time
Comments.
Full-experiment for Ef-* baselines, no calibration applied.
Plots of the uncalibrated amplitude and phase
against frequency channel
Comments.
Scalar averaged Ef-* baselines, each scan plotted separately. No calibration applied yet.
The uncalibrated amplitude and phase of the crosshand
correlations against frequency channel
Comments.
Scalar averaged Ef-* baselines for LR, each scan plotted separately. No calibration applied yet.
TSYS against time
Comments.
TY1 table, each IF/pol on a separate plot.
Telescope sensitivities
from the a priori TSYS and Gain
curves (the square of this number gives the antenna noise (SEFD) in Jy - the
smaller the better).
Comments.
Gain amplitude from CL2 table.
Fringe-fit phase solutions
(including Parallactic
Angle correction).
Comments.
CL3 station phase solutions -- CL3 = CL2+SN2, thus also includes the initial amplitude/parallactic angle calibration from CL2 and the fringe solutions from SN2.
Fringe-fit delay solutions
Comments.
SN2 station delay solutions for the fringed sources, each IF/pol on a separate plot.
Fringe-fit rate solutions
Comments.
SN2 station rate solutions.
Telescope bandpasses
Comments.
Bandpass table 1. 3C84, 0528+134, and DA193 were used for bandpass calibration.
Calibrated amplitude and phase against time
(a
priori amplitude calibration and fringe-fit solutions applied).
Comments.
Full-experiment for Ef-* baselines, calibrated with CL3.
Calibrated amplitude and phase against frequency
channel
Comments.
Ef-* baselines calibrated with CL3 and BP1. The amp and phaseplots self-scale, not necessarily going down to 0 in the case of the amps. LCP amplitude is higher than RCP amplitude for Sr-**.
Naturally weighted dirty map (not useful for bright sources)
produced before self-cal of:
J0313+4120:
pdf
, or
FITS
.
DA193: pdf (not available)
, or
FITS (not available)
.
0528+134: pdf (not available)
, or
FITS (not available)
.
3C84: pdf (not available)
, or
FITS (not available)
.
J0552+3754:
pdf
, or
FITS
.
Comments.
Naturally weighted dirty map of the targets.
Uniformly weighted dirty map (not useful for bright sources)
produced before self-cal of:
J0313+4120:
pdf
, or
FITS
.
DA193: pdf (not available)
, or
FITS (not available)
.
0528+134: pdf (not available)
, or
FITS (not available)
.
3C84: pdf (not available)
, or
FITS (not available)
.
J0552+3754:
pdf
, or
FITS
.
Comments.
Uniformly weighted dirty map of the targets.
Phase corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J0313+4120 (not available)
.
DA193
.
0528+134
.
3C84
.
J0552+3754 (not available)
.
Comments.
Plots of post-SPLIT tables SN1 for the sources.
Amplitude corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J0313+4120: pdf (not available)
, or
text file (not available)
, or
statistical summary (not available)
.
DA193:
pdf
, or
text file
, or
statistical summary
.
0528+134:
pdf
, or
text file
, or
statistical summary
.
3C84:
pdf
, or
text file
, or
statistical summary
.
J0552+3754: pdf (not available)
, or
text file (not available)
, or
statistical summary (not available)
.
Comments.
As above, but for the post-SPLIT table SN2.
Telescope sensitivities
(the total AMP gain applied
during both a priori and self calibration; the square of this number gives the
antenna noise (SEFD) in Jy).
Comments.
CL4 gain-amp.
Residual closure phase (visibility closure phase with model closure phase subtracted) for:
J0313+4120 (not available)
.
DA193
.
0528+134
.
3C84
.
J0552+3754 (not available)
.
Comments.
Separate files per (fringed) source, showing closure phase plots for all the triangles (not just Ef-*-*). Only stokes=I shown.
Calibrated visibilities and the source model of:
J0313+4120 (not available)
.
DA193
.
0528+134
.
3C84
.
J0552+3754 (not available)
.
Comments.
For each (fringed) source, plots of amp/phase on Ef-* baselines, calibrated with (post-SPLIT) table CL3, with a model-line overplotted.
Calibrated visibilities against u,v distance for:
J0313+4120:
pdf
, or
png
.
DA193:
pdf
, or
png
.
0528+134:
pdf
, or
png
.
3C84:
pdf
, or
png
.
J0552+3754:
pdf
, or
png
.
Comments.
For each source, a plot of amp vs. |uv| distance.
u,v coverage for:
J0313+4120:
pdf
, or
png
.
DA193:
pdf
, or
png
.
0528+134:
pdf
, or
png
.
3C84:
pdf
, or
png
.
J0552+3754:
pdf
, or
png
.
Comments.
For each source, a plot of the u-v coverage.
Crude maps of sources:
J0313+4120:
pdf
, or
FITS
.
DA193:
pdf
, or
FITS
.
0528+134:
pdf
, or
FITS
.
3C84:
pdf
, or
FITS
.
J0552+3754:
pdf
, or
FITS
.
Comments.
For each source, a CLEAN map resulting from the automated fringing and self-cal iterations (or phase-referencing) in the pipeline script.