EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EP088D_1. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Mon Jul 21 14:32:17 CEST 2014 campbell@jive.nl

General Comments. ( Brief data summary and scan listing )
EP088D had 13 good stations, 8 16MHz IFs, 4 polarizations, 32 frequency points per IF/pol, and 1s integrations. Considerably more information is included in the experiment's cover letter on the standard-plots portion of the EVN Archive. This pipelining corresponds to the non-multi-phase-center output for all the targets except NGC6090A,B. In the pipelining, the target sources were treated as phase-reference targets and were not separately fringe-fit. The SOLINT was set automatically to a value commensurate with a typical reference-source scan. Ef, and then Ys, were used as the reference stations.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.841 . ERI* = 0.841 . The losses include no fringes to Nt and Tr having no fringes in IF7-8/RCP.

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. A 1.5 minute plot-averaging was used.

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 showing 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. Some outliers in individual solints that throw off the automated phase-connection choices (e.g., Jb ~00:50, On ~05:00 in some IF/pol, Zc ~22:00), as reflected in the FRING_PHAS plot.

Telescope bandpasses
Comments.
Bandpass table 1. 3C454.3 and J1824+5651 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. The 1.5-min plot-averaging still applied.

Calibrated amplitude and phase against frequency channel
Comments.
Ef-* 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.

Naturally weighted dirty map (not useful for bright sources) produced before self-cal of:
J2108+1430: pdf (not available) , or FITS (not available) .
3C454.3: pdf (not available) , or FITS (not available) .
VV340A: pdf , or FITS .
J1102+2757: pdf (not available) , or FITS (not available) .
NGC6670A: pdf , or FITS .
J1453+2648: pdf (not available) , or FITS (not available) .
CGCG448: pdf , or FITS .
IRASF15250: pdf , or FITS .
IRAS10565: pdf , or FITS .
J1824+5651: pdf (not available) , or FITS (not available) .
J1522+3144: pdf (not available) , or FITS (not available) .
Comments.
Naturally-weighted dirty maps of the phase-referenced-to sources.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J2108+1430: pdf (not available) , or FITS (not available) .
3C454.3: pdf (not available) , or FITS (not available) .
VV340A: pdf , or FITS .
J1102+2757: pdf (not available) , or FITS (not available) .
NGC6670A: pdf , or FITS .
J1453+2648: pdf (not available) , or FITS (not available) .
CGCG448: pdf , or FITS .
IRASF15250: pdf , or FITS .
IRAS10565: pdf , or FITS .
J1824+5651: pdf (not available) , or FITS (not available) .
J1522+3144: pdf (not available) , or FITS (not available) .
Comments.
Uniformly-weighted dirty maps of the phase-referenced-to sources.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J2108+1430 .
3C454.3 .
VV340A (not available) .
J1102+2757 .
NGC6670A (not available) .
J1453+2648 .
CGCG448 (not available) .
IRASF15250 (not available) .
IRAS10565 (not available) .
J1824+5651 .
J1522+3144 .
Comments.
Plots of post-SPLIT tables SN1 for the sources that have been individually fringed.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J2108+1430: pdf , or text file , or statistical summary .
3C454.3: pdf , or text file , or statistical summary .
VV340A: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J1102+2757: pdf , or text file , or statistical summary .
NGC6670A: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J1453+2648: pdf , or text file , or statistical summary .
CGCG448: pdf (not available) , or text file (not available) , or statistical summary (not available) .
IRASF15250: pdf (not available) , or text file (not available) , or statistical summary (not available) .
IRAS10565: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J1824+5651: pdf , or text file , or statistical summary .
J1522+3144: pdf , or text file , or statistical summary .
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:
J2108+1430 .
3C454.3 .
VV340A (not available) .
J1102+2757 .
NGC6670A (not available) .
J1453+2648 .
CGCG448 (not available) .
IRASF15250 (not available) .
IRAS10565 (not available) .
J1824+5651 .
J1522+3144 .
Comments.
Separate files per (fringed) source, showing closure phase plots for all the triangles. Only stokes=I shown.

Calibrated visibilities and the source model of:
J2108+1430 .
3C454.3 .
VV340A (not available) .
J1102+2757 .
NGC6670A (not available) .
J1453+2648 .
CGCG448 (not available) .
IRASF15250 (not available) .
IRAS10565 (not available) .
J1824+5651 .
J1522+3144 .
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:
J2108+1430: pdf , or png .
3C454.3: pdf , or png .
VV340A: pdf , or png .
J1102+2757: pdf , or png .
NGC6670A: pdf , or png .
J1453+2648: pdf , or png .
CGCG448: pdf , or png .
IRASF15250: pdf , or png .
IRAS10565: pdf , or png .
J1824+5651: pdf , or png .
J1522+3144: pdf , or png .
Comments.
For each source, a plot of amp vs. |uv| distance.

u,v coverage for:
J2108+1430: pdf , or png .
3C454.3: pdf , or png .
VV340A: pdf , or png .
J1102+2757: pdf , or png .
NGC6670A: pdf , or png .
J1453+2648: pdf , or png .
CGCG448: pdf , or png .
IRASF15250: pdf , or png .
IRAS10565: pdf , or png .
J1824+5651: pdf , or png .
J1522+3144: pdf , or png .
Comments.
For each source, a plot of the u-v coverage.

Crude maps of sources:
J2108+1430: pdf , or FITS .
3C454.3: pdf , or FITS .
VV340A: pdf , or FITS .
J1102+2757: pdf , or FITS .
NGC6670A: pdf , or FITS .
J1453+2648: pdf , or FITS .
CGCG448: pdf , or FITS .
IRASF15250: pdf , or FITS .
IRAS10565: pdf , or FITS .
J1824+5651: pdf , or FITS .
J1522+3144: 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.