EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EG049B. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Fri Sep 16 11:19:45 CEST 2011 yang@jive.nl

General Comments. ( Brief data summary and scan listing )
EG049B was observed on 2011 Jun 3, had 13 stations Ef Jb Mc On Tr Wb Ys Hh Bd Sv Zc Sh Ur and observed at a datarate of 1 Gbps Considerably more information is included in the experiment's cover letter on the standard-plots portion of the EVN Archive. Ef was used as the reference station.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.57 (Ef=0, Mc=0, Ys=0) . ERI* = 0.57 .

Plots of the autocorrelations
Comments.
Each scan plotted separately, all stations.

plots of the uncalibrated amplitude and phase against time
Comments.
Full-experiment for Wb-* baselines, no calibration applied.

Plots of the uncalibrated amplitude and phase against frequency channel
Comments.
Scalar averaged Wb-* baselines, each scan plotted separately. No calibration applied yet.

The uncalibrated amplitude and phase of the crosshand correlations against frequency channel
Comments.
Scalar averaged Wb-* 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. M87 was used for bandpass calibration.

Calibrated amplitude and phase against time (a priori amplitude calibration and fringe-fit solutions applied).
Comments.
Full-experiment for Wb-* baselines, calibrated with CL3.

Calibrated amplitude and phase against frequency channel
Comments.
Wb-* baselines calibrated with CL3 and BP1. The amp and phaseplots 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:
0234+285: pdf (not available) , or FITS (not available) .
0239+175: pdf (not available) , or FITS (not available) .
0229+200: pdf (not available) , or FITS (not available) .
Comments.
Naturually weighted dirty map of the targets.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
0234+285: pdf (not available) , or FITS (not available) .
0239+175: pdf (not available) , or FITS (not available) .
0229+200: pdf (not available) , or FITS (not available) .
Comments.
Uniformly weighted dirty map of the targets.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
0234+285 .
0239+175 .
0229+200 .
Comments.
Plots of post-SPLIT tables SN1 for the sources.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
0234+285: pdf , or text file , or statistical summary .
0239+175: pdf , or text file , or statistical summary .
0229+200: 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:
0234+285 .
0239+175 .
0229+200 .
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:
0234+285 .
0239+175 .
0229+200 .
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:
0234+285: pdf , or png .
0239+175: pdf , or png .
0229+200: pdf , or png .
Comments.
For each source, a plot of amp vs. |uv| distance.

u,v coverage for:
0234+285: pdf , or png .
0239+175: pdf , or png .
0229+200: pdf , or png .
Comments.
For each source, a plot of the u-v coverage.

Crude maps of sources:
0234+285: pdf , or FITS .
0239+175: pdf , or FITS .
0229+200: 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.