EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment N12M2_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: Wed Feb 6 15:28:18 CET 2013 surcis@jive.nl

General Comments. ( Brief data summary and scan listing )
N12M2_1 had 8 stations, 16 x 8 MHz IFs, 4 polarizations, and used 32 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-finders and bandpass calibrators were '3C286' and '3C345'. The target sources 'J1329+3154' and 'G35.02' were calibrated using the phase-reference sources '3C286' and 'J1856+0610'.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.99 . ERI* = 0.99 . (EF=1, WB=1, JB=0.99, ON=1, MC=1, NT=1, TR=1, YS=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. No Fringes in all baselines JB-xx.

Plots of the uncalibrated amplitude and phase against frequency channel
Comments.
Scalar averaged Ef-* baselines, each scan plotted separately. No calibration applied yet. The maser G35.02 is in all the baseline but XX-JB.

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. No solutions for Jb.

Fringe-fit delay solutions
Comments.
SN2 station delay solutions for the fringed sources, each IF/pol on a separate plot. No solutions for Jb.

Fringe-fit rate solutions
Comments.
SN2 station rate solutions. No solutions for Jb.

Telescope bandpasses
Comments.
Bandpass table 1. J1751+0939 and J1748+0832 were used for bandpass calibration. No solutions for Jb.

Calibrated amplitude and phase against time (a priori amplitude calibration and fringe-fit solutions applied).
Comments.
Full-experiment for Ef-* baselines, calibrated with CL3. No JB in the plot.

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. Methanol masers in all the baselines.

Naturally weighted dirty map (not useful for bright sources) produced before self-cal of:
J1856+0610: pdf (not available) , or FITS (not available) .
G35.02: pdf , or FITS .
J1329+3154: pdf , or FITS .
3C286: pdf (not available) , or FITS (not available) .
3C345: 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:
J1856+0610: pdf (not available) , or FITS (not available) .
G35.02: pdf , or FITS .
J1329+3154: pdf , or FITS .
3C286: pdf (not available) , or FITS (not available) .
3C345: 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.
J1856+0610 .
G35.02 (not available) .
J1329+3154 (not available) .
3C286 .
3C345 .
Comments.
Plots of post-SPLIT tables SN1 for the sources.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1856+0610: pdf , or text file , or statistical summary .
G35.02: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J1329+3154: pdf (not available) , or text file (not available) , or statistical summary (not available) .
3C286: pdf , or text file , or statistical summary .
3C345: 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:
J1856+0610 .
G35.02 (not available) .
J1329+3154 (not available) .
3C286 .
3C345 .
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:
J1856+0610 .
G35.02 (not available) .
J1329+3154 (not available) .
3C286 .
3C345 .
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:
J1856+0610: pdf , or png .
G35.02: pdf , or png .
J1329+3154: pdf , or png .
3C286: pdf , or png .
3C345: pdf , or png .
Comments.
For each source, a plot of amp vs. |uv| distance.

u,v coverage for:
J1856+0610: pdf , or png .
G35.02: pdf , or png .
J1329+3154: pdf , or png .
3C286: pdf , or png .
3C345: pdf , or png .
Comments.
For each source, a plot of the u-v coverage.

Crude maps of sources:
J1856+0610: pdf , or FITS .
G35.02: pdf , or FITS .
J1329+3154: pdf , or FITS .
3C286: pdf , or FITS .
3C345: 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.