EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EH020. 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 Aug 17 15:28:18 CEST 2007 harvey@jive.nl

General Comments. ( Brief data summary and scan listing )

The EVN reliability indicator (ERI) for this experiment was ERI = 0.96 . ERI* = 0.96 . (CM=0.96, JB=0.96, EF=0.96, MC=0.96, ON=0.96, TR=0.96, NT=0.96, WB=0.96)

Plots of the autocorrelations
Comments.
Maser line visible in all plots of W3(OH). RFI also evident- this should be removed.

plots of the uncalibrated amplitude and phase against time
Comments.
normal

Plots of the uncalibrated amplitude and phase against frequency channel
Comments.

The uncalibrated amplitude and phase of the crosshand correlations against frequency channel (not available)
Comments.

TSYS against time
Comments.
EF was not focusing until 0500.

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.

Fringe-fit phase solutions (including Parallactic Angle correction).
Comments.

Fringe-fit delay solutions
Comments.

Fringe-fit rate solutions
Comments.

Telescope bandpasses
Comments.
looks ok

Calibrated amplitude and phase against time (a priori amplitude calibration and fringe-fit solutions applied).
Comments.
calibration looks good

Calibrated amplitude and phase against frequency channel
Comments.

Naturally weighted dirty map (not useful for bright sources) produced before self-cal of:
3C84: pdf (not available) , or FITS (not available) .
W3OH: pdf , or FITS .
DA193: pdf (not available) , or FITS (not available) .
J0244+6228: pdf (not available) , or FITS (not available) .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
3C84: pdf (not available) , or FITS (not available) .
W3OH: pdf , or FITS .
DA193: pdf (not available) , or FITS (not available) .
J0244+6228: pdf (not available) , or FITS (not available) .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C84 .
W3OH (not available) .
DA193 .
J0244+6228 .
Comments.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C84: pdf , or text file , or statistical summary .
W3OH: pdf (not available) , or text file (not available) , or statistical summary (not available) .
DA193: pdf , or text file , or statistical summary .
J0244+6228: pdf , or text file , or statistical summary .
Comments.

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.

Residual closure phase (visibility closure phase with model closure phase subtracted) for:
3C84 .
W3OH (not available) .
DA193 .
J0244+6228 .
Comments.

Calibrated visibilities and the source model of:
3C84 .
W3OH (not available) .
DA193 .
J0244+6228 .
Comments.

Calibrated visibilities against u,v distance for:
3C84: pdf , or png .
W3OH: pdf , or png .
DA193: pdf , or png .
J0244+6228: pdf , or png .
Comments.

u,v coverage for:
3C84: pdf , or png .
W3OH: pdf , or png .
DA193: pdf , or png .
J0244+6228: pdf , or png .
Comments.

Crude maps of sources:
3C84: pdf , or FITS .
W3OH: pdf , or FITS .
DA193: pdf , or FITS .
J0244+6228: pdf , or FITS .
Comments.
source visible