EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RSL01. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Thu May 22 15:00:43 CEST 2008 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
C-band e-VLBI run on 21 May 2008. Aggregate bitrate was 512 Mbps with 2-bit sampling, resulting in 8*8MHz subbands in both RCP and LCP. This was the first e-VLBI production run with 7 telescopes, and the first one with the 100m Effelsberg telescope. Fringe-finder was 3C454.3. The target source was phase-referenced to 3 sources using 4 different strategies -in these four parts of the experiment A, B, C, and D was added to the source names.

All stations performed well. The experiment started a few minutes late. Note that for this pipeline nominal gain and Tsys values were used.

The EVN reliability indicator (ERI) for this experiment was ERI = 1.00 . ERI* = 1.00 . (Cm=1, Ef=1, Jb2=1, Mc=1, On=1, Tr=1, Wb=1)

Plots of the autocorrelations
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plots of the uncalibrated amplitude and phase against time
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Plots of the uncalibrated amplitude and phase against frequency channel
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The uncalibrated amplitude and phase of the crosshand correlations against frequency channel
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TSYS against time
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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).
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Fringe-fit phase solutions (including Parallactic Angle correction).
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Fringe-fit delay solutions
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Fringe-fit rate solutions
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Telescope bandpasses
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Calibrated amplitude and phase against time (a priori amplitude calibration and fringe-fit solutions applied).
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Calibrated amplitude and phase against frequency channel
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Naturally weighted dirty map (not useful for bright sources) produced before self-cal of:
3C454.3: pdf (not available) , or FITS (not available) .
J2310+105A: pdf (not available) , or FITS (not available) .
J2310+105D: pdf (not available) , or FITS (not available) .
J2300+103B: pdf (not available) , or FITS (not available) .
J2300+103D: pdf (not available) , or FITS (not available) .
J2308+094C: pdf (not available) , or FITS (not available) .
NGC7479A: pdf , or FITS .
NGC7479B: pdf , or FITS .
NGC7479C: pdf , or FITS .
NGC7479D: pdf , or FITS .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
3C454.3: pdf (not available) , or FITS (not available) .
J2310+105A: pdf (not available) , or FITS (not available) .
J2310+105D: pdf (not available) , or FITS (not available) .
J2300+103B: pdf (not available) , or FITS (not available) .
J2300+103D: pdf (not available) , or FITS (not available) .
J2308+094C: pdf (not available) , or FITS (not available) .
NGC7479A: pdf , or FITS .
NGC7479B: pdf , or FITS .
NGC7479C: pdf , or FITS .
NGC7479D: pdf , or FITS .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C454.3 .
J2310+105A .
J2310+105D .
J2300+103B .
J2300+103D .
J2308+094C .
NGC7479A (not available) .
NGC7479B (not available) .
NGC7479C (not available) .
NGC7479D (not available) .
Comments.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C454.3: pdf , or text file , or statistical summary .
J2310+105A: pdf , or text file , or statistical summary .
J2310+105D: pdf , or text file , or statistical summary .
J2300+103B: pdf , or text file , or statistical summary .
J2300+103D: pdf , or text file , or statistical summary .
J2308+094C: pdf , or text file , or statistical summary .
NGC7479A: pdf (not available) , or text file (not available) , or statistical summary (not available) .
NGC7479B: pdf (not available) , or text file (not available) , or statistical summary (not available) .
NGC7479C: pdf (not available) , or text file (not available) , or statistical summary (not available) .
NGC7479D: pdf (not available) , or text file (not available) , or statistical summary (not available) .
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).
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Residual closure phase (visibility closure phase with model closure phase subtracted) for:
3C454.3 .
J2310+105A .
J2310+105D .
J2300+103B .
J2300+103D .
J2308+094C .
NGC7479A (not available) .
NGC7479B (not available) .
NGC7479C (not available) .
NGC7479D (not available) .
Comments.

Calibrated visibilities and the source model of:
3C454.3 .
J2310+105A .
J2310+105D .
J2300+103B .
J2300+103D .
J2308+094C .
NGC7479A (not available) .
NGC7479B (not available) .
NGC7479C (not available) .
NGC7479D (not available) .
Comments.

Calibrated visibilities against u,v distance for:
3C454.3: pdf , or png .
J2310+105A: pdf , or png .
J2310+105D: pdf , or png .
J2300+103B: pdf , or png .
J2300+103D: pdf , or png .
J2308+094C: pdf , or png .
NGC7479A: pdf , or png .
NGC7479B: pdf , or png .
NGC7479C: pdf , or png .
NGC7479D: pdf , or png .
Comments.

u,v coverage for:
3C454.3: pdf , or png .
J2310+105A: pdf , or png .
J2310+105D: pdf , or png .
J2300+103B: pdf , or png .
J2300+103D: pdf , or png .
J2308+094C: pdf , or png .
NGC7479A: pdf , or png .
NGC7479B: pdf , or png .
NGC7479C: pdf , or png .
NGC7479D: pdf , or png .
Comments.

Crude maps of sources:
3C454.3: pdf , or FITS .
J2310+105A: pdf , or FITS .
J2310+105D: pdf , or FITS .
J2300+103B: pdf , or FITS .
J2300+103D: pdf , or FITS .
J2308+094C: pdf , or FITS .
NGC7479A: pdf , or FITS .
NGC7479B: pdf , or FITS .
NGC7479C: pdf , or FITS .
NGC7479D: pdf , or FITS .
Comments.