EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RT009A. 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 Nov 27 10:39:23 CET 2009 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
C-band e-EVN run on 19 November 2009. The scheduled data rate was 1024 Mbps. Participating telescopes were Ef, Cm(+Da), Jb1, Mc, On, Tr and Wb. The Lovell Telescope and Darnhall were parked because of high winds. Cambridge was only available for limited time during the 24h run for the same reason, but it was available for most of the time in RT009A. Medicina and Yebes participated at 896 Mbps. This was achieved by dropping the highest subbands only from the initial 1024 Mbps data stream (because of the hard limit of 1000 Mbps for these telescopes).

The EVN reliability indicator (ERI) for this experiment was ERI = 0.55 . ERI* = 1.0 . (Cm=0.8/1 (Da=0/1), Jb1=0/1, Mc=1, Ef=1, On=1, Tr=1, Ys=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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Cm signal in IF2.

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:
1749+096: pdf (not available) , or FITS (not available) .
J1907+0127: pdf (not available) , or FITS (not available) .
AQLX-1: pdf , or FITS .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
1749+096: pdf (not available) , or FITS (not available) .
J1907+0127: pdf (not available) , or FITS (not available) .
AQLX-1: pdf , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
1749+096 .
J1907+0127 .
AQLX-1 (not available) .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
1749+096: pdf , or text file , or statistical summary .
J1907+0127: pdf , or text file , or statistical summary .
AQLX-1: pdf (not available) , or text file (not available) , or statistical summary (not available) .
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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:
1749+096 .
J1907+0127 .
AQLX-1 (not available) .
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Calibrated visibilities and the source model of:
1749+096 .
J1907+0127 .
AQLX-1 (not available) .
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Calibrated visibilities against u,v distance for:
1749+096: pdf , or png .
J1907+0127: pdf , or png .
AQLX-1: pdf , or png .
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u,v coverage for:
1749+096: pdf , or png .
J1907+0127: pdf , or png .
AQLX-1: pdf , or png .
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Crude maps of sources:
1749+096: pdf , or FITS .
J1907+0127: pdf , or FITS .
AQLX-1: pdf , or FITS .
Comments.