EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment N05K2. 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 15 15:13:07 CET 2006 soria@jive.nl


General Comments. ( Brief data summary and scan listing )
K-band Network Monitoring Experiment observed on the 26 October 2005 session 3/2005). The experiment was recorded at 256 Mbps using 2-bit sampling, dual polarization and 8 MHz bandwidth with 16 spectral channels. Six sources were observed: 1253-055, 1611+343, CEPA and the sources 3C345 and NRAO512 in phase referencing mode, which have been pipelined.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.36 . ERI* = 0.47 . (SH=0, EF=1, MC=1, JB=0.75, ON=1, NT=0, MH=1, UR=0.9)


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:
:postscript (not available) , or FITS (not available) .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
:postscript (not available) , or FITS (not available) .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
. (not available)
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
: postscript (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:
(not available) .
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Calibrated visibilities and the source model of:
(not available) .
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Calibrated visibilities against u,v distance for:
. postscript (not available) , or png (smaller) (not available)
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u,v coverage for:
. postscript (not available) , or png (smaller) (not available)
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Crude maps of sources:
:postscript (not available) , or FITS (not available) .
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