EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EM061E_2. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Mon Jun 25 15:58:52 CEST 2007 cimo@jive.nl

General Comments. ( Brief data summary and scan listing )
EM061E was observed on the 17th March 2007 and was processed in 2 passes. The continuum pass with 8 telescopes, 8 band x 2 pols., each with 128 points, and the line pass with 8 telescopes, 1 band and 2 pols., correlated with 1024 spectral channels.
8 stations participated. Mc had strong interference problems. Tr observed only in one channel and with high Tsys.

The EVN reliability indicator (ERI) for this experiment was ERI = 1 . ERI* = 1 . (JB=1, HH=1, CM=1, EF=1, WB=1, Mc=1, Nt=1, TR=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 (not available)
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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:
J1825-0737: pdf (not available) , or FITS (not available) .
J2253+1608: pdf (not available) , or FITS (not available) .
J2101+0341: pdf (not available) , or FITS (not available) .
J1751+0939: pdf (not available) , or FITS (not available) .
G23.01-0: pdf , or FITS .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J1825-0737: pdf (not available) , or FITS (not available) .
J2253+1608: pdf (not available) , or FITS (not available) .
J2101+0341: pdf (not available) , or FITS (not available) .
J1751+0939: pdf (not available) , or FITS (not available) .
G23.01-0: pdf , or FITS .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1825-0737 .
J2253+1608 .
J2101+0341 .
J1751+0939 .
G23.01-0 (not available) .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1825-0737: pdf , or text file , or statistical summary .
J2253+1608: pdf , or text file , or statistical summary .
J2101+0341: pdf , or text file , or statistical summary .
J1751+0939: pdf , or text file , or statistical summary .
G23.01-0: 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:
J1825-0737 .
J2253+1608 .
J2101+0341 .
J1751+0939 .
G23.01-0 (not available) .
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Calibrated visibilities and the source model of:
J1825-0737 .
J2253+1608 .
J2101+0341 .
J1751+0939 .
G23.01-0 (not available) .
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Calibrated visibilities against u,v distance for:
J1825-0737: pdf , or png .
J2253+1608: pdf , or png .
J2101+0341: pdf , or png .
J1751+0939: pdf , or png .
G23.01-0: pdf , or png .
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u,v coverage for:
J1825-0737: pdf , or png .
J2253+1608: pdf , or png .
J2101+0341: pdf , or png .
J1751+0939: pdf , or png .
G23.01-0: pdf , or png .
Comments.

Crude maps of sources:
J1825-0737: pdf , or FITS .
J2253+1608: pdf , or FITS .
J2101+0341: pdf , or FITS .
J1751+0939: pdf , or FITS .
G23.01-0: pdf , or FITS .
Comments.