EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EP061E. 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 Oct 3 11:52:55 CEST 2008 cimo@jive.nl

General Comments. ( Brief data summary and scan listing )
L band phase-referencing experiment, observed on 29 Feb 2008. Data rate was 1 Gbps (8 X 16 MHz subbands, dual polarization, two-bit sampling).
11 stations participated. Jb had a recording problem resulting to the loss of all data after UT 02:45 (15min). From 22:43 to 00:36 UT scans lost at Nt for MK5 failure.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.76 . ERI* = 0.76 . (JB=0.96, EF=1, WB=1, CM=0, ON=1, MC=1, NT=0.69, TR=1, UR=1, Sh=1, Hh=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:
IRAS1929: pdf , or FITS .
3C286: pdf (not available) , or FITS (not available) .
2134+004: pdf (not available) , or FITS (not available) .
J1941-0511: pdf (not available) , or FITS (not available) .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
IRAS1929: pdf , or FITS .
3C286: pdf (not available) , or FITS (not available) .
2134+004: pdf (not available) , or FITS (not available) .
J1941-0511: pdf (not available) , or FITS (not available) .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
IRAS1929 (not available) .
3C286 .
2134+004 .
J1941-0511 .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
IRAS1929: pdf (not available) , or text file (not available) , or statistical summary (not available) .
3C286: pdf , or text file , or statistical summary .
2134+004: pdf , or text file , or statistical summary .
J1941-0511: pdf , or text file , or statistical summary .
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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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Telescope sensitivities consistent with the EVN Status Table.

Residual closure phase (visibility closure phase with model closure phase subtracted) for:
IRAS1929 (not available) .
3C286 .
2134+004 .
J1941-0511 .
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Calibrated visibilities and the source model of:
IRAS1929 (not available) .
3C286 .
2134+004 .
J1941-0511 .
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Calibrated visibilities against u,v distance for:
IRAS1929: pdf , or png .
3C286: pdf , or png .
2134+004: pdf , or png .
J1941-0511: pdf , or png .
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u,v coverage for:
IRAS1929: pdf , or png .
3C286: pdf , or png .
2134+004: pdf , or png .
J1941-0511: pdf , or png .
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Crude maps of sources:
IRAS1929: pdf , or FITS .
3C286: pdf , or FITS .
2134+004: pdf , or FITS .
J1941-0511: pdf , or FITS .
Comments.