EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RSP06. 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 Dec 16 15:35:55 CET 2011 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
RSP06, L-band short e-VLBI run on 2011 Dec. 14.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.43 . ERI* = 0.79 . (Ef=1, Jb1=1, Mc=0.5, On=0/1, Tr=0.63/0.88, Wb=1 )

Plots of the autocorrelations
Comments.
IF2 strong RFI for all, especially Wb

plots of the uncalibrated amplitude and phase against time
Comments.
On: could not observe because of strong winds

Plots of the uncalibrated amplitude and phase against frequency channel
Comments.
Mc: because of a fiber cut, only 512 Mbps
Tr: IFs L5-6 missing (BBC#6 dead); IF7-8 very low amp (due to RFI?)

The uncalibrated amplitude and phase of the crosshand correlations against frequency channel
Comments.

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).
Comments.

Fringe-fit phase solutions (including Parallactic Angle correction).
Comments.

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:
J1545+5400: pdf (not available) , or FITS (not available) .
4C52.370: pdf , or FITS .
2MAS1542: pdf , or FITS .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J1545+5400: pdf (not available) , or FITS (not available) .
4C52.370: pdf , or FITS .
2MAS1542: pdf , or FITS .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1545+5400 .
4C52.370 (not available) .
2MAS1542 (not available) .
Comments.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1545+5400: pdf , or text file , or statistical summary (not available) .
4C52.370: pdf (not available) , or text file (not available) , or statistical summary (not available) .
2MAS1542: 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).
Comments.

Residual closure phase (visibility closure phase with model closure phase subtracted) for:
J1545+5400 .
4C52.370 (not available) .
2MAS1542 (not available) .
Comments.

Calibrated visibilities and the source model of:
J1545+5400 .
4C52.370 (not available) .
2MAS1542 (not available) .
Comments.

Calibrated visibilities against u,v distance for:
J1545+5400: pdf , or png .
4C52.370: pdf , or png .
2MAS1542: pdf , or png .
Comments.

u,v coverage for:
J1545+5400: pdf , or png .
4C52.370: pdf , or png .
2MAS1542: pdf , or png .
Comments.

Crude maps of sources:
J1545+5400: pdf , or FITS .
4C52.370: pdf , or FITS .
2MAS1542: pdf , or FITS .
Comments.