EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RP024A. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Tue Mar 8 16:00:34 CET 2016 zparagi@jive.eu

General Comments. ( Brief data summary and scan listing )
RP024A, L-band ToO e-VLBI experiment, 1st epoch on 1 February 2016. Participating telescopes were Arecibo, Effelsberg, Jodrell Bank (LT), Medicina, Onsala (25m), Torun, Westerbork (single dish). Unlike EP100, Arecibo did take part in the VLBI phase-referencing of the ms-transient candidate.

The target FRB121102 was phase-referenced to the ICRF calibrator J0518+3306. Additional calibrators and nearby calibrator candidates:
3C84
J0529+3209
J0530+3301
J0535+3249
J0535+3153
J0539+3308

The following test pulsars were observed for a short time (with their phase-reference calibrators):
Crab-J0534+2200 (J0535+1942)
J0614+2229 (J0604+2429)
J0629+2415 (J0637+2319)

Lost two telescopes: Jb1 and On were parked because of strong wind.
This pipeline shows results for the main calibrators, target, and the candidate nearby calibrators only.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.5 . ERI* = 1.0 . (Ef=1, Jb1=0/1, Mc=1, On=0/1, Tr=1, Wb=1, Ar=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
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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:
J0535+3153: pdf (not available) , or FITS (not available) .
J0535+3249: pdf (not available) , or FITS (not available) .
3C84: pdf (not available) , or FITS (not available) .
J0518+3306: pdf (not available) , or FITS (not available) .
J0530+3301: pdf (not available) , or FITS (not available) .
J0539+3308: pdf (not available) , or FITS (not available) .
FRB: pdf , or FITS .
J0529+3209: pdf (not available) , or FITS (not available) .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J0535+3153: pdf (not available) , or FITS (not available) .
J0535+3249: pdf (not available) , or FITS (not available) .
3C84: pdf (not available) , or FITS (not available) .
J0518+3306: pdf (not available) , or FITS (not available) .
J0530+3301: pdf (not available) , or FITS (not available) .
J0539+3308: pdf (not available) , or FITS (not available) .
FRB: pdf , or FITS .
J0529+3209: pdf (not available) , or FITS (not available) .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J0535+3153 .
J0535+3249 .
3C84 .
J0518+3306 .
J0530+3301 .
J0539+3308 .
FRB (not available) .
J0529+3209 .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J0535+3153: pdf , or text file , or statistical summary .
J0535+3249: pdf , or text file , or statistical summary .
3C84: pdf , or text file , or statistical summary .
J0518+3306: pdf , or text file , or statistical summary .
J0530+3301: pdf , or text file , or statistical summary .
J0539+3308: pdf , or text file , or statistical summary .
FRB: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J0529+3209: 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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Residual closure phase (visibility closure phase with model closure phase subtracted) for:
J0535+3153 .
J0535+3249 .
3C84 .
J0518+3306 .
J0530+3301 .
J0539+3308 .
FRB (not available) .
J0529+3209 .
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Calibrated visibilities and the source model of:
J0535+3153 .
J0535+3249 .
3C84 .
J0518+3306 .
J0530+3301 .
J0539+3308 .
FRB (not available) .
J0529+3209 .
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Calibrated visibilities against u,v distance for:
J0535+3153: pdf , or png .
J0535+3249: pdf , or png .
3C84: pdf , or png .
J0518+3306: pdf , or png .
J0530+3301: pdf , or png .
J0539+3308: pdf , or png .
FRB: pdf , or png .
J0529+3209: pdf , or png .
Comments.

u,v coverage for:
J0535+3153: pdf , or png .
J0535+3249: pdf , or png .
3C84: pdf , or png .
J0518+3306: pdf , or png .
J0530+3301: pdf , or png .
J0539+3308: pdf , or png .
FRB: pdf , or png .
J0529+3209: pdf , or png .
Comments.

Crude maps of sources:
J0535+3153: pdf , or FITS .
J0535+3249: pdf , or FITS .
3C84: pdf , or FITS .
J0518+3306: pdf , or FITS .
J0530+3301: pdf , or FITS .
J0539+3308: pdf , or FITS .
FRB: pdf , or FITS .
J0529+3209: pdf , or FITS .
Comments.