EVN User Experiment Pipeline Feedback
Last updated: vr dec 6 15:16:32 CET 2019
immer@jive.eu
General Comments.
(Brief data summary (not available)
and scan listing (not available)
)
Plots of the autocorrelations
(not available)
Comments.
Plots of the uncalibrated amplitude and phase
against time (not available)
Comments.
Plots of the uncalibrated amplitude and phase
against frequency channel
(not available)
Comments.
The uncalibrated amplitude and phase of the crosshand
correlations against frequency channel
(not available)
Comments.
TSYS against time
(not available)
Comments.
Telescope sensitivities (not available)
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 (not available)
(including Parallactic
Angle correction).
Comments.
Fringe-fit delay solutions
(not available)
Comments.
Fringe-fit rate solutions
(not available)
Comments.
Telescope bandpasses
(not available)
Comments.
Calibrated amplitude and phase against time (not available)
(a
priori amplitude calibration and fringe-fit solutions applied).
Comments.
Calibrated amplitude and phase against frequency
channel
(not available)
Comments.
Naturally weighted dirty map (not useful for bright sources)
produced before self-cal of:
Uniformly weighted dirty map (not useful for bright sources)
produced before self-cal of:
Phase corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
Comments.
Amplitude corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
Comments.
Telescope sensitivities (not available)
(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:
Calibrated visibilities and the source model of:
Calibrated visibilities against u,v distance for:
u,v coverage for:
Crude maps of sources: