EVN User Experiment Pipeline Feedback
Last updated: Thu Dec 17 12:14:22 CET 2009
zparagi@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
C-band e-VLBI run on 10 December 2009. The scheduled data rate was 1024 Mbps. Participating telescopes were Ef, Jb2, Mc, On, Sh, Tr, Ys and Wb. Because of a network problem in the UK, Jb2 could not transfer data during the EG047A part of the run. There were no fringes to Westerbork, because of a serious power failure at the station. Shanghai was limited to 512 Mbps. Medicina and Yebes were limited to 896 Mbps.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.42 . ERI* = 0.62 .
(Jb2=0/1, Mc=0.9, Ef=0.9, On=0.9, Sh=0.9, Tr=0.9, Ys=0.9, Wb=0)
Plots of the autocorrelations
Comments.
plots of the uncalibrated amplitude and phase
against time
Comments.
Plots of the uncalibrated amplitude and phase
against frequency channel
Comments.
The uncalibrated amplitude and phase of the crosshand
correlations against frequency channel
Comments.
TSYS against time
Comments.
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
Comments.
Fringe-fit rate solutions
Comments.
Telescope bandpasses
Comments.
Calibrated amplitude and phase against time
(a
priori amplitude calibration and fringe-fit solutions applied).
Comments.
Calibrated amplitude and phase against frequency
channel
Comments.
Naturally weighted dirty map (not useful for bright sources)
produced before self-cal of:
3C84: pdf (not available)
, or
FITS (not available)
.
Comments.
Uniformly weighted dirty map (not useful for bright sources)
produced before self-cal of:
3C84: pdf (not available)
, or
FITS (not available)
.
Comments.
Phase corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
3C84
.
Comments.
Amplitude corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
3C84:
pdf
, or
text file
, or
statistical summary
.
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:
3C84
.
Comments.
Calibrated visibilities and the source model of:
3C84
.
Comments.
Calibrated visibilities against u,v distance for:
3C84:
pdf
, or
png
.
Comments.
u,v coverage for:
3C84:
pdf
, or
png
.
Comments.
Crude maps of sources:
3C84:
pdf
, or
FITS
.
Comments.