EVN User Experiment Pipeline Feedback
Last updated: Fri Nov 20 13:08:57 CET 2015
zparagi@jive.eu
General Comments.
(
Brief data summary
and
scan listing
)
RG007A, C-band ToO e-VLBI experiment on 18 November 2015 (within the e-EVN run EM113 on 17-18 November). Participating telescopes were Effelsberg, Jodrell Bank (Mk2), Medicina, Onsala (25m), Torun, Yebes, Westerbork (single dish).
The target 151027A and the check source J1815+6127 were phase-referenced to the calibrator J1806+6141. Another bright calibrator was J1746+6226. Ef and Wb were parked during most of the experiment because of strong winds. Wb would not have seen the sources most of the time anyway because these were off limits. Lost some time to Ys because of network problems. Jb2 had low amplitudes during the run (corrected to first order in the pipeline ANTAB file; no measured Tsys).
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.64 . ERI* = 0.97 .
(Ef=0.5/1, Jb2=1, Mc=1, On=1, Tr=1, Ys=0.9, Wb=0.3/1)
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:
J1806+6141: pdf (not available)
, or
FITS (not available)
.
J1815+6127:
pdf
, or
FITS
.
J1746+6226: pdf (not available)
, or
FITS (not available)
.
151027A:
pdf
, or
FITS
.
Comments.
Uniformly weighted dirty map (not useful for bright sources)
produced before self-cal of:
J1806+6141: pdf (not available)
, or
FITS (not available)
.
J1815+6127:
pdf
, or
FITS
.
J1746+6226: pdf (not available)
, or
FITS (not available)
.
151027A:
pdf
, or
FITS
.
Comments.
Phase corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J1806+6141
.
J1815+6127 (not available)
.
J1746+6226
.
151027A (not available)
.
Comments.
Amplitude corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J1806+6141:
pdf
, or
text file
, or
statistical summary
.
J1815+6127: pdf (not available)
, or
text file (not available)
, or
statistical summary (not available)
.
J1746+6226:
pdf
, or
text file
, or
statistical summary
.
151027A: 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:
J1806+6141
.
J1815+6127 (not available)
.
J1746+6226
.
151027A (not available)
.
Comments.
Calibrated visibilities and the source model of:
J1806+6141
.
J1815+6127 (not available)
.
J1746+6226
.
151027A (not available)
.
Comments.
Calibrated visibilities against u,v distance for:
J1806+6141:
pdf
, or
png
.
J1815+6127:
pdf
, or
png
.
J1746+6226:
pdf
, or
png
.
151027A:
pdf
, or
png
.
Comments.
u,v coverage for:
J1806+6141:
pdf
, or
png
.
J1815+6127:
pdf
, or
png
.
J1746+6226:
pdf
, or
png
.
151027A:
pdf
, or
png
.
Comments.
Crude maps of sources:
J1806+6141:
pdf
, or
FITS
.
J1815+6127:
pdf
, or
FITS
.
J1746+6226:
pdf
, or
FITS
.
151027A:
pdf
, or
FITS
.
Comments.