EVN User Experiment Pipeline Feedback
Last updated: Mon Apr 7 10:27:38 CEST 2014
zparagi@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
EG079B, C-band e-VLBI run on 2014 Mar 25-26. Participating telescopes were Effelberg, Jodrell Bank 2, Medicina, Noto, Onsala, Shanghai, Torun, Yebes and Westerbork. Torun upper two RCP subbands were dead. Medicina lowest subband was flagged for bad data (RFI?). Mc observed at 512 Mbps - 1-bit sampling, all other 1024 Mbps with 2-bit sampling. There were 10 telescopes in the phased-up WSRT array; note for WSRT the target source was only visible at the very end of the experiment.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.94 . ERI* = 0.97 .
(Ef=1, Wb=1, Jb2=1, On=1, Mc=0.875/1, Nt=1, Tr=0.875, Ys=1, Sh=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:
J1927+6117: pdf (not available)
, or
FITS (not available)
.
J1933+6540: pdf (not available)
, or
FITS (not available)
.
1927+654:
pdf
, or
FITS
.
Comments.
Uniformly weighted dirty map (not useful for bright sources)
produced before self-cal of:
J1927+6117: pdf (not available)
, or
FITS (not available)
.
J1933+6540: pdf (not available)
, or
FITS (not available)
.
1927+654:
pdf
, or
FITS
.
Comments.
Phase corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J1927+6117
.
J1933+6540
.
1927+654 (not available)
.
Comments.
Amplitude corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J1927+6117:
pdf
, or
text file
, or
statistical summary
.
J1933+6540:
pdf
, or
text file
, or
statistical summary
.
1927+654: 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:
J1927+6117
.
J1933+6540
.
1927+654 (not available)
.
Comments.
Calibrated visibilities and the source model of:
J1927+6117
.
J1933+6540
.
1927+654 (not available)
.
Comments.
Calibrated visibilities against u,v distance for:
J1927+6117:
pdf
, or
png
.
J1933+6540:
pdf
, or
png
.
1927+654:
pdf
, or
png
.
Comments.
u,v coverage for:
J1927+6117:
pdf
, or
png
.
J1933+6540:
pdf
, or
png
.
1927+654:
pdf
, or
png
.
Comments.
Crude maps of sources:
J1927+6117:
pdf
, or
FITS
.
J1933+6540:
pdf
, or
FITS
.
1927+654:
pdf
, or
FITS
.
Comments.