EVN User Experiment Pipeline Feedback
Last updated: Fri May 20 18:42:02 CEST 2016
marcote@jive.eu
General Comments.
(
Brief data summary
and
scan listing
)
5cm experiment on 12 April 2016. RS002 was processed with two passes:
Pass1: "continuum" 8 2MHz bands X 2 pols, each with 128 points, 2 sec int.
Pass2: "line" 1 2MHz band X 2 pols, with 2048 points, 2 sec int.
This document summarises the "line" pass (es071c_2). J0530+1331 and 0234+2856 were used as fringe-finders and bandpass calibrators.
The source S255 was phase-referenced to J0603+1742 Note that the uvflg file for Wb has been edited to comment out line 1072.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.86 . ERI* = 0.86 .
The ERI* value takes into account that:
- Sr has no data from 16:15 to 18:00 UT - Jb, Nt missed a couple scans
The ERI value also takes into account losses that are outside the station's control, of which there were none for this experiment.
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
(not available)
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:
J0530+1331: pdf (not available)
, or
FITS (not available)
.
S255:
pdf
, or
FITS
.
J0603+1742: pdf (not available)
, or
FITS (not available)
.
Comments.
Uniformly weighted dirty map (not useful for bright sources)
produced before self-cal of:
J0530+1331: pdf (not available)
, or
FITS (not available)
.
S255:
pdf
, or
FITS
.
J0603+1742: pdf (not available)
, or
FITS (not available)
.
Comments.
Phase corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J0530+1331
.
S255 (not available)
.
J0603+1742
.
Comments.
Amplitude corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
J0530+1331:
pdf
, or
text file
, or
statistical summary
.
S255: pdf (not available)
, or
text file (not available)
, or
statistical summary (not available)
.
J0603+1742:
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:
J0530+1331
.
S255 (not available)
.
J0603+1742
.
Comments.
Calibrated visibilities and the source model of:
J0530+1331
.
S255 (not available)
.
J0603+1742
.
Comments.
Calibrated visibilities against u,v distance for:
J0530+1331:
pdf
, or
png
.
S255:
pdf
, or
png
.
J0603+1742:
pdf
, or
png
.
Comments.
u,v coverage for:
J0530+1331:
pdf
, or
png
.
S255:
pdf
, or
png
.
J0603+1742:
pdf
, or
png
.
Comments.
Crude maps of sources:
J0530+1331:
pdf
, or
FITS
.
S255:
pdf
, or
FITS
.
J0603+1742:
pdf
, or
FITS
.
Comments.