EVN User Experiment Pipeline Feedback
Last updated: Tue Feb 14 13:09:47 CET 2006
bignall@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
EM059A is a 22 GHz phase-referencing experiment observed on 26 October 2005 at 128 Mbps (one 16MHz IF, dual polarization, 2-bit sampling). Correlation produced 1024 spectral channels and 2s integration time.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.66 . ERI* = 0.66 .
(EF=1, JB=1, ON=0.93, MC=1, SH=0, MH=0.85, UR=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
(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 produced before self-cal of:
2007+402:
postscript
, or
FITS
.
2015+3710:
postscript
, or
FITS
.
2007+777:
postscript
, or
FITS
.
IRAS2012:
postscript
, or
FITS
.
2002+472:
postscript
, or
FITS
.
Comments.
Uniformly weighted dirty map produced before self-cal of:
2007+402:
postscript
, or
FITS
.
2015+3710:
postscript
, or
FITS
.
2007+777:
postscript
, or
FITS
.
IRAS2012:
postscript
, or
FITS
.
2002+472:
postscript
, or
FITS
.
Comments.
Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
2007+402.
2015+3710.
2007+777.
IRAS2012. (not available)
2002+472.
Comments.
Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
2007+402:
postscript
, or
text file
, or
statistical summary
.
2015+3710:
postscript
, or
text file
, or
statistical summary
.
2007+777:
postscript
, or
text file
, or
statistical summary
.
IRAS2012: postscript (not available)
, or text file (not available)
, or statistical summary
(not available)
.
2002+472: postscript (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:
2007+402
.
2015+3710
.
2007+777
.
IRAS2012
(not available)
.
2002+472
(not available)
.
Comments.
Calibrated visibilities and the source model of:
2007+402
.
2015+3710
.
2007+777
.
IRAS2012
(not available)
.
2002+472
(not available)
.
Comments.
Calibrated visibilities against u,v distance for:
2007+402.
postscript
, or
png (smaller)
2015+3710.
postscript
, or
png (smaller)
2007+777.
postscript
, or
png (smaller)
IRAS2012.
postscript
, or
png (smaller)
2002+472. postscript (not available)
, or png (smaller)
(not available)
Comments.
u,v coverage for:
2007+402.
postscript
, or
png (smaller)
2015+3710.
postscript
, or
png (smaller)
2007+777.
postscript
, or
png (smaller)
IRAS2012.
postscript
, or
png (smaller)
2002+472. postscript (not available)
, or png (smaller)
(not available)
Comments.
Crude maps of sources:
2007+402:
postscript
, or
FITS
.
2015+3710:
postscript
, or
FITS
.
2007+777:
postscript
, or
FITS
.
IRAS2012:
postscript
, or
FITS
.
2002+472:postscript
(not available)
, or
FITS
(not available)
.
Comments.