EVN User Experiment Pipeline Feedback
Last updated: Fri Jun 1 13:48:24 CEST 2012
yang@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
5 GHz phase-referencing experiment, observed on 8 March 2012. Data rate was 1 Gbps (8 X 16 MHz subbands, dual polarization, two-bit sampling). The target sources 'TDF' in correlation pass 1 and 'FIRST-1' in correlation pass 2 were calibrated using the phase-reference sources 'J1638+5720'. 'J1638+5720' were also observed as the bandpass calibrator.
11 stations participated.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.52 . ERI* = 0.63 .
See PI letter (Ys=0.13, ON=0.25*, Mc=0, Sv=0.7, Rest=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
(not available)
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 (not available)
(a
priori amplitude calibration and fringe-fit solutions applied).
Comments.
Calibrated amplitude and phase against frequency
channel
(not available)
Comments.
Naturally weighted dirty map (not useful for bright sources)
produced before self-cal of:
Uniformly weighted dirty map (not useful for bright sources)
produced before self-cal of:
Phase corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
Comments.
Amplitude corrections applied to a priori calibrated and
fringe-fitted data by self-calibration.
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:
Calibrated visibilities and the source model of:
Calibrated visibilities against u,v distance for:
u,v coverage for:
Crude maps of sources: