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UV_FITC
This task allows fitting of simple models directly from the visibil-
ities. The models are linear combinations of 2 radial distributions, as-
sumed to be centered on the current phase tracking center. Use tasks
UV_CENTER and UV_SHIFT if necessary before fitting.
A more flexible and more general fitting procedure is available in the
UVT task. This version is more suitable for plotting a fit over re-
binned visibilities.
The type of the first radial distribution. Available types are
NONE No function to fit (for 2nd function usually)
POINT Point source
GAUSS Gaussian sources
DISK Disk
RING Annulus
EXPONENT Exponential brightness
POWER-1 B = 1/r
POWER-2 B = 1/r^2
POWER-3 B = 1/r^3
PARABOLA Parabolic brightness distribution
Gildas manager
2014-07-01