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5.2.10 Parameter uvtaper
This controls the radial weighting of visibilities in the uv-plane (see § 5.2.11 below) through the multiplication of the visibilities by the Fourier transform of an elliptical Gaussian. This is itself a Gaussian, and thus the visibilities are “tapered” with weights decreasing as a function of uv-radius.
The uvtaper parameter expands the menu upon setting uvtaper=True to reveal the following sub-parameters:
outertaper = [] # uv-taper on outer baselines in uv-plane
innertaper = [] # uv-taper in center of uv-plane (not
implemented)
The sub-parameters specify the size and optionally shape and orientation of this Gaussian in the uv-plane or optionally the sky plane. The outertaper refers to a Gaussian centered on the origin of the uv-plane.
Some examples:
outertaper=[’5klambda’] # circular uv taper FWHM=5 kilo-lambda
outertaper=[’5klambda’,’3klambda’,’45.0deg’] # elliptical Gaussian
outertaper=[’10arcsec’] # on-sky FWHM 10"
outertaper=[’300.0’] # 300m in aperture plane
Note that if no units are given on the taper, then the default units are assumed to be meters in aperture plane.
ALERT: The innertaper option is not yet implemented.
More information about CASA may be found at the
CASA web page
Copyright © 2010 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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