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NRAO Home > CASA > CASA Toolkit Reference Manual |
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linearmosaic.defineoutputimage - Function
3.1.3 Set the output direction image parameters and name
Description
Define the direction axes output image parameters. The output image will get
the same number of spectral and polarization planes as the input images. This
function create a fresh new output image. If an image of the same name exist
on disk it will be erased. The spectral and polarization part of the image will
be identical to the images that are being mosaiced.
The output image will by default be flux correct and the weight image will be ∑ pAp2(θ) where the primary beam is Ap(θ)
Arguments
Inputs |
| ||
nx |
| Total number of spatial pixels in x
| |
| allowed: | int | |
| Default: | 128 |
|
ny |
| Total number of spatial pixels in y
| |
| allowed: | int | |
| Default: | -1 |
|
cellx |
| Cellsize in x (e.g. ’1arcsec’)
| |
| allowed: | any |
|
| Default: | variant 1.0 |
|
celly |
| Cellsize in y (e.g. ’1arcsec’)
| |
| allowed: | any |
|
| Default: | variant
|
|
imagecenter |
| Direction of phase center as a diretion measure
| |
| allowed: | any |
|
| Default: | variant 0 |
|
outputimage |
| output image name
| |
| allowed: | string |
|
| Default: |
|
|
outputweight |
| output weight image name
| |
| allowed: | string |
|
| Default: |
|
|
bool
Example
lm.defineoutputimage(nx=3000, cellx=’3arcsec’, imagecenter=’19h13m13.469 4d50m09.649’, outputimage=’test.linmos’, outputweight=’test.weightlinmos’)
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Copyright © 2016 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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