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NRAO Home > CASA > CASA Toolkit Reference Manual |
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deconvolver.fullclarkclean - Function
3.1.2 Make a clean image using the Clark Clean a threshold
Description
This is similar to clarkclean except that it accepts casa standard images. I.e it
has to have 4 axes with the canonical order of (direction1, direction2, stokes,
spectral). This function further will clean more than the quarter of the image
if the mask coverage is larger than a quarter of the image size. It is useful for
CLI level parallelization, i.e use imager to make a dirty image and psf and use
this function to deconvolve. If in doubt use clarkclean
Arguments
Inputs |
| ||
niter |
| Number of iterations | |
| allowed: | int |
|
| Default: | 1000 | |
gain |
| Loop Gain for CLEANing
| |
| allowed: | double | |
| Default: | 0.1 |
|
threshold |
| Flux level at which to stop CLEANing
| |
| allowed: | any |
|
| Default: | variant 0Jy |
|
model |
| Name of model image that will contain the clean
components
| |
| allowed: | string |
|
| Default: |
|
|
mask |
| Name of mask image used for CLEANing
| |
| allowed: | string |
|
| Default: |
|
|
cyclefactor |
| Factor to determine how deep to go in a Clark minor
cycle
| |
| allowed: | double |
|
| Default: | 1.5 |
|
record
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