imager.setmfcontrol - Function

2.3.1 Set various cycle control parameters for multi-field and wide-field imageing.
Description

Control parameters for mosaicing or wide-field imaging which are not required in single field deconvolution are set here to streamline the user interface. As multifield and widefield imaging is accomplished by deconvolution in cycles, many of these parameters control how the deconvolution cycles are ended.

cyclefactor: this parameter helps in lowering or increasing the threshold at which the deconvolution cycle will stop and degrid and subtract from the visibilities. For very bad PSFs you may want to reconcile with the visibilties often, thus a larger number is required here...(4 to 5). For very well behaved data you may want to deconvolve deep before reconciling: a lower number is used (1.5 to 2.0).
cyclespeedup: this is used if the PSF is not well behaved and you want clean to raise by 2 the threshold if it has not reached the threshold in this number of iteration
stoplargenegatives: This parameter is exclusively for when using multiscale clean. This is used to stop the component search when the largest scale has found this number of negative components. -1 here means that continue component search even if the largest component is negative.
stoppointmode: Again exclusively for when using multiscale clean. The clean will stop if the smallest scale receives this number of consecutive components.
minpb: This is to defined up to what level the voltage pattern is going to applied when using setvp. The default is 0.1 of the primary beam or the voltage pattern defined for the antenna.
scaletype: This parameter cab be NONE or SAULT. If NONE the image is not scaled, if SAULT is used the image is weighted so that the noise is kept uniform across the image. The next two parameters defines how the SAULT weighting is limited. Obviously then the flux scale is not uniform across the image. To get the right flux multiply the image with the fluxscale image.
constpb: this parameter defines up to what amplitude of the Primary beam the noise floor is kept uniform, when using SAULT as scaletype.
fluxscale: use this to give a filename to store the factor image to apply to the image to get the fluxscale right.

Arguments





Inputs

cyclefactor

Cycle threshold = this * max sidelobe * max resid

allowed:

double

Default:

1.5

cyclespeedup

Cycle threshold doubles in this number of iterations

allowed:

double

Default:

-1

stoplargenegatives

Stop the multiscale cycle for the first n cycles when a negative comp is found on the largest scale

allowed:

int

Default:

2

stoppointmode

Stop multiscale altogether if the smallest scale recieves this many consecutive components

allowed:

int

Default:

-1

minpb

Minimum PB level to use

allowed:

double

Default:

0.1

scaletype

Image plane flux scale type

allowed:

string

Default:

SAULT NONE NONE

constpb

In Sault weighting the flux scale is constant above this PB level

allowed:

double

Default:

0.4

fluxscale

Names of flux scale images for mosaicing

allowed:

stringArray

Default:

Returns
bool

Example

im.setmfcontrol(cyclefactor=2.0, cyclespeedup=niter/10,  
stoplargenegatives=T, stoppointmode=10, fluxscale=’image.fluxscale’);

Please send any comments or questions about CASA or AIPS++ to aips2-requests@nrao.edu

Copyright © 2008 Associated Universities Inc., Washington, D.C.

This code is available under the terms of the GNU General Public Lincense


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Updated daily during alpha development.