feather – Combine two images using their Fourier transforms – imaging task
Description
This task can be used as one method of combining single-dish and interferometric images after they have been separately made.
The algorithm converts each image to the gridded visibility plane, combines them, and reconverts them into an combined image. Each image must include a well-defined beam shape (clean beam) in order for feathering to work well. The two images must have the same flux density normalization scale.
Parameters
Parameter |
Default |
Description |
|---|---|---|
imagename |
|
Name of output feathered image |
highres |
|
Name of high resolution (interferometer) image |
lowres |
|
Name of low resolution (single dish) image |
sdfactor |
|
Scale factor to apply to Single Dish image |
effdishdiam |
|
New effective SingleDish diameter to use in m |
lowpassfiltersd |
|
Filter out the high spatial frequencies of the SD image |
Parameter Explanations
imagename
''
- Name of output feathered image
Default: none
Example: imagename=’orion_combined.im’
highres
''
- Name of high resolution (interferometer) image
Default: none
Example: imagename=’orion_vla.im’
lowres
''
- Name of low resolution (single dish) image
Default: none
Example: imagename=’orion_gbt.im’
sdfactor
float(1.0)
- Value by which to scale the Single Dish image.
Default: 1.0
Basically modifying the flux scale of the SD image
effdishdiam
float(-1.0)
- New effective SingleDish diameter to use in m
Default: -1.0 (leave as is)
Obviously one can only reduce the dish effective dish diameter in feathering.
lowpassfiltersd
False
- Filter out the high spatial frequencies of the SD image
Default: False
If True the high spatial frequency in the SD image is rejected.
Any data outside the maximum uv distance that the SD has illuminated is filtered out.