Description
This functions use an image from a single dish and make a model
(clean component) image out of it. This allows one to use this as the
starting model in a deconvoltion function e.g
clean or
mem
This provides an alternative to
feather.
The difference between the two is that in
feather the
interferometer image is deconvolved first and the single dish image is
put in at the end. Whereas if one starts with a model from the single
dish image it will give a different starting point for the deconvolving
algorithm to interpolate the missing short baseline.
The function setsdoptions to set
a factor by which to scale the SD image, if necessary.
The sdpsf parameter (optional) should be used if an external PSF image of the
single dish is needed to calculate the beam parameters of the primary
beam of the dish. This is usually needed if the dish image is from a
non standard telescope or the beam is not in the aips++ system.
This parameter should point to an image, if you have a vptable made from vpmanager then setvp should be used to define this beam.
The mask is a mask image that may be needed to be used for
clean. This is usually the case when the dish image does not fully
cover the field defined by setimage.
Arguments
sdimage |
in |
Single Dish image |
|
|
Allowed: |
String |
|
|
Default: |
'' |
modelimage |
in |
Name of output image to be used as model |
|
|
Allowed: |
String |
|
|
Default: |
'' |
sdpsf |
in |
PSF of Single Dish if needed |
|
|
Allowed: |
String |
|
|
Default: |
'' |
maskimage |
in |
mask image |
|
|
Allowed: |
String |
|
|
Default: |
'' |
Returns
Bool
Example
myim:=imager('orion\_only.ms')
myim.setdata(fieldid=[1:10], spwid=[1:2])
myim.setimage(nx=1000, ny=1000, cellx='1arcsec', celly='1arcsec', fieldid=5, spwid=[1,2])
myim.setvp(dovp=T)
myim.setoptions(ftmachine='mosaic')
myim.setscales(nscales=3)
myim.setsdoptions(scale=0.9);
myim.makemodelfromsd(sdimage='orion\_gbt.im', modelimage='orion\_model', maskimage='orion.mask')
myim.clean(algorithm='mfmultiscale', model='orion\_model',
residual='orion.residual', image='orion.restored', gain=0.2, niter=500, mask='orion.mask')
In the above example we are making a mosaic with the fields 1 to 10. A
single dish image orion_gbt.im is used scaled down by a factor 0.9 to
make the initial model that is passed to multi-scale clean.
Next: imager.mask - Function
Up: imager - Tool
Previous: imager.makeimage - Function
 
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2006-10-15