Documentation on mosmem
Task: mosmem
Purpose: Maximum Entropy deconvolution for a mosaiced image
Categories: deconvolution
MOSMEM is a MIRIAD task which performs a (joint) maximum entropy
deconvolution of a mosaiced image.
Key: map
The input dirty map, which should have units of Jy/beam, which was
produced by INVERTs mosaic mode.
Key: beam
The input dirty beam, also produced by INVERTs mosaic mode. No
default
Key: model
An initial estimate of the deconvolved image. For point sources,
giving a good initial model may help convergence. In principle,
this only helps convergence, but should not affect the final
solution. The model could be the output from a previous run of
MOSMEM or any other deconvolution task. It must have flux units of
Jy/pixel. The default is a flat estimate, with the correct flux.
Key: default
The default image. This is the image that the final solution will
tend towards. The final result will be influenced by this default
if the constrains that the data put on the solution are weak.
The default is a flat estimate, with the correct flux.
Key: out
The name of the output map. The units of the output will be Jy/pixel.
It can be input to RESTOR or MOSMEM (as a model, to continue the
deconvolution process).
Key: niters
The maximum number of iterations. The default is 30.
Key: region
This specifies the region to be deconvolved. See the Users Manual
for instructions on how to specify this. The default is the entire
image.
Key: measure
The entropy measure to be used, either "gull" (-p*log(p/e)) or
"cornwell" (-log(cosh(p)) -- also called the maximum emptiness
criteria).
Key: tol
Tolerance of solution. There is no need to change this from the
default of 0.01.
Key: q
An estimate of the number of points per beam. MOSMEM can usually
come up with a good, image-dependent estimate.
Key: rmsfac
MOSMEM knows the theoretical rms noise of the input dirty map, and
will, by default, attempt to reduce the residuals to have an rms of
this amount. If the true rms noise is different from the theoretical,
you may give the factor to multiply by to convert from theoretical
to true rms noise.
The theoretical rms will usually be an optimistic estimate of the
true noise level. The true noise will be increased by calibration
errors, confusion, poorly understood distant sidelobes, etc, so
rmsfac will usually give some `fudge factor' greater than 1.
Key: flux
An estimate of the total flux of the source. Giving a good total flux
will help MOSMEM find a good solution. On the other hand, giving
a poor value may do harm. Normally MOSMEM will NOT constrain the
total flux to be this value, but see the ``doflux'' option below.
The default is image-dependent for measure=gull, and zero for
measure=cornwell.
Key: options
Task enrichment parameters. Several can be given, separated by
commas. Minimum match is used. Possible values are:
doflux Constraint the flux to be that given by the "flux"
parameter. Normally the "flux" parameter value is only
used to determine the default image level.
verbose Give lots of messages during the iterations. The default
is to give a one line message at each iteration.
Generated by rsault@atnf.csiro.au on 11 Jul 1996