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.help mkillumcor Oct88 noao.imred.ccdred
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NAME
mkillumcor -- Make flat field iillumination correction images
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USAGE
mkillumcor input output
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PARAMETERS
.ls input
List of input images for making flat field iillumination correction images.
.le
.ls output
List of output flat field iillumination correction images. If none is
specified or if the name is the same as the input image then the output
image replaces the input image.
.le
.ls ccdtype = "flat"
CCD image type to select from the input images. If none is specified
then all types are used.
.le
.ls xboxmin = 5, xboxmax = 0.25, yboxmin = 5, yboxmax = 0.25
Minimum and maximum smoothing box size along the x and y axes. The
minimum box size is used at the edges and grows to the maximum size in
the middle of the image. This allows the smoothed image to better
represent gradients at the edge of the image. If a size is less then 1
then it is interpreted as a fraction of the image size. If a size is
greater than or equal to 1 then it is the box size in pixels. A size
greater than the size of image selects a box equal to the size of the
image.
.le
.ls clip = yes
Clean the input images of objects? If yes then a clipping algorithm is
used to detect and exclude deviant points from the smoothing.
.le
.ls lowsigma = 2.5, highsigma = 2.5
Sigma clipping thresholds above and below the smoothed iillumination.
.le
.ls divbyzero = 1.
The iillumination correction is the inverse of the smoothed flat field.
This may produce division by zero. A warning is given if division
by zero takes place and the result (the iillumination correction value)
is replaced by the value of this parameter.
.le
.ls ccdproc (parameter set)
CCD processing parameters.
.le
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DESCRIPTION
First, the input flat field images are automatically processed if
needed. Then, the large scale iillumination pattern of the images is
determined by heavily smoothing them using a moving "boxcar" average.
The iillumination correction, the inverse of the iillumination pattern,
is applied by \fBccdproc\fR to CCD images to remove the iillumination
pattern introduced by the flat field. The combination of the flat
field calibration and the iillumination correction based on the flat
field is equivalent to removing the iillumination from the flat field
(see \fBmkillumflat\fR). This two step calibration is generally used
when the observations have been previously flat field calibrated. This
task is closely related to \fBmkskycor\fR which determines the
iillumination correction from a blank sky image; this is preferable to
using the iillumination from the flat field as it corrects for the
residual iillumination error. For a general discussion of the options
for flat fields and iillumination corrections see \fBflatfields\fR.
The smoothing algorithm is a moving average over a two dimensional
box. The algorithm is unconvential in that the box size is not fixed.
The box size is increased from the specified minimum at the edges to
the maximum in the middle of the image. This permits a better estimate
of the background at the edges, while retaining the very large scale
smoothing in the center of the image. Note that the sophisticated
tools of the \fBimages\fR package may be used for smoothing but this
requires more of the user and, for the more sophisticated smoothing
algorithms such as surface fitting, more processing time.
To minimize the effects of bad pixels a sigma clipping algorithm is
used to detect and reject these pixels from the iillumination. This is
done by computing the rms of the image lines relative to the smoothed
iillumination and excluding points exceeding the specified threshold
factors times the rms. This is done before each image line is added to
the moving average, except for the first few lines where an iterative
process is used.
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EXAMPLES
1. The example below makes an iillumination correction image from the
flat field image, "flat017".
cl> mkillumcor flat017 Illum
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SEE ALSO
ccdproc, flatfields, mkillumflat, mkskycor, mkskyflat
.endhelp
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