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While the pre-launch version of Calnic C used a pre-computed model of
the background in space, it has since been replaced by empirical
estimates for each grism. These new estimates were computed by
medianing several sparse images together. Calnic C and NICMOSlook
scale these pre-defined backgrounds using a scaling factor that is
calculated by taking the mean flux values of a region surrounding each
spectrum, and dividing it by the mean of the background image in the
same region. The scaled background estimate is then subtracted from
the grism image prior to extracting each spectrum.
The region used to scale the background is the same one that is used
by the Interpolated Background Subtraction method described in
section 3.4.2. Figure 3.2 shows an example
of how Calnic C chose the region in a complex situation.
The uncertainty in the background estimate is computed from the error
plane of the grism image. The uncertainty is the square root of the
sum of the errors divided by the square root of the number of pixels.
Wolfram Freudling
5/29/1999