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One wants to
separate sources from the underlying
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sky
background, but:
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The background
is often far from homogeneous (halos from
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bright stars,
flat-field residuals), and it varies from exposure to
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exposure,
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The practical
definition of the background itself is ambiguous,
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especially in
crowded fields.
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One must rely on the crude assumption
that the
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background is
much “smoother” than the light
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distribution
of the overlying sources.
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