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