If temporal variation is spatially uniform, summing all frames in each group still gives independent Poisson distribution totals, but their means may now be with ratio . At high counts and negligible read noise, direct propagation gives
After dividing the ratio image by its measured mean , the appropriate estimator is
The original formula is recovered only for . Uniform brightness drift does not automatically create a spatial pattern or extra ratio scatter beyond these changed noise levels; its leading problem is unequal group normalization. Interleave the groups in time or pair exposures of comparable flux, measure their separate means, and propagate shot and read noise when rescaling. If the spatial pattern or photodetector sensitivity also evolves, the ratio develops systematic structure that must be modeled or those frames rejected. A normalization inferred from finitely many detector pixels introduces a small shared correlation, which vanishes in the large-pixel limit and can be included in a precise uncertainty analysis.

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