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Which mechanism limits achievable resolution when fitting functions to noisy interferometry data?

A)Heisenberg uncertainty regarding wavefront curvature
B)Nyquist limit obstructing fringe reconstruction
C)Wave function collapse biasing measurement
D)Superposition preventing deterministic deconvolution

💡 Explanation

The Nyquist limit restricts function fitting because undersampling high-frequency components causes aliasing, therefore correct wavefront phase reconstruction becomes impossible, rather than other limits affecting noise impact.

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