Optimal null-constrained source encoding in TRY interferometers is achieved by noise-weighted projection of the derivative response, retaining Fisher information reduced exactly by the factor 1-χ² where χ is the inverse-noise overlap.
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Optimal Null-Constrained Source-Basis Sensing in a Time-Reversed Young Interferometer
Optimal null-constrained source encoding in TRY interferometers is achieved by noise-weighted projection of the derivative response, retaining Fisher information reduced exactly by the factor 1-χ² where χ is the inverse-noise overlap.