Contrast vs. separation sensitivity curves showing our classical reference star differential imaging (RDI; in dotted–dashed orange), classical RDI reduction from S. G. Wolff et al. (2023; in dotted green), NMF reduction (in solid purple), and the photon limit (in thick solid gray). We note that the NMF curve has better contrast out to 3″, after which both classical RDI reductions perform better. Our reductions also extend to a smaller radial separation because of the occulter location we used in our observations.