Las Cumbres Observatory image of the host star HD 22946 in the rp filter. The ten sources identified by pink circles as T2 through T11 are within a 2.5′ radius of TOI-411 and are potentially bright enough (see text) to cause the TOI-411 b/c signals. The nine closest nearby sources are also displayed in Fig. 3 and fall just outside the automatic, SPOC-based aperture used in Sector 4.