Same as Fig. 2. HD 76460 has a single peak at 55.866 d⁻¹ (P = 26 min) not previously noted in the literature, with a significant amplitude of 58 ± 7 μmag. It could be a high-frequency δ Sct star, or a very low frequency roAp star. HD 85766 has no rotational variation, but does appear to have two, or more, very low amplitude δ Sct peaks not previously noted in the literature; the two with the highest amplitude are at 36.8877 d⁻¹ (A = 97 μmag) and 33.2056 d⁻¹ (A = 82 μmag). Most δ Sct stars show low frequency peaks in the g-mode range, but this star does not, supporting the Ap (SiCr) classification.