Observed and simulated photometry for NGC 4349 No. 127. Top: V magnitudes extracted from ASAS-3 plotted against time (colored dots). The color-coding is the same as in Fig. 4 and refers to the RV period. We also plot binned means (black rectangles) as well as the photometric variability predicted by the l = 1, m = 1 oscillation model (continuous multi-colored line). We further overplot a sinusoidal fit with period 2571 d in black. Bottom: ASAS-3 V magnitudes phase-folded to the 2571 d period.