Examples of two kinds of eclipses of the F1-type pulsator. Left: a “deep” eclipse. One star transits the pulsator between moments 1 and 5, while the other only from 2 to 4. They eclipse each other in 3. Right: a triple eclipse. One star transits the pulsator between moments 1 and 2, and later between 5 and 6. The other star transits between 3 and 4. The wave-like modulation comes from pulsations. Note the same vertical scale on both panels. The exact depths vary slightly from one event to the other. Short-cadence data are shown.