An interactive surface plot of the irradiation effect light-curve amplitudes of post-CE binary stars. The translucent plane is the approximate ground-based detection limit of 0.1 mag. The interactivity is available online, where the spectral type of the MS star can be changed to see its corresponding set of amplitudes, and the figure can be rotated and zoomed in and out. Hovering over a point reveals whether a binary with those parameters is eclipsing, and the detection limit can be toggled on or off.
An interactive version of this figure is available in the online journal.