Pulsational versus binary/atmospheric properties of the eclipsing binaries with g-modes. The plots in the left column show the distributions of N_ind and those in the right column show the distributions of f_max. The first row is a display of stacked histograms of N_ind and f_max, with the vertical axis representing the number of systems (N_*). For the first row of plots, systems where only g modes were detected are represented in blue, and systems where both p and g modes were detected are represented in orange. The 2nd, 3rd and 4th rows are displays of the variation of f_max and N_ind with respect to log P_orb (2nd row), T_eff (3rd row) and e (4th row). For the 2nd, 3rd and 4th rows of plots, stars where only g modes were detected are represented by blue circles, and stars where both p and g modes were detected are represented by orange triangles.