Stacked distributions (magnified by 30) of the secondary-only EB and occulting-only giant planets for their eclipse/transit depth (upper-left plot), eclipse/transit duration (upper-right plot), orbital period (middle-left plot), inclination (middle-right plot), eccentricity (lower-left plot), and argument of periastron (lower-right plot). The distribution have been normalized to represent the relative occurrence as computed in Table 1. Corresponding distributions of Kepler objects of interest (from Batalha et al. 2012, dashed black line) are also displayed, when known. The vertical dotted line in the upper-left plot represent the commonly-used 3% upper limit in depth of planetary transit candidates.