Fig. 5.
Summary of observations of the optical and near-infrared excess background over the integrated light of galaxies (ILG). The thick horizontal red bar indicates the lower limit we obtained. The solid black line represents the model ILG which includes all galaxies (Totani & Yoshii 2000; Matsumoto et al. 2005). (Color online)

Summary of observations of the optical and near-infrared excess background over the integrated light of galaxies (ILG). The thick horizontal red bar indicates the lower limit we obtained. The solid black line represents the model ILG which includes all galaxies (Totani & Yoshii 2000; Matsumoto et al. 2005). (Color online)

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