Fraction of light in CG+IGL (or ICL) compared to the total group light (f_{CG + IGL(or ICL)}) of the KiDS+GAMA groups at different redshifts from the 0^th order (p₀) background-subtracted images. The x-axis indicates the mean halo mass M₂₀₀ of the corresponding bins for this work (shaded regions), and the group/cluster halo mass for the previous works (different markers). Pink, yellow, and cyan shaded regions show the upper and lower limit of f_CG + IGL for the redshift ranges 0.09 < z < 0.15, 0.16 < z < 0.21, and 0.21 < z < 0.27, respectively. The diamonds, left-facing-triangles, and right-facing-triangles show previous works from Kluge et al. (2021), Furnell et al. (2021), and Gonzalez et al. (2007), respectively. The redshift ranges of the previous works are shown in the colourbar. Our results agree with a high f_CG + IGL value for low halo masses.