The intragroup light in KiDS+GAMA groups - A stacking analysis

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Table 1.

Measurements of IGL and CG+IGL for our KiDS+GAMA group sample shown in Figs. 9 and 10.

z	${log}_{10} (\frac{M_{200}}{M_{⊙}})$ $\log_{10}(\frac{M_{200}}{\mathrm{M}_\odot})$	CG Mag_r	L_IGL/L_Tot	L_CG + IGL/L_Tot
	12.79	−22.40	0.14–0.19	0.67–0.71
0.12	13.11	−22.93	0.05–0.16	0.63–0.76
	13.53	−23.43	0.02–0.07	0.58–0.70

	13.03	−22.33	0.11–0.21	0.59–0.63
0.18	13.40	−23.07	0.07–0.17	0.60–0.68
	13.85	−23.62	0.06–0.10	0.62–0.70

	13.38	−22.60	0.12–0.15	0.54–0.61
0.24	13.71	−23.27	0.11–0.19	0.51–0.56
	13.94	−23.81	0.04–0.07	0.65–0.67

Notes. First three columns show the mean redshift, halo mass, and r-band CG magnitudes of the CG M_r bins used in this work, respectively. The value ranges in L_IGL/L_Tot and L_CG + IGL/L_Tot columns show the lower and upper limits of our measurements as described in Sect. 5.5.

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