Table 1: Contribution to the CIB of $S_{24} \ge 60~\mu$ Jy galaxies. Sources of uncertainty come from photometry, calibration, and large scale structure. The CIB column gives the best estimate from the discussion in Sect. 4.1.
$\lambda$ $\nu I_{\nu}$ B $_{\lambda}$ CIB % CIB

$\mu$ m nW m^-2 sr^-1 MJy/sr MJy/sr resolved

24 $2.16 \pm 0.34$ $0.017 \pm 15$ % 0.022 79

70 $5.93 \pm 1.02$ $0.138 \pm 17$ % 0.15 92

160 $10.70 \pm 2.28$ $0.571 \pm 21$ % 0.82 69

**Table 1:** Contribution to the CIB of $S_{24} \ge 60~\mu$ Jy galaxies. Sources of uncertainty come from photometry, calibration, and large scale structure. The CIB column gives the best estimate from the discussion in Sect. 4.1.
$\lambda$	$\nu I_{\nu}$	B $_{\lambda}$	CIB	% CIB
$\mu$ m	nW m^-2 sr^-1	MJy/sr	MJy/sr	resolved
24	$2.16 \pm 0.34$	$0.017 \pm 15$ %	0.022	79
70	$5.93 \pm 1.02$	$0.138 \pm 17$ %	0.15	92
160	$10.70 \pm 2.28$	$0.571 \pm 21$ %	0.82	69

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