All Tables

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.
Table 2: Mean observed colors in $I_{\nu }$ of $S_{24} \ge 60~\mu$ Jy galaxies contributing to the CIB.
Table 3: Contributions of the 24 $~\mu$ m galaxies to the FIR CIB in nW m^-2 sr^-1. For the $S_{24} \le 60~\mu$ Jy galaxies, a simple color extrapolation has been used, as described in Sect. 5.