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Table 2:

Estimated fluxes in the 60 $\mu $m and 100 $\mu $m IRAS bands from the galaxy population of the SDSS-maxBCG clusters.

Spectral type
  F60 F100
    (Jy) (Jy)
-Early-type      
BCG   8.2 16.5
E/S0   31.1 62.9
(Total early-type)   (39.3) (79.4)
       
-Late-type      
Sa   36.4 58.6
Sb   259.5 621.3
Sc   333.9 1133.4
Starburst   15.4 12.1
(Total late-type)   (645.2) (1825.4)
       

Total
  $\rm 684.5_{-138.0}^{+211.3}$ $\rm 1904.8_{-429.1}^{+617.1}$
Observed   570.1 $\pm$ 36.1 1359.9 $\pm$ 249.1

Notes. We show the total fluxes and contribution of each galaxy population included in our model. The quoted errors on the total values correspond to the differences between our reference model and the conservative and extreme scenarios described in Sect. 3.4. The measurements by Giard et al. (2008) are reported together with their 1$\sigma$ error bars.


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