Table 1:

Log of Herschel observations.

Cluster
z Instrument $\lambda$ Obsid Flux
      ($\mu $m)   (mJy)
A1068 0.1386 PACS 70 1 342 187 051 542 $\pm$ 6
    PACS 100 1 342 187 053 757 $\pm$ 6
    PACS 160   769 $\pm$ 4
    SPIRE 250 1 342 187 321 376 $\pm$ 6
    SPIRE 350   135 $\pm$ 6
    SPIRE 500   56 $\pm$ 8
    SCUBA 450   39 $\pm$ 13
    SCUBA 850   5.3 $\pm$ 1.1
    Spitzer 24   74.5 $\pm$ 2.0
    Spitzer 70   941 $\pm$ 30
    IRAS 60   577 $\pm$ 52
    IRAS 100   958 $\pm$ 144
A2597 0.0821 PACS 70 1 342 187 118 57 $\pm$ 5
    PACS 100 1 342 187 120 67 $\pm$ 7
    PACS 160   86 $\pm$ 4
    SPIRE 250 1 342 187 329 30 $\pm$ 6
    SPIRE 350   15 $\pm$ 6
    SPIRE 500   <16
    SCUBA 850   14.5 $\pm$ 2.3
    Spitzer 24   2.1 $\pm$ 0.2
    Spitzer 70   49 $\pm$ 6
    Spitzer 160   52 $\pm$ 3
Zw3146 0.2906 PACS 70 1 342 187 043 94 $\pm$ 6
    PACS 100 1 342 187 045 150 $\pm$ 6
    PACS 160   139 $\pm$ 5
    SPIRE 250 1 342 187 326 81 $\pm$ 6
    SPIRE 350   30 $\pm$ 6
    SPIRE 500   <16
    SCUBA 450   <48
    SCUBA 850   6.6 $\pm$ 2.6
    Spitzer 24   4.1 $\pm$ 0.4
    Spitzer 70   68 $\pm$ 14
    Spitzer 160   157 $\pm$ 35

Notes. The Spitzer data are from Quillen et al. (2008), Donahue et al. (2007, priv. comm.) and Egami et al. (2006). The SCUBA data are from Edge (priv. comm.), Zemcov et al. (2007) and Chapman et al. (2002).


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