Free Access
Issue
A&A
Volume 539, March 2012
Article Number A155
Number of page(s) 35
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/201118312
Published online 12 March 2012

Online material

Table 1

Main properties of the PEP/HerMES fields used in this study.

Table 2

Main properties of the ancillary used in this study.

Table 3

Mid- and far-infrared properties of our GOODS-N SMG sample.

Table 4

Submm, radio and redshift properties for our GOODS-N SMG sample.

Table 5

Mid- and far-infrared properties of our GOODS-S SMG sample.

Table 6

Submm, radio and redshift properties for our GOODS-S SMG sample.

Table 7

Mid- and far-infrared properties of our LH SMG sample.

Table 8

Submm, radio and redshift properties for our LH SMG sample.

Table 9

Mid- and far-infrared properties of our COSMOS SMG sample.

Table 10

Submm, radio and redshift properties for our COSMOS SMG sample.

Table 11

Mid- and far-infrared properties of our lensed-SMG sample.

Table 12

Submm, radio, redshift and magnification properties for our lensed-SMG sample.

Table 13

Dust properties of our SMGs.

Appendix A: SED fits

thumbnail Fig. A.1

Spectral energy distribution of our SMGs. Red diamonds present the PACS and SPIRE measurements, while green squares present multi-wavelength ancillary data taken from the literature. The modified blackbody emission (β = 1.5) best-fitting the data are shown by dashed blue lines. The power-law temperature distribution model (β = 2.0, γ = 7.3 and R = 3   kpc) which best-fits the data are shown by solid red lines. Dotted lines present the CE01 SED template which best-fits the far-infrared observations.

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© ESO, 2012

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