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
Main properties of the PEP/HerMES fields used in this study.
Main properties of the ancillary used in this study.
Mid- and far-infrared properties of our GOODS-N SMG sample.
Submm, radio and redshift properties for our GOODS-N SMG sample.
Mid- and far-infrared properties of our GOODS-S SMG sample.
Submm, radio and redshift properties for our GOODS-S SMG sample.
Mid- and far-infrared properties of our LH SMG sample.
Submm, radio and redshift properties for our LH SMG sample.
Mid- and far-infrared properties of our COSMOS SMG sample.
Submm, radio and redshift properties for our COSMOS SMG sample.
Mid- and far-infrared properties of our lensed-SMG sample.
Submm, radio, redshift and magnification properties for our lensed-SMG sample.
Dust properties of our SMGs.
Appendix A: SED fits
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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. |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
© ESO, 2012
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