A Herschel view of the far-infrared properties of submillimetre galaxies

B. Magnelli; D. Lutz; P. Santini; A. Saintonge; S. Berta; M. Albrecht; B. Altieri; P. Andreani; H. Aussel; F. Bertoldi; M. Béthermin; A. Bongiovanni; P. Capak; S. Chapman; J. Cepa; A. Cimatti; A. Cooray; E. Daddi; A. L. R. Danielson; H. Dannerbauer; J. S. Dunlop; D. Elbaz; D. Farrah; N. M. Förster Schreiber; R. Genzel; H. S. Hwang; E. Ibar; R. J. Ivison; E. Le Floc’h; G. Magdis; R. Maiolino; R. Nordon; S. J. Oliver; A. Pérez García; A. Poglitsch; P. Popesso; F. Pozzi; L. Riguccini; G. Rodighiero; D. Rosario; I. Roseboom; M. Salvato; M. Sanchez-Portal; D. Scott; I. Smail; E. Sturm; A. M. Swinbank; L. J. Tacconi; I. Valtchanov; L. Wang; S. Wuyts

doi:10.1051/0004-6361/201118312

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Volume 539 (March 2012)

A&A, 539 (2012) A155

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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

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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