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Over half of the far-infrared background light comes from galaxies at z greater than or equal to 1.2

Mark J. Devlin, Peter A. R. Ade, Itziar Aretxaga, James J. Bock, Edward L. Chapin, Matthew Griffin, Joshua O. Gundersen, Mark Halpern, Peter C. Hargrave, David H. Hughes, Jeff Klein, Gaelen Marsden, Peter G. Martin, Philip Mauskopf, Lorenzo Moncelsi, Calvin B. Netterfield, Henry Ngo, Luca Olmi, Enzo Pascale, Guillaume Patanchon, Marie Rex, Douglas Scott, Christopher Semisch, Nicholas Thomas, Matthew D. P. Truch, Carole Tucker, Gregory S. Tucker, Marco P. Viero & Donald V. Wiebe

Nature 458, 737-739(9 April 2009)

doi:10.1038/nature07918

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Figure 1

Map showing the signal-to-noise ratio combination of all three BLAST bands for the entire BLAST GOODS-South observation.

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Figure 2

The differential source counts at a variety of submillimetre and far-infrared wavelengths.

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Table 1

Source confusion limits determined by BLAST

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Table 2

The results of the 24-microm stacked flux

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