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Home All issues Volume 557 (September 2013) A&A, 557 (2013) A66 Full HTML
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Fig. 4

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Effective SEDs of infrared galaxies used in our model at various redshifts. The upper panel shows the SEDs in νLν units normalized at LIR = 1  L⊙ as a function of rest-frame wavelength. The lower panel shows the ratio between the observed flux density and LIR as a function of observed wavelength.

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