Abstract
Abstract We apply a simple model, tested on local ultraluminous infrared galaxies (ULIRGs), to disentangle the active galactic nuclei (AGN) and starburst contributions in submillimetre and 24 εm-selected ULIRGs observed with the Spitzer–Infrared Spectrograph spectrometer. We quantitatively estimate the average AGN contribution to the stacked 6–8εm rest-frame spectra of these sources in different luminosity and redshift ranges and, under the assumption of similar infrared-to-bolometric ratios as in local ULIRGs, the relative AGN/starburst contributions to the total infrared luminosity. Though the starburst component is always dominant in submillimetre-selected ULIRGs, we find a significant increase of the AGN contribution at redshift z > 2.3 with respect to lower z objects. Finally, we quantitatively confirm that the mid-infrared emission of 24 εm-selected ULIRGs is dominated by the AGN component, but the starburst component contributes significantly to the bolometric luminosity.
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