Open Access
Fig. 4.
Decomposition of the ultraviolet, optical and near-infrared SED of the Seyfert-2 galaxy NGC 1068, including multi-aperture flux measurements taken from the NASA/IPAC Extragalactic Database (NED). Dust re-emission by the AGN circumnuclear region is not accounted for as it only becomes preponderant at λ > 1 μm.
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