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Fig. 1.


SED of AGS1 shown as an example. The solid black line represents the best fit, which can be decomposed into the IR dust contribution (brown line), a stellar component uncorrected for dust attenuation (dark blue line), synchrotron emission (purple line) and the AGN contribution (orange line). An extrapolation of the AGN model of Kirkpatrick et al. (2015) to shorter wavelengths is displayed with an orange dashed line. In addition, we show the best fit of a modified black body, with β = 1.5 (light blue line). The corrected UV emission is also shown in green. Bottom panel: residuals: (observation – model)/observation. The 34 other SEDs are given in the appendix (see Fig. A.1).

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