Fig. 7.
Comparison of the ratio of the total attenuation derived from the best-fit model of MAGPHYS to that of HYPERZ, the size ratio of Hα to the FIR continuum (left), and the total infrared luminosity (right). Data points are plotted along with their corresponding IDs, which have their field names removed for clarity. Sources that are identified to host an AGN are marked with an asterisk after the ID. We find a correlation between the ratio of attenuation and the infrared luminosity.
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