Best fits of the constructed SEDs of Astarte and Adonis along with their relative residuals. The SED of Astarte (left) is produced using the LF17 attenuation law. The SED of Adonis (right) is produced using the CF00 attenuation law. The best fit is shown in black. The unattenuated stellar emission is shown with the blue line. The filled region shows the difference between the unattenuated and the attenuated stellar emission, absorbed by dust. Red dots are the best-fit values of the observations, which are shown with the purple boxes. Upper limits are shown as purple triangles.