Panchromatic template SED of z > 0 QGs. Augmentation of the UV-to-MIR spectrum presented in this work with the FIR SED model of QGs presented in Magdis et al. (2021). The UV-to-MIR spectrum has been normalised to log(M_*/M_⊙) = 10 and the FIR model has been scaled to fit the MIR data resulting in a dust mass of log(M_dust/M_⊙) = 5.75 and a gas fraction of ≈0.5%. The full SED is shown as a solid black line and its associated uncertainty as a grey shaded region.