Broad-band SED of HE 1353−1917 and best-fit template models inferred with AGNFITTER (Calistro Rivera et al. 2016). The black points represent the observed photometric data with their associated error bars. One hundred representative template SEDs are overplotted from the MCMC sampling. The total SEDs are shown as red lines which are further split up into their sub-component, (1) the AGN optical-UV emission (blue lines), (2) the stellar continuum (yellow lines), (3) the hot torus emission (purple lines), and (4) the cold+warm dust emission from star formation (green lines).