Fig. 7.

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Multiwavelength SEDs of the MW versus NGC 3521 across UV to radio decameter ranges, shown as log10[λLλ(λ)/L⊙]. Black curve: Best theoretical SED for NGC 3521 (Sect. 5.1) converted to intrinsic luminosity assuming D = 10.7 Mpc, and including 28 MHz UTR-2 measurement as a constraint. Red curve: Intrinsic SED of MW obtained by Natale et al. (2022) (originally provided as Lν) and recast to λLλ/L⊙ without any distance scaling. Yellow star: MW 28 MHz UTR-2 flux density scaled to D = 10.7 Mpc and converted to intrinsic luminosity; plotted as λLλ/L⊙.
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