Physics

Infrared

Far ultraviolet

Infrared astronomy

Galaxy

Optics

Astronomy

Ultraviolet

Astrophysics

Spectral line

Far infrared

Monthly Notices of the Royal Astronomical Society

We combine the SHARK semi-analytic model of galaxy formation with the PROSPECT software tool for spectral energy distribution (SED) generation to study the multiwavelength emission of galaxies from the far-ultraviolet (FUV) to the far-infrared (FIR) at 0

From the far-ultraviolet to the far-infrared – galaxy emission at 0 ≤ z ≤ 10 in the shark semi-analytic model