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Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations
We present predictions from the COLIBRE cosmological hydrodynamical simulations of galaxy formation for the present-day galaxy luminosity functions (LFs) at wavelengths ranging from the far-ultraviolet (FUV) to the submillimetre. The simulations are post-processed with the radiative transfer code SK
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