Cosmological simulations predict that high-redshift galaxies transition between UV-bright and dusty IR-bright phases on roughly 100 Myr timescales, with ionizing escape fractions and metal-line luminosities fluctuating accordingly.
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Galaxy evolution and radiative properties in the early Universe: multi-wavelength analysis in cosmological simulations
Cosmological simulations predict that high-redshift galaxies transition between UV-bright and dusty IR-bright phases on roughly 100 Myr timescales, with ionizing escape fractions and metal-line luminosities fluctuating accordingly.