COLIBRE hydrodynamical simulations reproduce observed HI and H2 Kennicutt-Schmidt relations at z~0 and predict H2 depletion time drops by a factor of ~20 from z=0 to z=8 due to falling metallicity, matching observations to z=5.
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Different SED fitting techniques and data types produce stellar parameters and xi_ion values differing by up to 1.1 dex even for a homogeneous sample of z=3 EoR-analog galaxies, with apparent redshift evolution of xi_ion appearing only under consistent methodology.
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Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
COLIBRE hydrodynamical simulations reproduce observed HI and H2 Kennicutt-Schmidt relations at z~0 and predict H2 depletion time drops by a factor of ~20 from z=0 to z=8 due to falling metallicity, matching observations to z=5.
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Exploring biases in derived stellar parameters and the ionizing photon production efficiency
Different SED fitting techniques and data types produce stellar parameters and xi_ion values differing by up to 1.1 dex even for a homogeneous sample of z=3 EoR-analog galaxies, with apparent redshift evolution of xi_ion appearing only under consistent methodology.