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- W2160041804 abstract "We examine the star formation histories (SFHs) of galaxies in smoothed particle hydrodynamics (SPH) simulations, compare them to parametric models that are commonly used in fitting observed galaxy spectral energy distributions, and examine the efficacy of these parametric models as practical tools for recovering the physical parameters of galaxies. The commonly used �-model, with u M� / e (t t i)/� , provides a poor match to the SFH of our SPH galaxies, with a mismatch between early and late star formation that leads to systematic errors in predicting colours and stellar mass-to-light ratios. A one-parameter lin-exp model, with u" @default.
- W2160041804 created "2016-06-24" @default.
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- W2160041804 date "2014-04-01" @default.
- W2160041804 modified "2023-09-27" @default.
- W2160041804 title "Parametrising Star Formation Histories" @default.
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