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Conroy, Ch., Gunn, J. and White, M. (2009) The Propagation of Uncertainties in Stellar Population Synthesis Modeling I: The Relevance of Uncertain Aspects of Stellar Evolution and the IMF to the Derived Physical Properties of Galaxies. The Astrophysical Journal, 699, 486-506.
https://doi.org/10.1088/0004-637X/699/1/486

has been cited by the following article:

• TITLE: Cold or Warm Dark Matter?: A Study of Galaxy Stellar Mass Distributions

  AUTHORS: Bruce Hoeneisen

  KEYWORDS: Dark Matter, Warm Dark Matter, Dark Matter Properties, Galaxy Stellar Mass

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.10 No.2, April 3, 2020

  ABSTRACT: We compare the observed galaxy stellar mass distributions in the redshift range with expectations of the cold ΛCDM and warm ΛWDM dark matter models, and obtain the warm dark matter cut-off wavenumber:. This result is in agreement with the independent measurements with spiral galaxy rotation curves, confirms that kfs is due to warm dark matter free-streaming, and is consistent with the scenario of dark matter with no freeze-in and no freeze-out. Detailed properties of warm dark matter can be derived from kfs. The data disfavors the ΛCDM model.