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Impact of Uncertainties in Spectral Energy Distribution Modelling on Inferred Galaxy Properties
Gareth T. Jones, Conor M. Byrne, Elizabeth R. Stanway
Interpreting galaxy properties from astronomical surveys relies heavily on spectral energy distribution (SED) modelling, yet uncertainties in key model ingredients are often overlo…
What do we mean by stellar mass? The impact of the pre-main sequence on the mass to light ratio of young and intermediate age stellar populations
Elizabeth R. Stanway, Conor M. Byrne, Ankur Upadhyaya
Stellar population synthesis models are an essential tool with which galaxy physical parameters are extracted from observations. However they are built on assumptions designed for…
BPASS stellar evolution models incorporating -enhanced composition -- I. Single star models from 0.1 to 316 M
Conor M Byrne, Jan J Eldridge, Elizabeth R Stanway
Stellar evolution modelling is fundamental to many areas of astrophysics including stellar populations in both nearby and distant galaxies. It is heavily influenced by chemical com…