Open Access
Table A.1.
Different parametric forms of the star formation history that we used with BAGPIPES. Each model has its own parameters and we specify the uniform priors used in this work.
| SFH model | Priors |
|---|---|
| Constant | Maximum age ∈ [1 Myr, 1 Gyr] |
| Log-normal | Age of the Universe at peak SF ∈ [1 Myr, 1 Gyr] |
| Full width at half maximum SF ∈ [0, 1 Gyr] | |
| Exponentially Declining | Time since SFH began ∈ [1 Myr, 1 Gyr] |
| Timescale of decrease τ ∈ [0, 10 Gyr] | |
| Double-Power Law | Falling slope index ∈ [0, 10] |
| Rising slope index ∈ [0, 10] | |
| Age of the Universe at turnover τ ∈ [1 Myr, 1 Gyr] |
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