v0.2.0

StarFormationHistories v0.2.0

Diff since v0.1.1

Breaking changes

• This version transitions from separate fitting functions for different AMRs (e.g., fit_templates_mdf and fit_templates_logamr) to a single fitting function fit_sfh whose behavior is determined by arguments that set the metallicity evolution and dispersion models to use. This design enables more flexibility with respect to the types of AMR and MZR models that can be used. The HMC sampling routines have likewise been transitioned to a single sample_sfh function. For now the old methods are still included but will be deprecated in the future. The example notebook at examples/fitting1.ipynb has been updated to use these new interfaces.

Merged pull requests:

• Add method for arbitrary SFH to construct_x0_mdf (#48) (@cgarling)
• Number-weighted mdf_amr (#49) (@cgarling)
• Only fit free variables -- fix sampling methods (#54) (@cgarling)
• Refactor AMR code to use new generic interface (#56) (@cgarling)
• Implement mass-metallicity relations (#58) (@cgarling)

Closed issues:

• Redo threading in sampling methods (#19)
• Integrated metallicity distribution functions (#24)
• Consider removing LoopVectorization.jl (#26)
• Correct HMC sampling with fixed parameters (#53)