SFH sampling (sfh)#
The sfh module covers classes for a variety of models for the galactic star formation history, each of which
inherits from StarFormationHistory class. You can read more about each of these models below.

Classes#
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Class for a generic galactic star formation history model from which to sample |
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A star formation history that is a combination of multiple other star formation histories. |
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A star formation history based on a distribution function. |
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A semi-empirical model defined in Wagg+2022 (see Figure 1 and Section 2.2.1 for a detailed explanation.), heavily based on Frankel+2018. |
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A star formation history for a component of the Milky Way, based on Frankel+2018. |
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A star formation history for the low-alpha disc of the Milky Way, used in Wagg+2022 |
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A star formation history for the high-alpha disc of the Milky Way, used in Wagg+2022 |
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A star formation history for the bulge of the Milky Way used in Wagg+2022 |
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A star formation history for the Milky Way bar, based on Sormani+2022. |
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An extremely simple star formation history, with all stars formed at |
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A simple star formation history, with all stars formed at a constant rate between |
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A simple star formation history, with all stars formed at a constant rate between |
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Star formation history model based on a Quasi-Isothermal Disc distribution function from Sanders & Binney 2015. |
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An action-based model for dwarf spheroidal galaxies and globular clusters Pascale+2019. |
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A model for the Carina dwarf spheroidal galaxy based on Pascale+2019. |