Merging Dev1.6 for the upcoming hoki v1.6 release #76
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The complex stellar population subpackage is meant to combine bpass variables with a stelalr formation history to generate more complex populations. To this end, we're implementing a stellar formation history class. The basic SFH class for custom SFH is implemented using scipy splines. This basic class is also tested.
This method allows for the calculation of the event rate at a given lookback time. It uses the BPASS binning for this. This method is much faster, but suffers from a lack of accuracy.
Both functions are implemented for the BPASS spectra. However, the method is similar to the BPASS event rate calculation, which is sub optimal for the spectra calculation. It takes an extremely long time to do the calculation. A for loop of 100000 iterations is present, because each wavelength is seen as it's own "event type". It should be possible to remove this by implementing a function to take the separate wavelengths as a single unit. It would be interesting so see the influence of putting the for loop within a numba function, but thinking about restructuring the function is probably better. Including a "caching" of the BPASS spectra into a pickled DataFrame. Additional test files are required for this to run.
Agewizard errors
yaml update
Runs each individual python version separate
* Installs the requested python version (3.6 and 3.7) and uses `tox-gh-actions` to run the correct tox versions. * self import in `hoki.age.utils` fixed. * Add init files in test folders to account for similarly named test files.
Complex Stellar Populations
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Adding AgeWizard errors, the
agesubpackage, thedata_compiler.pymodule to compile models and do model search