Metadata-Version: 2.1
Name: minimint
Version: 0.3.0
Summary: MIST Isochrone interpolation
Home-page: http://github.com/segasai/minimint
Author: Sergey Koposov
Author-email: skoposov@ed.ac.uk
License: BSD
Keywords: isochrone interpolation
Platform: UNKNOWN
Classifier: Development Status :: 3 - Alpha
Classifier: Topic :: Utilities
Classifier: License :: OSI Approved :: BSD License
Description-Content-Type: text/markdown

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Minimint (MIni Mist INTerpolation)

Software to do simple interpolation of MIST isochrones.

Author: Sergey Koposov (2020-2021) skoposov __AT__ ed __DOT__ ac __DOT__ uk

# Instructions 

* Install minimint. You can either pip install the released version or install from github

```
pip install minimint
```

* Download and prepare isochrone files 
```
minimint.download_and_prepare()
```

That will download everything and process the evolutionary tracks and bolometric corrections by creating the necessary files for the package.

`minimint.download_and_prepare()` by default creates bolometric corrections for these filters
'DECam', 'GALEX', 'PanSTARRS', 'SDSSugriz', 'SkyMapper','UBVRIplus', 'WISE'
If you need additional filters, you can specify them using the filters parameter

``` minimint.download_and_prepare(filters=['JWST','WISE','DECam', 'GALEX', 'PanSTARRS', 'SDSSugriz', 'SkyMapper','UBVRIplus'])```
Check which filters are available on the MIST website http://waps.cfa.harvard.edu/MIST/model_grids.html
This will take some time (20-30 min) and will use some space (10-30 Gb).

If you want to put those processed isochrone files in a location different from the site-packages folder of minimint, you can use the outp_prefix parameter of `download_and_prepare`. You then will need to either specify the location each time when you construct the interpolators or with the MINIMINT_DATA_PATH environment variable

* Usage 

In order to create an interpolator object:

```i = minimint.Interpolator(['DECam_g','DECam_r'])```

The interpolator is a callable, so you can call it on mass, log10(age), feh 

``` ii(mass, logage,feh)``` 
 
This returns a dictionary with photometry and logg, logteff, logl and photometry.

You also can use the interpolator to find the maximum valid mass on the isochrone.

```ii.getMaxMass(logage, feh)```

## Examples 

See the [notebook](examples/Example.ipynb) in the examples folder

## Synthetic stellar populations
If you are interested in synthetic stellar populations you will need
the implementation of the IMF. For this you may want to use https://github.com/keflavich/imf


# Acknowledgement

Please cite the usage of this package using the zenodo reference: https://zenodo.org/record/4900576


