.. image:: https://travis-ci.com/timothydmorton/isochrones.svg?branch=master :target: https://travis-ci.com/timothydmorton/isochrones
Provides simple interface for interacting with stellar model grids.
https://isochrones.readthedocs.io
For simplest out-of-the-box usage after installation, make a file called star.ini
that
looks something like this::
Teff = 5770, 100
feh = 0.0, 0.15
logg = 4.5, 0.1
V = 10.0, 0.05
Any combination of spectroscopic or [supported] photometric properties, as well as parallax, can go as properties into this file.
Once you've made this file, type starfit
at the command line. Or if you want to be organized,
you can put star.ini
in a folder called mystar
[or whatever]
and run starfit mystar
from the command line. The starfit
script
will create an HDF5 file containing the saved StarModel
, which you
can load from python using StarModel.load_hdf
, as well as triangle
plots illustrating the fit.
If you use isochrones
in your research, please cite this ASCL reference <http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2015ascl.soft03010M&data_type=BIBTEX&db_key=AST&nocookieset=1>
_.