SPISEA is an python package that generates single-age, single-metallicity populations (i.e. star clusters). It gives the user control over many parameters:
Here is a brief list of things that SPISEA can do:
See documentation for details on installing and running SPISEA. We also provide jupyter notebooks with a quick-start tutorial and additional examples demonstrating how to use SPISEA.
If you use SPISEA in your research, please cite Hosek et al. (2020).
SPISEA is actively supported and is growing in functionality, and subsequently has had several updates since its initial release. See the main documentation page for the change log describing the updates in each release.
We welcome and encourage contributions to SPISEA! For feature additions, we ask that users make their own fork of the repository, make their changes, and then submit a pull request to the "dev" branch.
All contributions will be acknowledged on the contributors page (with permission). Contributors with features used in code releases will be co-authors in future SPISEA software papers.
This project is Copyright (c) Matthew Hosek Jr., Jessica Lu, Casey Lam, Abhimat Gautam, Kelly Lockhart, Dongwon Kim, and Siyao Jia and licensed under the terms of the GNU GPL v3+ license. This package is based upon the Astropy package template which is licensed under the BSD 3-clause license. See the licenses folder for more information. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.
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