Acknowledging

If you find this code useful, please cite both these papers:

Citation

• Muñoz 2023, [An Effective Model for the Cosmic-Dawn 21-cm Signal](https://arxiv.org/abs/2302.08506)

• Sklansky, Thélie, Muñoz, Cruz, Libanore, Venditti, in prep.

and include a link to [this Github](https://github.com/JulianBMunoz/Zeus21).

In addition, the following papers introduce multiple features into zeus21.

If you use the UVLF module, please cite:

Citation

• Muñoz, Mirocha, Furlanetto, Nashwan, 2023, [Breaking degeneracies in the first galaxies with clustering](https://arxiv.org/abs/2306.09403)

If you use relative velocites, Lyman-Werner feedback, or Population III stars, please cite:

Citation

• Cruz, Muñoz, Sabti, Kamionkowski, 2024, [The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars](https://arxiv.org/abs/2407.18294).