If you find this code useful, please cite:
An Effective Model for the Cosmic-Dawn 21-cm Signal. Muñoz 2023
@article{Munoz:2023kkg, author = "Mu~noz, Julian B.", title = "{An Effective Model for the Cosmic-Dawn 21-cm Signal}", eprint = "2302.08506", archivePrefix = "arXiv", primaryClass = "astro-ph.CO", doi = "10.1093/mnras/stad1512", month = "2", year = "2023" }
If additionally you use the UVLF functionality consider citing:
Breaking degeneracies in the first galaxies with clustering. Muñoz, Mirocha, Furlanetto, and Sabti 2023
@article{Munoz:2023cup, author = "Mu~noz, Julian B. and Mirocha, Jordan and Furlanetto, Steven and Sabti, Nashwan", title = "{Breaking degeneracies in the first galaxies with clustering}", eprint = "2306.09403", archivePrefix = "arXiv", primaryClass = "astro-ph.CO", month = "6", year = "2023" }
And if you use relative velocites, Lyman-Werner feedback, or Population III stars please cite:
The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars. Cruz, Muñoz, Sabti, and Kamionkowski 2024
@article{Cruz:2024fsv, author = "Cruz, Hector Afonso G. and Munoz, Julian B. and Sabti, Nashwan and Kamionkowski, Marc", title = "{The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars}", eprint = "2407.18294", archivePrefix = "arXiv", primaryClass = "astro-ph.CO", month = "7", year = "2024" }