If you use any of the global 21-cm signal or UV/X-ray radiation background stuff, you should cite:

    Mirocha, J., 2014, MNRAS, 443, 1211

@ARTICLE{2014MNRAS.443.1211M,
   author = {{Mirocha}, J.},
    title = "{Decoding the X-ray properties of pre-reionization era sources}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1406.4120},
 keywords = {methods: numerical, dark ages, reionization, first stars, diffuse radiation, X-rays: binaries, X-rays: diffuse background},
     year = 2014,
    month = sep,
   volume = 443,
    pages = {1211-1223},
      doi = {10.1093/mnras/stu1193},
   adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.443.1211M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

For the 1-D radiative transfer please cite:

    Mirocha, J., Skory, S., Burns, J.O., Wise, J.W., 2012, ApJ, 756, 94

@ARTICLE{2012ApJ...756...94M,
   author = {{Mirocha}, J. and {Skory}, S. and {Burns}, J.~O. and {Wise}, J.~H.
	},
    title = "{Optimized Multi-frequency Spectra for Applications in Radiative Feedback and Cosmological Reionization}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1204.1944},
 primaryClass = "astro-ph.CO",
 keywords = {dark ages, reionization, first stars, methods: numerical, radiative transfer},
     year = 2012,
    month = sep,
   volume = 756,
      eid = {94},
    pages = {94},
      doi = {10.1088/0004-637X/756/1/94},
   adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...756...94M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

For global 21-cm calculations using the UVLF-based model, please cite

@ARTICLE{2017MNRAS.464.1365M,
       author = {{Mirocha}, Jordan and {Furlanetto}, Steven R. and {Sun}, Guochao},
        title = "{The global 21-cm signal in the context of the high- z galaxy luminosity function}",
      journal = {\mnras},
     keywords = {galaxies: high-redshift, intergalactic medium, galaxies: luminosity function, mass function, dark ages, reionization, first stars, diffuse radiation, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jan,
       volume = {464},
       number = {2},
        pages = {1365-1379},
          doi = {10.1093/mnras/stw2412},
archivePrefix = {arXiv},
       eprint = {1607.00386},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017MNRAS.464.1365M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

and PopIII star formation

@ARTICLE{2018MNRAS.478.5591M,
       author = {{Mirocha}, Jordan and {Mebane}, Richard H. and {Furlanetto}, Steven R. and
         {Singal}, Krishma and {Trinh}, Donald},
        title = "{Unique signatures of Population III stars in the global 21-cm signal}",
      journal = {\mnras},
     keywords = {galaxies: high-redshift, intergalactic medium, galaxies: luminosity function, mass function, dark ages, reionization, first stars, diffuse radiation, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = aug,
       volume = {478},
       number = {4},
        pages = {5591-5606},
          doi = {10.1093/mnras/sty1388},
archivePrefix = {arXiv},
       eprint = {1710.02530},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.478.5591M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

If you use any of the more sophisticated galaxy modeling stuff, e.g., dust reddening, spectral synthesis, please consider citing

@ARTICLE{2020MNRAS.498.2645M,
       author = {{Mirocha}, Jordan and {Mason}, Charlotte and {Stark}, Daniel P.},
        title = "{Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models}",
      journal = {\mnras},
     keywords = {dust, extinction, galaxies: evolution, galaxies: high-redshift, galaxies: ISM, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = oct,
       volume = {498},
       number = {2},
        pages = {2645-2661},
          doi = {10.1093/mnras/staa2586},
archivePrefix = {arXiv},
       eprint = {2005.07208},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.2645M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}