Acknowledging ALPro

Acknowledging ALPro

If you use ALPro in your work, please acknowledge it and cite both the Zenodo DOI and the following paper:

J H Matthews et al 2022 “How do magnetic field models affect astrophysical limits on light axion-like particles? An X-ray case study with NGC 1275”, Accepted to ApJ.

Bibtex for the paper can be accessed in python via

import alpro; print (alpro.__citation__)

which prints out:

@ARTICLE{Matthews2022,
        author = {{Matthews}, James H. and {Reynolds}, Christopher S. and {Marsh}, M.~C. David and {Sisk-Reyn{\'e}s}, J{\'u}lia and {Rodman}, Payton E.},
        title = "{How do Magnetic Field Models Affect Astrophysical Limits on Light Axion-like Particles? An X-ray Case Study with NGC 1275}",
        journal = {arXiv e-prints},
        keywords = {Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology},
         year = 2022,
        month = feb,
          eid = {arXiv:2202.08875},
        pages = {arXiv:2202.08875},
        archivePrefix = {arXiv},
        eprint = {2202.08875},
        primaryClass = {astro-ph.HE},
        adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220208875M},
        adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

Bibtex for the Zenodo DOI can be accessed in python via

print (alpro.__zenodo__)

which prints out:

@software{alpro,
        author       = {James Matthews},
        title        = {{{{alpro: Axion-Like PROpagation}}}},
        month        = feb,
        year         = 2022,
        publisher    = {Zenodo},
        version      = {v1.1},
        doi          = {10.5281/zenodo.6137185},
        url          = {https://doi.org/10.5281/zenodo.6137185}
}

If you use the pruning scheme (an adaptive treatment for conservatively dealing with ALP resonances), please cite the paper where it is described:

J Sisk Reynes et al 2021 “New constraints on light axion-like particles using Chandra transmission grating spectroscopy of the powerful cluster-hosted quasar H1821+643”, MNRAS, 510, 64