Citing fiasco

If you use fiasco in your scientific work, we would appreciate you citing it in your publications. Please add the following line within your methods, conclusion or acknowledgements sections:

This research used version X.Y.Z (software citation) of the fiasco open source software package.

The software citation should be the specific Zenodo DOI for the version used within your work. The citation for the most current version on Zenodo is,

@software{Barnes2026,
   author       = {Will Barnes and
                   David Stansby and
                   Nick Murphy and
                   Jeffrey Reep and
                   Laura Hayes and
                   Stuart Mumford and
                   Nabil Freij},
   title        = {wtbarnes/fiasco: v0.8.0},
   month        = feb,
   year         = 2026,
   publisher    = {Zenodo},
   version      = {v0.8.0},
   doi          = {10.5281/zenodo. 18615537},
   url          = {https://doi.org/10.5281/zenodo.18615537}
}

You can also obtain this information with fiasco.__citation__.

In addition to citing fiasco, you should also cite the CHIANTI atomic database according to the instructions here.

Works Citing

The following works have used and cited the fiasco package:

[1]

Samuel T Hart. Understanding the Origins and Acceleration Mechanisms of 3He-Rich Solar Energetic Particle Events. PhD thesis, The University of Texas at San Antonio, 2024.

[2]

Luke Fushimi Benavitz, Jeffrey W. Reep, Lucas A. Tarr, and Andy S. H. To. Spatiotemporal Low First Ionization Potential Abundance: A Catalyst for Coronal Condensation. The Astrophysical Journal, 992(1):4, October 2025. arXiv:2504.05381, doi:10.3847/1538-4357/ae019d.

[3]

Callie A. García, Yeimy J. Rivera, Samuel T. Badman, John C. Raymond, Katharine K. Reeves, Tatiana Niembro, Kristoff W. Paulson, and Michael L. Stevens. Tracing a Multi-Temperature Quiescent Prominence's Thermodynamic Evolution from Sun to Earth. arXiv e-prints, pages arXiv:2512.09234, December 2025. arXiv:2512.09234, doi:10.48550/arXiv.2512.09234.

[4]

Graham S. Kerr, Säm Krucker, Joel C. Allred, Jenny M. Rodríguez-Gómez, Andrew R. Inglis, Daniel F. Ryan, Laura A. Hayes, Ryan O. Milligan, Adam F. Kowalski, Joseph E. Plowman, Peter R. Young, Therese A. Kucera, and Jeffrey W. Brosius. Spatial variation of energy transport mechanisms within solar flare ribbons. Nature Astronomy, January 2026. doi:10.1038/s41550-025-02747-9.

[5]

Yeimy J. Rivera, Samuel T. Badman, J. L. Verniero, Tania Varesano, Michael L. Stevens, Julia E. Stawarz, Katharine K. Reeves, Jim M. Raines, John C. Raymond, Christopher J. Owen, Stefano A. Livi, Susan T. Lepri, Enrico Landi, Jasper. S. Halekas, Tamar Ervin, Ryan M. Dewey, Rossana De Marco, Raffaella D'Amicis, Jean-Baptiste Dakeyo, Stuart D. Bale, and B. L. Alterman. Differentiating the Acceleration Mechanisms in the Slow and Alfvénic Slow Solar Wind. The Astrophysical Journal, 980(1):70, February 2025. arXiv:2501.02163, doi:10.3847/1538-4357/ada699.

[6]

Yeimy J. Rivera, John C. Raymond, Katharine K. Reeves, Susan T. Lepri, Roberto Lionello, Cooper Downs, Maurice L. Wilson, and Nicolas Trueba. 3D MHD Time-dependent Charge State Ionization and Recombination Modeling of the Bastille Day Coronal Mass Ejection. The Astrophysical Journal, 955(1):65, September 2023. doi:10.3847/1538-4357/aceef8.

[7]

Daniel F. Ryan, Laura A. Hayes, Hannah Collier, Graham S. Kerr, Andrew R. Inglis, David Williams, Andrew P. Walsh, Miho Janvier, Daniel Müller, David Berghmans, Cis Verbeeck, Emil Kraaikamp, Peter R. Young, Therese A. Kucera, Säm Krucker, Muriel Z. Stiefel, Daniele Calchetti, Katharine K. Reeves, Sabrina Savage, and Vanessa Polito. Solar Orbiter's 2024 Major Flare Campaigns: An Overview. Solar Physics, 300(11):152, November 2025. arXiv:2505.07472, doi:10.1007/s11207-025-02561-6.

[8]

T. Varesano, D. M. Hassler, N. Zambrana Prado, J. M. Laming, J. Plowman, D. J. Knipp, M. Molnar, K. Barczynski, and The SPICE consortium. FIP Bias Evolution in an Emerging Active Region as observed in SPICE Synoptic Observations. arXiv e-prints, pages arXiv:2502.12045, February 2025. arXiv:2502.12045, doi:10.48550/arXiv.2502.12045.