The project can be cited using the following BibTeX entry:

@ARTICLE{2024arXiv241020924B,
       author = {{Bugli}, M. and {Lopresti}, E.~F. and {Figueiredo}, E. and {Mignone}, A. and {Cerutti}, B. and {Mattia}, G. and {Del Zanna}, L. and {Bodo}, G. and {Berta}, V.},
        title = "{Relativistic reconnection with effective resistivity: I. Dynamics and reconnection rate}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - High Energy Astrophysical Phenomena, Physics - Plasma Physics},
         year = 2024,
        month = oct,
          eid = {arXiv:2410.20924},
        pages = {arXiv:2410.20924},
          doi = {10.48550/arXiv.2410.20924},
archivePrefix = {arXiv},
       eprint = {2410.20924},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2024arXiv241020924B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

If you use it in your own work, you may acknowledge the origin of the data obtained on the Galactica database like so:

This work reused datasets available on the Galactica simulations database
(http://www.galactica-simulations.eu)