Computations were carried out using GENCI via project 1623 for having provided the massive computing resources needed to perform this extensive study.

@ARTICLE{2017ApJ...836..192B,
       author = {{Brun}, Allan Sacha and {Strugarek}, Antoine and {Varela}, Jacobo and {Matt}, Sean P. and {Augustson}, Kyle C. and {Emeriau}, Constance and {DoCao}, Olivier Long and {Brown}, Benjamin and {Toomre}, Juri},
        title = "{On Differential Rotation and Overshooting in Solar-like Stars}",
      journal = {pj},
     keywords = {convection, hydrodynamics, stars: activity, stars: rotation, stars: solar-type, Astrophysics - Solar and Stellar Astrophysics},
         year = 2017,
        month = feb,
       volume = {836},
       number = {2},
          eid = {192},
        pages = {192},
          doi = {10.3847/1538-4357/aa5c40},
archivePrefix = {arXiv},
       eprint = {1702.06598},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017ApJ...836..192B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2022ApJ...926...21B,
       author = {{Brun}, Allan Sacha and {Strugarek}, Antoine and {Noraz}, Quentin and {Perri}, Barbara and {Varela}, Jacobo and {Augustson}, Kyle and {Charbonneau}, Paul and {Toomre}, Juri},
        title = "{Powering Stellar Magnetism: Energy Transfers in Cyclic Dynamos of Sun-like Stars}",
      journal = {pj},
     keywords = {2001, 1503, 1610, 1629, 1996, 1964, 299, 1966, 1941, 878, 558, Astrophysics - Solar and Stellar Astrophysics, Physics - Fluid Dynamics},
         year = 2022,
        month = feb,
       volume = {926},
       number = {1},
          eid = {21},
        pages = {21},
          doi = {10.3847/1538-4357/ac469b},
archivePrefix = {arXiv},
       eprint = {2201.13218},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...926...21B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2024A&A...684A.156N,
       author = {{Noraz}, Q. and {Brun}, A.~S. and {Strugarek}, A.},
        title = "{Magnetochronology of solar-type star dynamos}",
      journal = {ap},
     keywords = {dynamo, Sun: evolution, Sun: magnetic fields, stars: activity, stars: rotation, stars: solar-type, Astrophysics - Solar and Stellar Astrophysics},
         year = 2024,
        month = apr,
       volume = {684},
          eid = {A156},
        pages = {A156},
          doi = {10.1051/0004-6361/202347939},
archivePrefix = {arXiv},
       eprint = {2401.14460},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2024A&A...684A.156N},
      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)