The project can be cited with :

@ARTICLE{2020A&A...641A.112L,
       author = {{Lebreuilly}, U. and {Commer{\c{c}}on}, B. and {Laibe}, G.},
        title = "{Protostellar collapse: the conditions to form dust-rich protoplanetary disks}",
      journal = {\aap},
     keywords = {ISM: kinematics and dynamics, hydrodynamics, stars: formation, methods: numerical, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = sep,
       volume = {641},
          eid = {A112},
        pages = {A112},
          doi = {10.1051/0004-6361/202038174},
archivePrefix = {arXiv},
       eprint = {2007.06050},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...641A.112L},
      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)