Citation

If you have used data from the Quijote simulations you may consider citing the Quijote paper.

@ARTICLE{Quijote_sims,
         author = {{Villaescusa-Navarro}, Francisco and {Hahn}, ChangHoon and {Massara}, Elena and {Banerjee}, Arka and {Delgado}, Ana Maria and {Ramanah}, Doogesh Kodi and {Charnock}, Tom and {Giusarma}, Elena and {Li}, Yin and {Allys}, Erwan and {Brochard}, Antoine and {Uhlemann}, Cora and {Chiang}, Chi-Ting and {He}, Siyu and {Pisani}, Alice and {Obuljen}, Andrej and {Feng}, Yu and {Castorina}, Emanuele and {Contardo}, Gabriella and {Kreisch}, Christina D. and {Nicola}, Andrina and {Alsing}, Justin and {Scoccimarro}, Roman and {Verde}, Licia and {Viel}, Matteo and {Ho}, Shirley and {Mallat}, Stephane and {Wandelt}, Benjamin and {Spergel}, David N.},
         title = "{The Quijote Simulations}",
         journal = {\apjs},
         keywords = {N-body simulations, Cosmological parameters, Astrostatistics, Large-scale structure of the universe, Cosmological neutrinos, 1083, 339, 1882, 902, 338, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2020,
         month = sep,
         volume = {250},
         number = {1},
         eid = {2},
         pages = {2},
         doi = {10.3847/1538-4365/ab9d82},
         archivePrefix = {arXiv},
         eprint = {1909.05273},
         primaryClass = {astro-ph.CO},
         adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJS..250....2V},
         adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

If you use data from Molino, consider citing the Molino paper

@ARTICLE{Molino,
    author = {{Hahn}, ChangHoon and {Villaescusa-Navarro}, Francisco},
    title = "{Constraining M$_{{\ensuremath{\nu}}}$ with the bispectrum. Part II. The information content of the galaxy bispectrum monopole}",
    journal = {\jcap},
    keywords = {cosmological parameters from LSS, cosmological simulations, neutrino masses from cosmology, redshift surveys, Astrophysics - Cosmology and Nongalactic Astrophysics},
    year = 2021,
    month = apr,
    volume = {2021},
    number = {4},
    eid = {029},
    pages = {029},
    doi = {10.1088/1475-7516/2021/04/029},
    archivePrefix = {arXiv},
    eprint = {2012.02200},
    primaryClass = {astro-ph.CO},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021JCAP...04..029H},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

If you use data from Gigantes, consider citing the Gigantes paper

@ARTICLE{Gigantes,
    author = {{Kreisch}, Christina D. and {Pisani}, Alice and {Villaescusa-Navarro}, Francisco and {Spergel}, David N. and {Wandelt}, Benjamin D. and {Hamaus}, Nico and {Bayer}, Adrian E.},
    title = "{The GIGANTES dataset: precision cosmology from voids in the machine learning era}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
    year = 2021,
    month = jul,
    eid = {arXiv:2107.02304},
    pages = {arXiv:2107.02304},
    archivePrefix = {arXiv},
    eprint = {2107.02304},
    primaryClass = {astro-ph.CO},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210702304K},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

If you use data from Quijote-PNG (see Primordial non-Gaussianities), consider citing the Quijote-PNG papers: 2206.01619 and 2206.01624.

@ARTICLE{Quijote-PNG,
    author = {{Coulton}, William R and {Villaescusa-Navarro}, Francisco and {Jamieson}, Drew and {Baldi}, Marco and {Jung}, Gabriel and {Karagiannis}, Dionysios and {Liguori}, Michele and {Verde}, Licia and {Wandelt}, Benjamin D.},
    title = "{Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
    year = 2022,
    month = jun,
    eid = {arXiv:2206.01619},
    pages = {arXiv:2206.01619},
    archivePrefix = {arXiv},
    eprint = {2206.01619},
    primaryClass = {astro-ph.CO},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220601619C},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2022ApJ...940...71J,
   author = {{Jung}, Gabriel and {Karagiannis}, Dionysios and {Liguori}, Michele and {Baldi}, Marco and {Coulton}, William R. and {Jamieson}, Drew and {Verde}, Licia and {Villaescusa-Navarro}, Francisco and {Wandelt}, Benjamin D.},
   title = "{Quijote-PNG: Quasi-maximum Likelihood Estimation of Primordial Non-Gaussianity in the Nonlinear Dark Matter Density Field}",
   journal = {\apj},
   keywords = {Non-Gaussianity, Cosmological parameters from large-scale structure, Fisher's Information, 1116, 340, 1922, Astrophysics - Cosmology and Nongalactic Astrophysics},
   year = 2022,
   month = nov,
   volume = {940},
   number = {1},
   eid = {71},
   pages = {71},
   doi = {10.3847/1538-4357/ac9837},
   archivePrefix = {arXiv},
   eprint = {2206.01624},
   primaryClass = {astro-ph.CO},
   adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...940...71J},
   adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

If you use data from Quijote-ODD (see Parity-violation), consider citing the Quijote-ODD paper:

@ARTICLE{Quijote-ODD,
    author = {{Coulton}, William R. and {Philcox}, Oliver H.~E. and {Villaescusa-Navarro}, Francisco},
    title = "{Signatures of a Parity-Violating Universe}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology, High Energy Physics - Theory},
    year = 2023,
    month = jun,
    eid = {arXiv:2306.11782},
    pages = {arXiv:2306.11782},
    doi = {10.48550/arXiv.2306.11782},
    archivePrefix = {arXiv},
    eprint = {2306.11782},
    primaryClass = {astro-ph.CO},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2023arXiv230611782C},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}