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}
}