Journal
NATURE ASTRONOMY
Volume 2, Issue 8, Pages 680-687Publisher
NATURE PORTFOLIO
DOI: 10.1038/s41550-018-0502-4
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Funding
- Israel Science Foundation [1013/12]
- Institut Universitaire de France
- US National Science Foundation
- Space Telescope Science Institute
- Jet Propulsion Lab
- NASA
- Astronomy ESFRI and Research Infrastructure Cluster ASTERICS project
- European Commission under the Horizon 2020 Programme [GA 653477]
- l'Oreal-UNESCO Pour les Femmes et la Science
- Centre National d'Etudes Spatiales postdoctoral fellowship programmes
- MINECO/FEDER (Spain) [AYA2015-63810-P]
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The local Universe provides a unique opportunity for testing cosmology and theories of structure formation. As the velocities of galaxies respond to the distribution of matter-both visible and dark-the velocity field provides structural information. Here, we present an original method for the reconstruction of the quasi-linear matter density and velocity fields from galaxy peculiar velocities and apply it to the Cosmicflows-2 database of velocites. The method consists of constructing an ensemble of cosmological simulations, constrained by the standard cosmological model and the observational data. The quasi-linear density field is the geometric mean and variance of the fully nonlinear density fields of the simulations. The main nearby clusters (Virgo, Centaurus and Coma), superclusters (Shapley and Perseus-Pisces) and voids (Dipole Repeller) are robustly reconstructed. Galaxies are born 'biased' with respect to the underlying dark matter distribution. Using our quasi-linear framework, we demonstrate that the luminosity-weighted density field derived from the 2M++ redshift compilations is nonlinearly biased with respect to the matter density field. The bias diminishes in the linear regime.
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