Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
about
Earth-mass dark-matter haloes as the first structures in the early UniverseProperties of dark matter haloes in clusters, filaments, sheets and voidsGalactic Chemical EvolutionThe birth of a galaxy – III. Propelling reionization with the faintest galaxiesDark-ages reionization and galaxy formation simulation – IX. Economics of reionizing galaxiesScaling relations for galaxy clusters in the Millennium-XXL simulationMass assembly of galaxiesThe simulated 21 cm signal during the epoch of reionization: full modeling of the Ly-α pumpingThe inner structure of haloes in cold+warm dark matter modelsThe Gigaparsec WiggleZ simulations: characterizing scale-dependant bias and associated systematics in growth of structure measurements
P2860
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P2860
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
description
wetenschappelijk artikel
@nl
наукова стаття, опублікована в листопаді 2001
@uk
name
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
@en
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
@nl
type
label
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
@en
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
@nl
prefLabel
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
@en
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
@nl
P356
P1476
Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations
@en
P2093
Edmund Bertschinger
P356
10.1086/322526
P577
2001-11-01T00:00:00Z
P818
astro-ph/0103301
P819
2001ApJS..137....1B