Large scale bias and the peak background split
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- Type
- article
- Published
- 1999-01-11
- Cited by
- 2,335
- References
- 19
- Access
- Open access
- OpenAlex
- https://openalex.org/W2134712793
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:10389333
Keywords
Physics, Dark matter, Simple (philosophy), Astrophysics, Scale (ratio)
References
- Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation
- Biasing and the distribution of dark matter haloes
- THE ASSEMBLY OF MATTER IN GALAXY CLUSTERS
- Accurate Fitting Formula for the Two-Point Correlation Function of Dark Matter Halos
- An analytic model for the spatial clustering of dark matter haloes
- Excursion set mass functions for hierarchical Gaussian fluctuations
- The Cosmological Mass Distribution Function in the Zeldovich Approximation
- How Dark Matter Halos Cluster in Lagrangian Space
- The statistics of peaks of Gaussian random fields
- Merger rates in hierarchical models of galaxy formation – II. Comparison with N-body simulations
- Biased clustering in the cold dark matter cosmogony
- Gravitational clustering from scale-free initial conditions
- High-order correlations of peaks and haloes: a step towards understanding galaxy biasing
- Modelling the evolution of galaxy clustering
- Empirical constraints on the first stars and quasars
- Accurate Determination of the Lagrangian Bias for the Dark Matter Halos
- The bias field of dark matter haloes
- High-redshift galaxies, their active nuclei and central black holes
- High-redshift galaxies, their active nuclei and central black holes
- The Assembly of Matter in Galaxy Clusters
Cited by
- Higher Order Moments of the Cosmic Shear and Other Spin-2 Fields
- Galaxy clustering using the GAMA survey
- Clustering of galaxies: evolution, segregation and baryon acoustic oscillations
- Simulated versus observed UV emission at high redshift: a hint for a clumpy interstellar medium?
- Test des modèles d'Energie Noire et propriétés physiques des amas de galaxies
- The Matter Power Spectrum
- Empreintes de l'Énergie Noire sur la structuration de l'Univers
- The Non-Parametric Model for Linking Galaxy Luminosity with Halo/Subhalo Mass: Are First Brightest Galaxies Special?
- Fluctuations in Radiation Backgrounds at High Redshift and the First Stars
- Search for non-Gaussianity in Large Scale Structure surveys
- Neutrino constraints from clusters of galaxies and other probes
- Evidence for Merging or Disruption of Red Galaxies from the Evolution of Their Clustering
- The mass ratio distribution of MBH binaries in the hierarchical model
- Galaxy-dark matter structure relations in the standard cosmological model
- Precision cosmology with weak gravitational lensing
- Is the Universe Normal? Constraining Scale-Dependent Primordial Non-Gaussianity.
- High energy studies of active galactic nuclei with XMM-Newton.
- Cosmic Acceleration As Quantum Gravity Phenomenology
- The role of the dark matter haloes on the cosmic star formation rate
- Baryonic acoustic oscillations with emission line galaxies at intermediate redshift : the large-scale structure of the universe.
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