The halo mass function through the cosmic ages

Abstract

In this paper we investigate how the halo mass function evolves with redshift, based on a suite of very large (with N_p = 3072^3 - 6000^3 particles) cosmological N-body simulations. Our halo catalogue data spans a redshift range of z = 0-30, allowing us to probe the mass function from the dark ages to the present. We utilise both the Friends-of-Friends (FOF) and Spherical Overdensity (SO) halofinding methods to directly compare the mass function derived using these commonly used halo definitions. The mass function from SO haloes exhibits a clear evolution with redshift, especially during the recent era of dark energy dominance (z < 1). We provide a redshift-parameterised fit for the SO mass function valid for the entire redshift range to within ~20% as well as a scheme to calculate the mass function for haloes with arbitrary overdensities. The FOF mass function displays a weaker evolution with redshift. We provide a `universal' fit for the FOF mass function, fitted to data across the entire redshift range simultaneously, and observe redshift evolution in our data versus this fit. The relative evolution of the mass functions derived via the two methods is compared and we find that the mass functions most closely match at z=0. The disparity at z=0 between the FOF and SO mass functions resides in their high mass tails where the collapsed fraction of mass in SO haloes is ~80% of that in FOF haloes. This difference grows with redshift so that, by z>20, the SO algorithm finds a ~50-80% lower collapsed fraction in high mass haloes than does the FOF algorithm, due in part to the significant over-linking effects known to affect the FOF method.

v4, 16 pages, 16 colour figures. Changed to match MNRAS print version. NOTE: v1 of this paper has a typo in the fitting function. Please ensure you use the latest version

References in corpus (82)

• A Universal Density Profile from Hierarchical Clustering
• The cosmological simulation code GADGET-2
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Efficient Computation of CMB anisotropies in closed FRW models
• The Baryon Oscillation Spectroscopic Survey of SDSS-III
• Halo Models of Large Scale Structure
• Toward a halo mass function for precision cosmology: the limits of universality
• Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
• Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• Mass function of dark matter halos
• Using the Evolution of Clusters to Constrain Omega
• The Inner Structure of LambdaCDM Halos III: Universality and Asymptotic Slopes
• Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
• Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
• An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
• Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
• Ahf: Amiga's Halo Finder
• Formation of Galaxy Clusters
• The Diversity and Similarity of Simulated Cold Dark Matter Halos
• Merger rates in hierarchical models of galaxy formation. II: Comparison with N-body simulations
• Transients from Initial Conditions in Cosmological Simulations
• Halo concentrations in the standard LCDM cosmology
• The Structure of Dark Matter Haloes in Hierarchical Clustering Models
• Precision Determination of the Mass Function of Dark Matter Halos
• The redshift dependence of the structure of massive LCDM halos
• Scaling relations for galaxy clusters in the Millennium-XXL simulation
• Cosmological Constraints from the SDSS maxBCG Cluster Catalog
• The evolution substructure I: a new identification method
• Haloes gone MAD: The Halo-Finder Comparison Project
• Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample
• The halo mass function from the dark ages through the present day
• The PRIsm MUlti-Object Survey (PRIMUS) I: Survey Overview and Characteristics
• Unusually Large Fluctuations in the Statistics of Galaxy Formation at High Redshift
• The mass function
• The Halo Mass Function: High-Redshift Evolution and Universality
• Evolution of the Mass Function of Dark Matter Haloes
• Constraints on Omega_m, Omega_L, and Sigma_8, from Galaxy Cluster Redshift Distributions
• Planck Early Results XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
• The pseudo-evolution of halo mass
• The mass of a halo
• Simulating the Universe with MICE: The abundance of massive clusters
• Mass Function Predictions Beyond LCDM
• The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
• Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations
• The XMM Cluster Survey: Optical analysis methodology and the first data release
• The overdensity and masses of the friends-of-friends halos and universality of the halo mass function
• Planck Early Results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters
• High Performance P3M N-body code: CUBEP3M
• The Red-sequence Cluster Survey-2 (RCS-2): survey details and photometric catalog construction
• Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
• The Atacama Cosmology Telescope: A Measurement of the 600< ell <8000 Cosmic Microwave Background Power Spectrum at 148 GHz
• The Cosmic Code Comparison Project
• Robustness of Cosmological Simulations I: Large Scale Structure
• The effects of baryons on the halo mass function
• Constraining dark energy with Sunyaev-Zel'dovich cluster surveys
• Dark Matter Halo Growth II: Diffuse Accretion and its Environmental Dependence
• A model for the postcollapse equilibrium of cosmological structure: truncated isothermal spheres from top-hat density perturbations
• WINGS: A WIde-field Nearby Galaxy-cluster Survey. II. Deep optical photometry of 77 nearby clusters
• The Structure of Halos: Implications for Group and Cluster Cosmology
• The Postcollapse Equilibrium Structure of Cosmological Haloes in a Low-Density Universe
• Early Structure Formation and Reionization in a Cosmological Model with a Running Primordial Power Spectrum
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• What do cluster counts really tell us about the Universe?
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• An Extended Zel'dovich Model for the Halo Mass Function
• Cosmic Structure Formation at High Redshift
• Mass function of haloes: scale invariant models

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