An accurate tool for the fast generation of dark matter halo catalogs
arXiv:1305.1505 · doi:10.1093/mnras/stt907
Abstract
We present a new parallel implementation of the PINpointing Orbit Crossing-Collapsed HIerarchical Objects (PINOCCHIO) algorithm, a quick tool, based on Lagrangian Perturbation Theory, for the hierarchical build-up of Dark Matter halos in cosmological volumes. To assess its ability to predict halo correlations on large scales, we compare its results with those of an N-body simulation of a 3 Gpc/h box sampled with 2048^3 particles taken from the MICE suite, matching the same seeds for the initial conditions. Thanks to the FFTW libraries and to the relatively simple design, the code shows very good scaling properties. The CPU time required by PINOCCHIO is a tiny fraction (~1/2000) of that required by the MICE simulation. Varying some of PINOCCHIO numerical parameters allows one to produce a universal mass function that lies in the range allowed by published fits, although it underestimates the MICE mass function of FoF halos in the high mass tail. We compare the matter-halo and the halo-halo power spectra with those of the MICE simulation and find that these 2-point statistics are well recovered on large scales. In particular, when catalogs are matched in number density, agreement within ten per cent is achieved for the halo power spectrum. At scales k>0.1 h/Mpc, the inaccuracy of the Zel'dovich approximation in locating halo positions causes an underestimate of the power spectrum that can be modeled as a Gaussian factor with a damping scale of d=3 Mpc/h at z=0, decreasing at higher redshift. Finally, a remarkable match is obtained for the reduced halo bispectrum, showing a good description of nonlinear halo bias. Our results demonstrate the potential of PINOCCHIO as an accurate and flexible tool for generating large ensembles of mock galaxy surveys, with interesting applications for the analysis of large galaxy redshift surveys.
arXiv comment14 pages, 9 PDF figures, accepted by Monthly Notices of the Royal Astronomical Society. The PINOCCHIO code can be downloaded here: http://adlibitum.oats.inaf.it/monaco/Homepage/Pinocchio/index.html
References in corpus (48)
- The cosmological simulation code GADGET-2
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- Large scale bias and the peak background split
- Baryonic Features in the Matter Transfer Function
- SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
- Toward a halo mass function for precision cosmology: the limits of universality
- Mass function of dark matter halos
- Transients from Initial Conditions in Cosmological Simulations
- Halo concentrations in the standard LCDM cosmology
- Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
- Precision Determination of the Mass Function of Dark Matter Halos
- Accurate universal models for the mass accretion histories and concentrations of dark matter halos
- Scaling relations for galaxy clusters in the Millennium-XXL simulation
- Biasing and Hierarchical Statistics in Large-scale Structure
- The halo mass function from the dark ages through the present day
- The non-causal origin of the black hole-galaxy scaling relations
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: a large sample of mock galaxy catalogues
- Gravity and Large-Scale Non-local Bias
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of potential systematics
- Cosmology and the Bispectrum
- Mass and Redshift Dependence of Dark Halo Structure
- PINOCCHIO: pinpointing orbit-crossing collapsed hierarchical objects in a linear density field
- Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
- Simulating the Universe with MICE: The abundance of massive clusters
- Lightcone mock catalogues from semi-analytic models of galaxy formation - I. Construction and application to the BzK colour selection
- Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
- The onion universe: all sky lightcone simulations in spherical shells
- Primordial non-Gaussianity from the large scale structure
- Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
- On the origin of cold dark matter halo density profiles
- The Substructure Hierarchy in Dark Matter Haloes
- On The Assembly History of Dark Matter Haloes
- Constraints on the IMF of the first stars
- Lagrangian Dynamics in Non-Flat Universes and Non-Linear Gravitational Evolution
- The Mass Function of Cosmic Structures with Non-Spherical Collapse
- Shrinkage Estimation of the Power Spectrum Covariance Matrix
- A Lagrangian Dynamical Theory for the Mass Function of Cosmic Structures: I Dynamics
- Precision cosmology with a wide area XMM cluster survey
- PINOCCHIO and the hierarchical build-up of dark matter haloes
- The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
- A Lagrangian Dynamical Theory for the Mass Function of Cosmic Structures: II Statistics
- Measuring the neutrino mass from future wide galaxy cluster catalogues
- Modelling large-scale halo bias using the bispectrum
- Convergence of Galaxy Properties with Merger Tree Temporal Resolution
- Constraining neutrino properties with a Euclid-like galaxy cluster survey
- Tracing large-scale structure at high redshift with Lyman-alpha emitters: the effect of peculiar velocities
- Statistics of the Sunyaev-Zel'dovich Effect power spectrum
- A study of relative velocity statistics in Lagrangian perturbation theory with PINOCCHIO
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- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
- The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z=0.8 in the first data release
- The Mass-Concentration-Redshift Relation of Cold Dark Matter Halos
- FastPM: a new scheme for fast simulations of dark matter and halos
- EZmocks: extending the Zel'dovich approximation to generate mock galaxy catalogues with accurate clustering statistics
- Mock galaxy catalogs using the quick particle mesh method
- Modelling Baryon Acoustic Oscillations with Perturbation Theory and Stochastic Halo Biasing
- Large-scale dark matter simulations
- The Websky Extragalactic CMB Simulations
- ICE-COLA: Towards fast and accurate synthetic galaxy catalogues optimizing a quasi -body method
- The mass-Peak Patch algorithm for fast generation of deep all-sky dark matter halo catalogues and its N-Body validation
- Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
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- Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum
- Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
- Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
- SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the low-redshift sample
- HALOGEN: A tool for fast generation of mock halo catalogues
- A Lightcone Catalogue from the Millennium-XXL Simulation
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- Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection
- Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space
- Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment
- CARPool: fast, accurate computation of large-scale structure statistics by pairing costly and cheap cosmological simulations
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- The Formation of Supermassive Black Holes from Population III.1 Seeds. I. Cosmic Formation Histories and Clustering Properties
- FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
- Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
- Correlations between Triaxial Shapes and Formation History of Dark Matter Haloes
- ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
- Voronoi volume function: A new probe of cosmology and galaxy evolution
- Bias deconstructed: Unravelling the scale dependence of halo bias using real space measurements
- Nonlinear Bias of Cosmological Halo Formation in the Early Universe
- The Halo Bispectrum Multipoles in Redshift Space
- Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
- Bispectrum-window convolution via Hankel transform
- ICE-COLA: fast simulations for weak lensing observables
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- sCOLA: The N-body COLA Method Extended to the Spatial Domain
- Fast Weak Lensing Simulations with Halo Model
- Nonlinear 3D Cosmic Web Simulation with Heavy-Tailed Generative Adversarial Networks
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- Truthing the stretch: Non-perturbative cosmological realizations with multiscale spherical collapse
- Euclid: Modelling massive neutrinos in cosmology -- a code comparison
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- COVMOS: a new Monte Carlo approach for galaxy clustering analysis
- Towards cosmological constraints from the compressed modal bispectrum: a robust comparison of real-space bispectrum estimators
- Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
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- Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
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- Modelling the stochasticity of high-redshift halo bias
- Bayesian Control Variates for optimal covariance estimation with pairs of simulations and surrogates
- Deep learning reconstruction of three-dimensional galaxy distributions with intensity mapping observations
- Rapid Simulations of Halo and Subhalo Clustering
- A blind method to recover the mask of a deep galaxy survey
- MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
- One-point statistics of the Lagrangian displacement field
- Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
- Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
- Renormalization group and UV completion of cosmological perturbations: Gravitational collapse as a critical phenomenon
- Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
- The importance of the cosmic web and halo substructure for power spectra
- On general-relativistic Lagrangian perturbation theory and its non-perturbative generalization
- Beyond the Lognormal Approximation: a General Simulation Scheme
- Covariance matrices for variance-suppressed simulations
- Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
- Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
- Bayesian large-scale structure inference and cosmic web analysis
- Non-linear matter power spectrum without screening dynamics modelling in gravity
- Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
- Euclid preparation. Simulating thousands of Euclid spectroscopic skies
- Numerical implementation of the Cubic Galileon model in PINOCCHIO
- Fast and accurate collapse-time predictions for collisionless matter
- Uncertainty in the visibility mask of a survey and its effects on the clustering of biased tracers
- Evolution of dwarf galaxy observable parameters
- Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
- Euclid preparation. 3-dimensional galaxy clustering in configuration space. Part I. 2-point correlation function estimation
- On the tomographic cluster clustering as a cosmological probe
- SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport
- On the Robustness of Cluster Clustering Covariance Calibration
- An implementation of nDGP gravity in Pinocchio
- CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
- Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
- Euclid preparation. L. Calibration of the linear halo bias in CDM cosmologies
- Improving cosmological covariance matrices with machine learning
- Tracing cosmic voids with fast simulations
- Segmenting proto-halos with vision transformers