CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation

Abstract

Accurate theoretical prediction for halo mass function across a broad cosmological space is crucial for the forthcoming China Space Station Telescope (CSST) observations, which will capture cosmological information from multiple probes, e.g., cluster abundance, and weak lensing. In this work, we quantify the percent-level impact of different mass binning schemes when measuring the differential halo mass function from simulations, and demonstrate that the cumulative form of the halo mass function is independent of the binning scheme. Through the recently finished Kun simulation suite, we propose a generalized framework to construct multiple accurate halo mass function emulators for different halo mass definitions, including $M_{200m}$, $M_{vir}$, and $M_{200c}$. This extends our CSST Emulator to provide fast and accurate halo mass function predictions for halo mass $M\ge 10^{12}{h}^{-1}{M}_{\odot }$ up to $z=3.0$. For redshifts $z\le 1.0$, the accuracy is within $2\%$ for $M\le 10^{13}{h}^{-1}{M}_{\odot }$, $5\%$ for $M\le 10^{14}{h}^{-1}{M}_{\odot }$, and $10\%$ for $M\le 10^{15}{h}^{-1}{M}_{\odot }$, which is comparable with the statistical errors of training simulations. This tool is integrated in CSST Emulator and publicly available at https://github.com/czymh/csstemu, providing a fast and accurate theoretical tool to obtain unbiased cosmological constraints of the upcoming CSST survey.

12 pages, 8 figures, CSST Emulator at https://github.com/czymh/csstemu. Comments are welcome! Accepted by SCPMA

References in corpus (82)

• SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
• Array Programming with NumPy
• Exploring the Expansion History of the Universe
• Toward a halo mass function for precision cosmology: the limits of universality
• The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
• Observational Probes of Cosmic Acceleration
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Cosmological Parameters from Observations of Galaxy Clusters
• DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
• Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
• Formation of Galaxy Clusters
• redMaPPer I: Algorithm and SDSS DR8 Catalog
• Scaling relations for galaxy clusters in the Millennium-XXL simulation
• Rotation-Dependent Catastrophic Disruption of Gravitational Aggregates
• Dependence of the outer density profiles of halos on their mass accretion rate
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• The Quijote simulations
• The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum
• Weighing the Giants IV: Cosmology and Neutrino Mass
• Cosmology from the Chinese Space Station Optical Survey (CSS-OS)
• Measuring ${\Omega }_m$ with the ROSAT Deep Cluster Survey
• The halo mass function through the cosmic ages
• The universality of the virial halo mass function and models for non-universality of other halo definitions
• Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology
• Dark Energy Survey Year 1 Results: Weak Lensing Mass Calibration of redMaPPer Galaxy Clusters
• The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
• The 400 square degrees ROSAT PSPC galaxy cluster survey: Catalog and statistical calibration
• Evolution of the Mass Function of Dark Matter Haloes
• Splashback in accreting dark matter halos
• Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
• Cosmological $N$-body simulations with suppressed variance
• Cosmology with massive neutrinos II: on the universality of the halo mass function and bias
• Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
• Simulating the Universe with MICE: The abundance of massive clusters
• Mass Function Predictions Beyond LCDM
• The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog
• The REFLEX Galaxy Cluster Survey VII: Omega_m and sigma_8 from cluster abundance and large-scale clustering
• Large-scale dark matter simulations
• Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• The XXL Survey. II. The bright cluster sample: catalogue and luminosity function
• The Aemulus Project III: Emulation of the Galaxy Correlation Function
• The Aemulus Project II: Emulating the Halo Mass Function
• MassiveNuS: Cosmological Massive Neutrino Simulations
• On the Level of Cluster Assembly Bias in SDSS
• Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
• Cosmic Emulation: Fast Predictions for the Galaxy Power Spectrum
• Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
• Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-Square-Degree Survey
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from counts and stacked weak-lensing
• Constraining neutrino mass with tomographic weak lensing one-point probability distribution function and power spectrum
• Stringent ${\sigma }_8$ constraints from small-scale galaxy clustering using a hybrid MCMC+emulator framework
• Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
• Universal at last? The splashback mass function of dark matter halos
• Constraining neutrino mass with tomographic weak lensing peak counts
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Properties and Scaling Relations of Galaxy Clusters and Groups
• The BACCO simulation project: biased tracers in real space
• Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ
• The Mira-Titan Universe IV. High Precision Power Spectrum Emulation
• A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Non-universality of the mass function: dependence on the growth rate and power spectrum shape
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Machine Learning for Observational Cosmology
• Impact of systematics on cosmological parameters from future Galaxy Clusters surveys
• Cosmological constraints from abundance, weak-lensing and clustering of galaxy clusters: application to the SDSS
• First measurement of the characteristic depletion radius of dark matter haloes from weak lensing
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Fast simulations of cosmic large-scale structure with massive neutrinos
• Physical evolution of dark matter halo around the depletion boundary
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• A physical and concise halo model based on the depletion radius
• The Jiao Tong University Spectroscopic Telescope Project
• A Minimal Model for Massive Neutrinos in Newtonian N-body Simulations
• Constraints on dark energy from the CSST galaxy clusters
• Capturing primordial non-Gaussian signatures in the late Universe by multi-scale extrema of the cosmic log-density field
• Einasto profile as the halo model solution coupled to the depletion radius
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies

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