Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation

Abstract

We present the first results from the new Bolshoi N-body cosmological LCDM simulation that uses cosmological parameters favored by current observations. The Bolshoi simulation was done in a volume 250Mpc on a side using 8billion particles with mass and force resolution adequate to follow subhalos down to a completeness limit of Vcirc=50km/ s circular velocity. Using excellent statistics of halos and subhalos (10M at every moment and 50M over the whole history) we present accurate approximations for statistics such as the halo mass function, the concentrations for distinct halos and subhalos, abundance of halos as function of their circular velocity, the abundance and the spatial distribution of subhalos. We find that at high redshifts the concentration falls to a minimum of about 3.8 and then rises slightly for higher values of halo mass. We find that while the Sheth-Tormen approximation for the mass function of halos found by spherical overdensity is accurate at low redshifts, it over-predicts the abundance of halos by nearly an order of magnitude by z=10. We find that the number of subhalos scales with the circular velocity of the host halo as Vhost**0.5, and that subhalos have nearly the same radial distribution as dark matter particles at radii 0.3-2 times the host halo virial radius. The subhalo velocity function n(>V) behaves as V**(-3). We give normalization of this relation for different masses and redshifts. Finally, we use an abundance-matching procedure to assign r-band luminosities to dark matter halos as a function of halo Vcirc, and find that the luminosity-velocity relation is in remarkably good agreement with the observed Tully-Fisher relation for galaxies in the range 50-200km/s.

28 pages, 22 figures, accepted for publication in ApJ

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• Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Sensitivity of the Cherenkov Telescope Array to the detection of a dark matter signal in comparison to direct detection and collider experiments
• Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation
• Lessons from cosmic history: The case for a linear star formation -- H2 relation
• Extragalactic gamma-ray signal from Dark Matter annihilation: a power spectrum based computation
• FirstLight III: Rest-frame UV-optical spectral energy distributions of simulated galaxies at cosmic dawn
• Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles
• LCDM halo substructure properties revealed with high resolution and large volume cosmological simulations
• Post-Newtonian constraints on Lorentz-violating gravity theories with a MOND phenomenology
• A Novel Approach to Visualizing Dark Matter Simulations
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation
• Numerical simulations of dwarf galaxy merger trees
• Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model
• Identification of filamentary structures in the environment of superclusters of galaxies in the Local Universe
• Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
• Constraints on interacting dark energy models from galaxy Rotation Curves
• An extremely dense group of massive galaxies at the centre of the protocluster at z = 3.09 in the SSA22 field
• Relativistic SZ temperature scaling relations of groups and clusters derived from the BAHAMAS and MACSIS simulations
• Halo Mass Dependence of HI and OVI Absorption: Evidence for Differential Kinematics
• The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• Cosmic radiation backgrounds from primordial black holes
• The Relation Between Galaxy ISM and Circumgalactic OVI Gas Kinematics Derived from Observations and $\Lambda$CDM Simulations
• The Dark Matter Distribution in the Spiral $NGC3198$ out to 0.22 $R_{vir}$
• Forward and backward galaxy evolution in comoving number density space
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
• The most massive objects in the Universe
• The Optical Luminosity Function of Void Galaxies in the SDSS and ALFALFA Surveys
• Post-Newtonian Cosmological Modelling
• The Missing Satellite Problem in 3D
• SMBH Seeds from Dissipative Dark Matter
• The physical origins of low-mass spin bias
• Dependence of Halo Bias and Kinematics on Assembly Variables
• Non-universality of dark-matter halos: cusps, cores, and the central potential
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• Constraining the Warm Dark Matter Particle Mass through Ultra-Deep UV Luminosity Functions at z=2
• Tidal Tracks and Artificial Disruption of Cold Dark Matter Halos
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• The World Space Observatory Ultraviolet (WSO-UV), as a bridge to future UV astronomy
• A cosmological context for compact massive galaxies
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• Dwarf spheroidal galaxies and Bose-Einstein condensate dark matter
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• SatGen -- II. Assessing the impact of a disc potential on subhalo populations
• The contribution of HI-bearing ultra-diffuse galaxies to the cosmic number density of galaxies
• Groups in the Millennium Simulation and in SDSS DR7
• SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias
• A dynamics-based density profile for dark haloes -- II. Fitting function
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• The Sheet of Giants: Unusual Properties of the Milky Way's Immediate Neighbourhood
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• The optimal gravitational softening length for cosmological N-body simulations
• Dark Matter in Galaxies: evidences and challenges
• On Physical Scales of Dark Matter Halos
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• The Massive Satellite Population of Milky-Way Sized Galaxies
• Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Astrophysical and cosmological probes of dark matter
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Mass-concentration relation of clusters of galaxies from CFHTLenS
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• DGSAT: Dwarf Galaxy Survey with Amateur Telescopes II. A catalogue of isolated nearby edge-on disk galaxies and the discovery of new low surface brightness systems
• A matter of measurement: rotation velocities and the velocity function of dwarf galaxies
• Coarse-grained description of cosmic structure from Szekeres models
• The connection between the cusp-to-core transformation and observational universalities of DM halos
• Galaxy Mass, Metallicity, Radius and Star Formation Rates
• Understanding the non-linear clustering of high redshift galaxies
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• HACC Cosmological Simulations: First Data Release
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• On the evolution of cluster scaling relations
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
• Light versus dark in strong-lens galaxies: Dark matter haloes that are rounder than their stars
• Constructing high-fidelity halo merger trees in AbacusSummit
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• What sets the splashback radius of dark matter haloes: accretion history or other properties?
• Generating Synthetic Cosmological Data with GalSampler
• Cosmic variance in the nanohertz gravitational wave background
• Comparison between DAMA/LIBRA and COSINE-100 in the light of Quenching Factors
• Three-point galaxy-galaxy lensing as a probe of dark matter halo shapes
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• Sparse Bayesian mass-mapping with uncertainties: local credible intervals
• Dwarf Spheroidal Satellite Formation in a Reionized Local Group
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• Systematic uncertainties from halo asphericity in dark matter searches
• Constraints on shear and rotation with massive galaxy clusters
• Kinematics of the OVI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
• Comparison of Observed Galaxy Properties with Semianalytic Model Predictions using Machine Learning
• GalWeight: A New and Effective Weighting Technique for Determining Galaxy Cluster and Group Membership
• Likelihood-free Inference with Mixture Density Network
• Gravitational-wave dark siren cosmology systematics from galaxy weighting
• Clustering of star-forming galaxies detected in mid-infrared with the Spitzer wide-area survey
• The evolution of dwarf galaxy satellites with different dark matter density profiles in the ErisMod simulations. I. The early infalls
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• Spin-dependent sub-GeV Inelastic Dark Matter-electron scattering and Migdal effect: (I). Velocity Independent Operator
• The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
• The substructures in the local stellar halo from Gaia and LAMOST
• Long gamma-ray burst rate at very high redshift
• Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• The number of tidal dwarf satellite galaxies in dependence of bulge index
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Massive galaxy formation caught in action at z~5 with JWST
• Quantifying substructures in {\it Hubble Frontier Field} clusters: comparison with $\Lambda CDM$ simulations
• Subhaloes gone Notts: the clustering properties of subhaloes
• Another baryon miracle? Testing solutions to the "missing dwarfs" problem
• The Local Group in the cosmic web
• Modelling the matter bispectrum at small scales in modified gravity
• A Grand Design for Galaxy Clusters: Connections and Predictions
• Effects of Baryon Mass Loss on Profiles of Large Galactic Dark Matter Haloes
• Galaxy size trends as a consequence of cosmology
• Pushing down the low-mass halo concentration frontier with the Lomonosov cosmological simulations
• Effect of asphericity in caustic mass estimates of galaxy clusters
• Interaction between collisionless galactic discs and nonaxissymmetric dark matter haloes
• Impacts of biasing schemes in the one-loop integrated perturbation theory
• Metallicity and Kinematics of the Galactic halo from the LAMOST sample stars
• Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• On the dependence of galaxy morphologies on galaxy mergers
• Assessing the accuracy of cosmological parameters estimated from velocity -- density comparisons via simulations
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Some observational tests of a minimal galaxy formation model
• Ejection of supermassive black holes and implications for merger rates in fuzzy dark matter haloes
• Spatial Anisotropy of Galaxy Kinematics in Sloan Digital Sky Survey Galaxy Clusters
• Reversal of Fortune: Increased Star Formation Efficiencies in the Early Histories of Dwarf Galaxies?
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• A complete distribution of redshifts for sub-millimetre galaxies in the SCUBA-2 Cosmology Legacy Survey UDS field
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• Hierarchical structure of the cosmic web and galaxy properties
• The IllustrisTNG Simulations: Public Data Release
• Effects of Completeness and Purity on Cluster Dark Energy Constraints
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• Using member galaxy luminosities as halo mass proxies of galaxy groups
• New empirical constraints on the cosmological evolution of gas and stars in galaxies
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Virial halo mass function in the $Planck$ cosmology
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• On the environment of Low Surface Brightness galaxies at different scales
• The abundance of dark matter haloes down to Earth mass
• A Long Stream of Metal-Poor Cool Gas around a Massive Starburst Galaxy at z = 2.67
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• The density profiles of Dark Matter halos in Spiral Galaxies
• Modelling the shapes of the largest gravitationally bound objects
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• ALMA Observations of Lyman-alpha Blob 1: Multiple major-mergers and widely distributed interstellar media
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• A Precise Benchmark for Cluster Scaling Relations: Fundamental Plane, Mass Plane and IMF in the Coma Cluster from Dynamical Models
• Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S Field
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Halo assembly bias from a deep learning model of halo formation
• Imaging Spectroscopy of Ionized Gaseous Nebulae around Optically Faint AGN at Redshift z ~ 2
• Substructure within the SSA22 protocluster at $z\approx 3.09$
• How feedback shapes galaxies: an analytic model
• The kinematics of the Local Group in a cosmological context
• Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
• Chemo-dynamical simulations of dwarf galaxy evolution
• Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies
• On the Mass Assembly History of the Local Group
• The Califa and Hipass velocity function for all morphological galaxy types
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Differentiable Predictions for Large Scale Structure with SHAMNet
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Compact groups from semi-analytical models of galaxy formation -- I: a comparative study of frequency and nature
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• The bar rotation rate as a diagnostic of dark matter content in the centre of disc galaxies
• A new framework for numerical simulations of structure formation
• The Distribution of Mass in the Orion Dwarf Galaxy
• Prospects for Determining the Mass Distributions of Galaxy Clusters on Large Scales Using Weak Gravitational Lensing
• Giant Primeval Magnetic Dipoles
• An Accurate Comprehensive Approach to Substructure: I. Accreted Subhaloes
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• A universal angular momentum profile for dark matter haloes
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Constraints On Duty Cycles Of Quasars At Z $\sim$ 6
• Disentangling cosmic-ray and dark-matter induced gamma-rays in galaxy clusters?
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Sparse Bayesian mass-mapping with uncertainties: peak statistics and feature locations
• Investigating overdensities around z>6 galaxies through ALMA observations of [CII]
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• A Cosmological Solution to the Impossibly Early Galaxy Problem
• The Fabric of the Universe: Exploring the cosmic web in 3D prints and woven textiles
• Evolution of CIV Absorbers. II. Where does CIV live?
• Precision cosmology with baryons: non-radiative hydrodynamics of galaxy groups
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Impact of tidal environment on galaxy clustering in GAMA
• Cosmological applications of the Brown-York quasilocal mass
• Halo Mass-Concentration Relation at High-Mass End
• PHoToNs--A Parallel Heterogeneous & Threads oriented code for cosmological N-body simulation
• Constraint on dark matter annihilation with dark star formation using Fermi extragalactic diffuse gamma-ray background data
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• Testing core creation in hydrodynamical simulations using the HI kinematics of field dwarfs
• Setting the Stage: Structures from Gaussian Random Fields
• An Optical Analysis of the Merging Cluster Abell 3888
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Origin of reduced dynamical friction by dark matter halos with net prograde rotation
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• Mass Substructure in Abell 3128
• Dark Stars and Boosted Dark Matter Annihilation Rates
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• Voronoi Tessellation and Non-parametric Halo Concentration
• An Accurate Comprehensive Approach to Substructure: II. Stripped Subhaloes
• An Accurate Comprehensive Approach to Substructure: III. Masses and Formation Times of the Host Haloes
• Quantifying and controlling biases in dark matter halo concentration estimates
• Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• Characterizing SL2S galaxy groups using the Einstein radius
• Horizon Run 3: Topology as a Standard Ruler
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Rotation curves of galaxies and the stellar mass-to-light ratio
• Ridges in the Dark Energy Survey for cosmic trough identification
• Can a Satellite Galaxy Merger Explain the Active Past of the Galactic Center?
• Distortion of Infall Regions in Redshift Space-I
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• Transonic galactic outflows in a dark matter halo with a central black hole and its application to the Sombrero galaxy
• Constraining the mass-concentration relation through weak lensing peak function
• Low Density Structures in the Local Universe. I. Diffuse Agglomerates of Galaxies
• The abundance of Bullet-groups in LCDM
• Lagrangian Methods Of Cosmic Web Classification
• Angular Momentum Evolution in Dark Matter Halos
• Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
• Exploring galaxy dark matter halos across redshifts with strong quasar absorbers
• On the coldness of the local Hubble flow: the role of baryons
• SMBH Seeds: Model Discrimination with High Energy Emission Based on Scaling Relation Evolution
• The mass accretion history of dark matter haloes down to Earth mass
• RAiSERed: radio continuum redshifts for lobed AGNs
• The impact of the cosmological constant on past and future star formation
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Effects of tidal gravitational fields in clustering dark energy models
• Gravitational Lensing in More Realistic Dark Matter Halo Models
• Baryonic Post-Processing of N-body Simulations, with Application to Fast Radio Bursts
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• Studying galaxy cluster morphological metrics with Mock-X
• Halos in Dark Ages: formation and chemistry
• "Non-Local" Effects from Boosted Dark Matter in Indirect Detection
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• An efficient and robust method to estimate halo concentration
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• Halo Growth and Merger Rates as a Cosmological Test
• Tests of Acoustic Scale Shifts in Halo-based Mock Galaxy Catalogues
• Evolution of Low Mass Galactic Subhalos and Dependence on Concentration
• The velocity function of dark matter halos at r=20 kpc: Remarkably little evolution since z ~ 4
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Nonlinear structure formation in Bound Dark Energy
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• Smooth halos in the cosmic web
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• Direct Gravitational Imaging of Intermediate Mass Black Holes in Extragalactic Halos
• An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
• The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
• Semi-analytical frameworks for subhalos from the smallest to the largest scale
• Cluster Assembly Times as a Cosmological Test
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Complementary Cosmological Simulations
• A mass threshold in the number density of passive galaxies at z$\sim$2
• Joint constraints on galaxy bias and ${\sigma }_8$ through the N-pdf of the galaxy number density
• Disk Mass-to-Light ratio distribution from stellar population synthesis: Application to rotation curve decomposition of NGC 5278 (KPG 390A)
• Partial Rate Matrix for Dark Matter Scattering
• Wavelet-Harmonic Integration Methods
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
• Detecting Adiabatic Contraction in Rotation Curves
• Issues in the Investigations of the Dark Matter Phenomenon in Galaxies: Parcere Personis, Dicere de Vitiis
• Galaxy formation from a timescale perspective
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Mass - concentration relation and weak lensing peak counts
• Constraining cosmology with the velocity function of low-mass galaxies
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Universal multi-stream radial structures of cold dark matter halos
• Semi analytical description of formation of galaxies and clusters of galaxies
• Evolution of Star Cluster Within Galaxy using Self-consistent Hybrid Hydro/N-body Simulation
• Unified dark matter: constraints from galaxies and clusters
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
• Fundamental properties of the dark and the luminous matter from Low Surface Brightness discs
• Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters
• Thermodynamics of gravitational clustering phenomena: $N$-body self-gravitating gas on the sphere ${\mathbb{S}}^3\subset {\mathbb{R}}^4$
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• Sample variance in N--body simulations and impact on tomographic shear predictions
• Hierarchical Bayesian inference of the Initial Mass Function in Composite Stellar Populations
• High-Performance Astrophysical Simulations and Analysis with Python
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• Dark matter halo concentrations: a short review
• An optically-dark merging system at z~6 detected by JWST
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• Post-Newtonian Gravity in Cosmology
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• Inferring the density and membership of stellar streams with flexible models: The GD-1 stream in Gaia Data Release 3
• FLORAH: A generative model for halo assembly histories
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$\alpha$ Emitters
• Barions and $\Lambda$CDM Model Problems
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• ELG$\times$LRG distribution through dark matter halo dynamics
• Hermeian haloes: extreme objects with two interactions in the past
• Toward Gravitational Lensing in Modified Theories of Gravity
• Primordial Black Hole Mergers as Probes of Dark Matter in Galactic Center
• Delensing for Precision Cosmology: Optimizing Future CMB B-mode Surveys to Constrain r
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• On the evolution of Betti curves in the Cosmic web
• COSMOS2025: Machine Learning Classification of Early- and Late-type Galaxies at 0 < z < 3
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• NebulOS: A Big Data Framework for Astrophysics
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Tensor anisotropy as a tracer of cosmic voids
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• Approximating Density Probability Distribution Functions Across Cosmologies
• The Sizes of Globular Clusters as Tracers of Galactic Halo Potentials
• Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
• The Redshift Evolution of LCDM Halo Parameters
• Extended Hernquist-Springel formalism for cosmic star formation
• Halo growth and the NFW profile
• Correlations in the matter distribution in CLASH galaxy clusters
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Timing Mass of the Local Group
• The impact of cosmic filaments on the abundance of satellite galaxies
• An Accurate Comprehensive Approach to Substructure: IV. Dynamical Friction
• Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory
• Effect of the cubic torus topology on cosmological perturbations
• Effect of Neutrinos on Angular Momentum of Dark Matter Halo
• The orbital dynamics of the LMC and SMC about the Milky Way
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• COSMOS2025: A Machine Learning Census of Massive Quiescent Galaxies at $2.5<\text{z}<5$
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• Cylindrical cosmological simulations with StePS
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• Phase-space perturbation theory for cosmic large-scale structure
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
• Excess of substructure due to primordial black holes
• Using Unreal Engine to Visualize a Cosmological Volume
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• On the Evolution of Dark Matter Halo Properties Following Major and Minor Mergers
• Compact Groups in GDM Cosmological Simulations
• A Mass Dependent Density Profile from Dwarfs to Clusters
• Cosmic Reionization On Computers: Baryonic Effects on Halo Concentrations During the Epoch of Reionization
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Constraining the shape of Milky Way satellites with distance gradients
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• Initial Mass Function for Massive Galaxies at z$\sim$1
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos
• Sparse Bayesian mass-mapping with uncertainties: hypothesis testing of structure