Concentrations of Dark Halos from their Assembly Histories

Abstract

(abridged) We study the relation between the density profiles of dark matter halos and their mass assembly histories, using a statistical sample of halos in a high-resolution N-body simulation of the LCDM cosmology. For each halo at z=0, we identify its merger-history tree, and determine concentration parameters c_vir for all progenitors, thus providing a structural merger tree for each halo. We fit the mass accretion histories by a universal function with one parameter, the formation epoch a_c, defined when the log mass accretion rate dlogM/dloga falls below a critical value S. We find that late forming galaxies tend to be less concentrated, such that c_vir ``observed'' at any epoch a_o is strongly correlated with a_c via c_vir=c_1*a_o/a_c. Scatter about this relation is mostly due to measurement errors in c_v and a_c, implying that the actual spread in c_vir for halos of a given mass can be mostly attributed to scatter in a_c. We demonstrate that this relation can also be used to predict the mass and redshift dependence of c_v, and the scatter about the median c_vir(M,z), using accretion histories derived from the Extended Press-Schechter (EPS) formalism, after adjusting for a constant offset between the formation times as predicted by EPS and as measured in the simulations;this new ingredient can thus be easily incorporated into semi-analytic models of galaxy formation. The correlation found between halo concentration and mass accretion rate suggests a physical interpretation: for high mass infall rates the central density is related to the background density; when the mass infall rate slows, the central density stays approximately constant and the halo concentration just grows as R_vir. The tight correlation demonstrated here provides an essential new ingredient for galaxy formation modeling.

19 pages, 18 figures, uses emulateapj5.tex. ApJ, in press; revised to match accepted version

References in corpus (3)

• An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
• The Power Spectrum Dependence of Dark Matter Halo Concentrations
• The Phase-Space Density Profiles of Cold Dark Matter Halos

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• Cores and Cusps in Warm Dark Matter Halos
• Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
• The Galaxy Clustering Crisis in Abundance Matching
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• Angular momentum distribution of hot gas and implications for disk galaxy formation
• The Swift/BAT AGN Spectroscopic Survey -- IX. The Clustering Environments of an Unbiased Sample of Local AGN
• Bar-Halo Friction in Galaxies III: Halo Density Changes
• The clustering of SDSS galaxy groups: mass and color dependence
• Thermal Balance in the Intracluster Medium: Is AGN Feedback Necessary?
• IDCS J1426.5+3508: Sunyaev-Zel'dovich Measurement of a Massive IR-selected Cluster at z=1.75
• Baryonic Conversion Tree: The global assembly of stars and dark matter in galaxies from the SDSS
• A two-phase scenario for bulge assembly in LCDM cosmologies
• The scatter and evolution of the global hot gas properties of simulated galaxy cluster populations
• Dark halo response and the stellar initial mass function in early-type and late-type galaxies
• The baryonic Tully-Fisher relation and galactic outflows
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• Properties of Dark Matter Halos as a Function of Local Environment Density
• The Edge of the Galaxy
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• The angular momentum of dark halos: merger and accretion effects
• The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
• Genetically modified halos: towards controlled experiments in $\Lambda$CDM galaxy formation
• Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z~1
• The Distribution of Dark Matter in Galaxies: a Constant-Density Halo around DDO 47
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes II: Global Properties
• Constraints on the mass-concentration relation of cold dark matter halos with 11 strong gravitational lenses
• The Dynamics of Merging Clusters: A Monte Carlo Solution Applied to the Bullet and Musket Ball Clusters
• Dynamical and photometric imprints of feedback processes on the early evolution of E/S0 galaxies
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• The Environmental Dependence of the Evolving S0 Fraction
• Faint extended Lyalpha emission due to star formation at the centre of high-column density QSO absorption systems
• Cosmology: small scale issues revisited
• Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• A Tale of Dwarfs and Giants: Using a z=1.62 Cluster to Understand How the Red Sequence Grew Over The Last 9.5 Billion Years
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• NIHAO XII: galactic uniformity in a ΛCDM universe
• The SLUGGS Survey: Dark matter fractions at large radii and assembly epochs of early-type galaxies from globular cluster kinematics
• MOKA: a new tool for Strong Lensing Studies
• 3D Spectroscopy with VLT/GIRAFFE - IV: Angular Momentum and Dynamical Support of Intermediate Redshift Galaxies
• The Three Hundred Project: The evolution of galaxy cluster density profiles
• An analytical model for the accretion of dark matter subhalos
• Dissipationless Merging and the Assembly of Central Galaxies
• Constraints on the Proper Motion of the Andromeda Galaxy Based on the Survival of Its Satellite M33
• The spherical collapse model and cluster formation beyond the $\Lambda$ cosmology: Indications for a clustered dark energy?
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Empirical constraints on the formation of early-type galaxies
• Deep XMM and Chandra observations of ClJ1226.9+3332: A detailed X-ray mass analysis of a z=0.89 galaxy cluster
• Modeling dark matter subhalos in a constrained galaxy: Global mass and boosted annihilation profiles
• A First Look at Galaxy Flyby Interactions: I. Characterizing the Frequency of Flybys in a Cosmological Context
• Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• The collision velocity of the bullet cluster in conventional and modified dynamics
• Central mass and luminosity of Milky Way satellites in the LCDM model
• Further evidence for large central mass-to-light ratios in early-type galaxies: the case of ellipticals and lenticulars in the Abell~262 cluster
• Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
• The Scale-Dependence of Halo Assembly Bias
• The physical nature of the cosmic accretion of baryons and dark matter into halos and their galaxies
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• Quantum fluctuations masquerade as halos: Bounds on ultra-light dark matter from quadruply-imaged quasars
• Merger induced scatter and bias in the cluster mass - Sunyaev-Zeldovich effect scaling relation
• Dissection of the collisional and collisionless mass components in a mini sample of CLASH and HFF massive galaxy clusters at $z\approx 0.4$
• Halo Histories vs. Galaxy Properties at z=0 II: Large-Scale Galactic Conformity
• Cosmology in 2D: the concentration-mass relation for galaxy clusters
• Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?
• TheHaloMod: An online calculator for the halo model
• Self-interacting dark matter cusps around massive black holes
• The Red Sequence Luminosity Function in Massive Intermediate Redshift Galaxy Clusters
• Prediction of the 21-cm signal from reionization: comparison between 3D and 1D radiative transfer schemes
• The dependence of halo bias on age, concentration and spin
• Stellar orbits and the survival of metallicity gradients in simulated dwarf galaxies
• An Effective Model for the Cosmic-Dawn 21-cm Signal
• Star Clusters Around Recoiled Black Holes in the Milky Way Halo
• Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies
• Interpreting the Clustering of Distant Red Galaxies
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• Two-Phase Galaxy Formation
• Implications of Recent Measurements of the Milky Way Rotation for the Orbit of the Large Magellanic Cloud
• CosmicGrowth Simulations---Cosmological simulations for structure growth studies
• Late Gas accretion onto Primordial Minihalos: a Model for Leo T, Dark Galaxies and Extragalactic High-Velocity Clouds
• Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
• A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations
• Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Gravitational Lensing Statistics in Universes Dominated by Dark Energy
• Imprints of mass accretion on properties of galaxy clusters
• Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• The Impact of Halo Properties, Energy Feedback and Projection Effects on the Mass-SZ Flux Relation
• Dark matter subhaloes as gamma-ray sources and candidates in the first Fermi-LAT catalogue
• The Evolution of Dusty Star formation in Galaxy Clusters to z = 1: Spitzer IR Observations of the First Red-Sequence Cluster Survey
• Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. III. Nurture shapes up the Hubble sequence in the Great Wall
• Disk settling and dynamical heating: histories of Milky Way-mass stellar disks across cosmic time in the FIRE simulations
• The Role of Penetrating Gas Streams in Setting the Dynamical State of Galaxy Clusters
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• Rapid growth of seed black holes during early bulge formation
• The gravitational field of X-COP galaxy clusters
• Cold accretion flows and chemical bimodality of the Milky Way galaxy
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• Simulated ΛCDM analogues of the thin Plane of Satellites around the Andromeda galaxy are not kinematically coherent structures
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Effects of the Non-Equipartition of Electrons and Ions in the Outskirts of Relaxed Galaxy Clusters
• Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Luminosity Functions and Density Profiles
• Predicting the density profiles of the first halos
• An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS field (AS2COSPEC): Survey Description and First Results
• Formation times and masses of dark matter haloes
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• Imprints of Dark Energy on Cosmic Structure Formation: III. Sparsity of Dark Matter Halo Profiles
• The primordial matter power spectrum on sub-galactic scales
• On the Origin of the Inner Structure of Halos
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• Sunyaev Zel'dovich Effect Observations of Strong Lensing Galaxy Clusters: Probing the Over-Concentration Problem
• The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
• An interpretable machine learning framework for dark matter halo formation
• Exploring the liminality: properties of haloes and subhaloes in borderline $f(R)$ gravity
• A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope
• The Tully-Fisher relation and its evolution with redshift in cosmological simulations of disc galaxy formation
• Ultimate age-dating method for galaxy groups; clues from the Millennium Simulations
• Using dwarf satellite proper motions to determine their origin
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters
• Fingerprints of the initial conditions on the density profiles of cold and warm dark matter haloes
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• The nature of dark matter and the density profile and central behavior of relaxed halos
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• Predicting Merger-Induced Gas Motions in Lambda-CDM Galaxy Clusters
• Modeling color-dependent galaxy clustering in cosmological simulations
• Feedback from galactic stellar bulges and hot gaseous haloes of galaxies
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• Dark Matter Halo Profiles in Scale-Free Cosmologies
• Accurate Realizations of the Ionized Gas in Galaxy Clusters: Calibrating Feedback
• Constraints on the Process that Regulates the Growth of Supermassive Black Holes Based on the Intrinsic Scatter in the M_bh-sigma Relation
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• Dark Matter Microhalos From Simplified Models
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
• The central dark matter content of early-type galaxies: scaling relations and connections with star formation histories
• Uncertainties associated with the backward integration of dwarf satellites using simple parametric potentials
• On the common mass scale of the Milky Way satellites
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• gamma-rays from annihilating dark matter in galaxy clusters: stacking vs single source analysis
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Comprehensive Assessment of the Too-Big-to-Fail Problem
• Status of Cold Dark Matter Cosmology
• The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
• Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories
• Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
• Assembly bias in the local PNG halo bias and its implication for $f_{\mathrm{NL}}$ constraints
• Mass and Redshift Dependence of Star Formation in Relaxed Galaxy Clusters
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• Relating the structure of dark matter halos to their assembly and environment
• Galaxy density profiles and shapes -- I. simulation pipeline for lensing by realistic galaxy models
• Priors on red galaxy stochasticity from hybrid effective field theory
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• Disentangling the dark matter halo from the stellar halo
• Entropy of gas and dark matter in galaxy clusters
• Probing Dark Energy at Galactic and Cluster Scales
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters I: Analysis with the Three Hundred Simulations
• Galaxy downsizing evidenced by hybrid evolutionary tracks
• Are Clusters Standard Candles? Galaxy Cluster Scaling Relations With the Sunyaev-Zeldovich Effect
• Connecting the structure of dark matter haloes to the primordial power spectrum
• Precision Cosmology
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• The Galaxy Cluster Concentration-Mass Scaling Relation
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Evolution of Characteristic Quantities for Dark Matter Halo Density Profiles
• A Wide-Field Study of the z~0.8 Cluster RX J0152.7-1357: the Role of Environment in the Formation of the Red-Sequence
• On the stability of tidal streams in action space
• A Plane of High Velocity Galaxies Across the Local Group
• Theoretical dark matter halo density profile
• Formation of Dwarf Spheroidal Galaxies Via Mergers of Disky Dwarfs
• On the reliability of merger-trees and the mass growth histories of dark matter haloes
• Element segregation in giant galaxies and X-ray clusters
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters II: Measurements from SPT-SZ + Planck Compton-y Map
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• Bright and Dark Matter in Elliptical Galaxies: Mass and Velocity Distributions from Self-consistent Hydrodynamical Simulations
• Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
• Weak lensing in the second post-Newtonian approximation: Gravitomagnetic potentials and the integrated Sachs-Wolfe effect
• Mass models from high-resolution HI data of the dwarf galaxy NGC 1560
• The Nature of Dark Matter in Elliptical Galaxies: Chandra Observations of NGC 4636
• Bar instability in cosmological halos
• Cosmological structure formation in scalar field dark matter with repulsive self-interaction: The Incredible Shrinking Jeans Mass
• Unbound Particles in Dark Matter Halos
• Strong lensing constraints on the velocity dispersion and density profile of elliptical galaxies
• The Dark Matter Distribution in the Spiral $NGC3198$ out to 0.22 $R_{vir}$
• On the Origin of Dark Matter Cores in Dwarf Galaxies
• Dependence of Halo Bias and Kinematics on Assembly Variables
• Signatures of clumpy dark matter in the global 21 cm background signal
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• Connecting Cluster Substructure in Galaxy Cluster Cores at z=0.2 With Cluster Assembly Histories
• Finding Fossil Groups: Optical Identification and X-ray Confirmation
• Predictably Missing Satellites: Subhalo Abundance in Milky Way-like Halos
• The Relation Between Halo Shape, Velocity Dispersion and Formation Time
• The MUSIC of Galaxy Clusters III: Properties, evolution and Y-M scaling relation of protoclusters of galaxies
• Massive Low Surface Brightness Galaxies in the EAGLE Simulation
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• SMBH Seeds from Dissipative Dark Matter
• Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8
• Preprocessing Among the Infalling Galaxy Population of EDisCS Clusters
• An optical and X-ray study of the fossil group RX J1340.6+4018
• The twisted dark matter halo of the Milky Way
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• LYRA III: The smallest Reionization survivors
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• A cosmological context for compact massive galaxies
• Refining the M_BH-V_c scaling relation with HI rotation curves of water megamaser galaxies
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Fast Weak Lensing Simulations with Halo Model
• Globular cluster numbers in dark matter haloes in a dual formation scenario: an empirical model within EMERGE
• Hierarchical probabilistic inference of cosmic shear
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Formation of Supermassive Black Holes in Galactic Bulges: A Rotating Collapse Model Consistent with the $\mbh-σ$ Relation
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• Local gravitational redshifts can bias cosmological measurements
• A dynamics-based density profile for dark haloes -- II. Fitting function
• Halo assembly bias from Separate Universe simulations
• Impact of astrophysical processes on the gamma-ray background from dark matter annihilations
• Long-term orbital evolution of Galactic satellites and the effects on their star formation histories
• The Lack of Structural and Dynamical Evolution of Elliptical Galaxies since z ~ 1.5: Clues from Self-Consistent Hydrodynamical Simulations
• The portrait of Malin 2: a case study of a giant low surface brightness galaxy
• Non-universality of halo profiles and implications for dark matter experiments
• Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass
• On the algorithms of radiative cooling in semi-analytic models
• Composition of Low Redshift Halo Gas
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• The mass accretion rate of galaxy clusters: a measurable quantity
• Scale Radii and Aggregation Histories of Dark Haloes
• On Physical Scales of Dark Matter Halos
• The Influence of Concentration and Dynamical State on Scatter in the Galaxy Cluster Mass-Temperature Relation
• Effect of Helium Sedimentation on X-ray Measurements of Galaxy Clusters
• Massive elliptical galaxies : From cores to haloes
• The SLUGGS Survey: Multi-population dynamical modelling of the elliptical galaxy NGC 1407 from stars and globular clusters
• Constraining the substructure of dark matter haloes with galaxy-galaxy lensing
• Sensitivity of dark matter haloes to their accretion histories
• Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
• Probing the galaxy-halo connection with total satellite luminosity
• 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
• Lensing constraints on ultradense dark matter halos
• Constrained Cosmological Simulations of Dark Matter Halos
• An investigation of star formation and dust attenuation in major mergers using ultraviolet and infrared data
• Kinematical Structure of the Magellanic System
• First measurement of the characteristic depletion radius of dark matter haloes from weak lensing
• Lensed arc statistics: comparison of Millennium-simulation galaxy clusters to Hubble Space Telescope observations of an X-ray selected sample
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• Discovery of a new fundamental plane dictating galaxy cluster evolution from gravitational lensing
• Disk Assembly and the M_BH-sigma Relation of Supermassive Black Holes
• The probability distribution function of the SZ power spectrum: an analytical approach
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• On the dynamics of the satellite galaxies in NGC 5044
• Evolution of compact and fossil groups of galaxies from semi-analytical models of galaxy formation
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• Some assembly required: assembly bias in massive dark matter halos
• The Accretion and Cooling of Preheated Gas in Dark Matter Halos
• On the evolution of cluster scaling relations
• Clues on Regularity in the Structure and Kinematics of Elliptical Galaxies from Self-consistent Hydrodynamical Simulations: the Dynamical Fundamental Plane
• Cannibalism's lingering imprint on the matter power spectrum
• Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
• The Halo Shape and Evolution of Polar Disc Galaxies
• DM haloes in the fifth-force cosmology
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• The effects of Non-Gaussian initial conditions on the structure and substructure of Cold Dark Matter halos
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• The Origin of Dark Matter Halo Profiles
• Dynamical signatures of infall around galaxy clusters: a generalized Jeans equation
• The connection between the host halo and the satellite galaxies of the Milky Way
• Comparing Simulations of AGN Feedback
• The galaxy-halo size relation of low-mass galaxies in FIRE
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
• Redshift evolution of the dark matter haloes shapes
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Observational Measures of Halo Properties Beyond Mass
• Baryonic mass budgets for haloes in the EAGLE simulation, including ejected and prevented gas
• Constraining interacting dark energy models with the halo concentration-mass relation
• Merger rates in primordial black hole clusters without initial binaries
• What sets the splashback radius of dark matter haloes: accretion history or other properties?
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Helium Sedimentation and the UV Upturn in Brightest Cluster Galaxies
• Dwarf Spheroidal Satellite Formation in a Reionized Local Group
• The degeneracy between star-formation parameters in dwarf galaxy simulations and the Mstar-Mhalo relation
• Dark matter halo response to the disk growth
• Magnetic field amplification and X-ray emission in galaxy minor mergers
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Precision Cosmology: Successes and Challenges
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• Photoionized Gas in Dark-Matter Minihalos in the Galactic Halo and Local Group
• A Local Leaky-box Model for the Local Stellar Surface Density - Gas Surface Density - Gas Phase Metallicity Relation
• Universal Merger Histories of Dark-Matter Haloes
• How many arcminute-separation lenses are expected in the 2dF QSO survey?
• The Shape of Galaxy Cluster Dark Matter Haloes: Systematics of Its Imprint on Cluster Gas, and Comparison to Observations
• A Bayesian Hierarchical Approach to Galaxy-Galaxy Lensing
• Boosting hierarchical structure formation with scalar-interacting dark matter
• Classifying orbits in galaxy models with a prolate or an oblate dark matter halo component
• Subhaloes gone Notts: the clustering properties of subhaloes
• The survival of globular clusters in a cuspy Fornax
• Re-Examining Astrophysical Constraints on the Dark Matter Model
• Modelling Baryonic Effects on Galaxy Cluster Mass Profiles
• The concentration-velocity dispersion relation in galaxy groups
• Passive Evolution of Galaxy Clustering
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The Cosmological History of Accretion onto Dark Halos and Supermassive Black Holes
• Stirred, not Clumped: Evolution of Temperature Profiles in the Outskirts of Galaxy Clusters
• Probing of the Interactions Between the Hot Plasmas and Galaxies in Clusters from z=0.1 to 0.9
• What Sets Temperature Gradients in Galaxy Clusters? Implications for non-thermal pressure support and mass-observable scaling relations
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• Insights into the origin of halo mass profiles from machine learning
• New views of the distant stellar halo
• The density of dark matter haloes of early-type galaxies in low-density environments
• The thermalisation of massive galaxy clusters
• Cluster Lensing of QSOs as a Probe of LCDM and Dark Energy Cosmologies
• Pushing down the low-mass halo concentration frontier with the Lomonosov cosmological simulations
• Dynamical modelling of the twisted galaxy PGC 046832
• Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
• Exploring Simulated Early Star Formation in the Context of the Ultrafaint Dwarf Galaxies
• Dark Matter Halos from the Inside Out
• Seeding supermassive black holes with a non-vortical dark-matter subcomponent
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• The First Galaxies and the Likely Discovery of their Fossils in the Local Group
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• Major mergers between dark matter haloes -- I. Predictions for size, shape, and spin
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. V. Properties and Frequency of Merging Satellites and Centrals in Different Environments
• Photometric Properties of the Most Massive High-Redshift Galaxies
• Simulation view of galaxy clusters with low X-ray surface brightness
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• The Impact of Cluster Structure and Dynamical State on Scatter in the Sunyaev-Zel'dovich Flux-Mass Relation
• Analytical halo model of galactic conformity
• Dynamical flows through Dark Matter Haloes II: one and two points statistics at the virial radius
• Dark Matter Minihalos from Primordial Magnetic Fields
• QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at $z\sim 0.7$
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• NIHAO XXVI: Nature versus nurture, the Star Formation Main Sequence and the origin of its scatter
• Mass accretion rates of clusters of galaxies: CIRS and HeCS
• Constraints on dark matter annihilation and decay from the large-scale structure of the nearby universe
• Evolution of subhalo orbits in a smoothly-growing host halo potential
• A tale of a rich cluster at z$\sim$0.8 as seen by the Star Formation Histories of its ETGs
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Kinematics of cluster galaxies and their relation to galaxy evolution
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• Orbital and escape dynamics in barred galaxies - I. The 2D system
• RELICS: ICL Analysis of the $z=0.566$ merging cluster WHL J013719.8-08284
• A new fitting-function to describe the time evolution of a galaxy's gravitational potential
• Explaining dark matter halo density profiles with neural networks
• On the Redshift Evolution of MgII Absorption Systems
• Dynamical invariants and diffusion of merger substructures in time-dependent gravitational potentials
• The role of AGN on the structure, kinematics and evolution of ETGs in the Horizon simulations
• Merger history trees of dark matter haloes in moving barrier models
• Impact of substructure on local dark matter searches
• COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
• Close Pairs as Proxies for Galaxy Cluster Mergers
• Evolution of stellar-gaseous disks in cosmological haloes
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• The dark matter halo density profile, spiral arm morphology and black hole mass of M33
• A shallow dark matter halo in Ultra Diffuse Galaxy AGC 242019: are UDGs structurally similar to low surface brightness galaxies?
• Statistical properties of dark matter mini-haloes at z >= 15
• Probing the Metal Enrichment of the Intergalactic Medium at $z=5-6$ Using the Hubble Space Telescope
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• X-ray Signatures of Non-Equilibrium Ionization Effects in Galaxy Cluster Accretion Shock Regions
• The probability distribution of cluster formation times and implied Einstein Radii
• Two Body Relaxation in Simulated Cosmological Haloes
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• AXES-SDSS: comparison of SDSS galaxy groups with all-sky X-ray extended sources
• The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars
• When Should We Treat Galaxies as Isolated?
• The evolution of chaos in active galaxy models with an oblate or a prolate dark halo component
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• The Impact of Molecular Hydrogen Cooling on the Galaxy Formation Threshold
• Analytical halo models of cosmic tidal fields
• Chemical Abundance Patterns and the Early Environment of Dwarf Galaxies
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Probing gaseous galactic halos through the rotational kSZ effect
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Large-Scale Gas Dynamics in the Adhesion Model: Implications for the Two-Phase Massive Galaxy Formation Scenario
• Evolution of the gas mass fraction in galaxy clusters
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling
• The SFR-radius connection: data and implications for wind strength and halo concentration
• Growing the First Galaxies' Merger Trees
• Galaxy cluster mass accretion rates from IllustrisTNG
• Disentangling cosmic-ray and dark-matter induced gamma-rays in galaxy clusters?
• The impact of environment on the dynamical structure of satellite systems
• The Halo Density Profiles with Non-Standard N-body Simulations
• A tale of two tails: insights from simulations into the formation of the peculiar dwarf galaxy NGC 1427A
• The cosmology dependence of the concentration-mass-redshift relation
• Absence of Dwarf Galaxies at High Redshifts: Evidence from a Galaxy Group
• The distribution of dark galaxies and spin bias
• Efficient and accurate force replay in cosmological-baryonic simulations
• Spectroscopy of Luminous Compact Blue Galaxies in Distant Clusters I. Spectroscopic Data
• Galactic orbital motions of star clusters: static versus semicosmological time-dependent Galactic potentials
• Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
• Neutron star mass in dark matter clumps
• GHASP: an H$\alpha$ kinematics survey of spiral galaxies - XII. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using R${}_c$-band photometry
• Star formation and bar instability in cosmological haloes
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• Impact of tidal environment on galaxy clustering in GAMA
• The mass and temperature functions in a moving barrier model
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Environmental Effects of Dark Matter Haloes: The Clustering-Substructure relation of Group-size Haloes
• Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Galactic halos in cosmology with long-range scalar DM interaction
• Testing DARKexp against energy and density distributions of Millennium-II halos
• High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
• A Two-Parameter Matching Scheme for Massive Galaxies and Dark Matter Haloes
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Halo Concentrations and the New Baseline X-ray Luminosity-Temperature and Mass Relations of Galaxy Clusters
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies I: A catalogue of morphological parameters
• Extended Press-Schechter theory and the density profiles of dark matter haloes
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Photometry and Dynamics of the Minor Merger AM1219-430 with Gemini GMOS-S
• SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• AXES-2MRS: A new all-sky catalogue of extended X-ray galaxy groups
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• Using Strong Gravitational Lensing to Identify Fossil Group Progenitors
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Modeling the Void H I Column Density Spectrum
• Do Bound Structures Brake Cosmic Acceleration?
• Voronoi Tessellation and Non-parametric Halo Concentration
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Rotation curves of galaxies and the stellar mass-to-light ratio
• Photometry and dynamics of the minor mergers AM\,1228-260 and AM\,2058-381
• The dark matter halo concentration and stellar initial mass function of a CASSOWARY group
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• Halo formation and evolution in scalar field dark matter and cold dark matter: New insights from the fluid approach
• The mass accretion history of dark matter haloes down to Earth mass
• Galaxy Infall by Interacting with its Environment: a Comprehensive Study of 340 Galaxy Clusters
• Self-Consistent Theory of Halo Mergers - II: CDM Power Spectra
• Characterizing simulated galaxy stellar mass histories
• On the Apparent Power Law in CDM Halo Pseudo Phase Space Density Profiles
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• Dark halos acting as chaos controllers in asymmetric triaxial galaxy models
• Close Galaxy Pairs at z = 3: A Challenge to UV Luminosity Abundance Matching
• Galaxy Formation and Dark Matter
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• An efficient and robust method to estimate halo concentration
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• A Random Walk Model for Dark Matter Halo Concentrations
• Response of the LMC's Bar to a Recent SMC Collision and Implications for the SMC's Dark Matter Profile
• Beyond Mass: Detecting Secondary Halo Properties with Galaxy-Galaxy Lensing
• The Radial Distribution of Mono-Metallicity Populations in the Galactic Disk as Evidence for Two-Phase Disk Formation
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• The Evolution of Radio Galaxies and X-ray Point Sources in Coma Cluster Progenitors Since z~1.2
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• The distribution of annihilation luminosities in dark matter substructure
• The velocity function of dark matter halos at r=20 kpc: Remarkably little evolution since z ~ 4
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• Semi-analytical frameworks for subhalos from the smallest to the largest scale
• Cluster Assembly Times as a Cosmological Test
• Fitting functions for a disk-galaxy model with different LCDM-halo profiles
• Massive Galaxies at High-z: Assembly Patterns, Structure & Dynamics in the Fast Phase of Galaxy Formation
• Evolution of Low Mass Galactic Subhalos and Dependence on Concentration
• An expanded merger-tree description of cluster evolution
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• Secular evolution versus hierarchical merging: galaxy evolution along the Hubble sequence, in the field and rich environments
• The mass distribution in Spiral galaxies
• Simulation studies of dark energy clustering induced by the formation of dark matter halos
• Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
• Understanding Galaxy Formation and Evolution
• Local reionizations histories with merger tree of HII regions
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• The kinetic Sunyaev-Zel'dovich effect from the diffuse gas in the Local Group
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• The distinguishing factor for gravity models: stellar population synthesis
• Temporal Self-Organization in Galaxy Formation
• Protoclusters at z=5.7: A view from the MultiDark galaxies
• Spectroscopy of Luminous Compact Blue Galaxies in Distant Clusters II. Physical Properties of dE Progenitor Candidates
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Redshift estimation of clusters by wavelet decomposition of their Sunyaev-Zel'dovich morphology
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• Halo Concentrations and the Fundamental Plane of Galaxy Clusters
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• CHEX-MATE: Multi-probe analysis of Abell 1689
• A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium
• Can radial motions in the stellar halo constrain the rate of change of mass in the Galaxy?
• N-body simulations of dark matter-baryon interactions
• The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters
• Shape and connectivity of groups and clusters: Impact of dynamical state and accretion history
• The SRG/eROSITA All-Sky Survey: Exploring halo assembly bias with X-ray selected superclusters
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Is Abell 2261 a fossil galaxy cluster in a transitional dynamical state?
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• Simulation-based marginal likelihood for cluster strong lensing cosmology
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Subhalos are Anisotropically Distributed and Aligned with the Smooth Matter Distribution of Their Host Halos
• Constraint on Matter Power Spectrum on $10^6-10^9{M}_{\odot }$ Scales from ${\tau }_e$
• Beyond the Halo: Redefining environment with unbound matter in N-body simulations
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• The cusp-halo relation
• The connection between halo concentrations and assembly histories: a probe of gravity?
• On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies
• Constraining blazar heating with the 2<z<3 Lyman-$\alpha$ forest
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• Chemo-dynamical substructure in the M31 inner halo globular clusters: Further evidence for a recent accretion event
• A Gravitational Double Scattering Mechanism for Generating High Velocity Objects
• Dark matter halo concentrations: a short review
• Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
• Dark halo densities, substructure, and the initial power spectrum
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Properties of Barred Galaxies with the Environment: II. The case of the Cosmic Web around the Virgo cluster
• Searching for Dark Matter Annihilation with IceCube and P-ONE
• JWST Discovery of Strong Lensing from a Galaxy Cluster at Cosmic Noon: Giant Arcs and a Highly Concentrated Core of XLSSC 122
• The galaxy-environment connection revealed by constrained simulations
• Formation of galactic bulges from the cold gas filaments in high-redshift dark matter halos
• The Sizes of Globular Clusters as Tracers of Galactic Halo Potentials
• Mass function and assembly of dark halos: an approach to inventory isolated overdense regions in random fields
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• New insights on low-mass dark matter subhalo tidal tracks via numerical simulations
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• Cosmo-Paleontology: Statistics of Fossil Groups in a Gravity-Only Simulation
• The Multidimensional Milky Way
• Cored Dark Matter halos in the Cosmic Neutrino Background
• Correlations in the matter distribution in CLASH galaxy clusters
• The intracluster light analysis of the most evolved systems of galaxies: fossil groups
• On the Assembly Bias of Cool Core Clusters Traced by H$\alpha$ Nebulae
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
• Hot accretion onto spiral galaxies: the origin of extended and warped HI discs
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• Baryonic Collapse within Dark Matter Halos and the Formation of Gaseous Galactic Disks
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos
• Transition between order and chaos in a composite disk galaxy model with a massive nucleus and a dark matter halo
• Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams
• Testing subhalo abundance matching with galaxy kinematics
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• The eventful life journey of galaxy clusters. II. Impact of mass accretion on the thermodynamical structure of the ICM
• The life and times of dark matter haloes: what will I be when I grow up?
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• Dark Matter Density in Disk Galaxies
• Viscous Dark Energy Accretion Activities : Sonic Speed, Angular Momentum and Mach Number Studies
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Morphological diversity of spiral galaxies originating in the cold gas inflow from cosmic webs
• Cosmic Reionization On Computers: Baryonic Effects on Halo Concentrations During the Epoch of Reionization
• Numerical approaches to star formation and SuperNovae energy feedback in simulations of galaxy clusters
• Predicting Halo Formation Time Using Machine Learning
• Independent Evidence for earlier formation epochs of fossil groups of galaxies through the intracluster light: the case for RX J100742.53+380046.6
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• Do gas-poor galaxy clusters have different galaxy populations? The positive covariance of hot and cold baryons
• Chandra Study of the Massive and Distant Galaxy Cluster SDSS J0150-1005
• Determination of Dark Matter Properties at High-Energy Colliders