Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Abstract

We compare the results of Eulerian hydrodynamic simulations of cluster formation against virial scaling relations between four bulk quantities: the cluster mass, the dark matter velocity dispersion, the gas temperature and the cluster luminosity. The comparison is made for a large number of clusters at a range of redshifts in three different cosmological models (CHDM, CDM and OCDM). We find that the analytic formulae provide a good description of the relations between three of the four numerical quantities. The fourth (luminosity) also agrees once we introduce a procedure to correct for the fixed numerical resolution. We also compute the normalizations for the virial relations and compare extensively to the existing literature, finding remarkably good agreement. The Press-Schechter prescription is calibrated with the simulations, again finding results consistent with other authors. We also examine related issues such as the size of the scatter in the virial relations, the effect of metallicity with a fixed pass-band, and the structure of the halos. All of this is done in order to establish a firm groundwork for the use of clusters as cosmological probes. Implications for the models are briefly discussed.

23 pages, 17 figures, accepted for publication in ApJ

References in corpus (1)

• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

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• The Formation of the First Stars in the Universe
• Antiprotons from dark matter annihilation in the Galaxy: astrophysical uncertainties
• Two-Temperature Intracluster Medium in Merging Clusters of Galaxies
• The time-scales probed by star formation rate indicators for realistic, bursty star formation histories from the FIRE simulations
• Satellite Dwarf Galaxies in a Hierarchical Universe: The Prevalence of Dwarf-Dwarf Major Mergers
• Satellite quenching timescales in clusters from projected phase space measurements matched to simulated orbits
• Baryon Content in a Sample of 91 Galaxy Clusters Selected by the South Pole Telescope at 0.2 < z < 1.25
• Dissecting Galaxy Formation: I. Comparison Between Pure Dark Matter and Baryonic Models
• Satellites of Simulated Galaxies: survival, merging, and their relation to the dark and stellar halos
• Galaxy Groups
• Gas density and X-ray surface brightness profiles of clusters of galaxies from dark matter halo potentials: beyond the isothermal beta model
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Populating Dark Matter Haloes with Galaxies: Comparing the 2dFGRS with Mock Galaxy Redshift Surveys
• A Testable Conspiracy: Simulating Baryonic Effects on Self-Interacting Dark Matter Halos
• Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution
• Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: cosmological implications
• The IRX-Beta Dust Attenuation Relation in Cosmological Galaxy Formation Simulations
• Modelling galaxy clustering: halo occupation distribution versus subhalo matching
• Formation of the Black Holes in the Highest Redshift Quasars
• Mass Accretion and its Effects on the Self-Similarity of Gas Profiles in the Outskirts of Galaxy Clusters
• The Eating Habits of Milky Way Mass Halos: Destroyed Dwarf Satellites and the Metallicity Distribution of Accreted Stars
• Disentangling galaxy environment and host halo mass
• On the Detectability of Turbulence and Bulk Flows in X-ray Clusters
• Scaling Relations from Sunyaev-Zel'dovich Effect and Chandra X-ray measurements of high-redshift galaxy clusters
• Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
• The sizes of $z\sim 6-8$ lensed galaxies from the Hubble Frontier Fields Abell 2744 data
• The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile
• Quenching as a Contest between Galaxy Halos and their Central Black Holes
• A Deep XMM-Newton Study of the Hot Gaseous Halo Around NGC 1961
• A Stellar Feedback Origin for Neutral Hydrogen in High-Redshift Quasar-Mass Halos
• XMM-Newton observation of the distant (z=0.6) galaxy cluster RX J1120.1+4318
• The Halo Boundary of Galaxy Clusters in the SDSS
• An XMM-Newton view of the cluster of galaxies Abell 85
• On the radiative efficiencies, Eddington ratios, and duty cycles of luminous high-redshift quasars
• The evolution of the cluster X-ray scaling relations in the WARPS sample at 0.6<z<1.0
• The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
• The Dark Side of Galaxy Color: evidence from new SDSS measurements of galaxy clustering and lensing
• New constraints on light Axion-Like Particles using Chandra Transmission Grating Spectroscopy of the powerful cluster-hosted quasar H1821+643
• Future Galaxy Cluster Surveys: The Effect of Theory Uncertainty on Constraining Cosmological Parameters
• The impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
• Evolution of shocks and turbulence in major cluster mergers
• Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
• Overconsumption, outflows and the quenching of satellite galaxies
• $S^5$: Probing the Milky Way and Magellanic Clouds potentials with the 6-D map of the Orphan-Chenab stream
• The Formation of Isolated Ultra-Diffuse Galaxies in Romulus25
• Cosmological AMR MHD with Enzo
• Disc galaxy evolution models in a hierarchical formation scenario: structure and dynamics
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• LoCuSS: The Sunyaev-Zel'dovich Effect and Weak Lensing Mass Scaling Relation
• A Comparison of Cosmological Codes: Properties of Thermal Gas and Shock Waves in Large Scale Structures
• A model for the postcollapse equilibrium of cosmological structure: truncated isothermal spheres from top-hat density perturbations
• A Simple Model for Quasar Demographics
• Resolving the Lyman-alpha Forest
• Cooling flow solutions for the circumgalactic medium
• The Angular Momentum Distribution of Gas and Dark Matter in Galactic Halos
• Pressure of the hot gas in simulations of galaxy clusters
• Dynamics of the Magellanic Clouds in a LCDM Universe
• The Distribution of Dark Matter in the Milky Way's Disk
• A mass-dependent slope of the galaxy size-mass relation out to z~3: further evidence for a direct relation between median galaxy size and median halo mass
• Evolution of violent gravitational disc instability in galaxies: Late stabilization by transition from gas to stellar dominance
• The Impact of Cooling and Feedback on Disc Galaxies
• On the identification of merger debris in the {\it Gaia} Era
• Hunting for Galaxies and Halos in simulations with VELOCIraptor
• Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties
• The Luminosity Dependence of Quasar Clustering
• The splashback radius of halos from particle dynamics. I. The SPARTA algorithm
• The local dark matter phase-space density and impact on WIMP direct detection
• Effect of turbulent diffusion on iron abundance profiles
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
• The history of chemical enrichment in the intracluster medium from cosmological simulations
• The Three Hundred Project: Backsplash galaxies in simulations of clusters
• Strong lensing in the MareNostrum Universe: biases in the cluster lens population
• Physical properties underlying observed kinematics of satellite galaxies
• The Accuracy of Subhalo Detection
• SIDM on FIRE: Hydrodynamical Self-Interacting Dark Matter simulations of low-mass dwarf galaxies
• Cosmological Constraints from the ROSAT Deep Cluster Survey
• Supermassive Black Holes in the Hierarchical Universe: A General Framework and Observational Tests
• Gas inflow and metallicity drops in star-forming galaxies
• Dependence of Halo Properties on Interaction History, Environment and Cosmology
• Diffuse Baryons in Groups and Clusters of Galaxies
• The Clustering Properties of Lyman-Break Galaxies at Redshift z~3
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey
• What Causes The Formation of Disks and End of Bursty Star Formation?
• Dark matters on the scale of galaxies
• Cosmological Origin of the Stellar Velocity Dispersions in Massive Early-Type Galaxies
• Effect of halo modelling on WIMP exclusion limits
• The Most Massive Galaxies and Black Holes Allowed by $\Lambda$CDM
• Effects of large-scale structure on the accuracy of weak lensing mass measurements
• Hydrodynamic Simulation of the Cosmological X-ray Background
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• The Large-scale Distribution of Cool Gas around Luminous Red Galaxies
• Exploring the Energetics of Intracluster Gas with a Simple and Accurate Model
• Supermassive Black Hole Formation at High Redshifts via Direct Collapse: Physical Processes in the Early Stage
• Observations of High-Redshift X-Ray Selected Clusters with the Sunyaev-Zel'dovich Array
• Scaling Properties of Galaxy Groups
• Close Galaxy Counts as a Probe of Hierarchical Structure Formation
• Quenching of Satellite Galaxies at the Outskirts of Galaxy Clusters
• Low-Redshift Lyman Limit Systems as Diagnostics of Cosmological Inflows and Outflows
• The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations
• Hot Gas in Clusters of Galaxies: the Punctuated Equilibria Model
• The X-ray/SZ view of the virial region. I. Thermodynamic properties
• Isolating Triggered Star Formation
• Constraining the LRG Halo Occupation Distribution using Counts-in-Cylinders
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the Halo Occupation Distribution model for Emission Line Galaxies
• How do galaxies acquire their mass?
• CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding Structures
• Tree-Particle-Mesh: an adaptive, efficient, and parallel code for collisionless cosmological simulation
• Evolution of the atomic and molecular gas content of galaxies in dark matter haloes
• Kinematics of Circumgalactic Gas: Feeding Galaxies and Feedback
• The High-$z$ Universe Confronts Warm Dark Matter: Galaxy Counts, Reionization and the Nature of Dark Matter
• Constraints on Assembly Bias from Galaxy Clustering
• \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities
• A Sunyaev-Zel'dovich take on cluster radio haloes -- I. Global scaling and bi-modality using Planck data
• The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos
• X-ray and Sunyaev-Zel'dovich scaling relations in galaxy clusters
• Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
• Why do high-redshift galaxies show diverse gas-phase metallicity gradients?
• PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
• XMM-Newton observations of three poor clusters: Similarity in dark matter and entropy profiles down to low mass
• Coming of Age in the Dark Sector: How Dark Matter Haloes grow their Gravitational Potential Wells
• Cosmological Simulations of Decaying Dark Matter: Implications for Small-scale Structure of Dark Matter Halos
• Constraining dark matter halo properties using lensed SNLS supernovae
• A hydrodynamical halo model for weak-lensing cross correlations
• The extent of chemically enriched gas around star-forming dwarf galaxies
• The Direct Collapse of a Massive Black Hole Seed Under the Influence of an Anisotropic Lyman-Werner Source
• On the Evolution of the Velocity-Mass-Size Relations of Disk-Dominated Galaxies over the Past 10 Billion Years
• Modeling evolution of dark matter substructure and annihilation boost
• Constraining the primordial black hole abundance with 21cm cosmology
• Gemini/GMOS Spectroscopy of 26 Strong Lensing Selected Galaxy Cluster Cores
• The outer profile of dark matter halos: an analytical approach
• Self-regulated black hole accretion, the M-sigma relation, and the growth of bulges in galaxies
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• nIFTy Cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics
• Relations Between the Sizes of Galaxies and their Dark Matter Halos at Redshifts $0<z<3$
• Sunyaev-Zel'dovich clusters in Millennium Gas simulations
• The predicted luminous satellite populations around SMC and LMC-mass galaxies - A missing satellite problem around the LMC?
• Identifying the Reionization Redshift from the Cosmic Star Formation Rate
• Fermi-LAT constraints on dark matter annihilation cross section from observations of the Fornax cluster
• Mass Modeling of Disk Galaxies: Constraints, Degeneracies and Adiabatic Contraction
• Heating of the intracluster medium by quasar outflows
• Scaling relations and mass calibration of the X-ray luminous galaxy clusters at z~0.2: XMM-Newton observations
• Scalar Field Dark Matter: Helping or Hurting Small-Scale Problems in Cosmology?
• The Evolution of the Dark Halo Spin Parameters lambda and lambda' in a LCDM Universe: The Role of Minor and Major Mergers
• Where are the Low-Mass Population III Stars ?
• The Postcollapse Equilibrium Structure of Cosmological Haloes in a Low-Density Universe
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• The evolution of clusters in the CLEF cosmological simulation: X-ray structural and scaling properties
• The M-sigma Relation for Nucleated Galaxies
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• EVLA Observations of Galactic Supernova Remnants: Wide-field Continuum and Spectral-index Imaging
• Observing the End of Cold Flow Accretion using Halo Absorption Systems
• Dark Matter Halos of Disk Galaxies: Constraints from the Tully-Fisher Relation
• The SAMI Galaxy Survey: Quenching of star formation in clusters I. Transition galaxies
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• An analytic model for the bispectrum of galaxies in redshift space
• The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
• Velocity Dispersions of CNOC Clusters and the Evolution of the Cluster Abundance
• Magnetic field amplification during gravitational collapse - Influence of initial conditions on dynamo evolution and saturation
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• Cosmological constraints from evolution of cluster baryon mass function at z~0.5
• The Alignment between Satellites and Central Galaxies: Theory vs. Observations
• Column Density Profiles of Multi-Phase Gaseous Halos
• AGN feedback in dwarf galaxies?
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes
• MAGIICAT III. Interpreting Self-Similarity of the Circumgalactic Medium with Virial Mass using MgII Absorption
• The Three Causes of Low-Mass Assembly Bias
• The observability of gamma-rays from neutralino annihilations in Milky Way substructure
• The X-ray Properties of Nearby Abell Clusters from the ROSAT All-Sky Survey: The Sample and Correlations with Optical Properties
• A VLT spectroscopic survey of RX J0152.7-1357, a forming cluster of galaxies at z=0.837
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• MultiDark-Galaxies: data release and first results
• CoMaLit III. Literature Catalogs of weak Lensing Clusters of galaxies (LC^2)
• Suppressed effective viscosity in the bulk intergalactic plasma
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• Blazars in the early Universe
• Properties of Intra-group Stars and Galaxies in Galaxy Groups: "Normal" versus "Fossil" Groups
• A Deficit of High-Redshift, High-Luminosity X-Ray Clusters: Evidence for a High Value of Omega_m?
• Cosmology from the Thermal Sunyaev-Zel'dovich Power Spectrum: Primordial non-Gaussianity and Massive Neutrinos
• The radial structure of galaxy groups and clusters
• A Census of Baryons and Dark Matter in an Isolated, Milky Way-sized Elliptical Galaxy
• An Extreme Metallicity, Large-Scale Outflow from a Star-Forming Galaxy at z ~ 0.4
• Dwarf Galaxies in CDM, WDM, and SIDM: Disentangling Baryons and Dark Matter Physics
• How important is the dark matter halo for black hole growth?
• The tidal evolution of dark matter substructure -- II. The impact of artificial disruption on subhalo mass functions and radial profiles
• Nonthermal Particles and Radiation Produced by Cluster Merger Shocks
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• Inside Out and Upside-Down: The Roles of Gas Cooling and Dynamical Heating in Shaping the Stellar Age-Velocity Relation
• Major Mergers Going Notts: Challenges for Modern Halo Finders
• A Census of Stellar Mass in 10 Massive Haloes at z~1 from the GCLASS Survey
• Nuclear Star Clusters from Clustered Star Formation
• A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes
• The build up of the correlation between halo spin and the large scale structure
• The maximum accretion rate of hot gas in dark matter halos
• Non-linear evolution of the cosmic neutrino background
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• Reionization in Technicolor
• The Absence of Adiabatic Contraction of the Radial Dark Matter Profile in the Galaxy Cluster A2589
• Do Mergers Spin up Dark Matter Halos?
• Surveying the Sky with the Arcminute MicroKelvin Imager: Expected Constraints on Galaxy Cluster Evolution and Cosmology
• Evolution at z>0.5 of the X-ray properties of simulated galaxy clusters: comparison with the observational constraints
• XMM-Newton Observations of Evolution of Cluster X-Ray Scaling Relations at z=0.4-0.7
• Assessing the redshift evolution of massive black holes and their hosts
• The Effect of Cooling on the Density Profile of Hot Gas in Clusters of Galaxies: Is Additional Physics Needed?
• Large Einstein Radii: A Problem for LambdaCDM
• Modeling Dynamical Dark Energy
• Resolved Dwarf Galaxy Searches within ~5 Mpc with the Vera Rubin Observatory and Subaru Hyper Suprime-Cam
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• Escape of Lyman-alpha and continuum photons from star-forming galaxies
• Dissecting the Evolution of Dark Matter Subhaloes in the Bolshoi Simulation
• H_2 Suppression with Shocking Inflows: Testing a Pathway for Supermassive Black Hole Formation
• Chemical evolution in a model for the joint formation of quasars and spheroids
• The impact of Early Dark Energy on non-linear structure formation
• Predicting the locations of possible long-lived low-mass first stars: Importance of satellite dwarf galaxies
• Metal-Poor, Cool Gas in the Circumgalactic Medium of a z = 2.4 Star-Forming Galaxy: Direct Evidence for Cold Accretion?
• Constraints on the annihilation cross section of dark matter particles from anisotropies in the diffuse gamma-ray background measured with Fermi-LAT
• Gas Loss by Ram Pressure Stripping and Internal Feedback From Low Mass Milky Way Satellites
• Quasars: What turns them off?
• Mass profiles and galaxy orbits in nearby galaxy clusters from the analysis of the projected phase-space
• Radial Temperature Profiles of X-Ray--Emitting Gas Within Clusters of Galaxies
• The Need for Speed: Escape velocity and dynamical mass measurements of the Andromeda galaxy
• Effective Models for Statistical Studies of Galaxy-Scale Gravitational Lensing
• The angular momentum of cold dark matter haloes with and without baryons
• Rapid disc settling and the transition from bursty to steady star formation in Milky Way-mass galaxies
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the low-redshift sample
• On the Physical Origin of Galactic Conformity
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• The Mass Assembly History of Spheroidal Galaxies: Did Newly-Formed Systems Arise Via Major Mergers?
• A Complete Census of Circumgalactic MgII at Redshift z<~ 0.5
• Turbulent Velocity Fields in SPH--simulated Galaxy Clusters
• Strong Gravitational Lensing and Dark Energy
• Galaxies lacking dark matter produced by close encounters in a cosmological simulation
• Signatures of Velocity-Dependent Dark Matter Self-Interactions in Milky Way-mass Halos
• Accretion Shocks in Clusters of Galaxies and their SZ Signature from Cosmological Simulations
• Omega-Matter from the Temperature-Redshift Distribution of EMSS Clusters of Galaxies
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Precision Scaling Relations for Disk Galaxies in the Local Universe
• Mass functions in coupled Dark Energy models
• Gas depletion in Local Group dwarfs on ~250 kpc scales: Ram pressure stripping assisted by internal heating at early times
• The halo model for cosmology: a pedagogical review
• The dynamics of tidal tails from massive satellites
• An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB
• The Mass-Temperature Relation of 22 Nearby Clusters
• The Three Hundred Project: correcting for the hydrostatic-equilibrium mass bias in X-ray and SZ surveys
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Preventing Star Formation in Early-Type Galaxies with Late-Time Stellar Heating
• On the dynamical state of galaxy clusters: insights from cosmological simulations II
• Density profiles of dark matter haloes on Galactic and Cluster scales
• Measuring the Cosmic Equation of State with Counts of Galaxies
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Evolution of Galaxy Shapes from Prolate to Oblate through Compaction Events
• Shock Waves and Cosmic Ray Acceleration in the Outskirts of Galaxy Clusters
• Absorption-Line Detections of $10^{5-6}$ K Gas in Spiral-Rich Groups of Galaxies
• Where Do Galaxies End?
• Galaxy Infall Kinematics as a Test of Modified Gravity
• Anisotropic dark matter distribution functions and impact on WIMP direct detection
• Modeling Tidal Streams in evolving dark matter halos
• Cosmological Effects of Powerful AGN Outbursts in Galaxy Clusters: Insights from an XMM-Newton Observation of MS0735+7421
• Dark-Matter Decays and Self-Gravitating Halos
• Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
• Cross-Correlation of Cosmic Shear and Extragalactic Gamma-ray Background: Constraints on the Dark Matter Annihilation Cross-Section
• The First Stars
• The Galaxy Clustering Crisis in Abundance Matching
• Morphologies of ~190,000 Galaxies at z=0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
• The X-ray surface brightness profiles of hot galaxy clusters up to z~0.8: evidence for self-similarity and constraints on Omega_0
• LambdaCDM Halo Density Profiles: where do actual halos converge to NFW ones?
• The interplay of Self-Interacting Dark Matter and baryons in shaping the halo evolution
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• On the Self-Similar Appearance of Galaxy Clusters in X-rays
• Angular momentum distribution of hot gas and implications for disk galaxy formation
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• High-Redshift Galaxies: Their Predicted Size and Surface Brightness Distributions and Their Gravitational Lensing Probability
• Gas infall and radial transport in cosmological simulations of Milky Way-mass disks
• How accurately can the SZ effect measure peculiar cluster velocities and bulk flows?
• Reignition of Star Formation in Dwarf Galaxies
• Scaling relations of Fuzzy Dark Matter haloes I: individual systems in their cosmological environment
• The halo model in a massive neutrino cosmology
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• How well does the Friends-of-Friends algorithm recover group properties from galaxy catalogs limited in both distance and luminosity?
• Universal at last? The splashback mass function of dark matter halos
• Is the Number of Giant Arcs in LCDM Consistent With Observations?
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• A two-phase scenario for bulge assembly in LCDM cosmologies
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• Contributions to the Power Spectrum of Cosmic Microwave Background from Fluctuations Caused by Clusters of Galaxies
• A Dichotomy in Satellite Quenching Around L* Galaxies
• The Edge of the Galaxy
• On the mass of the Local Group
• Discovery of Multi-Phase Cold Accretion in a Massive Galaxy at z=0.7
• Effects of Strong Gravitational Lensing on Millimeter-Wave Galaxy Number Counts
• The Origins of Off-Centre Massive Black Holes in Dwarf Galaxies
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• Testing the Cosmological Principle with CatWISE Quasars: A Bayesian Analysis of the Number-Count Dipole
• Boosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling
• Reconciling observed and simulated stellar halo masses
• Tracing the first stars and galaxies of the Milky Way
• The impact of baryons on the direct detection of dark matter
• The Multiphase Intergalactic Medium towards PKS 2155-304
• X-ray scaling relations of early-type galaxies
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• Runaway Stars and the Escape of Ionizing Radiation from High-Redshift Galaxies
• Puffing up early-type galaxies by baryonic mass loss: numerical experiments
• Properties of Resonantly Produced Sterile Neutrino Dark Matter Subhalos
• Nonthermal Emission from Accreting and Merging Clusters of Galaxies
• On the shape of dark matter halos from MultiDark Planck simulations
• Emulating galaxy clustering and galaxy-galaxy lensing into the deeply nonlinear regime: methodology, information, and forecasts
• Localized massive halo properties in Bahamas and Macsis simulations: scalings, log-normality, and covariance
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• NIHAO XII: galactic uniformity in a ΛCDM universe
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• The Atacama Cosmology Telescope: Detection of Sunyaev-Zel'dovich Decrement in Groups and Clusters Associated with Luminous Red Galaxies
• Cosmic variance of the galaxy cluster weak lensing signal
• Simulating the X-ray Forest
• The sizes of mini-voids in the local universe: an argument in favor of a warm dark matter model?
• MOKA: a new tool for Strong Lensing Studies
• Future Evolution of Bound Superclusters in an Accelerating Universe
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• The Three Hundred Project: The evolution of galaxy cluster density profiles
• The phase-space distribution of infalling dark matter subhalos
• Heating groups and clusters of galaxies: the role of AGN jets
• On the Segregation of Dark Matter Substructure
• The XMM--NEWTON Omega Project: I. The X-ray Luminosity - Temperature Relation at z>0.4
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Disentangling the Cosmic Web Towards FRB 190608
• Exploring SMBH Assembly with Semi-analytic Modelling
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Interpreting Short Gamma Ray Burst Progenitor Kicks and Time Delays Using the Host Galaxy-Dark Matter Halo Connection
• 3D simulations with boosted primordial power spectra and ultracompact minihalos
• Off-Center Mergers of Clusters of Galaxies and Nonequipartition of Electrons and Ions in Intracluster Medium
• Intensity Mapping as a Probe of Axion Dark Matter
• Numerical and Analytical Predictions for the Large-Scale Sunyaev-Zel'dovich Effect
• Empirical constraints on the formation of early-type galaxies
• Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
• Chandra X-Ray Observatory Observation of the High-Redshift Cluster MS 1054-0321
• A robust estimate of the Milky Way mass from rotation curve data
• A simluated TCDM cosmology cluster catalogue: the NFW profile and the temperature-mass scaling relations
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way
• A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
• A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• Bailing Out the Milky Way: Variation in the Properties of Massive Dwarfs Among Galaxy-Sized Systems
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions
• The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect
• Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ
• Tracing the Gas to the Virial Radius (R100) in a Fossil Group
• Numerical Simulations of High Redshift Star Formation in Dwarf Galaxies
• Cosmological Constraints from the Clustering Properties of the X-Ray Brightest Abell-type Cluster Sample
• Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation
• The physical nature of the cosmic accretion of baryons and dark matter into halos and their galaxies
• Growing Live Disks Within Cosmologically Assembling Asymmetric Halos: Washing Out the Halo Prolateness
• Born this way: thin disc, thick disc, and isotropic spheroid formation in FIRE-2 Milky-Way-mass galaxy simulations
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• Mock Lightcones and Theory Friendly Catalogs for the CANDELS Survey
• A2163: Merger events in the hottest Abell galaxy cluster I. Dynamical analysis from optical data
• Dark Photon Dark Matter in the Presence of Inhomogeneous Structure
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Systematic biases on galaxy haloes parameters from Yukawa-like gravitational potentials
• The environmental dependence of galaxy colors in intermediate redshift X-ray-selected clusters
• Detection of the Entropy of the Intergalactic Medium: Accretion Shocks in Clusters, Adiabatic Cores in Groups
• Mass and Concentration estimates from Weak and Strong Gravitational Lensing: a Systematic Study
• Sharpening the Precision of the Sunyaev-Zel'dovich Power Spectrum
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• Characterizing the abundance, properties, and kinematics of the cool circumgalactic medium of galaxies in absorption with SDSS DR16
• The nature of voids: II. Tracing underdensities with biased galaxies
• Parameter Tests Within Cosmological Simulations of Galaxy Formation
• Globular Clusters and Dark Satellite Galaxies through the Stream Velocity
• How Gas Accretion Feeds Galactic Disks
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• Cosmic Evolution of Virial and Stellar Mass in Massive Early-Type Galaxies
• Does circumgalactic OVI trace low-pressure gas beyond the accretion shock? Clues from HI and low-ion absorption, line kinematics, and dust extinction
• A Systematic Search for High Surface Brightness Giant Arcs in a Sloan Digital Sky Survey Cluster Sample
• The Self-Similarity of the Circumgalactic Medium with Galaxy Virial Mass: Implications for Cold-Mode Accretion
• Calcium H & K Induced by Galaxy Halos
• COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at $z=2.77$
• TheHaloMod: An online calculator for the halo model
• The dependence of halo bias on age, concentration and spin
• The accretion of dark matter subhaloes within the cosmic web: primordial anisotropic distribution and its universality
• Pressure balance in the multiphase ISM of cosmologically simulated disk galaxies
• Multiscale probability mapping: groups, clusters and an algorithmic search for filaments in SDSS
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• The splashback boundary of haloes in hydrodynamic simulations
• Substructure Boosts to Dark Matter Annihilation from Sommerfeld Enhancement
• How Biased Are Halo Properties in Cosmological Simulations?
• An XMM-Newton observation of the massive, relaxed galaxy cluster ClJ1226.9+3332 at z=0.89
• Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation
• Constraints on the small-scale power spectrum of density fluctuations from high-redshift gamma-ray bursts
• Constraints on Dark Matter Annihilation in Clusters of Galaxies from Diffuse Radio Emission
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Formation, vertex deviation and age of the Milky Way's bulge: input from a cosmological simulation with a late-forming bar
• Optical selection bias and projection effects in stacked galaxy cluster weak lensing
• Bispectrum of the Sunyaev-Zel'dovich Effect
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• Gravitational recoil: effects on massive black hole occupation fraction over cosmic time
• On the origin of surprisingly cold gas discs in galaxies at high redshift
• The Co-Evolution of Galaxies and the Cool Circumgalactic Medium Probed with the SDSS and DESI Legacy Imaging Surveys
• Chandra and XMM-Newton Observations of the Double Cluster Abell 1758
• Thermal evolution of the primordial clouds in warm dark matter models with keV sterile neutrinos
• The Young and the Wild: What happens to Protoclusters forming at z = 4?
• A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations
• Probing small-scale cosmological fluctuations with the 21 cm forest: effects of neutrino mass, running spectral index and warm dark matter
• An Improved Model for the Dynamical Evolution of Dark Matter Subhaloes
• Understanding Cluster Gas Evolution and Fine-Scale CMB Anisotropy with Deep Sunyaev-Zel'dovich Effect Surveys
• Evolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters II. The Effects of Cluster Size and Dynamical State
• Tracing the X-ray emitting intra-cluster medium of clusters of galaxies beyond r_200
• The X-ray Size-Temperature Relation for Intermediate Redshift Galaxy Clusters
• Dark matter subhaloes as gamma-ray sources and candidates in the first Fermi-LAT catalogue
• The Origin of Weak Lensing Convergence Peaks
• The Impact of Halo Properties, Energy Feedback and Projection Effects on the Mass-SZ Flux Relation
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• The Role of Penetrating Gas Streams in Setting the Dynamical State of Galaxy Clusters
• The Mass of the Milky Way from the H3 Survey
• The XMM--NEWTON Omega Project: II.Cosmological implications from the high redshift L-T relation of X-ray clusters
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies
• On Galaxy-Cluster Sizes and Temperatures
• Radio spectral study of the cluster of galaxies Abell 2255
• Rhapsody. II. Subhalo Properties and the Impact of Tidal Stripping From a Statistical Sample of Cluster-Size Halos
• Cosmology dependency of halo masses and concentrations in hydrodynamic simulations
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• A self-consistent phase-space distribution function for the anisotropic Dark Matter halo of the Milky Way
• Evolution of star clusters in a cosmological tidal field
• Virial scaling of galaxies in clusters: bright to faint is cool to hot
• XMM-Newton study of the lensing cluster of galaxies CL0024+17
• Cosmic Ballet III: halo spin evolution in the cosmic web
• Cosmological baryon transfer in the SIMBA simulations
• Constraints on the circumburst environments of short gamma-ray bursts
• Compact groups from the Millennium Simulations: I. Their Nature and the completeness of the Hickson sample
• Mass-Temperature Relation of Galaxy Clusters: A Theoretical Study
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
• Mapping Extragalactic Dark Matter Annihilation with Galaxy Surveys: A Systematic Study of Stacked Group Searches
• Mapping the allowed parameter space for decaying dark matter models
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• Joint analysis of the thermal Sunyaev-Zeldovich effect and 2MASS galaxies: Probing gas physics in the local Universe and beyond
• Cluster Tempreature Evolution: The Mass-Temperature Relation
• Dissipative Dark Matter on FIRE: I. Structural and kinematic properties of dwarf galaxies
• Including beyond-linear halo bias in halo models
• Was the Cosmic Web of Protogalactic Material Permeated by Lobes of Radio Galaxies During the Quasar Era?
• Lensing Magnification: Implications for Counts of Submillimeter Galaxies and SZ Clusters
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Cold Dark Matter Substructures in Early-Type Galaxy Halos
• The Abundance and Structure of Subhaloes near the Free Streaming Scale and Their Impact on Indirect Dark Matter Searches
• Dark-matter decays and Milky Way satellite galaxies
• Effects of the Non-Equipartition of Electrons and Ions in the Outskirts of Relaxed Galaxy Clusters
• Unabsorbed Seyfert 2 galaxies: the case of "naked" AGN
• Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• What sets the central structure of dark matter haloes?
• Thermodynamical properties of the ICM from hydrodynamical simulations
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• Self-consistent semi-analytic models of the first stars
• The X-ray surface brightness distribution from diffuse gas
• Testing adiabatic contraction of dark matter in fossil group candidates
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• The evolution of the stellar mass versus halo mass relationship
• The Role of Baryons in Creating Statistically Significant Planes of Satellites around Milky Way-Mass Galaxies
• Weak lensing constraints on splashback around massive clusters
• The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• On the origin of the angular momentum properties of gas and dark matter in galactic halos and its implications
• Self-similarity of clusters of galaxies and the L_X-T relation
• Non-parametric strong lens inversion of SDSS J1004+4112
• A rumble in the dark: signatures of self-interacting dark matter in Super-Massive Black Hole dynamics and galaxy density profiles
• Missing baryons traced by the galaxy luminosity density in the large-scale WHIM filaments
• Small-scale Intensity Mapping: Extended Ly$\alpha$, H$\alpha$ and Continuum emission as a Probe of Halo Star Formation in High-redshift Galaxies
• Quenched Cold Accretion of a Large Scale Metal-Poor Filament due to Virial Shocking in the Halo of a Massive z=0.7 Galaxy
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• Young and turbulent: the early life of massive galaxy progenitors
• X-Ray Constraints on the Warm_hot Intergalactic Medium
• Thermal and non-thermal traces of AGN feedback: results from cosmological AMR simulations
• Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• A theoretical study of the mass temperature relation for clusters of galaxies
• Clusters of galaxies in the microwave band: influence of the motion of the Solar System
• Constraints on small-scale primordial power by annihilation signals from extragalactic dark matter minihalos
• Supernovae and AGN driven galactic outflows
• Angular power spectrum of galaxies in the 2MASS Redshift Survey
• The nature of dark matter and the density profile and central behavior of relaxed halos
• Joint likelihood function of cluster counts and $n$-point correlation functions: Improving their power through including halo sample variance
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Gas in Simulations of High Redshift Galaxies and Minihalos
• Reexamination of the galaxy formation-regulated gas evolution model in groups and clusters
• Newtonian acceleration scales in spiral galaxies
• The Smith Cloud: high-velocity accretion and dark-matter confinement
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• Redshifted 21 Centimeter Emission from Minihalos Before Reionization
• Feedback from galactic stellar bulges and hot gaseous haloes of galaxies
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• On stellar mass loss from galaxies in groups and clusters
• Fuzzy Dark Matter at Cosmic Dawn: New 21-cm Constraints
• Accurate Analytic Model for the Weak Lensing Convergence One-Point Probability Distribution Function and its Auto-Covariance
• The Three Hundred Project: quest of clusters of galaxies morphology and dynamical state through Zernike Polynomials
• A joint model for the emission and absorption properties of damped Lyman alpha absorption systems
• Radio source feedback in galaxy evolution
• Weak Lensing as a Calibrator of the Cluster Mass-Temperature Relation
• The ELIXR Galaxy Survey. II: Baryons and Dark Matter in an Isolated Elliptical Galaxy
• Dynamical Evolution of Primordial Dark Matter Haloes through Mergers
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• Dissecting the Gamma-Ray Background in Search of Dark Matter
• Uncertainties associated with the backward integration of dwarf satellites using simple parametric potentials
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Core-Envelope Haloes in Scalar Field Dark Matter with Repulsive Self-Interaction: Fluid Dynamics Beyond the de Broglie Wavelength
• Dark matter scaling relations in intermediate z haloes
• Cosmological SPH simulations with four million particles: statistical properties of X-ray clusters in a low-density universe
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• Constraints on Dark Matter Annihilation/Decay from the Isotropic Gamma-Ray Background
• Bias deconstructed: Unravelling the scale dependence of halo bias using real space measurements
• Comprehensive Assessment of the Too-Big-to-Fail Problem
• The Physical Origins of the Identified and Still Missing Components of the Warm-Hot Intergalactic Medium: Insights from Deep Surveys in the Field of Blazar 1ES1553+113
• Reconstructing the radial profiles of gas density and temperature in clusters of galaxies from high-resolution X-ray and radio observations
• Astrometric Microlensing by Local Dark Matter Subhalos
• ASOHF: a new adaptive spherical overdensity halo finder
• Low Angular Momentum in Clumpy, Turbulent Disk Galaxies
• Satellites in MW-like hosts: Environment dependence and close pairs
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• Stellar splashback: the edge of the intracluster light
• Neutrinos in IceCube/KM3NeT as probes of Dark Matter Substructures in Galaxy Clusters
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Neutral CGM as damped Lyα absorbers at high redshift
• Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
• Gemini and Chandra observations of Abell 586, a relaxed strong-lensing cluster
• Ultraviolet Background Radiation from Cosmic Structure Formation
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• The Secondary Spin Bias of Dark Matter Haloes
• A Critical Assessment of Solutions to the Galaxy Diversity Problem
• The Bright SHARC Survey: The X-ray Cluster Luminosity Function
• Weakly Lensed Gravitational Waves: Probing Cosmic Structures with Wave-Optics Features
• Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars
• Testing phenomenological and theoretical models of dark matter density profiles with galaxy clusters
• Relating the structure of dark matter halos to their assembly and environment
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• The Main Sequence and the Fundamental Metallicity Relation in MaGICC Galaxies: Evolution and Scatter
• The CGM${}^2$ Survey: Circumgalactic O VI from dwarf to massive star-forming galaxies
• Angular correlations in the cosmic gamma-ray background from dark matter annihilation around intermediate-mass black holes
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Closing in on Omega_0: The Amplitude of Mass Fluctuations from Galaxy Clusters and the Lyman-alpha Forest
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• The Contribution of Halos with Different Mass Ratios to the Overall Growth of Cluster-Sized Halos
• Can simulations reproduce the observed temperature-mass relation for clusters of galaxies?
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• The Effect of radiative cooling on the scale-dependence of global stellar and gas contents of groups and clusters of galaxies
• Signatures of Galaxy Formation in the Intracluster Medium
• Do Cosmic Rays Heat the Early Intergalactic Medium?
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters I: Analysis with the Three Hundred Simulations
• Are Clusters Standard Candles? Galaxy Cluster Scaling Relations With the Sunyaev-Zeldovich Effect
• Cross-correlation of the thermal Sunyaev-Zel'dovich effect and weak gravitational lensing: Planck and Subaru Hyper Suprime-Cam first-year data
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• Deconstructing Thermal Sunyaev-Zel'dovich - Gravitational Lensing Cross-Correlations: Implications for the Intracluster Medium
• Probing Cosmology with the X-ray Forest
• Galaxy cluster mergers
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• The DEEP2 Galaxy Redshift Survey: Probing the Evolution of Dark Matter Halos around Isolated Galaxies at z ~ 1
• The Dark Matter Annihilation Signal from Dwarf Galaxies and Subhalos
• Adiabatic scaling relations of galaxy clusters
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Modelling the Milky Way through adiabatic compression of cold dark matter halo
• The Galaxy Cluster Concentration-Mass Scaling Relation
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Cold Fronts and Shocks Formed by Gas Streams in Galaxy Clusters
• Lyman continuum leaking galaxies - Search strategies and local candidates
• The effects of baryonic cooling on the concentration-mass relation
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• Towards a characterization of X-ray galaxy clusters for cosmology
• The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud
• A Deep Learning Approach to Infer Galaxy Cluster Masses from Planck Compton$-y$ parameter maps
• Theoretical dark matter halo density profile
• The Challenges of Identifying Population III Stars in the Early Universe
• The Redshift Distribution of Distant Supernovae and its Use in Probing Reionization
• CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
• The Gravitational-Wave contribution to the CMB anisotropies
• On the decreasing fraction of Strong Ly$\alpha$ Emitters around $z$ $\sim$ $6$-$7$
• The Angular Momentum of Gas in Proto-Galaxies: II -- The Impact of Preheating
• New Light on the Baryon Fraction in Galaxy Clusters
• Anisotropic cosmic optical background bound for decaying dark matter in light of the LORRI anomaly
• Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations
• Post-Newtonian constraints on Lorentz-violating gravity theories with a MOND phenomenology
• Bright and Dark Matter in Elliptical Galaxies: Mass and Velocity Distributions from Self-consistent Hydrodynamical Simulations
• Magnetic Fields on FIRE: Comparing B-fields in the multiphase ISM and CGM of Simulated L${}_{\ast }$ Galaxies to Observations
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• High redshift X-ray galaxy clusters. II. The L_X-T relationship revisited
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• The generalized scaling relations for X-ray galaxy clusters: the most powerful mass proxy
• Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
• Confronting Galactic and Extragalactic $\gamma$-ray observed by Fermi-LAT with Annihilating Dark Matter in Inert Higgs Doublet Model
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04
• Mass models from high-resolution HI data of the dwarf galaxy NGC 1560
• On the accretion history of galaxy clusters: temporal and spatial distribution
• Halo Mass Dependence of HI and OVI Absorption: Evidence for Differential Kinematics
• Models of Disk Evolution: Confrontation with Observations
• Abell 611: I. weak lensing analysis with LBC
• Cosmological Lower Bound on Dark Matter Masses from the Soft Gamma-ray Background
• Discovery of a Solitaire Dwarf Galaxy in the APPLES Survey
• Cluster scaling relations from cosmological hydrodynamic simulations in dark energy dominated universe
• Predicting the Clustering of X-Ray Selected Galaxy Clusters in Flux-Limited Surveys
• The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
• Soft X-ray and ultra-violet metal-line emission from the gas around galaxies
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• Astrophysics & Cosmology from Line Intensity Mapping vs Galaxy Surveys
• Massive black hole and Population III galaxy formation in over-massive dark matter halos with violent merger histories
• Non-Thermal Production of WIMPs, Cosmic $e^{\pm }$ Excesses and $\gamma$-rays from the Galactic Center
• Adaptive mesh refinement simulations of a galaxy cluster merger - I. Resolving and modelling the turbulent flow in the cluster outskirts
• Merging Galaxy Clusters: Offset Between the Sunyaev-Zel'dovich Effect and X-ray Peaks
• Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Subaru Weak Lensing survey -- II: Multi-object Spectroscopy and Cluster Masses
• Unbound Particles in Dark Matter Halos
• How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
• Comparisons of Cosmological MHD Galaxy Cluster Simulations to Radio Observations
• Mass distribution in the most X-ray-luminous galaxy cluster RX J1347.5-1145 studied with XMM-Newton
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• Cosmology with clusters of galaxies
• SZE Signals in Cluster Models
• Cosmic filaments delay quenching inside clusters
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• Neutrino clustering in the Milky Way and beyond
• The DESI $N$-body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Constraining SIDM with halo shapes: revisited predictions from realistic simulations of early-type galaxies
• The scatter in the galaxy-halo connection: a machine learning analysis
• Amplified J-factors in the Galactic Center for velocity-dependent darkmatter annihilation in FIRE simulations
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Thermal Instability in the CGM of $L_{\star }$ Galaxies: Testing "Precipitation" Models with the FIRE Simulations
• The earliest galaxies seen in 21 cm line absorption
• Modelling the cosmic neutral hydrogen from DLAs and 21 cm observations
• Ram-Pressure Stripping of Galaxies in High-Redshift Clusters and Influence of ICM Heating
• Evolution of Dark Matter Halos and their Radio Emissions
• A divergence-cleaning scheme for cosmological SPMHD simulations
• Redshift Evolution in the Iron Abundance of the Intracluster Medium
• The power spectrum amplitude from clusters revisited: σ_8 using simulations with preheating and cooling
• What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• Turbulence in the Intergalactic Medium
• Magneto-Hydrodynamical Effects on Nuclear Deflagration Fronts in Type Ia Supernovae
• SMBH Seeds from Dissipative Dark Matter
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• LoCuSS: A Herschel view of obscured star formation in Abell 1835
• The physical origins of low-mass spin bias
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^{\ast }$ Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
• Conditions for detecting lensed Population III galaxies in blind surveys with the James Webb Space Telescope, the Roman Space Telescope and Euclid
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations
• Dark matter haloes in modified gravity and dark energy: interaction rate, small-, and large-scale alignment
• Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
• Re-ionizing the Universe without Stars
• Neutrino Halos in Clusters of Galaxies and their Weak Lensing Signature
• Cool circumgalactic gas of passive galaxies from cosmological inflow
• Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of the Thermal Sunyaev-Zel'dovich Effect and Weak Lensing
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• The Angular Momentum Distribution within Halos in Different Dark Matter Models
• On the Distribution of X-ray Surface Brightness from Diffuse Gas
• Merger and Ring Galaxy Formation Rates at z<=2
• Mapping "out-of-the-box" the properties of the baryons in massive halos
• Modeling the Phase-Space Distribution around Massive Halos
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• The mass function dependence on the dynamical state of dark matter haloes
• A Possible Origin of Magnetic Fields in Galaxies and Clusters: Strong Magnetic fields at z~10?
• The polytropic approximation and X-ray scaling relations: constraints on gas and dark matter profiles for galaxy groups and clusters
• Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems
• The Most Massive Black Holes in the Universe: Effects of Mergers in Massive Galaxy Clusters
• The importance of preventive feedback: inference from observations of the stellar masses and metallicities of Milky Way dwarf galaxies
• Impact of astrophysical processes on the gamma-ray background from dark matter annihilations
• (No) dimming of X-ray clusters beyond z~1 at fixed mass: crude redhshifts and masses from raw X-ray and SZ data
• Fast Weak Lensing Simulations with Halo Model
• Testing Strict Hydrostatic Equilibrium in Simulated Clusters of Galaxies: Implications to Abell 1689
• SatGen -- II. Assessing the impact of a disc potential on subhalo populations
• Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations
• Critical spin periods of sub-km-sized cohesive rubble-pile asteroids: dependencies on material parameters
• The size evolution of galaxy discs formed within Lambda Cold Dark Matter haloes
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• Remapping dark matter halo catalogues between cosmological simulations
• Globular Cluster Formation from Colliding Substructure
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
• Virial shocks are suppressed in cosmic ray-dominated galaxy halos
• SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias
• Galaxy Formation in Heavily Overdense Regions at z~10: the Prevalence of Disks in Massive Halos
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• A Multi-frequency analysis of dark matter annihilation interpretations of recent anti-particle and gamma-ray excesses in cosmic structures
• Cosmological shock waves: clues to the formation history of haloes
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• On the algorithms of radiative cooling in semi-analytic models
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• Massive elliptical galaxies : From cores to haloes
• Constraining the substructure of dark matter haloes with galaxy-galaxy lensing
• Scale Radii and Aggregation Histories of Dark Haloes
• Dissecting Galaxy Formation: II. Comparing Substructure in Pure Dark Matter and Baryonic Models
• Cosmology dependence of galaxy cluster scaling relations
• Halo Exclusion Criteria Impacts Halo Statistics
• On Physical Scales of Dark Matter Halos
• Radio Point Sources and the Thermal SZ Power Spectrum
• The Influence of Concentration and Dynamical State on Scatter in the Galaxy Cluster Mass-Temperature Relation
• Highly-Ionized Oxygen Absorbers in the Intergalactic Medium
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• The Sheet of Giants: Unusual Properties of the Milky Way's Immediate Neighbourhood
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• Mapping Compound Cosmic Telescopes Containing Multiple, Projected Cluster-Scale Halos
• The imprint of dark matter haloes on the size and velocity dispersion evolution of early-type galaxies
• Relative velocity of dark matter and barions in clusters of galaxies and measurements of their peculiar velocities
• The Global Star-Formation Law by Supernova Feedback
• The void halo mass function: a promising probe of neutrino mass
• Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Modeling star formation in dwarf spheroidal galaxies: a case for extended dark matter halos
• Cosmology with the pairwise kinematic SZ effect: Calibration and validation using hydrodynamical simulations
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Computational Cosmology: from the Early Universe to the Large Scale Structure
• Where are the Cosmic Metals at z~3?
• Shapes of Milky-Way-Mass Galaxies with Self-Interacting Dark Matter
• A LABOCA survey of submillimeter galaxies behind galaxy clusters
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Mass Variance from Archival X-ray Properties of Dark Energy Survey Year-1 Galaxy Clusters
• A model of spectral line broadening in signal forecasts for line-intensity mapping experiments
• One Thousand and One Clusters: Measuring the Bulk Flow with the Planck ESZ and X-Ray Selected Galaxy Cluster Catalogs
• On the dynamics of the satellite galaxies in NGC 5044
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
• The correlation function of X-ray galaxy clusters in the RASS1 Bright Sample
• Gravitational lens candidates in the E-CDFS
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Dark Matter in Astrophysics/Cosmology
• Effects of the halo concentration distribution on strong-lensing optical depth and X-ray emission
• First measurement of the characteristic depletion radius of dark matter haloes from weak lensing
• Can Virialization Shocks be Detected Around Galaxy Clusters Through the Sunyaev-Zel'dovich Effect?
• 21-cm observations and warm dark matter models
• Soliton Merger Rates and Enhanced Axion Dark Matter Decay
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• Heating of the Hot Intergalactic Medium by Powerful Radio Galaxies and Associated High Energy Gamma-Ray Emission
• The halo light cone catalogues of \Abacus{AbacusSummit}
• Improved Mixed Dark Matter Halo Model for Ultralight Axions
• Predictions of the causal entropic principle for environmental conditions of the universe
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• Properties of Wide-separation Lensed Quasars by Clusters of Galaxies in the SDSS
• Some assembly required: assembly bias in massive dark matter halos
• Moderate Steepening of Galaxy Cluster Dark Matter Profiles by Baryonic Pinching
• On the evolution of cluster scaling relations
• Friends-of-Friends Groups and Clusters in the 2SLAQ Catalogue
• Clues on Regularity in the Structure and Kinematics of Elliptical Galaxies from Self-consistent Hydrodynamical Simulations: the Dynamical Fundamental Plane
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Joint X-Ray and Optical Measurements of the Mass Distribution of the Distant Galaxy Cluster CLJ 0152.7-1357
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• What to expect from dynamical modelling of cluster haloes II. Investigating dynamical state indicators with Random Forest
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Characteristic density contrasts in the evolution of superclusters. The case of A2142 supercluster
• The giant arc statistics in the three year WMAP cosmological model
• LoCuSS: The splashback radius of massive galaxy clusters and its dependence on cluster merger history
• Lyalpha heating and its impact on early structure formation
• Measuring the Cosmic Equation of State with Galaxy Clusters in the DEEP2 Redshift Survey
• Using the Topology of Large Scale Structure to constrain Dark Energy
• The galaxy-halo size relation of low-mass galaxies in FIRE
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• Cluster counts: calibration issue or new physics?
• Dianoga SIDM: galaxy cluster self-interacting dark matter simulations
• The connection between the host halo and the satellite galaxies of the Milky Way
• Dynamical signatures of infall around galaxy clusters: a generalized Jeans equation
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• The global mass - to - light ratio of SLACS lenses
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• Signatures of Cosmic Reionization on the 21cm 2- and 3-point Correlation Function I: Quadratic Bias Modeling
• OVI Traces Photoionized Streams With Collisionally Ionized Boundaries in Cosmological Simulations of $z\sim 1$ Massive Galaxies
• From the core to the outskirts: structure analysis of three massive galaxy clusters
• Troubled cosmic flows: turbulence, enstrophy and helicity from the assembly history of the intracluster medium
• SZ polarisation as a probe of the intracluster medium
• Alone on a wide wide sea. The origin of SECCO 1, an isolated star-forming gas cloud in the Virgo cluster
• The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters
• Strongly lensed cluster substructures are not in tension with $\Lambda$CDM
• Massive relic galaxies prefer dense environments
• Is MS1054-03 an exceptional cluster? A new investigation of ROSAT/HRI X-ray data
• Dark Matter in Elliptical Galaxies
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• Milky Way-est: Cosmological Zoom-in Simulations with Large Magellanic Cloud and Gaia-Sausage-Enceladus Analogs
• Photometric Mass Estimation and the Stellar Mass-Halo Mass Relation for Low Mass Galaxies
• The Dark Matter Haloes of Chandra X-ray Galaxy Clusters and Baryons Effect
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Phase-space shapes of clusters and rich groups of galaxies
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• Numerical convergence of physical variables in hydrodynamical simulations of cooling clusters
• Observational Measures of Halo Properties Beyond Mass
• Accuracy of Mesh Based Cosmological Hydrocodes: Tests and Corrections
• The detection of sub-solar mass dark matter halos
• Clues on the Physical Origin of the Fundamental Plane from Self-consistent Hydrodynamical Simulations
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) V: The Virial Temperature Does Not Describe Gas in a Virialized Galaxy Halo
• The 21-cm forest as a simultaneous probe of dark matter and cosmic heating history
• Observing the First Stars and Black Holes
• Halo based reconstruction of the cosmic mass density field
• Into the Lyα jungle: exploring the circumgalactic medium of galaxies at z ~ 4-5 with MUSE
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Physical evolution of dark matter halo around the depletion boundary
• 21 cm Forest Constraints on Primordial Black Holes
• Fragmentation in Dusty Low-Metallicity Star Forming Halos
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Possibilities and Limitations of Kinematically Identifying Stars from Accreted Ultra-Faint Dwarf Galaxies
• Systematic uncertainties from halo asphericity in dark matter searches
• X-ray Measurement of Dark Matter "Temperature" in Abell 1795
• Is it possible to tell the difference between fermionic and bosonic hot dark matter?
• Weak lensing peak count as a probe of f(R) theories
• Beyond Ultra-diffuse Galaxies. I. Mass--Size Outliers among the Satellites of Milky Way Analogs
• Multipolar moments of weak lensing signal around clusters. Weighing filaments in harmonic space
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• Dark Matter-baryon segregation in the non-linear evolution of coupled Dark Energy model
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• Two phase galaxy formation: The Gas Content of Normal Galaxies
• Where can we really find the First Stars' Remnants today?
• Perturbation theory with dispersion and higher cumulants: non-linear regime
• Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories
• Cosmological Implications of the Fundamental Relations of X-ray Clusters
• What galaxy masses perturb the local cosmic expansion?
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations
• The Effect of Galactic Feedback on Gas Accretion and Wind Recycling
• Kinematics of the OVI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
• The Three Hundred project: Galaxy groups do not survive cluster infall
• The neutral hydrogen distribution in large-scale haloes from 21-cm intensity maps
• Hydrostatic equilibrium profiles for gas in elliptical galaxies
• The evolution of dwarf galaxy satellites with different dark matter density profiles in the ErisMod simulations. I. The early infalls
• SZ and X-ray combined analysis of a distant galaxy cluster, RX J2228+2037
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• The Shape of Galaxy Cluster Dark Matter Haloes: Systematics of Its Imprint on Cluster Gas, and Comparison to Observations
• The peculiar velocities of satellites of external disk galaxies
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Tidal disruption events can power the observed AGN in dwarf galaxies
• Practical Cosmology with Lenses
• GalWeight: A New and Effective Weighting Technique for Determining Galaxy Cluster and Group Membership
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• How identifying circumgalactic gas by line-of-sight velocity instead of the location in 3D space affects O VI measurements
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• The concentration-velocity dispersion relation in galaxy groups
• Cold accretion in early galaxy formation and its Lyman-alpha signatures
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• The Effect of Thermal Velocities on Structure Formation in N-body Simulations of Warm Dark Matter
• Modelling the asymmetry of the halo cross-correlation function with relativistic effects at quasi-linear scales
• Halo orbits in cosmological disk galaxies: tracers of formation history
• The AGORA High-resolution Galaxy Simulations Comparison Project. V: Satellite Galaxy Populations In A Cosmological Zoom-in Simulation of A Milky Way-mass Halo
• Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• A determination of dark matter bispectrum with a large set of N-body simulations
• The Effect of Radiative Cooling on the Sunyaev-Zel'dovich Cluster Counts and Angular Power Spectrum: Analytic Treatment
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Evaluating Galaxy Dynamical Masses From Kinematics and Jeans Equilibrium in Simulations
• The In-situ Origins of Dwarf Stellar Outskirts in FIRE-2
• Effects of Baryon Mass Loss on Profiles of Large Galactic Dark Matter Haloes
• Observing Merger Trees in a New Light
• Determine the galaxy bias factors on large scales using bispectrum method
• Study of gravitational fields and globular cluster systems of early-type galaxies
• Diffuse gamma-ray background and cosmic-ray positrons from annihilating dark matter
• Detecting low-mass haloes with strong gravitational lensing II: constraints on the density profiles of two detected subhaloes
• A simple model for the evolution of super-massive black holes and the quasar population
• A theoretical study of the luminosity temperature relation for clusters of galaxies
• The Variation of Gas Mass Distribution in Galaxy Clusters: Effects of Preheating and Shocks
• Galaxy cluster luminosities and colours, and their dependence on cluster mass and merger state
• Insights into the origin of halo mass profiles from machine learning
• Tracing stars in Milky Way satellites with A-SLOTH
• $\gamma$-ray and $\nu$ searches for dark matter subhalos in the Milky Way with a baryonic potential
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Orbital distribution of infalling satellite halos across cosmic time
• The thermalisation of massive galaxy clusters
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• AGN Jet Power, Formation of X-ray Cavities, and FR I/II Dichotomy in Galaxy Clusters
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail
• The anatomy of the NGC 5044 group - I. Group membership and dynamics
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Groups of Galaxies in AEGIS: The 200 ksec Chandra Extended X-ray Source catalogue
• The trajectories of galaxies in groups: mass loss and preprocessing
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos
• Anisotropic q-Gaussian velocity distributions in LambdaCDM halos
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• 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
• An Accurate Analytic Model for the Thermal Sunyaev-Zel'dovich One-Point PDF
• The First Compact Objects in the $\Lambda$-dominated Universe
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• An emission map of the disk-circumgalactic medium transition in starburst IRAS 08339+6517
• Renormalisation of linear halo bias in N-body simulations
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• Constraining the primordial curvature perturbation using dark matter substructure
• Reignited star formation in dwarf galaxies quenched during reionization
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• Lyα Halos around [O III]-Selected Galaxies in HETDEX
• Sizing from the Smallest Scales: The Mass of the Milky Way
• The Cosmic Ultraviolet Baryon Survey (CUBS) II: Discovery of an H${}_2$-Bearing DLA in the Vicinity of an Early-Type Galaxy at z = 0.576
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• Direct-collapse black hole formation induced by internal radiation of host halos
• X-ray Constraints on Galaxy-Gas-Jet Interactions in the Dumbbell Galaxies NGC4782 and NGC4783 in the LGG316 Group
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Characterizing the Circumgalactic Medium of the Lowest-Mass Galaxies: A Case Study of IC 1613
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• Backlighting extended gas halos around luminous red galaxies: kinematic Sunyaev-Zel'dovich effect from DESI Y1 x ACT
• On the growth of supermassive black holes formed from the gravitational collapse of fermionic dark matter cores
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• Mass accretion rates of clusters of galaxies: CIRS and HeCS
• Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription
• Tangential Velocity of the Dark Matter in the Bullet Cluster from Precise Lensed Image Redshifts
• Evolution of subhalo orbits in a smoothly-growing host halo potential
• On the Probability Distribution of Cosmological Microlensing Optical Depths
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• Phase spirals in cosmological simulations of Milky Way-size galaxies
• Modeling Redshift-Space Clustering with Abundance Matching
• The abundance of dark matter haloes down to Earth mass
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• Virial halo mass function in the $Planck$ cosmology
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• The Effect of Formation Redshifts on the Cluster Mass-Temperature Relation
• Dynamics of Stellar Disk Tilting from Satellite Mergers
• Observing H2 Emission in Forming Galaxies
• Spin and structural halo properties at high redshift in a LCDM Universe
• Mass of clusters in simulations
• The galaxy - halo connection in low mass halos
• A Subgrid Turbulent Mean Field Dynamo Model for Cosmological Galaxy Formation Simulations
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Entrainment of Hot Gas into Cold Streams: The Origin of Excessive Star-formation Rates at Cosmic Noon
• HIR4: cosmology from a simulated neutral hydrogen full sky using Horizon Run 4
• The Universal Specific Merger Rate of Dark Matter Halos
• Cosmic rays, lithium abundance and excess entropy in galaxy clusters
• Strong Evolution in the Luminosity-Velocity Relation at z>1?
• A Long Stream of Metal-Poor Cool Gas around a Massive Starburst Galaxy at z = 2.67
• Can radiative cooling and nongravitational heating explain simultaneously the global X-ray properties of clusters and the unresolved cosmic X-ray background ?
• Internal dark matter structure of the most massive galaxy clusters
• The time-scales of major mergers from simulations of isolated binary galaxy collisions
• Stacking weak lensing signals of SZ clusters to constrain cluster physics
• Constraints on ${\Omega }_{\mathrm{m}}$ and ${\sigma }_8$ from the potential-based cluster temperature function
• Superclusters with thermal SZ effect surveys
• Validity of strong lensing statistics for constraints on the galaxy evolution model
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• The X-ray Luminosity Function of Nearby Rich and Poor Clusters of Galaxies: A Cosmological Probe
• Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
• High-Entropy Polar Regions Around the First Protostars
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Extraction of cluster parameters with future Sunyaev-Zel'dovich observations
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• Discriminating power of milli-lensing observations for dark matter models
• Multiple regimes and coalescence timescales for massive black hole pairs ; the critical role of galaxy formation physics
• Closing up the cluster tension?
• On the choice of the most suitable indicator for the assembly state of dark matter haloes through cosmic time
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• Radial structure, inflow & central mass of stationary radiative galaxy clusters
• Evidence for new physics from clusters ?
• Dust attenuation in galaxies at cosmic dawn from the FirstLight simulations
• An improved prescription for merger time-scales from controlled simulations
• Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
• The outermost edges of the Milky Way halo from galaxy kinematics
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Analytical approach to core-halo structure of fuzzy dark matter
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Galaxy Bulge Formation: Interplay with Dark Matter Halo and Central Supermassive Black Hole
• Massive galaxy clusters as gravitational telescopes for distant supernovae
• Replacing dark energy by silent virialisation
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• Disentangling the multi-phase circumgalactic medium shared between a dwarf and a massive star-forming galaxy at z~0.4
• An Accurate Comprehensive Approach to Substructure: I. Accreted Subhaloes
• Mass estimation in the outer non-equilibrium region of galaxy clusters
• Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy
• Clusters of galaxies: setting the stage
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• Light or heavy supermassive black hole seeds: the role of internal rotation in the fate of supermassive stars
• Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey
• Transient Weak-Lensing by Cosmological Dark Matter Microhaloes
• Culminating the peak CUSP to descry the dark side of halos
• Accurate mass estimates from the proper motions of dispersion-supported galaxies
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• Clumpiness enhancement of charged cosmic rays from dark matter annihilation with Sommerfeld effect
• Primordial magnetic fields with X-ray and S-Z cluster survey
• Probing gaseous galactic halos through the rotational kSZ effect
• Implications of Halo Inside-out Growth on the X-Ray Properties of Nearby Galaxy Systems within the Preheating Scenario
• The Impact of Molecular Hydrogen Cooling on the Galaxy Formation Threshold
• Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
• Galactic satellite systems in CDM, WDM and SIDM
• The XMM Cluster Survey: evolution of the velocity dispersion -- temperature relation over half a Hubble time
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• Where are the missing baryons in clusters?
• Cuspy dark matter density profiles in massive dwarf galaxies
• Hierarchical Structure Formation and Chemical Evolution of Galaxies
• A universal angular momentum profile for dark matter haloes
• Impact of thermal diffusion and other abundance anomalies on cosmological uses of galaxy clusters
• Toward a Physical Understanding of Galaxy-Halo Alignment
• Constraining cluster masses from the stacked phase space distribution at large radii
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• Properties of galaxy halos in Clusters and Voids
• SIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations
• Diagnostics of Baryonic Cooling in Lensing Galaxies
• Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling
• A New Dynamical Mass Measurement for the Virgo Cluster using the Radial Velocity Profile of the Filament Galaxies
• Galaxy And Mass Assembly (GAMA): The group HI mass as a function of halo mass
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
• A census of dwarf galaxy satellites around LMC-mass galaxy NGC 2403
• SASHIMI-SIDM: Semi-analytical subhalo modelling for self-interacting dark matter at sub-galactic scales
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• ICM properties and AGN distribution in high-z RCS clusters
• Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts
• Constraining the Minimum Luminosity of High Redshift Galaxies through Gravitational Lensing
• On the Origin of the Rotation Curves of Dark-Matter-Dominated Galaxies
• Cluster abundance and large scale structure
• Distribution of Dust around Galaxies: An Analytic Model
• Expectations for SZ cluster counts: mass function versus X-ray luminosity function
• CARMA follow-up of the northern unconfirmed PLANCK galaxy cluster candidates
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• Evolution of CIV Absorbers. II. Where does CIV live?
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Predicting the clustering properties of galaxy clusters detectable for the Planck satellite
• Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect
• CLUES about M33: the reversed radial stellar age gradient in the outskirts of Triangulum galaxy
• Beacons In the Dark: Using Novae and Supernovae to Detect Dwarf Galaxies in the Local Universe
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Mass Dependence of Galaxy-Halo Alignment in LOWZ and CMASS
• A Spectroscopic Census of X-ray Systems in the COSMOS Field
• Smooth Boundaries to Cosmological HII Regions from Galaxy Clustering
• The Past History of Galaxy Clusters told by their present neighbors
• Statistical properties of substructures around Milky Way-sized haloes and their implications for the formation of stellar streams
• Contribution of Radio Halos to the Foreground for SKA EoR Experiments
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• The virialization density of peaks with general density profiles under spherical collapse
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• A Two-Parameter Matching Scheme for Massive Galaxies and Dark Matter Haloes
• Constraints on the winds of hot subdwarf stars from X-ray observations of two sdB binaries with compact companions: CD -30 11223 and PG 1232-136
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic survey. II. Morphology, Color and Size Dependences of the Stellar-halo Mass Relation for Massive Galaxies
• The spherical collapse model with shell crossing
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Modification of the halo mass function by kurtosis associated with primordial non-Gaussianity
• Relating galaxies across different redshift to study galaxy evolution
• Serendipitous XMM-Newton discovery of a cluster of galaxies at z=0.28
• The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
• Gas mass fraction from XMM-Newton and Chandra high redshift clusters and its use as a cosmological test
• Halo Concentrations and the New Baseline X-ray Luminosity-Temperature and Mass Relations of Galaxy Clusters
• The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
• The ecology of dark matter haloes I: The rates and types of halo interactions
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• VIMOS-VLT Integral Field Kinematics of the Giant Low Surface Brightness Galaxy ESO 323-G064
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• X-ray galaxy clusters abundance and mass temperature scaling
• Remapping simulated halo catalogues in redshift space
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Extended Press-Schechter theory and the density profiles of dark matter haloes
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Can the splashback radius be an observable boundary of galaxy clusters?
• High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• Cosmology with Galaxy Cluster Properties using Machine Learning
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
• Impacts of Source Properties on Strong Lensing by Rich Galaxy Clusters
• An Accurate Comprehensive Approach to Substructure: III. Masses and Formation Times of the Host Haloes
• Do Bound Structures Brake Cosmic Acceleration?
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Sunyaev-Zel'dovich scaling relations from a simple phenomenological model for galaxy clusters
• Inferring dark matter halo properties for HI-selected galaxies
• Constraining Intra-cluster Gas Models with AMiBA13
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• A new test for the stable clustering hypothesis
• Suzaku Measurements of Hot Halo Emission at Outskirts for Two Poor Galaxy Groups: NGC 3402 and NGC 5129
• Kinematic effect in gravitational lensing by clusters of galaxies
• Excess entropy and energy feedback from within cluster cores up to r${}_{200}$
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• XMM-Newton observation of the cluster ZW 1305.4+2941 in the field SA 57
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• Unifying static analysis of gravitational structures with a scale-dependent scalar field gravity as an alternative to dark matter
• On the phase-space structure of galaxy clusters from cosmological simulations
• Collisional interaction limits between dark matters and baryons in `cooling flow' clusters
• Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
• Cosmological constraints from a 2D SZ catalog
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Line-of-sight Elongation and Hydrostatic Mass Bias of the Frontier Fields Galaxy Cluster Abell 370
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• Dark matter halos and the M-σrelation for supermassive black holes
• An Accurate Comprehensive Approach to Substructure: II. Stripped Subhaloes
• Beyond Ultra-diffuse Galaxies. II. Environmental Quenching of Mass-Size Outliers among the Satellites of Milky Way Analogs
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• 2-D Magnetohydrodynamic Simulations of Induced Plasma Dynamics in the Near-Core Region of a Galaxy Cluster
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• An Evolving Entropy Floor in the Intracluster Gas?
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Cross-correlation between the soft X-ray background and SZ Sky
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• On the coldness of the local Hubble flow: the role of baryons
• Optical inverse-Compton emission from clusters of galaxies
• Cosmological test of local position invariance from the asymmetric galaxy clustering
• Joint Strong and Weak Lensing Analysis of the Massive Cluster Field J0850+3604
• Strong lensing by subhalos in the dwarf-galaxy mass range I: Image separations
• Evidence for line-of-sight structure in a comparison of X-ray and optical observations of the high-redshift cluster RCS043938-2904.7
• Constraints on structure formation models from Sunyaev-Zel'dovich Effect
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• Close Galaxy Pairs at z = 3: A Challenge to UV Luminosity Abundance Matching
• Exploring galaxy dark matter halos across redshifts with strong quasar absorbers
• Ultra-fine dark matter structure in the Solar neighbourhood
• A simple analytical model for the abundance of damped Ly-αabsorbers
• Modeling the core-halo mass relation in fuzzy dark matter halos
• GalRotpy: an educational tool to understand and parametrize the rotation curve and gravitational potential of disk-like galaxies
• Spiral galaxies rotation curves in the Horava - Lifshitz gravity theory
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Can electron distribution functions be derived through the Sunyaev-Zel'dovich effect?
• Detecting First Star Lyman-$\alpha$ Spheres through Gravitational Telescopes
• Highly-magnified, Multiply-imaged radio counterparts of the Sub-mm Starburst Emission in the Cluster-Lens MS0451.6-0305
• Bracketing the soliton-halo relation of ultralight dark matter
• The Chemical Evolution of Very Metal-Poor Damped Lyman-$\alpha$ Systems
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Heating of X-Ray Hot Gas in Groups by Blast Waves
• CLMM: a LSST-DESC Cluster weak Lensing Mass Modeling library for cosmology
• The Structure of Cold Dark Matter Halos: Recent Insights from High Resolution Simulations
• Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
• Correlations of the feedback energy and BCG radio luminosity in galaxy clusters
• Quantification of the multi-streaming effect in Redshift Space Distortion
• A Random Walk Model for Dark Matter Halo Concentrations
• Haloes at the ragged edge: The importance of the splashback radius
• The Effects of Linear Matter Power Spectrum Enhancement on Dark Matter Substructure
• Optimizing the yield of Sunyaev-Zel'dovich cluster surveys
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
• Stochastic Model of the Spin Distribution of Dark Matter Halos
• Mass accretion rates of the HectoMAP clusters of galaxies
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Steady-state conduction-driven temperature profile in clusters of galaxies
• Profiles of dark-matter haloes at high redshift
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• A break in the high-redshift stellar mass Tully-Fisher relation
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• A Cluster of Galaxies hiding behind M31: XMM-Newton observations of RX J0046.4+4204
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster
• Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
• Evolution of Low Mass Galactic Subhalos and Dependence on Concentration
• The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
• A public grid of radiative transfer simulations for Lyman-alpha and metal lines in idealised galactic outflows
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• Strong Lensing In The Inner Halo Of Galaxy Clusters
• Angular momentum in cluster Spherical Collapse Model
• Intracluster gas pressure, entropy injection and redshift evolution
• The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
• Fitting functions for a disk-galaxy model with different LCDM-halo profiles
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Exploring the role of cosmological shock waves in the Dianoga simulations of galaxy clusters
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• How complex is the cosmic web?
• COZMIC. II. Cosmological Zoom-in Simulations with Fractional non-CDM Initial Conditions
• Improvements in the M-T relation and mass function and the measured Omega_m through clusters evolution
• Autocorrelation function of the soft X-ray background produced by warm-hot gas in dark halos
• Machine Learning Etudes in Astrophysics: Selection Functions for Mock Cluster Catalogs
• The effect of finite halo size on the clustering of neutral hydrogen
• Massive Galaxies at High-z: Assembly Patterns, Structure & Dynamics in the Fast Phase of Galaxy Formation
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Semi-analytical frameworks for subhalos from the smallest to the largest scale
• Halo Profile Evolution and Velocity Bias
• Cosmic accretion shocks as a tool to measure the dark matter mass of galaxy clusters
• Scaling relations of clusters and groups, and their evolution
• Measuring the Hubble constant through the galaxy pairwise peculiar velocity
• Mass - concentration relation and weak lensing peak counts
• COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions
• Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• The size function of massive satellites from the $R_e-R_h$ and $M_{star}-M_h$ relations: constraining the role of environment
• The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
• Entropy of the intracluster medium at high redshift
• Living with Neighbors. IV. Dissecting the Spin$-$Orbit Alignment of Dark Matter Halos: Interacting Neighbors and the Local Large-scale Structure
• "Observing" Unrelaxed Clusters in Dark Matter Simulations
• Baryon Pasting the Uchuu Lightcone Simulation
• Angular momentum loss of primordial gas in Lyman-alpha radiation field
• Influence of AGN Outbursts on the Surrounding Galaxies
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Einasto profile as the halo model solution coupled to the depletion radius
• The Contribution of EUV from Clusters of Galaxies to the Cosmic Ionizing Background
• Morphological Redshift Estimates for Galaxy Clusters in a Sunyaev-Zel'dovich Effect Survey
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• A large thermal energy reservoir in the nascent intracluster medium at a redshift of 4.3
• 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
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Nucleation regions in the Large-Scale Structure I. A catalogue of cores in nearby rich superclusters
• RXJ0256.5+0006: a merging cluster of galaxies at z=0.36 observed with XMM-Newton
• The information on halo properties contained in spectroscopic observations of late-type galaxies
• Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• Accurate halo mass functions from the simplest excursion set theory
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Cluster mass estimation through Fair Galaxies
• Spin transfer from dark matter to gas during halo formation
• Kinematic scaling relations of disc galaxies from ionised gas at $z\sim 1$ and their connection with dark matter haloes
• Measuring neutrino mass and asymmetry with matter pairwise velocities
• Simulation-based marginal likelihood for cluster strong lensing cosmology
• Can QCD Axion Stars explain Subaru HSC microlensing?
• The eventful life journey of galaxy clusters. I. Impact of DM halo and ICM properties on their full assembly histories
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Dark matter model favoured by reionization data: 7 keV sterile neutrino vs cold dark matter
• Gravitational wave lensing: probing Fuzzy Dark Matter with LISA
• Heating of the intracluster medium by buoyant bubbles and sound waves
• Angular momentum - mass relation for dark matter haloes
• Halo Concentrations and the Fundamental Plane of Galaxy Clusters
• Improved Halo Model Calibrations for Mixed Dark Matter Models of Ultralight Axions
• The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at $1<z<5$
• Evolution of dwarf galaxy observable parameters
• Massive Black Hole Mergers
• Discovery of a damped Ly$\alpha$ absorber originating in a spectacular interacting dwarf galaxy pair at $z=0.026$
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• Cluster outskirts and their connection to the cosmic web
• Kinematics of Circumgalactic O VI Gas and Disk Rotation of $z\approx 0.2$ Star-forming Galaxies
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Dynamical friction in rotating ultralight dark matter galactic cores
• Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters
• Improving lensing cluster mass estimate with flexion
• Semi analytical description of formation of galaxies and clusters of galaxies
• A full reconstruction of two galaxy clusters intra-cluster medium with strong gravitational lensing
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• Cooling and Clusters: When Is Heating Needed?
• The Generation of Magnetic Fields and X-ray Observations
• Hermeian haloes: extreme objects with two interactions in the past
• Lagrangian Volume Deformations around Simulated Galaxies
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Galaxy cluster mass bias from projected mass maps: The Three Hundred-NIKA2 LPSZ twin samples
• Halo Properties from Observable Measures of Environment: I. Halo and Subhalo Masses
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• Cosmological perturbation theory for large scale structure in phase space
• Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Testing for evolution in scaling relations of galaxy clusters: Cross analysis between X-ray and SZ observations
• Effects of Formation Epoch Distribution on X-Ray Luminosity and Temperature Functions of Galaxy Clusters
• The imprints of galaxy cluster internal dynamics on the Sunyaev-Zeldovich effect
• Strong Evidence for Cosmic Ray-Supported $\sim$L${}^{\ast }$ Galaxy Halos via X-ray \& tSZ Constraints
• Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals
• A graph model for the clustering of dark matter halos
• CLASH-VLT: The variance in the velocity anisotropy profiles of galaxy clusters
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Diversity of the Lyman continuum escape fractions of high-$z$ galaxies and its origins
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• An implementation of nDGP gravity in Pinocchio
• Mass function and assembly of dark halos: an approach to inventory isolated overdense regions in random fields
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• Metamorphosis of dwarf halo density profile under dark matter decays
• Contamination of Cluster Radio Sources in the Measurement of the Thermal Sunyaev-Zel'dovich Angular Power Spectrum
• Testing an entropy estimator related to the dynamical state of galaxy clusters
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Semianalytic model for decaying dark matter halos
• Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
• Estimating the evolution of gas in the Fornax dwarf spheroidal galaxy from its star formation history: an illustrative example
• On the spin distributions of $\Lambda$CDM haloes
• Selection Function of Clusters in Dark Energy Survey Year 3 Data from Cross-Matching with South Pole Telescope Detections
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• Evolution of the degree of substructures in simulated galaxy clusters
• A feedback compression star formation model and the black hole - bulge relations
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• Segue 2 Recently Collided with the Cetus-Palca Stream: New Opportunities to Constrain Dark Matter in an Ultra-Faint Dwarf
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• The largest virialized dark halo in the universe
• The distribution of lenticular galaxies in the phase space of present-day galaxy cluster regions
• The dynamical evolution of the stellar clumps in the Sparkler galaxy
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• The Complexity and Information Content of Simulated Universes
• Machine Learning the Dark Matter Halo Mass of Milky Way-Like Systems
• COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS
• Timing Mass of the Local Group
• Layered dark structure with a Structuring Field: A $Z_4$-symmetric Inert Doublet-Singlet realization and implications for the $S_8$ tension
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Photometric Objects Around Cosmic Webs (PAC). VI. High Satellite Fraction of Quasars
• MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of $z\sim 1$ star-forming galaxies
• The Formation of Dwarf Galaxy Disks
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter
• MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• An Accurate Comprehensive Approach to Substructure: IV. Dynamical Friction
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: II. dwarf spheroidal galaxy
• Morphology of dark matter haloes beyond triaxiality
• A hierarchical clustering method for quantifying satellite abundance
• Constraining cosmic ray transport models using circumgalactic medium properties and observables
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• The mass profile of NGC 3377 from a Bayesian approach
• Cosmological Implications of Galaxy Clusters in X-Ray, Millimeter, and Submillimeter Bands
• The Role of Mass and Environment on Satellite distributions around Milky Way analogs in the Romulus25 simulation
• On the virialization threshold for halo mass functions
• On the Size Evolution of a Galactic Disk in Hierarchical Merging of Cold Dark Matter Halos
• Radial Transport in High-Redshift Disk Galaxies Dominated by Inflowing Streams
• Observed versus Simulated Halo c-Mvir Relations
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
• AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
• Studying the gaseous outskirts of galaxy groups with coherent Ly alpha absorption patterns
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales
• Timing the last major merger of galaxy clusters with large halo sparsity
• The halo finding problem revisited: a deep revision of the ASOHF code
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Internal dark matter structure of the most massive galaxy clusters since redshift 1
• Cosmological constraints from clustering properties of galaxy clusters
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• Revisiting the relation between the number of globular clusters and galaxy mass for low mass galaxies
• Warm, not Fuzzy: Generalized Ultralight Dark Matter Limits from Milky Way Satellites
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
• Scaling Relations in the Phase-Space Structure of Dark Matter Haloes
• The orbital dynamics of the LMC and SMC about the Milky Way
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• The signature of major mergers on the hydrostatic mass bias of galaxy clusters
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Analysis of shape and angular orientation parameters of velocity-dependent dark matter annihilation signals in Galactic Centers for FIRE simulations
• The life and times of dark matter haloes: what will I be when I grow up?
• Super Interacting Dark Sector: An Improvement on Self-Interacting Dark Matter via Scaling Relations of Galaxy Clusters
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• A redshift distortion free correlation function at third order in the nonlinear regime
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• The eventful life journey of galaxy clusters. II. Impact of mass accretion on the thermodynamical structure of the ICM
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\mathrm{X}}$--$T$ relation of early-type galaxies
• The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• Mapping the z>=5 SiIV Column Density Distribution onto the Galaxy Stellar Mass Function Using the Cumulative Absorption Cross Section
• Testing subhalo abundance matching with galaxy kinematics
• Cylindrical cosmological simulations with StePS
• Gravitational collapse and non-self similarity in the L-T relation
• Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies
• Panchromatic Studies of Distant Clusters of Galaxies
• Luminosity-Temperature Relation as a Probe for Modified Gravity
• 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