Populating a cluster of galaxies - I. Results at z=0

Abstract

We simulate the assembly of a massive rich cluster and the formation of its constituent galaxies in a flat, low-density universe. Our most accurate model follows the collapse, the star-formation history and the orbital motion of all galaxies more luminous than the Fornax dwarf spheroidal, while dark halo structure is tracked consistently throughout the cluster for all galaxies more luminous than the SMC. Within its virial radius this model contains about 2.0e7 dark matter particles and almost 5000 distinct dynamically resolved galaxies. Simulations of this same cluster at a variety of resolutions allow us to check explicitly for numerical convergence both of the dark matter structures produced by our new parallel N-body and substructure identification codes, and of the galaxy populations produced by the phenomenological models we use to follow cooling, star formation, feedback and stellar aging. This baryonic modelling is tuned so that our simulations reproduce the observed properties of isolated spirals outside clusters. Without further parameter adjustment our simulations then produce a luminosity function, a mass-to-light ratio, luminosity, number and velocity dispersion profiles, and a morphology-radius relation which are similar to those observed in real clusters. In particular, since our simulations follow galaxy merging explicitly, we can demonstrate that it accounts quantitatively for the observed cluster population of bulges and elliptical galaxies.

28 pages, submitted to MNRAS

Cited by in corpus (2082)

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• Satellites of Simulated Galaxies: survival, merging, and their relation to the dark and stellar halos
• Velocity-dependent Self-interacting Dark Matter from Groups and Clusters of Galaxies
• Asymmetries in the inner regions of LCDM haloes
• Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$
• Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution
• Galaxy Shapes and Intrinsic Alignments in The MassiveBlack-II Simulation
• The Atacama Cosmology Telescope: Dynamical Masses and Scaling Relations for a Sample of Massive Sunyaev-Zel'dovich Effect Selected Galaxy Clusters
• Thermal conduction in cosmological SPH simulations
• The Impact of Galactic Feedback on the Circumgalactic Medium
• The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $\Lambda$CDM
• Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2
• Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
• On the puzzling plateau in the specific star formation rate at z=2-7
• Limitations to the "basic'' HOD model and beyond
• Galaxy Luminosity Functions from Deep Spectroscopic Samples of Rich Clusters
• Are peculiar velocity surveys competitive as a cosmological probe?
• Radiative Feedback from high mass X-ray binaries on the formation of the first galaxies and early reionization
• Star Formation and Metallicity Gradients in Semi-analytic Models of Disk Galaxy Formation
• Metal Enrichment of the ICM: a 3-D Picture of Chemical and Dynamical Properties
• The cosmic history of the spin of dark matter haloes within the large scale structure
• The origin of diverse $\alpha$-element abundances in galaxy discs
• The Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• The assembly of dusty galaxies at $z\ge 4$: statistical properties
• The Dynamical State and Mass-Concentration Relation of Galaxy Clusters
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• Anomalous Flux Ratios in Gravitational Lenses: For or Against CDM?
• The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
• On the nature of the Milky Way satellites
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: II. The clustering of quasars and their dark environment
• The link between galaxy and black hole growth in the EAGLE simulation
• The impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
• Cosmological simulation with dust formation and destruction
• The phase-space structure of a dark-matter halo: Implications for dark-matter direct detection experiments
• A census of cool core galaxy clusters in IllustrisTNG
• The fundamental plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
• Simulating the Formation of the Local Galaxy Population
• The Mass Assembly of Fossil Groups of Galaxies in the Millennium Simulation
• The evolution of substructure II: linking dynamics to environment
• Dark Matter Halo Growth II: Diffuse Accretion and its Environmental Dependence
• Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• The effect of baryons on the inner density profiles of rich clusters
• Dark Matter Subhaloes in Numerical Simulations
• Not too big, not too small: the dark halos of the dwarf spheroidals in the Milky Way
• Pressure of the hot gas in simulations of galaxy clusters
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors
• Strong lensing optical depths in a LCDM universe II: the influence of the stellar mass in galaxies
• The Effects of Photoionization on Galaxy Formation -- III: Environmental Dependence in the Luminosity Function
• Hunting for Galaxies and Halos in simulations with VELOCIraptor
• Gas cooling in simulations of the formation of the galaxy population
• The Growth in Size and Mass of Cluster Galaxies since z=2
• Revealing the galaxy-halo connection in IllustrisTNG
• RASS-SDSS Galaxy Cluster Survey. VII. On the Cluster Mass to Light ratio and the Halo Occupation Distribution
• The impact of baryonic processes on the two-point correlation functions of galaxies, subhaloes and matter
• The assembly bias of dark matter haloes to higher orders
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• The effect of magnetic fields on properties of the circumgalactic medium
• Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
• The relation between galaxy morphology and colour in the EAGLE simulation
• The Influence of Streaming Velocities on the Formation of the First Stars
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• The Abundance and Radial Distribution of Satellite Galaxies
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• The Source Density and Observability of Pair-Instability Supernovae from the First Stars
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• Elemental Abundances in Milky Way-like Galaxies from a Hierarchical Galaxy Formation Model
• Galaxy Formation Spanning Cosmic History
• Satellite Systems around Galaxies in Hydrodynamic Simulations
• The masses and metallicities of stellar haloes reflect galactic merger histories
• Galaxy Populations and Evolution in Clusters II: Defining Cluster Populations
• The Accuracy of Subhalo Detection
• Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration
• The influence of streaming velocities and Lyman-Werner radiation on the formation of the first stars
• Intracluster stellar population properties from N-body cosmological simulations -- I. Constraints at $z=0$
• The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with 3-point correlation functions
• The statistics of the subhalo abundance of dark matter haloes
• Gas-phase metallicity gradients of TNG50 star-forming galaxies
• Disruption of giant molecular clouds and formation of bound star clusters under the influence of momentum stellar feedback
• Kinematics of Simulated Galaxies I: Connecting Dynamical and Morphological Properties of Early-Type Galaxies at Different Redshifts
• The Link between Galactic Satellite Orbits and Subhalo Accretion
• Massive Close Pairs Measure Rapid Galaxy Assembly in Mergers at High Redshift
• The origin of failed subhaloes and the common mass scale of the Milky Way satellite galaxies
• Constrained simulations of the Local Group: on the radial distribution of substructures
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Alignment between galaxies and large-scale structure
• The core-cusp problem: a matter of perspective
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• The low-mass end of the baryonic Tully-Fisher relation
• The effect of minihaloes on cosmic reionization
• First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
• Subaru Weak-Lensing Survey of Dark Matter Subhalos in the Coma Cluster : Subhalo Mass Function and Statistical Properties
• Enhanced cluster lensing models with measured galaxy kinematics
• The mass assembly of galaxy groups and the evolution of the magnitude gap
• The First Galaxies: Assembly of Disks and Prospects for Direct Detection
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• Recovery from population III supernova explosions and the onset of second generation star formation
• \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities
• Origin of strong magnetic fields in Milky-Way like galactic haloes
• Are Great Disks Defined by Satellite Galaxies in Milky-Way Type Halos Rare in $\Lambda$CDM model?
• A model for the formation of stellar associations and clusters from giant molecular clouds
• Galaxy Cluster Mass Reconstruction Project: I. Methods and first results on galaxy-based techniques
• The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE
• Assembly Bias and Splashback in Galaxy Clusters
• Large-scale mass distribution in the Illustris simulation
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF
• First Simulations of Axion Minicluster Halos
• Orbital parameters of infalling satellite haloes in the hierarchical $\Lambda$CDM model
• Preheating by Previrialization and its Impact on Galaxy Formation
• Satellite abundances around bright isolated galaxies II: radial distribution and environmental effects
• On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
• Missing dark matter in dwarf galaxies?
• The rapid growth phase of supermassive black holes
• Satellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matter
• Environmental Dependence of Galaxy Merger Rate in ΛCDM Universe
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
• Constraints on the identity of the dark matter from strong gravitational lenses
• Composite Luminosity Functions Based on the Sloan Digital Sky Survey "Cut & Enhance" Galaxy Cluster Catalog
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Voids in the Simulated Local Universe
• Intrinsic alignments of galaxies in the MassiveBlack-II simulation: analysis of two-point statistics
• Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter
• The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• Dissecting and Modelling Galaxy Assembly Bias
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• Log-normal star formation histories in simulated and observed galaxies
• Comparing approximate methods for mock catalogues and covariance matrices I: correlation function
• Satellite Galaxies and Fossil Groups in the Millennium Simulation
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• Intrinsic alignments of galaxies in the EAGLE and cosmo-OWLS simulations
• Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
• A dynamical model of supernova feedback: gas outflows from the interstellar medium
• Ultra-diffuse galaxies in the Auriga simulations
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• Are mergers responsible for universal halo properties?
• The X-ray luminous galaxy cluster XMMU J1007.4+1237 at z=1.56 - The dawn of starburst activity in cluster cores
• The environmental dependence of gas accretion onto galaxies: quenching satellites through starvation
• The Aurora radiation-hydrodynamical simulations of reionization: calibration and first results
• Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
• How common is the Milky Way - satellite system alignment?
• Dwarf galaxy populations in present-day galaxy clusters: I. Abundances and red fractions
• Simulated Milky Way analogues: implications for dark matter indirect searches
• Substructure in lensing clusters and simulations
• Tracing Galaxies Through Cosmic Time with Number Density Selection
• Populations of filaments from the distribution of galaxies in numerical simulations
• A Systematic Analysis of Caustic Methods for Galaxy Cluster Masses
• Baryon Dynamics, Dark Matter Substructure, and Galaxies
• The First Galaxies: Assembly under Radiative Feedback from the First Stars
• The formation of low metallicity globular clusters in dwarf galaxy mergers
• How Rare is the Bullet Cluster?
• The inner structure of early-type galaxies in the Illustris simulation
• Dry Mergers: A Crucial Test for Galaxy Formation
• Mergers and the outside-in formation of dwarf spheroidals
• The Alignment between Satellites and Central Galaxies: Theory vs. Observations
• A Common Origin for Globular Clusters and Ultra-faint Dwarfs in Simulations of the First Galaxies
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• MultiDark-Galaxies: data release and first results
• Early Structure Formation and Reionization in a Cosmological Model with a Running Primordial Power Spectrum
• Self-Consistent Theory of Halo Mergers
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• Ram pressure stripping in a galaxy formation model. I. A novel numerical approach
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• Steep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 and the Implications for Reionisation
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• Galaxy mergers in EAGLE do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN
• Dynamical difference between the cD galaxy and the stellar diffuse component in simulated galaxy clusters
• How robust are predictions of galaxy clustering?
• The properties of "dark" ΛCDM halos in the Local Group
• The signature of substructure on gravitational lensing in the LCDM cosmological model
• Dust scaling relations in a cosmological simulation
• The tidal evolution of dark matter substructure -- II. The impact of artificial disruption on subhalo mass functions and radial profiles
• Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE project
• The build up of the correlation between halo spin and the large scale structure
• The Varied Fates of z~2 Star-forming Galaxies
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation
• The Evolution of Assembly Bias
• A comparison of observed and simulated absorption from HI, CIV, and SiIV around $z\approx 2$ star-forming galaxies suggests redshift-space distortions are due to inflows
• Major Mergers Going Notts: Challenges for Modern Halo Finders
• The XMM Cluster Survey: The interplay between the brightest cluster galaxy and the intra-cluster medium via AGN feedback
• The Clustering of Galaxies around Quasars
• Non-linear evolution of the cosmic neutrino background
• The statistical properties of LCDM halo formation
• Properties of the galaxy population in hydrodynamical simulations of clusters
• Times, environments and channels of bulge formation in a LambdaCDM cosmology
• Formation histories of stars, clusters and globular clusters in the E-MOSAICS simulations
• A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
• A z=2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments
• The separate and combined effects of baryon physics and neutrino free-streaming on large-scale structure
• Quenching star formation in cluster galaxies
• Universality of dark matter haloes shape over six decades in mass: Insights from the Millennium XXL and SBARBINE simulations
• Realistic simulations of gravitational lensing by galaxy clusters: extracting arc parameters from mock DUNE images
• The fate of disk galaxies in IllustrisTNG clusters
• Scaling relations and mass bias in hydrodynamical f(R) gravity simulations of galaxy clusters
• The impact of Early Dark Energy on non-linear structure formation
• SZE Observables, Pressure Profiles and Center Offsets in Magneticum Simulation Galaxy Clusters
• The Dynamics of Galaxy Pairs in a Cosmological Setting
• X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations
• Mass assembly of galaxies: Smooth accretion versus mergers
• The Onset of Gravothermal Core Collapse in Velocity Dependent Self-Interacting Dark Matter Subhaloes
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier
• Clarifying the effects of interacting dark energy on linear and nonlinear structure formation processes
• Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
• The distribution of gas in the Local Group from constrained cosmological simulations: the case for Andromeda and the Milky Way galaxies
• On the linearity of tracer bias around voids
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• First results from SMAUG: Uncovering the Origin of the Multiphase Circumgalactic Medium with a Comparative Analysis of Idealized and Cosmological Simulations
• The angular momentum of cold dark matter haloes with and without baryons
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• The fully connected N-dimensional skeleton: probing the evolution of the cosmic web
• The colors of satellite galaxies in the Illustris Simulation
• Velocity distributions in clusters of galaxies
• Effects of dynamical evolution on the distribution of substructures
• Weak Lensing Light-Cones in Modified Gravity simulations with and without Massive Neutrinos
• The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
• The Effect of Gravitational Recoil on Black Holes Forming in a Hierarchical Universe
• The nebular emission of star-forming galaxies in a hierarchical universe
• Globular Cluster Formation Within The Aquarius Simulation
• Subhalo destruction in the Apostle and Auriga simulations
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• Towards an understanding of the evolution of the scaling relations for supermassive black holes
• Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
• On the dynamical state of galaxy clusters: insights from cosmological simulations II
• On ths assembly history of stellar components in massive galaxies
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Quantifying Cosmic Superstructures
• Weighing neutrinos with cosmic neutral hydrogen
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• Constraining the Projected Radial Distribution of Galactic Satellites with the Sloan Digital Sky Survey
• The CAMELS project: public data release
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• The origin of dust in galaxies across cosmic time
• The origin of pseudobulges in cosmological simulations of galaxy formation
• GALICS -- VI. Modelling Hierarchical Galaxy Formation in Clusters
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Galaxy shapes and alignments in the MassiveBlack-II hydrodynamic and dark matter-only simulations
• Halo Shapes From Weak Lensing: The Impact of Galaxy--Halo Misalignment
• Peaks above the Maxwellian Sea: A New Approach to Finding Substructure in N-Body Haloes
• Probing recent star formation with absorption-line strengths in hierarchical models and observations
• Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses
• The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way
• Scaling relations of Fuzzy Dark Matter haloes I: individual systems in their cosmological environment
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• A semi-analytic model comparison - gas cooling and galaxy mergers
• Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
• The spin alignment of galaxies with the large-scale tidal field in hydrodynamic simulations
• Statistical properties of paired fixed fields
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• A Comparison of Galaxy Merger History Observations and Predictions from Semi-Analytic Models
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• Semi-analytic Simulations of Galactic Winds: Volume Filling Factor, Ejection of Metals and Parameter Study
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- I: Halo Gas Properties and the Role of SMBH Feedback
• The atomic Hydrogen content of the post-reionization Universe
• The 21cm bispectrum during reionization: a tracer of the ionization topology
• A Lightcone Catalogue from the Millennium-XXL Simulation
• Genetically modified halos: towards controlled experiments in $\Lambda$CDM galaxy formation
• Intrinsic alignments of disk and elliptical galaxies in the MassiveBlack-II and Illustris simulations
• The Edge of the Galaxy
• Numerical resolution limits on subhalo abundance matching
• The imprint of cosmic reionisation on the luminosity function of galaxies
• Secondary Infall and the Pseudo-Phase-Space Density Profiles of Cold Dark Matter Halos
• Tidal dwarf galaxies in cosmological simulations
• The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
• The Birth and Growth of Neutralino Haloes
• Numerical Galaxy Catalog -I. A Semi-analytic Model of Galaxy Formation with N-body simulations
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes II: Global Properties
• Quantifying the Cosmic Web I: The large-scale halo ellipticity-ellipticity and ellipticity-direction correlations
• Seeding Black Holes in Cosmological Simulations
• The Hierarchical Origins of Observed Galaxy Morphology
• The Impact of Galactic Winds on the Angular Momentum of Disk Galaxies in the Illustris Simulation
• Characterization of Dark-Matter-induced anisotropies in the diffuse gamma-ray background
• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• Hydrogen Reionization in the Illustris universe
• Inverted initial conditions: exploring the growth of cosmic structure and voids
• Redshift-space distortions with split densities
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• The Millennium Run Observatory: First Light
• How does our choice of observable influence our estimation of the centre of a galaxy cluster? Insights from cosmological simulations
• The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• Phase-space structures II: Hierarchical Structure Finder
• L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
• High redshift galaxies and the Lyman-alpha forest in a CDM universe
• The growth of disks and bulges during hierarchical galaxy formation. I: fast evolution vs secular processes
• The Baryons in the Milky Way Satellites
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• The Frequency of Dwarf Galaxy Multiples at Low Redshift in SDSS vs. Cosmological Expectations
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• The radial profiles of the different mass components in galaxy clusters
• Impact of Baryonic Processes on Weak Lensing Cosmology: Power Spectrum, Non-Local Statistics, and Parameter Bias
• The phase-space distribution of infalling dark matter subhalos
• Photometric Properties of Lyman-break Galaxies at z=3 in Cosmological SPH Simulations
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• MOKA: a new tool for Strong Lensing Studies
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• Moving mesh cosmology: properties of neutral hydrogen in absorption
• Introducing a new, robust galaxy finder algorithm for simulations
• Warm dark matter signatures on the 21cm power spectrum: Intensity mapping forecasts for SKA
• Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
• Massive galaxies in cosmological simulations: UV-selected sample at redshift z=2
• Environmental Effects on Evolution of Cluster Galaxies in a LCDM Universe
• Barred Galaxies in the IllustrisTNG Simulation
• Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• Ellipsoidal halo finders and implications for models of triaxial halo formation
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations
• Central stellar populations of early-type galaxies in low-density environments
• Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations
• An Extreme Starburst in Close Proximity to the Central Galaxy of a Rich Galaxy Cluster at z=1.7
• Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies
• Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
• The evolution of galaxy cluster X-ray scaling relations
• Probing Evolutionary Mechanisms in Galaxy Clusters: Neutral Atomic Hydrogen in Abell 1367
• An analytical model for the accretion of dark matter subhalos
• The origin and properties of massive prolate galaxies in the Illustris simulation
• Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
• Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
• The contributions of matter inside and outside of haloes to the matter power spectrum
• A First Look at Galaxy Flyby Interactions: I. Characterizing the Frequency of Flybys in a Cosmological Context
• A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
• Dark-Halo Cusp: Asymptotic Convergence
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• Witnessing galaxy assembly in an extended z~3 structure
• Extensions to models of the galaxy-halo connection
• Extragalactic gamma-ray background radiation from dark matter annihilation
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey
• Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
• Abundance of substructure in clusters of galaxies
• Massive and old quiescent galaxies at high redshift
• Chemical evolution of Local Group dwarf galaxies in a cosmological context -- I. A new modelling approach and its application to the Sculptor dwarf spheroidal galaxy
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA
• The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
• The Metallicity and Elemental Abundance Gradients of Simulated Galaxies, and their Environmental Dependence
• The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last $\approx$10 Gyr
• On the Dynamical Origin of the ICM Metallicity Evolution
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• Stellar Halos in Illustris- Probing the Histories of Milky Way-Mass Galaxies
• A Realistic Model for Spatial and Mass Distributions of Dark Halo Substructures: An Analytic Approach
• Streams in the Aquarius stellar haloes
• A New Halo Finding Method for N-Body Simulations
• Strong magnetic fields and large rotation measures in protogalaxies by supernova seeding
• Modeling The Star Forming Universe at z=2: Impact of Cold Accretion Flows
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• Galactic inflow and wind recycling rates in the EAGLE simulations
• The Hydrodynamic Feedback of Cosmic Reionization on Small-Scale Structures and Its Impact on Photon Consumption during the Epoch of Reionization
• Identifying and Analysing Protostellar Disc Fragments in Smoothed Particle Hydrodynamics Simulations
• Tracing the Quenching History in Galaxy Clusters in the EAGLE Simulation
• The stability of stellar disks in Milky-Way sized dark matter halos
• To beta or not to beta: can higher-order Jeans analysis break the mass-anisotropy degeneracy in simulated dwarfs?
• The shape of dark matter subhalos in the Aquarius simulations
• Formation and evolution of young massive clusters in galaxy mergers: the SMUGGLE view
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• How Gas Accretion Feeds Galactic Disks
• The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
• Pairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matter Model using the Bullet Cluster
• Dwarf galaxy populations in present-day galaxy clusters - II. The history of early-type and late-type dwarfs
• Cosmology in 2D: the concentration-mass relation for galaxy clusters
• Predictions for local PNG bias in the galaxy power spectrum and bispectrum and the consequences for $f_{\mathrm{NL}}$ constraints
• Group finding in the stellar halo using M-giants in 2MASS: An extended view of the Pisces Overdensity?
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• Enriching the hot circumgalactic medium
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• The splashback boundary of haloes in hydrodynamic simulations
• Learning cosmology and clustering with cosmic graphs
• The accretion of dark matter subhaloes within the cosmic web: primordial anisotropic distribution and its universality
• The first galaxies: simulating their feedback-regulated assembly
• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• Detailed Cluster Mass and Light profiles of A1703, A370 and RXJ1347-11 from Deep Subaru Imaging
• Expected number of massive galaxy relics in the present-day Universe
• The diverse nature and formation paths of slow rotator galaxies in the EAGLE simulations
• Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Resolution-independent modeling of environmental effects in semi-analytic models of galaxy formation that include ram-pressure stripping of both hot and cold gas
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Origin and evolution of ultra-diffuse galaxies in different environments
• PHEW: a parallel segmentation algorithm for three-dimensional AMR datasets - application to structure detection in self-gravitating flows
• The SLUGGS Survey: A comparison of total-mass profiles of early-type galaxies from observations and cosmological simulations, to $\sim$4 effective radii
• Evolution of the Colour--Radius Relation and the Morphology--Radius Relation in the SDSS Galaxy Clusters
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• The Young and the Wild: What happens to Protoclusters forming at z = 4?
• The impact of galaxy formation on X-ray groups
• Evolution of giant molecular clouds across cosmic time
• An Improved Model for the Dynamical Evolution of Dark Matter Subhaloes
• Duty Cycle and the Increasing Star Formation History of z>=6 Galaxies
• Where do "red and dead" early-type void galaxies come from?
• Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
• Shapley Optical Survey. I: Luminosity Functions in the Supercluster Environment
• How to add massive neutrinos to your $\Lambda$CDM simulation -- extending cosmology rescaling algorithms
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• Impact of baryons on the cluster mass function and cosmological parameter determination
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• On the relative bias of void tracers in the Dark Energy Survey
• The specific star formation rate of high redshift galaxies: the case for two modes of star formation
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• High Redshift Galaxy Populations and their Descendants
• Origin of the galaxy HI size-mass relation
• First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at $z\ge 5$
• Sussing Merger Trees: the influence of the halo finder
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• The earliest stars and their relics in the Milky Way
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• Structure of Axion Miniclusters
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• The origin of the enhanced metallicity of satellite galaxies
• Virial scaling of galaxies in clusters: bright to faint is cool to hot
• Cosmic Ballet III: halo spin evolution in the cosmic web
• AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
• Building a control sample for galaxy pairs
• The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulations
• Galaxy evolution in protoclusters
• The Padova-Millennium Galaxy and Group Catalogue (PM2GC): the group-finding method and the PM2GC catalogues of group, binary and single field galaxies
• Galactic Chemical Evolution of Radioactive Isotopes
• Cosmology dependency of halo masses and concentrations in hydrodynamic simulations
• The competition between confinement and ram pressure and its implications for galaxies in groups and clusters
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Fossil stellar streams and their globular cluster populations in the E-MOSAICS simulations
• CLASH-VLT: Abell~S1063. Cluster assembly history and spectroscopic catalogue
• The strong correlation between post-starburst fraction and environment
• The filling factor of intergalactic metals at redshift z=3
• Prospects for Detecting Neutrino Signals from Annihilating/Decaying Dark Matter to Account for the PAMELA and ATIC results
• On the galaxy-halo connection in the EAGLE simulation
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• The origin of the 'blue tilt' of globular cluster populations in the E-MOSAICS simulations
• Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
• Evolution of the cold gas properties of simulated post-starburst galaxies
• The journey of QSO haloes from z=6 to the present
• The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies
• Galaxies going MAD: The Galaxy-Finder Comparison Project
• Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• Investigating Galaxy-Filament Alignments in Hydrodynamic Simulations using Density Ridges
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
• A first constraint on the average mass of ultra diffuse galaxies from weak gravitational lensing
• Massive Milky Way Satellites in Cold and Warm Dark Matter: Dependence on Cosmology
• Tidal evolution of galaxies in the most massive cluster of IllustrisTNG-100
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes III: Comparison with Simulations
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• Internal kinematics of spiral galaxies in distant clusters Part I
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• Line strengths of early-type galaxies
• Galaxies lacking dark matter in the Illustris simulation
• Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation
• Shallow Dark Matter Cusps in Galaxy Clusters
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Reionization History from Coupled CMB/21cm Line Data
• A tale of two populations: the stellar mass of central and satellite galaxies
• Predicting Hα emission line galaxy counts for future galaxy redshift surveys
• Cosmology with Equivalence Principle Breaking in the Dark Sector
• The cold circumgalactic medium in emission: MgII halos in TNG50
• The Effects of Patchy Reionization on Satellite Galaxies of the Milky Way
• The evolution of the oxygen abundance gradients in star-forming galaxies in the EAGLE simulations
• Barred galaxies in the Illustris-1 and TNG100 simulations
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• Chemical enrichment in very low-metallicity environments: Bootes I
• Robust Field-level Likelihood-free Inference with Galaxies
• Ultimate age-dating method for galaxy groups; clues from the Millennium Simulations
• Einasto Profiles and the Dark Matter Power Spectrum
• The many lives of active galactic nuclei-II: The formation and evolution of radio jets and their impact on galaxy evolution
• The evolution of the stellar mass versus halo mass relationship
• Simulating galaxy Clusters -II: global star formation histories and galaxy populations
• SPIDER IX - Classifying Galaxy Groups according to their Velocity Distribution
• Structure formation simulations with momentum exchange: alleviating tensions between high-redshift and low-redshift cosmological probes
• 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• Characterizing hydrostatic mass bias with Mock-X
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• Effects of Baryon Dissipation on the Dark Matter Virial Scaling Relation
• Cosmology with one galaxy?
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• Great Balls of FIRE I: The formation of star clusters across cosmic time in a Milky Way-mass galaxy
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• Satellite Alignment: I. Distribution of Substructures and Their Dependence On Assembly History From N-Body Simulations
• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• Splotch: Visualizing Cosmological Simulations
• Multicomponent and Variable Velocity Galactic Outflow in Cosmological Hydrodynamic Simulations
• Modelling Galaxy Merger Timescales and Tidal Destruction
• On the measurements of assembly bias and splashback radius using optically selected galaxy clusters
• The Cluster-EAGLE project: velocity bias and the velocity dispersion - mass relation of cluster galaxies
• Modeling color-dependent galaxy clustering in cosmological simulations
• ALMA will determine the spectroscopic redshift z>8 with FIR [O III] emission lines
• A Halo Expansion (HEX) Technique for Approximating Simulated Dark Matter Haloes
• An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• Subhalo statistics of galactic halos: beyond the resolution limit
• Subhaloes gone Notts: Spin across subhaloes and finders
• The nature of assembly bias - III. Observational properties
• The mass dependence of dark matter halo alignments with large-scale structure
• Young star cluster populations in the E-MOSAICS simulations
• The effect of massive neutrinos on the Sunyaev-Zeldovich and X-ray observables of galaxy clusters
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• Iron in galaxy groups and clusters: Confronting galaxy evolution models with a newly homogenised dataset
• The effect of dwarf galaxies disruption in semi-analytic models
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• Satellites Around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations Versus Simulations
• The nature of assembly bias - II. Halo spin
• The origin of compact galaxies with anomalously high black hole masses
• Baryon effects on void statistics in the EAGLE simulation
• On the common mass scale of the Milky Way satellites
• Simulating Momentum Exchange in the Dark Sector
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Galactic Tides and the Shape and Orientation of Dwarf Galaxy Satellites
• Astrometric Microlensing by Local Dark Matter Subhalos
• Revealing the properties of void galaxies and their assembly using the EAGLE simulation
• The diversity of rotation curves of simulated galaxies with cusps and cores
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Gas distribution from clusters to filaments in IllustrisTNG
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• Properties and Evolution of Dual and Offset AGN in the ASTRID Simulation at $z\sim 2$
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• Massive Dark Matter Halos around Bright Isolated Galaxies in the 2dFGRS
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• ASOHF: a new adaptive spherical overdensity halo finder
• Measuring the slopes of mass profiles for dwarf spheroidals in triaxial CDM potentials
• Stellar splashback: the edge of the intracluster light
• Impact of Supernova feedback on the Tully-Fisher relation
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
• Decoupling the rotation of stars and gas -- I: the relationship with morphology and halo spin
• The specific star formation rate and stellar mass fraction of low-mass central galaxies in cosmological simulations
• Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
• The build-up of pseudobulges in a hierarchical universe
• Pre-processing, group accretion and the orbital trajectories of associated subhaloes
• The offsets between galaxies and their dark matter in Lambda-CDM
• Modeling the gravitational potential of a cosmological dark matter halo with stellar streams
• Effects of metal enrichment and metal cooling in galaxy growth and cosmic star formation history
• Semi-Analytic Model Predictions of the Galaxy Population in Proto-clusters
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• The halo mass function in interacting Dark Energy models
• Brighter galaxy bias: underestimating the velocity dispersions of galaxy clusters
• Damped Lyman alpha systems and galaxy formation models - II. High ions and Lyman limit systems
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Towards a general parametrization of the warm dark matter halo mass function
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• Accretion of Galaxy Groups into Galaxy Clusters
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Mergers and Star Formation: The environment and Stellar Mass Growth of the Progenitors of Ultra-Massive Galaxies since z = 2
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Globular clusters as tracers of the dark matter content of dwarfs in galaxy clusters
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• Evolution of Characteristic Quantities for Dark Matter Halo Density Profiles
• The boundary of cosmic filaments
• Properties of fossil groups in cosmological simulations and galaxy formation models
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• Galaxy formation in the brane world I: overview and first results
• Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
• Connecting the structure of dark matter haloes to the primordial power spectrum
• Dark Matter Signatures in the Anisotropic Radio Sky
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• The Impact of Gas Stripping and Stellar Mass Loss on Satellite Galaxy Evolution
• Physical Properties of UDF12 Galaxies in Cosmological simulations
• The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• The pairwise velocity dispersion of galaxies: luminosity dependence and a new test of galaxy formation models
• Investigating the Relation between Galaxy Properties and the Gaussianity of the Velocity Distribution of Groups and Clusters
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• Kinematics of Simulated Galaxies II: Probing the Stellar Kinematics of Galaxies out to Large Radii
• A measurement of galaxy halo mass from the surrounding HI Lyα absorption
• The [α/Fe]-[Fe/H] relation in the E-MOSAICS simulations: its connection to the birth place of globular clusters and the fraction of globular cluster field stars in the bulge
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• MUSE sneaks a peek at extreme ram-pressure stripping events - IV. Hydrodynamic and gravitational interactions in the Blue Infalling Group
• Radiative properties of the first galaxies: rapid transition between blue and red
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• PICS: Simulations of Strong Gravitational Lensing in Galaxy Clusters
• The rise and fall of a challenger: the Bullet Cluster in $\Lambda$ Cold Dark Matter simulations
• Accreted or Not Accreted? The Fraction of Accreted Mass in Galaxies from Simulations and Observations
• The bright end of the colour-magnitude relation of cluster galaxies
• Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys
• Effects of cosmological parameters and star formation models on the cosmic star formation history in LambdaCDM cosmological simulations
• Properties and Origin of Galaxy Velocity Bias in the Illustris Simulation
• Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• The eROSITA view of the Abell 3391/95 field: a case study from the Magneticum cosmological simulation
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Finding universal relations in subhalo properties with artificial intelligence
• Bound and unbound substructures in Galaxy-scale Dark Matter haloes
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• The SIBELIUS Project: E Pluribus Unum
• From large-scale environment to CGM angular momentum to star forming activities -- I: star-forming galaxies
• Strong lensing statistics in large, z~<0.2 surveys: bias in the lens galaxy population
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• Formation and Morphology of the First Galaxies in the Cosmic Morning
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Soft X-ray and ultra-violet metal-line emission from the gas around galaxies
• Semi-analytic galaxy formation in f(R)-gravity cosmologies
• The origin of abundance gradients in the Milky Way: the predictions of different models
• The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
• Measuring the Tidal Response of Structure Formation: Anisotropic Separate Universe Simulations using TreePM
• Color Dependence in the Spatial Distribution of Satellite Galaxies
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Small-scale galaxy clustering in the EAGLE simulation
• Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• X-ray line tomography of AGN-induced motion in clusters of galaxies
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Cosmic voids detection without density measurements
• Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin
• The First Quiescent Galaxies in TNG300
• Influence of baryons on the orbital structure of dark matter haloes
• Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
• The innate origin of radial and vertical gradients in a simulated galaxy disc
• Unbound Particles in Dark Matter Halos
• Quenching Timescales in the IllustrisTNG Simulation
• The Intrinsic Alignment of Dark Halo Substructures
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• Testing strong lensing subhalo detection with a cosmological simulation
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• Baryon history and cosmic star formation in non-Gaussian cosmological models: numerical simulations
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Simulating the effect of photoheating feedback during reionization
• Mapping the Universe: The 2010 Russell Lecture
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• Effects of initial density profiles on massive star cluster formation in giant molecular clouds
• First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
• The scatter in the galaxy-halo connection: a machine learning analysis
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Linear bias forecasts for emission line cosmological surveys
• Adaptive gravitational softening in GADGET
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• The Bound Mass of Substructures in Dark Matter Halos
• Cosmic velocity--gravity relation in redshift space
• Massive Low Surface Brightness Galaxies in the EAGLE Simulation
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in $f(R)$ gravity
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• The impact of galactic feedback on the shapes of dark-matter haloes
• Convergence of Galaxy Properties with Merger Tree Temporal Resolution
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• Nebular line emission from z > 7 galaxies in cosmological simulations: rest-frame UV to Optical lines
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Dark matter haloes in modified gravity and dark energy: interaction rate, small-, and large-scale alignment
• The Formation of Low-Mass Cluster Galaxies and the Universal Initial Galaxy Mass Function
• The Effect of Coupled Dark Energy on the Alignment between Dark Matter and Galaxy Distributions in Clusters
• Abell 2744: Too much substructure for Lambda CDM?
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• The evolution of the galaxy content of dark matter haloes
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• What determines large scale galaxy clustering: halo mass or local density?
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• Gravitational redshift and asymmetric redshift-space distortions for stacked clusters
• Urchin: A Reverse Ray Tracer for Astrophysical Applications
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• Joining X-ray to lensing: an accurate combined analysis of MACS J0416.1$-$2403
• Linking haloes to galaxies: how many halo properties are needed?
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Identification of galaxy cluster substructures with the Caustic method
• Mapping "out-of-the-box" the properties of the baryons in massive halos
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• Suppression of accretion onto low-mass Population III stars
• Structure and rotation of young massive star clusters in a simulated dwarf starburst
• LYRA III: The smallest Reionization survivors
• On the fragmentation boundary in magnetised self-gravitating discs
• Study of galaxies on large-scale filaments in simulations
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
• Why Cosmic Voids Matter: Nonlinear Structure & Linear Dynamics
• The Physical Origin of Galactic Conformity: From Theory to Observation
• The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
• The evolution of barred galaxies in the EAGLE simulations
• On the small scale turbulent dynamo in the intracluster medium: A comparison to dynamo theory
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
• The cosmological dependence of halo and galaxy assembly bias
• The spatial distribution of Milky Way satellites, gaps in streams and the nature of dark matter
• Understanding the Results of Galaxy-Galaxy Lensing using Galaxy-Mass Correlation in Numerical Simulations
• Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• Fast Weak Lensing Simulations with Halo Model
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• Dilution in elliptical galaxies: Implications for the relation between metallicity, stellar mass and star formation rate
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• BSG alignment of SDSS galaxy groups
• On the orbital and internal evolution of cluster galaxies
• Evolution and Role of Mergers in the BCG-Cluster Alignment. A View from Cosmological Hydro-Simulations
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• The importance of galaxy formation histories in models of reionization
• Insights on the origin of ORCs from cosmological simulations
• Constraining the halo mass function with observations
• Dissecting Galaxy Formation: II. Comparing Substructure in Pure Dark Matter and Baryonic Models
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Dark-ages reionization & galaxy formation simulation V: morphology and statistical signatures of reionization
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• The impact of the Large Magellanic Cloud on dark matter direct detection signals
• Testing LSST Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics
• Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass
• The mass accretion rate of galaxy clusters: a measurable quantity
• The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity
• Gas cooling in semi-analytic models and SPH simulations: are results consistent?
• How AGN feedback drives the size growth of the first quasars
• Detecting neutral hydrogen in emission at redshift z ~ 1
• Cosmology dependence of galaxy cluster scaling relations
• Cosmological insights into the assembly of the radial and compact stellar halo of the Milky Way
• Deep spectroscopy in nearby galaxy clusters: III Orbital structure of galaxies in Abell 85
• ELUCID V. Lighting dark matter halos with galaxies
• The evolution of galaxy groups and of galaxies therein
• Stellar feedback from HMXBs in cosmological hydrodynamical simulations
• Euclid: The search for primordial features
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• Evolution and Statistics of Non-Sphericity of Dark Matter Halos from Cosmological N-Body Simulation
• Galactic conformity measured in semi-analytic models
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Multifrequency radiation hydrodynamics simulations of H2 line emission in primordial, star-forming clouds
• Lyman-alpha Emitters in Cosmological Simulations I: Lyman-alpha Escape Fraction and Statistical Properties at z=3.1
• Towards an improved model of self-interacting dark matter haloes
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Cosmology with the pairwise kinematic SZ effect: Calibration and validation using hydrodynamical simulations
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• How accurate is it to update the cosmology of your halo catalogues?
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• The physical drivers of gas turbulence in simulated disc galaxies
• Probing the dark-matter halos of cluster galaxies with weak lensing
• DEMNUni: The imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing
• Relative velocity of dark matter and barions in clusters of galaxies and measurements of their peculiar velocities
• Parallel HOP: A Scalable Halo Finder for Massive Cosmological Data Sets
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Evolution of compact and fossil groups of galaxies from semi-analytical models of galaxy formation
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• The galaxy population in cold and warm dark matter cosmologies
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Fast Identification of Bound Structures in Large N-body Simulations
• On the dynamics of the satellite galaxies in NGC 5044
• The Transition Region between Brightest Cluster Galaxies and Intra-Cluster Light in Galaxy Groups and Clusters
• The Lives of High Redshift Mergers
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Why are AGN found in High Mass Galaxies?
• Dynamical flows through Dark Matter Haloes: Inner perturbative dynamics, secular evolution, and applications
• Evolution of galaxy groups in the Illustris simulation
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Cosmic evolution of bars in simulations of galaxy formation
• Highly r-process enhanced stars in ultra-faint dwarf galaxies
• The orbital PDF: the dynamical state of Milky Way sized haloes and the intrinsic uncertainty in the determination of their masses
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• Where do galaxies end? Comparing measurement techniques of hydrodynamic-simulation galaxies' integrated properties
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• The stellar populations of high-redshift dwarf galaxies
• Modeling the kinematics of globular cluster systems
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• GalICS V : Low and high order clustering in mock SDSS's
• Are Passive Spiral Galaxies Truly "Passive" and "Spiral"? : Near-Infrared Perspective
• On the Mass Distribution of the Intra-Cluster Light in Galaxy Groups and Clusters
• The effects of halo alignment and shape on the clustering of galaxies
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• The evolution of galaxy intrinsic alignments in the MassiveBlack II universe
• The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
• Subhaloes in Scale-Free Cosmologies
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• The eROSITA view of the Abell 3391/95 field: The Northern Clump. The largest infalling structure in the longest known gas filament observed with eROSITA, XMM-Newton, and Chandra
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• Dianoga SIDM: galaxy cluster self-interacting dark matter simulations
• The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo
• Influence of baryonic physics on the merger time-scale of galaxies in N-body/hydrodynamical simulations
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• Blind Search of The Solar Neighborhood Galactic Disk within 5kpc: 1,179 new Star clusters found in Gaia DR3
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• Modeling Intrinsic Galaxy Alignment in the MICE Simulation
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Are fossil groups early-forming galaxy systems?
• Measuring the Cosmic Equation of State with Galaxy Clusters in the DEEP2 Redshift Survey
• The segregation of baryons and dark matter during halo assembly
• Signature of the first galaxies in JWST deep field observations
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Dust evolution with MUPPI in cosmological volumes
• Constructing high-fidelity halo merger trees in AbacusSummit
• Velocity-dependent J-factors for annihilation radiation from cosmological simulations
• Dark-matter-deficient galaxies in hydrodynamical simulations
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
• Comparison of cosmological simulations and deep submillimetre galaxy surveys
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• Lensing Model of MACS J1149.5+2223 - I. Cluster mass reconstruction
• Phase-space structures I: A comparison of 6D density estimators
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• Redshift evolution of the dark matter haloes shapes
• Massive relic galaxies prefer dense environments
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• Gravitational Wave Signal from Assembling the Lightest Supermassive Black Holes
• Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
• Strongly lensed cluster substructures are not in tension with $\Lambda$CDM
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• Properties of brightest group galaxies in cosmic web filaments
• The VLT LBG Redshift Survey - IV. Gas and galaxies at z ~ 3 in observations and simulations
• Galaxies at Redshift ~0.5 Around Three Closely Spaced Quasar Sightlines
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Supersymmetric dark matter in M31: can one see neutralino annihilation with CELESTE?
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• SOAP: A Python Package for Calculating the Properties of Galaxies and Halos Formed in Cosmological Simulations
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• Zoomed cosmological simulations of Milky Way sized halos in f(R)-gravity
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• A stream come true: Connecting tidal tails, shells, streams, and planes with galaxy kinematics and formation history
• Origins of carbon-enhanced metal-poor stars
• Star clusters forming in a low metallicity starburst -- rapid self-enrichment by (very) massive stars
• The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
• Galaxy properties in the cosmic web of EAGLE simulation
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• The peculiar velocities of satellites of external disk galaxies
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• The origin of X-ray coronae around simulated disc galaxies
• Calibrated, cosmological hydrodynamical simulations with variable IMFs III: Spatially-resolved properties and evolution
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Dark matter halo occupation: environment and clustering
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs
• The galaxy morphology-density relation in the EAGLE simulation
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• The assembly bias of emission line galaxies
• Smoothing Algorithms and High-order Singularities in Gravitational Lensing
• The First Billion Years project: dark matter haloes going from contraction to expansion and back again
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• Subhaloes gone Notts: the clustering properties of subhaloes
• Semi-analytic galaxy formation in early dark energy cosmologies
• Present-day scaling relations of submm galaxies: origin of spheroidal sytems
• On the inconsistency between the estimates of cosmic star formation rate and stellar mass density of high redshift galaxies
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Formalism for the Subhalo Mass Function in the Tidal-limit Approximation
• Passive Evolution of Galaxy Clustering
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• How identifying circumgalactic gas by line-of-sight velocity instead of the location in 3D space affects O VI measurements
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• The Indirect Influence of Quasars on Reionization
• Sussing Merger Trees: Stability and Convergence
• One simulation to have them all: performance of the Bias Assignment Method against N-body simulations
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• The low abundance and insignificance of dark discs in simulated Milky Way galaxies
• Galaxies with monstrous black holes in galaxy cluster environments
• Satellite galaxies in groups in the CIELO Project I. Gas removal from galaxies and its re-distribution in the intragroup medium
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Subhaloes gone Notts: Subhaloes as tracers of the dark matter halo shape
• From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass
• The Milky Way and Andromeda galaxies in a constrained hydrodynamical simulation: morphological evolution
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• Santa Barbara Cluster Comparison Test with DISPH
• First Structure Formation under the Influence of Gas-Dark Matter Streaming Velocity and Density: Impact of the Baryons-trace-dark matter Approximation
• A high-resolution cosmological simulation of a strong gravitational lens
• Orbital distribution of infalling satellite halos across cosmic time
• Beta-Skeleton Analysis of the Cosmic Web
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• II. Apples to apples $A^2$: cluster selection functions for next-generation surveys
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• A Baryonic Effect on the Merger Timescale of Galaxy Clusters
• Effects of Multiphase Gas and Projection on X-ray Observables in Simulated Galaxy Clusters as Seen by eROSITA
• A New Model for Dark Matter Halos Hosting Quasars
• Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
• The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• Assembly history of subhalo populations in galactic and cluster sized dark haloes
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Dust and Power: Unravelling the merger - active galactic nucleus connection in the second half of cosmic history
• A 4% measurement of $H_0$ using the cumulative distribution of strong-lensing time delays in doubly-imaged quasars
• Numerical investigation of lenses with substructures using the perturbative method
• Testing dark energy using pairs of galaxies in redshift space
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• A general framework to test gravity using galaxy clusters III: Observable-mass scaling relations in $f(R)$ gravity
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe
• The lopsided distribution of satellites of isolated central galaxies
• The cosmic web connection to the dark matter halo distribution through gravity
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• Globular Clusters and Streaming Velocities: Testing the new formation channel in high-resolution cosmological simulations
• Through a Smoother Lens: An expected absence of LCDM substructure detections from hydrodynamic and dark matter only simulations
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• Tidal features of classical Milky Way satellites in a $\Lambda$CDM universe
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar halo
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• The MIP Ensemble Simulation: Local Ensemble Statistics in the Cosmic Web
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Simulation view of galaxy clusters with low X-ray surface brightness
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Assessing the Predictive Power of Galaxy Formation Models: A Comparison of Predicted and Observed Rest-Frame Optical Luminosity Functions at 2.0<z<3.3
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• How do galactic winds affect the Lyalpha forest?
• First Light And Reionisation Epoch Simulations (FLARES) XIII: The Lyman-continuum emission of high-redshift galaxies
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Milky Way type galaxies in a LCDM cosmology
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Structure formation with primordial black holes: collisional dynamics, binaries, and gravitational waves
• Intra-cluster Globular Clusters in a Simulated Galaxy Cluster
• On the operation of the chemothermal instability in primordial star-forming clouds
• Probability Friends-of-Friends (PFOF) Group Finder: Performance Study and Observational Data Applications on Photometric Surveys
• Direct-collapse black hole formation induced by internal radiation of host halos
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• The spatial distribution of X-ray selected AGN in the Chandra deep fields: a theoretical perspective
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• The Cosmic Web Around The Brightest Galaxies During The Epoch Of Reionization
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• The abundance of dark matter haloes down to Earth mass
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• The Dispersion Measure Contributions of the Cosmic Web
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• The Breakdown Scale of HI Bias Linearity
• Alignments of dark matter halos with large-scale tidal fields: mass and redshift dependence
• The evolutionary pathways of disk galaxies with different sizes
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Testing Dark Matter Halo Models of Quasars With Thermal Sunyaev-Zeldovich Effect
• Fingerprints of the hierarchical building up of the structure on the gas kinematics of galaxies
• Two channels for the formation of compact dwarf galaxies in clusters of galaxies
• The Effect of Assembly Bias on Redshift Space Distortions
• Compact groups in theory and practice - II. Comparing the observed and predicted nature of galaxies in compact groups
• Constraints on ${\Omega }_{\mathrm{m}}$ and ${\sigma }_8$ from the potential-based cluster temperature function
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Cosmological Probes of Structure Growth and Tests of Gravity
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• The Cluster-EAGLE project: a comparison of dynamical mass estimators using simulated clusters
• Warm Dark Haloes Accretion Histories and their Gravitational Signatures
• Rosella: A mock catalogue from the P-Millennium simulation
• Self-similarity in the chemical evolution of galaxies and the delay time distribution of SNe Ia
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• A Merger Tree with Microsolar Mass Resolution: Application to $\gamma$-ray Emission from Subhalo Population
• Multi-Scale Morphological Analysis of SDSS DR5 Survey using the Metric Space Technique
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Connections between galaxy properties and halo formation time in the cosmic web
• POLAR -- I: linking the 21-cm signal from the epoch of reionization to galaxy formation
• Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogs
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• Statistical properties of dark matter mini-haloes at z >= 15
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• A warm mode of gas accretion on forming galaxies
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Benchmarks and Explanations for Deep Learning Estimates of X-ray Galaxy Cluster Masses
• Star formation in mergers with cosmologically motivated initial conditions
• Inferring Gravitational Potentials from Mass Densities in Cluster-sized Halos
• Stacking Caustic Masses from Galaxy Clusters
• Introducing the Photometric Maximum Likelihood Method: Galaxy Luminosity Functions at z<1.2 in MUSYC-ECDFS
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• Galaxy Evolution in the Environment of ABCG 209
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• N-body simulations of gravitational redshifts and other relativistic distortions of galaxy clustering
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Constraining CMB-consistent primordial voids with cluster evolution
• The effect of gas-dynamics on semi-analytic modeling of cluster galaxies
• The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model. II. The colour-density relation up to z=1.5
• Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo Cluster
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• Heating and enriching the intracluster medium
• The magnetised and thermally unstable tails of jellyfish galaxies
• Indra: a Public Computationally Accessible Suite of Cosmological $N$-body Simulations
• The impact of Self-Interacting Dark Matter on the Intrinsic Alignments of Galaxies
• Merging galaxy clusters in IllustrisTNG
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Blooming Trees: Substructures and Surrounding Groups of Galaxy Clusters
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• Keck Spectroscopy of Globular Clusters in the Virgo Cluster Dwarf Elliptical VCC 1386
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• Luminosity Distribution of Gamma-Ray Burst Host Galaxies at redshift z=1 in Cosmological Smoothed Particle Hydrodynamic Simulations: Implications for the Metallicity Dependence of GRBs
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
• Globular cluster metallicity distributions in the E-MOSAICS simulations
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• The Cosmic Evolution of Halo Pairs: I. Global Trends
• Calibrated, cosmological hydrodynamical simulations with variable IMFs II: Correlations between the IMF and global galaxy properties
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Semi-Analytic Galaxy Formation in Massive Neutrino Cosmologies
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Dynamical analysis of clusters of galaxies from cosmological simulations
• The imprint of galaxy mergers on satellite planes in a cosmological context
• Degeneracies between baryons and dark matter: the challenge of constraining the nature of dark matter with JWST
• Simulations of structure formation in interacting dark energy cosmologies
• The First Billion Years project: gamma-ray bursts at z>5
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
• A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
• Mock HUBS observations of hot gas with IllustrisTNG
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Ram pressure stripping in the EAGLE simulation
• The Kinematic State of the Local Volume
• Massive Quiescent Galaxies at z>3 in The Millennium Simulation Populated by A Semi-analytic Galaxy Formation Model
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• Do satellite galaxies trace matter in galaxy clusters?
• The impact of magnetic fields on cosmological galaxy mergers -- II. Modified angular momentum transport and feedback
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• Evolution of central galaxy alignments in simulations
• A too-many dwarf satellite galaxies problem in the MATLAS low-to-moderate density fields
• Why weak lensing cluster shapes are insensitive to self-interacting dark matter
• An Accurate Comprehensive Approach to Substructure: I. Accreted Subhaloes
• The distribution and properties of DLAs at z $\le$ 2 in the EAGLE simulations
• Machine Learning to identify ICL and BCG in simulated galaxy clusters
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• Host galaxies of long gamma-ray bursts in the Millennium Simulation
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• The cosmology dependence of the concentration-mass-redshift relation
• Galactic satellite systems in CDM, WDM and SIDM
• Ultramassive black holes formed by triple quasar mergers at $z\sim 2$
• The Origin of Neutral Hydrogen Clouds in Nearby Galaxy Groups: Exploring the Range Of Galaxy Interactions
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Formation of a barred galaxy in a major merger: The role of AGN feedback
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Matching the mass function of Milky Way satellites in competing dark matter models
• Toward a Physical Understanding of Galaxy-Halo Alignment
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• NGC 1436: the making of a lenticular galaxy in the Fornax cluster
• Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ΛCDM
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• A new gas cooling model for semi-analytical galaxy formation models
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• The Local Void: for or against LCDM?
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Testing the fidelity of simulations of black hole - galaxy co-evolution at z ~ 1.5 with observations
• Disk flaring with TNG50: diversity across Milky Way and M31 analogs
• Impact of Primordial Black Hole Dark Matter on Gas Properties at Very High Redshift: A Semi-Analytical Model
• UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?
• The impact of environment on the dynamical structure of satellite systems
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Zooming in on the Circumgalactic Medium with GIBLE: the Topology and Draping of Magnetic Fields around Cold Clouds
• The origin of star-gas misalignments in simulated galaxies
• Exploring the effects of primordial non-Gaussianity at galactic scales
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• The Size Evolution of Elliptical Galaxies
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• Debiased Galaxy Cluster Pressure Profiles from X-ray Observations and Simulations
• Galaxy stellar and total mass estimation using machine learning
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• The Galactic positron flux and dark matter substructures
• Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate
• Tracking the orbit of unresolved subhalos for semi-analytic models
• The effect of interacting dark energy on local measurements of the Hubble constant
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• Merger Effects on the Spin and Shape Alignments of Galaxy Stellar, Cold and Hot Gas, and Dark Matter Components
• Intrinsic alignments of bulges and discs
• Gas stripping and mixing in galaxy clusters: A numerical comparison study
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• Galaxy-group (halo) alignments from SDSS DR7 and the ELUCID simulation
• Testing the Impact of Satellite Anisotropy on Large and Small Scale Intrinsic Alignments using Hydrodynamical Simulations
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• The scale dependence of mass assembly in galaxies
• Uncovering substructure with wavelets: proof of concept using Abell 2744
• Three-point intrinsic alignments of dark matter halos in the IllustrisTNG simulation
• Radio views of cosmic reionization
• The CO universe: Modelling CO emission and H${}_2$ abundance in cosmological galaxy formation simulations
• An empirical model to form and evolve galaxies in dark matter halos
• An IllustrisTNG View of the Caustic Technique for Galaxy Cluster Mass Estimation
• The signal of decaying dark matter with hydrodynamical simulations
• Classification of cosmic structures for galaxies with deep learning: connecting cosmological simulations with observations
• Overdensity of VVV galaxies behind the Galactic bulge
• SDSS-IV MaNGA: Stellar population correlates with stellar root-mean-square velocity $V_{\mathrm{rms}}$ gradients or total-density-profile slopes at fixed effective velocity dispersion ${\sigma }_{\mathrm{e}}$
• Probing the assembly of dwarf galaxies through cosmic time with damped Lyman-$\alpha$ absorption spectroscopy
• A new analytic ram pressure profile for satellite galaxies
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Merge and strip: dark matter-free dwarf galaxies in clusters can be formed by galaxy mergers
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Setting the Stage: Structures from Gaussian Random Fields
• Star Formation and Chemical Enrichment in Protoclusters
• Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• An environment-dependent halo mass function as a driver for the early quenching of $z\ge 1.5$ cluster galaxies
• Modelling the dynamical friction timescale of sinking satellite
• A panchromatic view of star cluster formation in a simulated dwarf galaxy starburst
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Rotation in Gravitational Lenses
• Relating galaxies across different redshift to study galaxy evolution
• Starburst galaxies in semi-analytic models of galaxy formation and evolution
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
• Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector
• History of the gas fuelling star formation in eagle galaxies
• A consistent model for both the HI and stellar mass functions of galaxies
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• Extracting galaxy merger timescales I: Tracking haloes with WhereWolf and spinning orbits with OrbWeaver
• Gas clumping and its effect on hydrostatic bias in the MACSIS simulations
• A common origin for the Fundamental Plane of quiescent and star-forming galaxies in the EAGLE simulations
• The inhomogenous reionization of the inter-galactic medium by metal-poor globular clusters
• Using galaxy pairs as cosmological tracers
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
• Formation of super-thin galaxies in Illustris-TNG
• A robust determination of halo environment in the cosmic field
• Measuring the BAO peak position with different galaxy selections
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
• Semi-analytic galaxy formation in coupled dark energy cosmologies
• GABE: Galaxy Assembly with Binary Evolution
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Environmental dependence of X-ray and optical properties of galaxy clusters
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Implications of galaxy buildup for putative IMF variations in massive galaxies
• Galaxy shapes in Magneticum. I. Connecting stellar and dark matter shapes to dynamical and morphological galaxy properties and the large-scale structure
• Demographics of Sloan Digital Sky Survey galaxies along the Hubble sequence
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• Probabilistic model for dynamic galaxy decomposition
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Cosmology with Galaxy Cluster Properties using Machine Learning
• Using angular momentum maps to detect kinematically distinct galactic components
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- I. Constraining physical processes in local star-forming galaxies
• MEGA: Merger graphs of structure formation
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• On the phase-space structure of galaxy clusters from cosmological simulations
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• On merger bias and the clustering of quasars
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Mergers all the way down: stellar collisions and kinematics of a dense hierarchically forming massive star cluster in a dwarf starburst
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• Formation and fate of low metallicity stars in IllustrisTNG50
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• Luminous satellite galaxies in gravitational lenses
• On the reliability of photometric and spectroscopic tracers of halo relaxation
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• The chemical imprint of the bursty nature of Milky Way's progenitors
• The origin and properties of red spirals: Insights from cosmological simulations
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• Baryonic Effects on Lagrangian Clustering and Angular Momentum Reconstruction
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Ecology of dark matter haloes -II. Effects of interactions on the alignment of halo pairs
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• Playing with FIRE: A Galactic Feedback-Halting Experiment Challenges Star Formation Rate Theories
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• L-GALAXIES 2020: The formation and chemical evolution of stellar haloes in Milky Way Analogues and galaxy clusters
• Impact of Cosmological Satellites on Stellar Discs: Dissecting One Satellite at a Time
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Can substructure in the Galactic Halo explain the ATIC and PAMELA results?
• Characterizing simulated galaxy stellar mass histories
• Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
• The parametrization of gas flows in discs in the Auriga simulations
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Reconstructing the Triaxial Shapes of Dark Matter Halos from the Anisotropic Spatial Distributions of their Substructures in the Concordance Cosmology
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• Mass-morphology relation of TNG50 galaxies
• Zooming in on the Circumgalactic Medium with GIBLE: Tracing the Origin and Evolution of Cold Clouds
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• Galaxy populations of ProtoClusters in cosmological hydrodynamical simulations
• The diverse physical origins of stars in the dynamically hot bulge: CALIFA vs. IllustrisTNG
• The perils of stacking optically selected groups in eROSITA data. The Magneticum perspective
• Galaxy populations in protoclusters at cosmic noon
• Radial X-ray profiles of simulated galaxies: Contributions from hot gas and XRBs
• Spin speed correlations and the evolution of galaxy-halo systems
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• An efficient and robust method to estimate halo concentration
• Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
• A new test of gravity -- I: Introduction to the method
• Triple and Quadruple Black Holes in the ASTRID Simulation at $z\sim 2$
• Anisotropic correlation functions as tracers of central galaxy alignments in simulations
• Halo mass function in scale invariant models
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Differentiating small-scale subhalo distributions in CDM and WDM models using persistent homology
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
• The impact of filaments on dwarf galaxy properties in the Auriga simulations
• Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• Studying galaxy cluster morphological metrics with Mock-X
• Connection Between Galaxies and HI in the Circumgalactic and Intergalactic Media: Variation According to Galaxy Stellar Mass and Star-formation Activity
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• Setting the scene for BUFFALO: A study of the matter distribution in the HFF galaxy cluster MACS J0416.1-2403 and its parallel field
• The impact of the cosmological constant on past and future star formation
• MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
• A deep learning approach to halo merger tree construction
• SCONCE: A cosmic web finder for spherical and conic geometries
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• The Effect of the Remnant Mass in Estimating Stellar Mass of Galaxies
• Clustering in the Phase Space of Dark Matter Haloes. I. Results from the Aquarius simulations
• Confronting predictions of the galaxy stellar mass function with observations at high-redshift
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Fluorescent rings in star-free dark matter haloes
• Haloes at the ragged edge: The importance of the splashback radius
• The LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap I. The Spectroscopic Redshift Catalog
• Evidence of Turbulence-like Universality on the Formation of Galaxy-sized Dark Matter Haloes
• Color, spectral and morphological transformations of galaxies in clusters
• The origin of redshift asymmetries: How LambdaCDM explains anomalous redshift
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Constraining supersymmetry from the satellite experiments
• Gamma rays from dark matter spikes in EAGLE simulations
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• The history and mass content of cluster galaxies in the EAGLE simulation
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Preprocessing in small groups: Three simulated galaxies interacting prior to cluster infall
• Modeling the Alignment Profile of Satellite Galaxies in Clusters
• Boosting Line Intensity Map Signal-to-Noise with the Ly-$\alpha$ Forest Cross-Correlation
• SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
• Influence of mergers on LyC escape of high redshift galaxies
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• The Degeneracy of Galaxy Formation Models
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• Simulating Kilonovae in the ΛCDM Universe
• Complementary Cosmological Simulations
• Sensitivity of Halo Shape Measurements
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• The relationship between substructure in 2D X-ray surface brightness images and weak lensing mass maps of galaxy clusters: A simulation study
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• Detecting the dark matter annihilation at the ground EAS detectors
• Astrophysics with the Laser Interferometer Space Antenna
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• The quantity of dark matter in early-type galaxies and its relation to the environment
• Satellite galaxy abundance dependency on cosmology in Magneticum simulations
• CSST Cosmological Emulator III: Hybrid Lagrangian Bias Expansion Emulation of Galaxy Clustering
• Exploring the physical origins of halo assembly bias from early times
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• The effects of the orbital configurations of mergers on reshaping galaxy structures
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Finding proto-clusters to trace galaxy evolution: I. The finder and its performance
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Chemical abundances and spatial distribution of Long Gamma-Ray Bursts
• Evolution of Low Mass Galactic Subhalos and Dependence on Concentration
• The Glow of Axion Quark Nugget Dark Matter: (II) Galaxy Clusters
• A two-phase model of galaxy formation: III. The formation of globular clusters
• Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution
• Thinking outside the halo: Tracing the large-scale distribution of diffuse cosmic metals with semi-analytic models
• Cross-Correlation between Damped Ly-alpha Systems and Ly-break Galaxies in Cosmological SPH Simulations
• Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
• Velocity-dependent J-factors for Milky Way dwarf spheroidal analogues in cosmological simulations
• Local variations of the Stellar Velocity Ellipsoid-I: the disc of galaxies in the Auriga simulations
• Anisotropy and characteristic scales in halo density gradient profiles
• Performance Optimisation of Smoothed Particle Hydrodynamics Algorithms for Multi/Many-Core Architectures
• Galaxy Groups: Proceedings from a Swinburne University Workshop
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Co-Interacting Dark Matter
• What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Protoclusters at z=5.7: A view from the MultiDark galaxies
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Fast multiscale galaxy cluster detection with weak lensing: towards a mass-selected sample
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• A study on the multicolour evolution of Red Sequence galaxy populations: insights from hydrodynamical simulations and semi-analytical models
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• A Study of the Properties and Dynamics of the Disk of Satellites in a Milky-Way-like Galaxy System
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Breaking the Dark Degeneracy with the Drifting Coefficient of the Field Cluster Mass Function
• The formation and disruption of globular cluster populations in simulations of present-day $L^{\ast }$ galaxies with controlled assembly histories
• CEMPlifying reionization
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• Constraints on the Dark Matter Annihilations by Neutrinos with Substructure Effects Included
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• AuriDESI: Mock Catalogues for the DESI Milky Way Survey
• Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• The influence of baryons on low-mass haloes
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Local variations of the Stellar Velocity Ellipsoid-II: the effect of the bar in the inner regions of Auriga galaxies
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Building Blocks of the Milky Way's Accreted Spheroid
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Proca-stinated Cosmology II: Matter, Halo, and Lensing Statistics in the vector Galileon
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Cosmic filament spin -- I: a comparative study in observation
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at $1<z<5$
• Probing Satellite Halos with Weak Gravitational Lensing
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Simulations of the accreted stellar halos of low-mass field galaxies
• Kickstarting Reionization with the First Black Holes: the effects of second-order perturbation theory in pre-reionization volumes
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• Detection of the Intrinsic Spin Alignments in Isolated Spiral Pairs
• Environmental effects on associations of dwarf galaxies
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Dark matter haloes: a multistream view
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• Mock Observations: Three Different Types of Galaxy Alignment in TNG100 Simulations
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• Solving the puzzle of subhalo spins
• The Coarse Geometry of Merger Trees in ΛCDM
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• The Impact of Baryons on the Large-Scale Structure of the Universe
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• The "Building Blocks" of Stellar Halos
• The Formation and Evolution of Massive Galaxies
• Machine Learning and Structure Formation in Modified Gravity
• Alignment between Satellite and Central Galaxies in the EAGLE Simulation: Dependence on the Large-Scale Environments
• Reoriented Memory of Galaxy Spins for the Early Universe
• The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• The eROSITA view on the halo mass-temperature relation: From low-mass groups to massive clusters
• The S-PLUS Fornax Project (S+FP): Mapping H$\alpha$+[NII] emission in 77 Fornax galaxy members reaching $\sim$4 Rvir
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• Spin alignment around TNG300-1 voids
• Making use of sub-resolution halos in N-body simulations
• The imprint of dark subhaloes on the circumgalactic medium
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Beyond the Halo: Redefining environment with unbound matter in N-body simulations
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• Modelling the Evolution of Ly$\alpha$ Blobs and Ly$\alpha$ Emitters
• Negligible Effects of Baryons on the Angular Momentum Scaling Relations of Galactic Dark Matter Halos
• Probing the shape and internal structure of dark matter halos with the halo-shear-shear three-point correlation function
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing
• The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective
• On the Spin Bias of Satellite Galaxies in the Local Group-like Environment
• Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi
• High-redshift AGN population in radiation-hydrodynamics simulations
• The velocity--shape alignment of clusters and the kinetic Sunyaev--Zeldovich effect
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• Associations of dwarf galaxies in a $\Lambda$CDM Universe
• The role of magnetic fields in ram pressure stripping of satellite galaxies in the circumgalactic medium around massive galaxies
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• The evolution of the barred galaxy population in the TNG50 simulation
• How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• Physically motivated modeling of LyC escape fraction during reionization
• Evidence for axion miniclusters with an increased central density
• The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies
• Average energy of the X-ray spectrum as a model-independent proxy for the mass of galaxy clusters
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• CGCG 480-022: A distant lonesome merger?
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• Infant Galaxy Clusters at Low Redshifts?
• Cosmology with One Galaxy: Auto-Encoding the Galaxy Properties Manifold
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Study of dependence of ram pressure stripping on the orbital parameters of the galaxies
• HIKER: a halo-finding method based on kernel-shift algorithm
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• Estimating infall times of galaxies around clusters: how accurately can it be done with observational data?
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• On the effects of parameters on galaxy properties in CAMELS and the predictability of ${\Omega }_{\mathrm{m}}$
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• Three-dimensional shapelets and an automated classification scheme for dark matter haloes
• The AIDA-TNG project: 3D halo shapes
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Inferring halo masses with Graph Neural Networks
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• Bulgeless Evolution And the Rise of Discs (BEARD) II. The role of mergers in shaping the Milky Way analogues in TNG50
• SubDLe: identification of substructures in cosmological simulations with deep learning
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Gaussian Lagrangian Galaxy Bias
• Identifying Halos in Cosmological Simulations with Continuous Wavelet Analysis: The 2D Case
• The Boosted Potential
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Large, fast and accurate HI intensity maps with latent overlap diffusion
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• Environment matters: stronger magnetic fields in satellite galaxies
• The Effect of Corner Modes in the Initial Conditions of Cosmological Simulations
• Evolution of the degree of substructures in simulated galaxy clusters
• Constraints on the galaxy formation models during epoch of reionization with high redshift observations
• Dynamics of merging: Post-merger mixing and relaxation of an Illustris galaxy
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Dust contribution to the panchromatic galaxy emission
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• On the Robustness of Cluster Clustering Covariance Calibration
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods
• The Hierarchical Structure of Galactic Haloes: Generalised N-Dimensional Clustering with CluSTAR-ND
• STRAWBERRY: Finding haloes in the gravitational potential
• Cosmological simulations with rare and frequent dark matter self-interactions
• The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
• The impact of cosmic filaments on the abundance of satellite galaxies
• The effect of hydrodynamics alone on the subhalo population in a $\Lambda$CDM rich cluster sized dark matter halo
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• Towards Precision Cosmology With Improved PNLF Distances Using VLT-MUSE. III. Impact of Stellar Populations in Early-Type Galaxy
• The progenitor galaxies of stellar haloes as "failed" Milky Ways
• Galaxy-halo internal alignments across cosmic time
• Angular momentum and morphological sequence of massive galaxies through Dark Sage
• A group finder algorithm optimised for the study of local galaxy environment
• RIGEL: Feedback-regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• Predicting halo occupation and galaxy assembly bias with machine learning
• Probing the spatial and velocity anisotropies in stellar halos from the Aquarius simulations
• Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue
• Halo cluster shapes: Insights from simulated galaxies and ICL with prospects for weak lensing applications
• The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
• The major merger-active galactic nucleus connection up to the cosmic noon
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• Tracing black hole and galaxy growth across environments since cosmic noon
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Constructing Merger Trees of Density Peaks Using Phase-Space Watershed Segmentation Algorithm
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• Subhalo abundance and satellite spatial distribution in Milky Way-Andromeda-like paired haloes
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• "Observing and Analyzing" Images From a Simulated High Redshift Universe
• Halo detection via large-scale Bayesian inference
• Disc instability and bar formation: view from the IllustrisTNG simulations
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• The Galaxy and its stellar halo - insights from a hybrid cosmological approach
• Baryon-driven decontraction in Milky Way mass haloes
• The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Extended Hernquist-Springel formalism for cosmic star formation
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• The PARADIGM project II: The lifetimes and quenching of satellites in Milky Way-mass haloes
• Go with the Flow: The Self-Similar and Non-Linear Behaviour of Large-Scale In- and Outflows and the Impact of Accretion Shocks from Galaxies to Galaxy Clusters
• Investigating the Relationship Between the Hot Gas and the Dark Matter Components of Galaxy Clusters
• Cosmic Web-Halo Connection Between Twin Universes
• Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• The halo finding problem revisited: a deep revision of the ASOHF code
• Galaxies in the central regions of simulated galaxy clusters
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Primordial Galaxy Formation and IGM Reionization
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• Intrinsic alignments of galaxies in multiple projections
• Mimicking the halo-galaxy connection using machine learning
• Simulated X-ray Emission in Galaxy Clusters with Feedback from Active Galactic Nuclei
• Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• The dynamical lineage of ultra-diffuse galaxies from TNG50-1
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• Towards a universal model for the density profiles of dark matter haloes
• Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
• Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
• The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Identification of Compact Groups of Galaxies in IllustrisTNG300
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• White dwarfs in the building blocks of the Galactic spheroid
• 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
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• cosmokdtree: a flexible OpenMP-parallelized k-d tree for computational astrophysics applications
• The black hole occupation fraction as a fossil record of seeding, dynamics, and galaxy assembly
• Tracing cosmic voids with fast simulations
• Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
• POLAR-II: modeling star formation history of galaxies on the 21-cm signal from Epoch of Reionization
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• DeepVoid: A Deep Learning Void Detector
• Stellar populations of stellar halos: Results from the Illustris simulation
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• CWTHF: Subhalo Identification with Continuous Wavelet Transform
• Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
• Modeling the High-z Universe: Probing Galaxy Formation
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Off-center black hole seed formation? Implications for high and low redshift massive black holes
• Probing gravity with non-linear clustering in redshift space
• Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions