Resolving Cosmic Structure Formation with the Millennium-II Simulation

Abstract

We present the Millennium-II Simulation (MS-II), a very large N-body simulation of dark matter evolution in the concordance LCDM cosmology. The MS-II assumes the same cosmological parameters and uses the same particle number and output data structure as the original Millennium Simulation (MS), but was carried out in a periodic cube one-fifth the size (100 Mpc/h) with 5 times better spatial resolution (a Plummer equivalent softening of 1.0 kpc/h) and with 125 times better mass resolution (a particle mass of 6.9 \times 10^6 Msun/h). By comparing results at MS and MS-II resolution, we demonstrate excellent convergence in dark matter statistics such as the halo mass function, the subhalo abundance distribution, the mass dependence of halo formation times, the linear and nonlinear autocorrelations and power spectra, and halo assembly bias. Together, the two simulations provide precise results for such statistics over an unprecedented range of scales, from halos similar to those hosting Local Group dwarf spheroidal galaxies to halos corresponding to the richest galaxy clusters. The "Milky Way" halos of the Aquarius Project were selected from a lower resolution version of the MS-II and were then resimulated at much higher resolution. As a result, they are present in the MS-II along with thousands of other similar mass halos. A comparison of their assembly histories in the MS-II and in resimulations of 1000 times better resolution shows detailed agreement over a factor of 100 in mass growth. We publicly release halo catalogs and assembly trees for the MS-II in the same format within the same archive as those already released for the MS.

16 pages, 13 figures; matches version published in MNRAS. Halo catalogs and merger trees, along with movies, images, and additional information, are available at http://www.mpa-garching.mpg.de/galform/millennium-II

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• The hierarchical formation of the brightest cluster galaxies
• The redshift dependence of the structure of massive LCDM halos
• The spin and shape of dark matter haloes in the Millennium simulation of a LambdaCDM universe
• Effects of Baryons and Dissipation on the Matter Power Spectrum
• Assembly bias in the clustering of dark matter haloes
• The halo mass function from the dark ages through the present day
• The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth
• The Halo Mass Function: High-Redshift Evolution and Universality
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• Full-Sky Weak Lensing Simulation with 70 Billion Particles
• The Clustering of Massive Halos
• The assembly bias of dark matter haloes to higher orders
• Dark matter halo abundances, clustering and assembly histories at high redshift

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• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Very Compact Dense Galaxy Overdensity with δ ~ 130 Identified at z ~ 8: Implications for Early Protocluster and Cluster-Core Formation
• Spatial and luminosity distributions of galactic satellites
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Forward and backward galaxy evolution in comoving number density space
• Stability of Cool Cores During Galaxy Cluster Growth: A Joint $Chandra$/SPT Analysis of 67 Galaxy Clusters Along a Common Evolutionary Track Spanning 9 Gyr
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z=0.975 - Observing the assembly of a massive system
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Convergence of Galaxy Properties with Merger Tree Temporal Resolution
• Adaptive gravitational softening in GADGET
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• SMBH Seeds from Dissipative Dark Matter
• Abell 2744: Too much substructure for Lambda CDM?
• Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
• Cool circumgalactic gas of passive galaxies from cosmological inflow
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• The physical drivers of the atomic hydrogen-halo mass relation
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• Dilution in elliptical galaxies: Implications for the relation between metallicity, stellar mass and star formation rate
• BSG alignment of SDSS galaxy groups
• The Physical Origin of Galactic Conformity: From Theory to Observation
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• Strong stellar-driven outflows shape the evolution of galaxies at cosmic dawn
• The fraction of early-type galaxies in low redshift groups and clusters of galaxies
• Dwarf spheroidal galaxies and Bose-Einstein condensate dark matter
• OTELO Survey: Deep BVRI broadband photometry of the Groth strip. II Properties of X-ray Emitters
• Groups in the Millennium Simulation and in SDSS DR7
• ODIN: Where Do Lyman-alpha Blobs Live? Contextualizing Blob Environments within the Large-Scale Structure
• On the orbital and internal evolution of cluster galaxies
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Non-fiducial cosmological test from geometrical and dynamical distortions around voids
• Dark Matter Subhalos and the X-ray Morphology of the Coma Cluster
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
• On Physical Scales of Dark Matter Halos
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Void profile from Planck lensing potential map
• Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data
• What to expect from dynamical modelling of galactic haloes II: the spherical Jeans equation
• Galactic conformity measured in semi-analytic models
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• The Lives of High Redshift Mergers
• The connection between the cusp-to-core transformation and observational universalities of DM halos
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• Effects of voids on the reconstruction of the equation of state of Dark Energy
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• Cosmology on all scales: a two-parameter perturbation expansion
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Effect of inhomogeneities on high precision measurements of cosmological distances
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• The initial mass spectrum of old globular clusters in dwarf galaxies
• Tidal disruption events from massive black hole binaries: predictions for ongoing and future surveys
• Population III Star Clusters in the Reionized Universe
• MAMMOTH: Confirmation of Two Massive Galaxy Overdensities at $z=2.24$ with H$\alpha$ Emitters
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• The effects of halo alignment and shape on the clustering of galaxies
• The cross-power spectrum between 21cm emission and galaxies in hierarchical galaxy formation models
• Driving the Growth of the Earliest Supermassive Black Holes with Major Mergers of Host Galaxies
• The mass discrepancy acceleration relation in early-type galaxies: extended mass profiles and the phantom menace to MOND
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• Extended X-ray study of M49: the frontier of the Virgo Cluster
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
• Gravitationally Bound Bose Condensates with Rotation
• The median density of the Universe
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• The halo mass function of late-type galaxies from HI kinematics
• Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
• Cosmological parameter constraints from CMB lensing with cosmic voids
• The Structure of Reionization in Hierarchical Galaxy Formation Models
• Galaxy formation in the Planck cosmology II. Star formation histories and post-processing magnitude reconstruction
• Extending the halo mass resolution of $N$-body simulations
• Known Unknowns of Dark Matter Annihilation over Cosmic Time
• Ursa Major II - Reproducing the observed properties through tidal disruption
• Towards Cosmological Simulations of Dark Matter on Quantum Computers
• Velocity and mass bias in the distribution of dark matter halos
• A Possible Formation Scenario for Dwarf Spheroidal Galaxies I: Fiducial Model
• Clustering in the Phase Space of Dark Matter Haloes. II. Stable Clustering and Dark Matter Annihilation
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• Fossil groups in the Millennium simulation. From the brightest to the faintest galaxies during the past 8 Gyr
• On the Universality of the Bound-Zone Peculiar Velocity Profile
• Planes of satellites around simulated disc galaxies: I.- Finding high-quality planar configurations from positional information and their comparison to MW/M31 data
• The Carnegie-Irvine Galaxy Survey. IV. A Method to Determine the Average Mass Ratio of Mergers That Built Massive Elliptical Galaxies
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• Viscosity in cosmic fluids
• On the Nature of AGN and Star Formation Enhancement in the $z=3.1$ SSA22 Protocluster: The HST WFC3 IR View
• The Massively Accreting Cluster A2029
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Subhaloes gone Notts: Subhaloes as tracers of the dark matter halo shape
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• What to expect from dynamical modelling of galactic haloes
• Signatures of quenching in dwarf galaxies in local galaxy clusters
• The outermost stellar halo of NGC 5128 (Centaurus A): Radial structure
• Massive galaxy formation caught in action at z~5 with JWST
• Assembly history of subhalo populations in galactic and cluster sized dark haloes
• Dark Matter implications of Fermi-LAT measurement of anisotropies in the diffuse gamma-ray background
• Galaxy size trends as a consequence of cosmology
• 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
• Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• The virial mass distribution of ultra-diffuse galaxies in clusters and groups
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• Simulation view of galaxy clusters with low X-ray surface brightness
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity
• Cosmological Constraints from applying SHAM to rescaled cosmological simulations
• Diffuse Radio Sources in a Statistically Complete Sample of High Redshift Galaxy Clusters
• The $z\lesssim 1$ drop of cosmic dust abundance in a semi-analytic framework
• The MIP Ensemble Simulation: Local Ensemble Statistics in the Cosmic Web
• Effects of Completeness and Purity on Cluster Dark Energy Constraints
• A correlation between the number of satellites and the baryonic bulge-to-total ratio extending beyond the Local Group
• The Stellar Age Dependence of X-ray Emission from Normal Star-Forming Galaxies in the GOODS Fields
• Configuration entropy of the Cosmic Web: Can voids mimic the dark energy?
• Finding Strong Gravitational Lenses Through Self-Attention
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Network Analysis of Cosmic Structures : Network Centrality and Topological Environment
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Cosmic explosions, life in the Universe and the Cosmological Constant
• Constraints on dark matter annihilation and decay from the large-scale structure of the nearby universe
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Modelling the shapes of the largest gravitationally bound objects
• Estimating the Turn-Around Radii of Six Isolated Galaxy Groups in the Local Universe
• Self-similarity in the chemical evolution of galaxies and the delay time distribution of SNe Ia
• Rosella: A mock catalogue from the P-Millennium simulation
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• ENISALA: II. Distinct Star Formation and Active Galactic Nucleus Activity in Merging and Relaxed Galaxy Clusters
• The number of dwarf satellites of disk galaxies versus their bulge mass in the standard model of cosmology
• Life and death of a hero - Lessons learned from modeling the dwarf spheroidal Hercules: an incorrect orbit?
• A Versatile and Accurate Method for Halo Mass Determination from Phase-Space Distribution of Satellite Galaxies
• Joint reconstruction of galaxy clusters from gravitational lensing and thermal gas I. Outline of a non-parametric method
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Gravitational entropy and the cosmological no-hair conjecture
• The frequency of very young galaxies in the local Universe: II. The view from SDSS spectra
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• A methodology to select galaxies just after the quenching of star formation
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• Chemo-dynamical simulations of dwarf galaxy evolution
• Internal Cluster Structure
• Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo Cluster
• Hot Gas, Cold Gas and Sub-Halos in a Lyman-alpha Blob at Redshift 2.38
• The Cosmic Evolution of Halo Pairs: I. Global Trends
• What kind of science is cosmology?
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• The large-scale structure around the Fornax-Eridanus Complex
• HST F160W Imaging of Very Massive Galaxies at $1.5<z<3.0$: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates
• Stability of Satellite Planes in M31 II: Effects of the Dark Subhalo Population
• Massive Quiescent Galaxies at z>3 in The Millennium Simulation Populated by A Semi-analytic Galaxy Formation Model
• Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
• Group galaxy number density profiles far out: is the 'one-halo' term NFW out to $>10$ virial radii?
• Assembly Bias of Dwarf-sized Dark Matter Haloes
• Compact groups from semi-analytical models of galaxy formation -- I: a comparative study of frequency and nature
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Transient Weak-Lensing by Cosmological Dark Matter Microhaloes
• The miniJPAS survey: The galaxy populations in the most massive cluster in miniJPAS, mJPC2470-1771
• Void Galaxy Distribution: A Challenge for $\Lambda$CDM
• Comparing Galactic Center MSSM dark matter solutions to the Reticulum II gamma-ray data
• Leo IV & V - A possible dwarf galaxy pair ?
• Variation in the escape fraction of ionising photons from galaxies and the redshifted 21-cm power spectrum during reionization
• The impact of environment on the dynamical structure of satellite systems
• Compact groups from semi-analytical models of galaxy formation -- II: Different assembly channels
• Galaxy cluster mass accretion rates from IllustrisTNG
• Demographics of Tidal Disruption Events with L-Galaxies: I. Volumetric TDE rates and the abundance of Nuclear Star Clusters
• The Shape of Velocity Dispersion Profiles and the Dynamical State of Galaxy Clusters
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• Terapixel imaging of cosmological simulations
• The Size Evolution of Elliptical Galaxies
• Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
• TEGLIE: Transformer encoders as strong gravitational lens finders in KiDS
• Testing DARKexp against energy and density distributions of Millennium-II halos
• On the Evolution of the Bi-Modal Distribution of Galaxies in the Plane of Specific Star Formation Rate versus Stellar Mass
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Uncovering substructure with wavelets: proof of concept using Abell 2744
• The Stellar Halo and Tidal Streams of Messier 63
• The Massive and Distant Clusters of WISE Survey IX: High Radio Activity in a Merging Cluster
• An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies
• Star Formation and Chemical Enrichment in Protoclusters
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• Non-Parametric Spherical Jeans Mass Estimation with B-splines
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• Cusps in the center of galaxies: a real conflict with observations or a numerical artefact of cosmological simulations?
• Gemini IFU, VLA, and HST observation of the OH Megamaser Galaxy IRAS17526+3253
• A consistent model for both the HI and stellar mass functions of galaxies
• The Large-scale Effect of Environment on Galactic Conformity
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• The Tully-Fisher relation for flat galaxies
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Horizon Run 3: Topology as a Standard Ruler
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Prospects of Probing Dark Matter Condensates with Gravitational Waves
• Ridges in the Dark Energy Survey for cosmic trough identification
• SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
• On the influence of environment on star forming galaxies
• 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
• Ecology of dark matter haloes -II. Effects of interactions on the alignment of halo pairs
• Ultra-fine dark matter structure in the Solar neighbourhood
• Angular Momentum Evolution in Dark Matter Halos
• Close Galaxy Pairs at z = 3: A Challenge to UV Luminosity Abundance Matching
• Are compact groups hostile towards faint galaxies?
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• The spatial distribution of satellites in galaxy clusters
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• Co-evolution of supermassive black holes with galaxies from semi-analytic model: stochastic gravitational wave background and black hole clustering
• The mass accretion history of dark matter haloes down to Earth mass
• Interacting dark energy collapse with matter components separation
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• Lyman Alpha line properties at $z\simeq 3.78$ and their environmental dependence: a case study around a massive proto-cluster
• 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
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• Ubiquity of density slope oscillations in the central regions of galaxy and cluster-sized systems
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Clustering in the Phase Space of Dark Matter Haloes. I. Results from the Aquarius simulations
• Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
• The velocity function of dark matter halos at r=20 kpc: Remarkably little evolution since z ~ 4
• Evolution of Low Mass Galactic Subhalos and Dependence on Concentration
• Satellite galaxy abundance dependency on cosmology in Magneticum simulations
• VisIVOWeb: A WWW Environment for Large-Scale Astrophysical Visualization
• A hybrid multi resolution scheme to efficiently model the structure of reionization on the largest scales
• Psi-GAN: A power-spectrum-informed generative adversarial network for the emulation of large-scale structure maps across cosmologies and redshifts
• Enabling Radiative Transfer on AMR grids in CRASH
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Growth of Linear Perturbations in a Universe with Superfluid Dark Matter
• Complementary Cosmological Simulations
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• A two-phase model of galaxy formation: III. The formation of globular clusters
• Determining the time before or after a galaxy merger event
• Understanding the cosmic web
• Statistical Mechanics of Collisionless Orbits. V. The approach to equilibrium for idealized self-gravitating systems
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• Predicting the Merger Fraction of Lyman alpha Emitters from Redshift z~3 to z~7
• The Circular Velocity Function of Group Galaxies
• Growth and disruption in the Lyra complex
• The Schr$\ddot{o}$dinger-Poisson equations as the large-N limit of the Newtonian N-body system: applications to the large scale dark matter dynamics
• The cosmological distribution of compact object mergers from dynamical interactions with SMBH binaries
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• Is the correlation between the bulge-to-total stellar mass ratio and the number of dwarf galaxies in tension with $\Lambda$CDM?
• New radial velocities for dwarf galaxies in the Local Volume
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Satellite galaxies as better tracers of the Milky Way halo mass
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Solving the puzzle of subhalo spins
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• Cosmology and the Dark Matter Frontier
• 21 cm Intensity Mapping with the DSA-2000
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• The effect of environment on the mass assembly history of the Milky Way and M31
• On the Spin Bias of Satellite Galaxies in the Local Group-like Environment
• On the behaviour of streams in angle and frequency spaces in different potentials
• Dark Matter implications of the Fermi-LAT measurement of anisotropies in the diffuse gamma-ray background: status report
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• Merger rates of dark matter haloes: a comparison between EPS and N-body results
• Modelling the Evolution of Ly$\alpha$ Blobs and Ly$\alpha$ Emitters
• A Ly-alpha nebula at z~3.3
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• Extremely Isolated Galaxies I. Sample and Simulation Analysis
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• VEGA: Voids idEntification using Genetic Algorithm
• Low-resolution near-infrared spectroscopic signatures of unresolved ultracool companions to M dwarfs
• Consistent explanation for the cosmic-ray positron excess in p-wave Sommerfeld-enhanced dark matter annihilation
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• Indirect dark matter searches at ultrahigh energy neutrino detectors
• ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09
• The size and mass evolution of the massive galaxies over cosmic time
• Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9
• Large-k Limit of Multi-Point Propagators in the RG Formalism
• Independent Measurements of the Dynamical Masses of Six Galaxy Clusters in the Local Universe
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• The Way to Quench: Galaxy evolution in Abell 2142
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Does stellar mass assembly history vary with environment?
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• First use of large area SiPM matrices coupled with NaI(Tl) scintillating crystal for low energy dark matter search
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Back to basics: Little Red Dots as galaxies and dust-obscured AGNs in a synthetic NIRCam sky simulated with L-GalaxiesBH
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Subhalo abundance and satellite spatial distribution in Milky Way-Andromeda-like paired haloes
• The Angular Correlation Function as measured by the GLEAM-X Survey
• A Model For Intergalactic Filaments and Galaxy Formation During the First Gigayear
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• Predicting large scale cosmological structure evolution with generative adversarial network-based autoencoders
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• UHECR Acceleration in Dark Matter Filaments of Cosmological Structure Formation
• Universality of the halo mass function in modified gravity cosmologies
• 130GeV gamma-ray line through axion conversion
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• The structural elements of the cosmic web
• Fueling and feedback mechanisms at the nodes of the cosmic web
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• The Fornax Deep Survey (FDS) with the VST: III. Low Surface Brightness (LSB) dwarfs and Ultra Diffuse Galaxies (UDGs) in the center of the Fornax cluster
• Implications of the correlation between bulge-to-total baryonic mass ratio and the number of satellites for SAGA galaxies
• Off-center black hole seed formation? Implications for high and low redshift massive black holes
• The Distribution of Satellite Galaxies in the TNG100 Simulation