Ahf: Amiga's Halo Finder

Abstract

Cosmological simulations are the key tool for investigating the different processes involved in the formation of the universe from small initial density perturbations to galaxies and clusters of galaxies observed today. The identification and analysis of bound objects, halos, is one of the most important steps in drawing useful physical information from simulations. In the advent of larger and larger simulations, a reliable and parallel halo finder, able to cope with the ever-increasing data files, is a must. In this work we present the freely available MPI parallel halo finder AHF. We provide a description of the algorithm and the strategy followed to handle large simulation data. We also describe the parameters a user may choose in order to influence the process of halo finding, as well as pointing out which parameters are crucial to ensure untainted results from the parallel approach. Furthermore, we demonstrate the ability of AHF to scale to high resolution simulations.

18 pages, 18 figures. Accepted for publication in ApJS

References in corpus (8)

• The Population of Dark Matter Subhaloes: Mass Functions and Average Mass Loss Rates
• Initial Conditions for Large Cosmological Simulations
• The Structure of Halos: Implications for Group and Cluster Cosmology
• VOBOZ: An Almost-Parameter-Free Halo-Finding Algorithm
• On the Correlation between Spin Parameter and Halo Mass
• Dark Matter Halo Profiles in Scale-Free Cosmologies
• The Bound Mass of Substructures in Dark Matter Halos
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum

Cited by in corpus (695)

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• Baryons Matter: Why Luminous Satellite Galaxies Have Reduced Central Masses
• The Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs
• ELVIS: Exploring the Local Volume in Simulations
• Why Baryons Matter: The Kinematics of Dwarf Spheroidal Satellites
• NIHAO IV: Core creation and destruction in dark matter density profiles across cosmic time
• The CAMELS project: Cosmology and Astrophysics with MachinE Learning Simulations
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• NIHAO XI: Formation of Ultra-Diffuse Galaxies by outflows
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• The Evolution of Central Group Galaxies in Hydrodynamical Simulations
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• Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space
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• CLARA's view on the escape fraction of Lyman-Alpha photons in high redshift galaxies
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• A general framework to test gravity using galaxy clusters I: Modelling the dynamical mass of haloes in $f(R)$ gravity
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• Cosmological simulation in tides: power spectra and halo shape responses, and shape assembly bias
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• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
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• Effects of large-scale environment on the assembly history of central galaxies
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• Unbound Particles in Dark Matter Halos
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• Do dark matter halos explain lensing peaks?
• Impacts of the physical data model on the forward inference of initial conditions from biased tracers
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• The Three Hundred Project: the stellar and gas profiles
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• Reconstructing cosmological initial conditions from galaxy peculiar velocities. II. The effect of observational errors
• Sowing black hole seeds: Direct collapse black hole formation with realistic Lyman-Werner radiation in cosmological simulations
• Dark matter haloes in modified gravity and dark energy: interaction rate, small-, and large-scale alignment
• Simulating the H2 content of high-redshift galaxies
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• Cosmological Structure Formation in Decaying Dark Matter Models
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• Probing Cosmic Dawn: Modelling the Assembly History, SEDs, and Dust Content of Selected $z\sim 9$ Galaxies
• Characterising the intra-cluster light in The Three Hundred simulations
• The cosmic web for density perturbations of various scales
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• Systematic Problems With Using Dark Matter Simulations to Model Stellar Halos
• On Physical Scales of Dark Matter Halos
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
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• The formation of entropy cores in non-radiative galaxy cluster simulations: SPH versus AMR
• Modified Gravity Spins Up Galactic Halos
• Cosmology inference at the field level from biased tracers in redshift-space
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Measuring nonlocal Lagrangian peak bias
• Galaxy clusters in simulations of the local Universe: a matter of constraints
• Constraints on decaying dark matter from weak lensing and cluster counts
• Galaxy clusters in local Universe simulations without density constraints: a long uphill struggle
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• The imprint of dark matter haloes on the size and velocity dispersion evolution of early-type galaxies
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• Parallel HOP: A Scalable Halo Finder for Massive Cosmological Data Sets
• NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• The velocity field in MOND cosmology
• The Effects of X-Ray Feedback from AGN on Host Galaxy Evolution
• Computation of the Halo Mass Function Using Physical Collapse Parameters: Application to Non-Standard Cosmologies
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• The formation and evolution of star clusters in interacting galaxies
• Where do galaxies end? Comparing measurement techniques of hydrodynamic-simulation galaxies' integrated properties
• DM haloes in the fifth-force cosmology
• The Halo Shape and Evolution of Polar Disc Galaxies
• The Dawn of Disk Formation in a Milky Way-sized Galaxy Halo: Thin Stellar Disks at $z>4$
• The stellar halo in Local Group Hestia simulations II. The accreted component
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• The stellar populations of high-redshift dwarf galaxies
• What to expect from dynamical modelling of cluster haloes II. Investigating dynamical state indicators with Random Forest
• Halo Abundance and Assembly History with Extreme-Axion Wave Dark Matter at $z\ge 4$
• The reionization of galactic satellite populations
• Clustering and lifetime of Lyman Alpha Emitters in the Epoch of Reionization
• Bayesian Inference of Initial Conditions from Non-Linear Cosmic Structures using Field-Level Emulators
• Constructing high-fidelity halo merger trees in AbacusSummit
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• A first estimate of the Milky Way dark matter halo spin
• High resolution simulations of the reionization of an isolated Milky Way - M31 galaxy pair
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• The segregation of baryons and dark matter during halo assembly
• The galaxy-halo size relation of low-mass galaxies in FIRE
• The Three Hundred: Cluster Dynamical States and Relaxation Time Scale
• An alternative method to generate pre-initial conditions for cosmological $N$-body simulations
• High-redshift quasars and their host galaxies II: multiphase gas and stellar kinematics
• Constraining interacting dark energy models with the halo concentration-mass relation
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• A hidden population of massive black holes in simulated dwarf galaxies
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Redshift evolution of the dark matter haloes shapes
• Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
• How to Build a Catalogue of Linearly-Evolving Cosmic Voids
• Running with BICEP2: Implications for Small-Scale Problems in CDM
• Bullet Clusters in the MareNostrum Universe
• Modelling the fraction of Lyman Break Galaxies with strong Lyman alpha emission at 5 < z < 7
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• Comparing galactic satellite properties in hydrodynamical and Nbody simulations
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Enhanced star formation in $z\sim 6$ quasar companions
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• Tidal evolution of cored and cuspy dark matter halos
• The evolution of dwarf galaxy satellites with different dark matter density profiles in the ErisMod simulations. I. The early infalls
• On the radial acceleration relation of $\Lambda$CDM satellite galaxies
• Gravitational wave fossils in nonlinear regime: halo tidal bias and intrinsic alignments from gravitational wave separate universe simulations
• Vector dark energy and high-z massive clusters
• Quintessential Scale Dependence from Separate Universe Simulations
• Quadratic shape biases in three-dimensional halo intrinsic alignments
• Spatial variations of the fine-structure constant in symmetron models
• Subhaloes gone Notts: Subhaloes as tracers of the dark matter halo shape
• Sussing Merger Trees: Stability and Convergence
• The Three Hundred project: A Machine Learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps
• Subhaloes gone Notts: the clustering properties of subhaloes
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• Boosting hierarchical structure formation with scalar-interacting dark matter
• Probing modified gravity via the mass-temperature relation of galaxy clusters
• Delayed Photons from Binary Evolution Help Reionize the Universe
• Observing Merger Trees in a New Light
• The Three Hundred Project: The gas disruption of infalling objects in cluster environments
• Realistic HI scale heights of Milky Way-mass galaxies in the FIREbox cosmological volume
• Halo orbits in cosmological disk galaxies: tracers of formation history
• Satellite galaxies in groups in the CIELO Project I. Gas removal from galaxies and its re-distribution in the intragroup medium
• Effective Window Function for Lagrangian Halos
• Hydrodynamical structure formation in Milgromian cosmology
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• Dissecting the spin distribution of Dark Matter halos
• Leavers and remainers: Galaxies split by group-exit
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• First Structure Formation under the Influence of Gas-Dark Matter Streaming Velocity and Density: Impact of the Baryons-trace-dark matter Approximation
• Beta-Skeleton Analysis of the Cosmic Web
• Dark matter halos in the multicomponent model. I. Substructure
• Toward an Optimal Sampling of Peculiar Velocity Surveys For Wiener Filter Reconstructions
• The history of stellar metallicity in a simulated disc galaxy
• Seeking Observable Imprints of Small-Scale Structure on the Properties of Dark Matter Haloes
• Cold versus Warm Dark Matter simulations of a galaxy group
• Enabling parallel computing in CRASH
• The cosmological free-free signal from galaxy groups and clusters
• Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• The Three Hundred Project: the evolution of physical baryon profiles
• On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters
• Through a Smoother Lens: An expected absence of LCDM substructure detections from hydrodynamic and dark matter only simulations
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• Reionization of the Milky Way, M31, and their satellites I: reionization history and star formation
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• Towards Accurate Field-Level Inference of Massive Cosmic Structures
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Brightest Cluster Galaxies Trace Weak Lensing Mass Bias and Halo Triaxiality in The Three Hundred Project
• Magnetogenesis at Cosmic Dawn: Tracing the Origins of Cosmic Magnetic Fields
• An accurate method of modeling cluster scaling relations in modified gravity
• One-Two Quench: A Double Minor Merger Scenario
• Volume Statistics as a Probe of Large-Scale Structure
• Probing Theories of Gravity with Phase Space-Inferred Potentials of Galaxy Clusters
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Dynamics of Stellar Disk Tilting from Satellite Mergers
• The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function
• Warm Dark Haloes Accretion Histories and their Gravitational Signatures
• EDGE: The shape of dark matter haloes in the faintest galaxies
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• Effective Dark Matter Halo catalog in $f(R)$ gravity
• Explaining the chemical trajectories of accreted and in-situ halo stars of the Milky Way
• Measurement of Void Bias Using Separate Universe Simulations
• Tracking Halo Orbits and Their Mass Evolution around Large-scale Filaments
• The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $\le z\le$ 0.60 and $4\times 10^{14}$ M${}_{\odot }$ $\le {\text{M}}_{500}\le 30\times 10^{14}$ M${}_{\odot }$
• Stellar cluster formation in a Milky Way-sized galaxy at z>4 -- I. The proto-globular cluster population and the imposter amongst us
• Testable predictions of outside-in age gradients in dwarf galaxies of all types
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• Virgo: an unlikely cluster of galaxies because of its environment
• Simplified galaxy formation with mesh-less hydrodynamics
• Revisiting the screening mechanism in $f(R)$ gravity
• Merger types forming the Virgo cluster in recent gigayears
• Estimation of the masses in the Local Group by Gradient Boosted Decision Trees
• Analytic and numerical realisations of a disk galaxy
• Star Formation and Gas Phase History of the Cosmic Web
• Particle tagging and its implications for stellar population dynamics
• Decaying warm dark matter and structure formation
• The luminosity function of diverse satellite galaxy systems
• The Observable Thermal and Kinetic Sunyaev-Zel'dovich Effect in Merging Galaxy Clusters
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Is there a disk of satellites around the Milky Way?
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Simulating Globular Clusters in Dark Matter Sub-Halos
• A high fidelity Milky Way simulation with Kraken, Gaia-Enceladus, and Sequoia analogues: clues to their accretion histories
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Dark matter halos in the multicomponent model. II. Density profiles of galactic halos
• Metallicity profiles of Ultra Diffuse Galaxies in NIHAO simulations
• Local Group progenitors: Lyman Alpha bright?
• The Origin of Neutral Hydrogen Clouds in Nearby Galaxy Groups: Exploring the Range Of Galaxy Interactions
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• Galactic halos in cosmology with long-range scalar DM interaction
• The Past History of Galaxy Clusters told by their present neighbors
• Numerical simulations of bar formation in the Local Group
• Effective dark matter power spectra in $f(R)$ gravity
• Halo abundances and shear in void models
• The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations I: Unique Galaxy Morphologies in Imaging
• The tangential velocity of M31: CLUES from constrained simulations
• Anisotropic satellite accretion onto the Local Group with HESTIA
• CLUES about M33: the reversed radial stellar age gradient in the outskirts of Triangulum galaxy
• A study on Cubic Galileon Gravity Using N-body Simulations
• The features of the Cosmic Web unveiled by the flip-flop field
• Rapid Simulations of Halo and Subhalo Clustering
• N-body simulations, halo mass functions, and halo density profile in $f(T)$ gravity
• Gravitational lensing in WDM cosmologies: The cross section for giant arcs
• A deeper look into the structure of ΛCDM haloes: correlations between halo parameters from Einasto fits
• The Sunyaev-Zeldovich effect in superclusters of galaxies using gasdynamical simulations: the case of Corona Borealis
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• The undiscovered ultra-diffuse galaxies of the Local Group
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Probing modified gravity in cosmic filaments
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies
• Carbon envelopes around merging galaxies at z ~ 4.5
• Cornerstone: Octree Construction Algorithms for Scalable Particle Simulations
• The tilting rate of the Milky Way's disc
• Origin of stellar prolate rotation in a cosmologically simulated faint dwarf galaxy
• Estimates of cluster masses in screened modified gravity
• MEGA: Merger graphs of structure formation
• Mass Estimation of Planck Galaxy Clusters using Deep Learning
• Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
• Modified Baryonic Dynamics: two-component cosmological simulations with light sterile neutrinos
• Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters
• Validating galaxy clustering models with Fixed & Paired and Matched-ICs simulations: application to Primordial Non-Gaussianities
• On the coldness of the local Hubble flow: the role of baryons
• Predicting the frequencies of young and of tiny galaxies
• Angular Momentum Evolution in Dark Matter Halos
• A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
• Universal subhalo accretion in cold and warm dark matter cosmologies
• Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
• Simulated vs. observed UV emission at high redshift: a hint for a clumpy ISM?
• Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• Velocity dispersion vs cluster mass: a new scaling law with The Three Hundred clusters
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• N-body Simulations of $\gamma$ Gravity
• Halo Growth and Merger Rates as a Cosmological Test
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• Correlation between centre offsets and gas velocity dispersion of galaxy clusters in cosmological simulations
• The infall region as a complementary probe to cluster abundance
• Subhalo abundance matching in $f(R)$ gravity
• The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations
• Haloes at the ragged edge: The importance of the splashback radius
• The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
• A comparison of ${\text{H}}_2$ formation models at high redshift
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• Constrained simulations and excursion sets: understanding the risks and benefits of `genetically modified' haloes
• The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
• Massive Galaxies at High-z: Assembly Patterns, Structure & Dynamics in the Fast Phase of Galaxy Formation
• Cluster Assembly Times as a Cosmological Test
• Relative baryon-dark matter velocities in cosmological zoom simulations
• Diverse Properties of Interstellar Medium Embedding Gamma-Ray Bursts at the Epoch of Reionization
• Higher moments of primordial non-Gaussianity and N-body simulations
• CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments
• Massive Gravity wrapped in the Cosmic Web
• Are there more galaxies than we see around high-$z$ quasars?
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Over-cooled haloes at z > 10: a route to form low-mass first stars
• A MARVEL-ous study of how well galaxy shapes reflect Dark Matter halo shapes in Cold Dark Matter Simulations
• Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• Identifying Galaxy Cluster Mergers with Deep Neural Networks using Idealized Compton-y and X-ray maps
• The emergence of globular clusters and globular-cluster-like dwarfs
• Exploring the centre of mass properties of LG-like galaxies
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
• Great Balls of FIRE IV. The contribution of massive star clusters to the astrophysical population of merging binary black holes
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations II: Unique Stellar Kinematics in Integral Field Unit Spectroscopy
• Degeneracies between Modified Gravity and Baryonic Physics
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Tensor classification of structure in smoothed particle hydrodynamics density fields
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• CLUES to the past: Local Group progenitors amongst high-redshift Lyman Break Galaxies
• Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
• Angular momentum - mass relation for dark matter haloes
• Milky Way Halo Vibrations and Incommensurate Stream Velocities
• The THREEHUNDRED project: the effect of baryon processes at galaxy cluster scale
• Dark matter haloes: a multistream view
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Solving the puzzle of subhalo spins
• The Three Hundred Project: The stellar angular momentum evolution of cluster galaxies
• Probabilistic Estimators of Lagrangian Shape Biases: Universal Relations and Physical Insights
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Scalable Streaming Tools for Analyzing $N$-body Simulations: Finding Halos and Investigating Excursion Sets in One Pass
• Beyond the Halo: Redefining environment with unbound matter in N-body simulations
• A Simulated Annealing algorithm to quantify patterns in astronomical data
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• The Three Hundred: The existence of massive dark matter-deficient satellite galaxies in cosmological simulations
• How do dwarf galaxies acquire their mass & when do they form their stars?
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• Intermediate Mass Ratio Inspirals in Milky Way Galaxies
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• HIKER: a halo-finding method based on kernel-shift algorithm
• Identifying Halos in Cosmological Simulations with Continuous Wavelet Analysis: The 2D Case
• Metamorphosis of dwarf halo density profile under dark matter decays
• A Generative Model for Realistic Galaxy Cluster X-ray Morphologies
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• Cosmic wallflowers: the circumgalactic origins of isolated ultra-compact star clusters at $z>7$
• Chameleon Screening Depends on the Shape and Structure of NFW Halos
• Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
• Inference of morphology and dynamical state of nearby $Planck$-SZ galaxy clusters with Zernike polynomials
• The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
• Cosmological Simulations of Satellites around Isolated Dwarf Galaxies
• The Role of Mass and Environment on Satellite distributions around Milky Way analogs in the Romulus25 simulation
• The effects on structure of a momentum coupling between dark matter and quintessence
• Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• Cosmological simulations with rare and frequent dark matter self-interactions
• The PARADIGM project II: The lifetimes and quenching of satellites in Milky Way-mass haloes
• The Hierarchical Structure of Galactic Haloes: Generalised N-Dimensional Clustering with CluSTAR-ND
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• Variable gravitational potential of Milky Way analogues in HESTIA suite
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• Constructing Merger Trees of Density Peaks Using Phase-Space Watershed Segmentation Algorithm
• The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology
• Segmenting proto-halos with vision transformers
• Generating Galaxy Clusters Mass Density Maps from Mock Multiview Images via Deep Learning
• Cosmic voids and BAO with relative baryon-CDM perturbations
• Reionization in HESTIA: Studying reionization in the LG through zoom simulations
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• The origin of the intra-cluster light in The Three Hundred simulations
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• Predicting Halo Formation Time Using Machine Learning
• Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
• The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?
• Ginnungagap -- a massively parallel cosmological initial conditions generator
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• CWTHF: Subhalo Identification with Continuous Wavelet Transform
• Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales
• The halo finding problem revisited: a deep revision of the ASOHF code
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• The Nun Path: The Evolution and Quenching of Satellite Galaxies
• An anti-correlation between barycentre offsets and velocity dispersion for highest overdensity subhalos in cosmological simulations
• Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints
• Tidal adaptive softening and artificial fragmentation in cosmological simulations
• An Anti-halo Void Catalogue of the Local Super-Volume
• CHEX-MATE: Morphological analysis of the sample
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations