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

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• The Assembly of Matter in Galaxy Clusters
• First Structure Formation: A Simulation of Small Scale Structure at High Redshift
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Cited by in corpus (696)

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