Gravitationally Consistent Halo Catalogs and Merger Trees for Precision Cosmology
arXiv:1110.4370 · doi:10.1088/0004-637X/763/1/18
Abstract
We present a new algorithm for generating merger trees and halo catalogs which explicitly ensures consistency of halo properties (mass, position, and velocity) across timesteps. Our algorithm has demonstrated the ability to improve both the completeness (through detecting and inserting otherwise missing halos) and purity (through detecting and removing spurious objects) of both merger trees and halo catalogs. In addition, our method is able to robustly measure the self-consistency of halo finders; it is the first to directly measure the uncertainties in halo positions, halo velocities, and the halo mass function for a given halo finder based on consistency between snapshots in cosmological simulations. We use this algorithm to generate merger trees for two large simulations (Bolshoi and Consuelo) and evaluate two halo finders (ROCKSTAR and BDM). We find that both the ROCKSTAR and BDM halo finders track halos extremely well; in both, the number of halos which do not have physically consistent progenitors is at the 1-2% level across all halo masses. Our code is publicly available at http://code.google.com/p/consistent-trees . Our trees and catalogs are publicly available at http://hipacc.ucsc.edu/Bolshoi/ .
15 pages, 12 figures. Minor revisions to match ApJ accepted version
References in corpus (9)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The hierarchical formation of the brightest cluster galaxies
- The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
- Building Merger Trees from Cosmological N-body Simulations
- The Nearly Universal Merger Rate of Dark Matter Haloes in Lambda-CDM Cosmology
- The growth of dark matter halos: evidence for significant smooth accretion
- Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
- The statistical properties of LCDM halo formation
- Bayesian inference of galaxy formation from the K-band luminosity function of galaxies: tensions between theory and observation
Cited by in corpus (476)
- The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
- Physical Models of Galaxy Formation in a Cosmological Framework
- UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
- CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST
- The Illustris Simulation: Public Data Release
- Rotation-Dependent Catastrophic Disruption of Gravitational Aggregates
- Dependence of the outer density profiles of halos on their mass accretion rate
- EMERGE - An empirical model for the formation of galaxies since
- Simulating cosmic structure formation with the GADGET-4 code
- A White Paper on keV Sterile Neutrino Dark Matter
- The Connection between Galaxies and Dark Matter Structures in the Local Universe
- A universal model for halo concentrations
- Not so lumpy after all: modeling the depletion of dark matter subhalos by Milky Way-like galaxies
- The size - virial radius relation of galaxies
- ELVIS: Exploring the Local Volume in Simulations
- The Relation Between SFR and Stellar Mass for Galaxies at 3.5 6.5 in CANDELS
- Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
- The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations
- An accurate physical model for halo concentrations
- Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results
- Too Big to Fail in the Local Group
- The Galaxy-Halo Connection Over The Last 13.3 Gyrs
- Halo and Subhalo Demographics with Planck Cosmological Parameters: Bolshoi-Planck and MultiDark-Planck Simulations
- Formation of massive black holes in rapidly growing pre-galactic gas clouds
- Splashback in accreting dark matter halos
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Modeling the clustering and halo occupation distribution of BOSS-CMASS galaxies in the Final Data Release
- Galaxy Assembly Bias: A Significant Source of Systematic Error in the Galaxy-Halo Relationship
- Milky Way Satellite Census. II. Galaxy--Halo Connection Constraints Including the Impact of the Large Magellanic Cloud
- The Dark Side of Galaxy Color
- N-body Dark Matter Haloes with simple Hierarchical Histories
- The upper bound on the lowest mass halo
- Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection
- Sweating the small stuff: simulating dwarf galaxies, ultra-faint dwarf galaxies, and their own tiny satellites
- A Simple Technique for Predicting High-Redshift Galaxy Evolution
- The angular momentum distribution and baryon content of star forming galaxies at z~1-3
- Characterizing mass, momentum, energy and metal outflow rates of multi-phase galactic winds in the FIRE-2 cosmological simulations
- A Critical Assessment of Stellar Mass Measurement Methods
- Disentangling satellite galaxy populations using orbit tracking in simulations
- The First Population II Stars Formed in Externally Enriched Mini-halos
- Quasars Probing Quasars VI. Excess HI Absorption Within One Proper Mpc of z~2 Quasars
- Star cluster formation in cosmological simulations. I. Properties of young clusters
- The Universe at z>10: Predictions for JWST from the UniverseMachine DR1
- Using Cumulative Number Densities to Compare Galaxies across Cosmic Time
- Organized Chaos: Scatter in the relation between stellar mass and halo mass in small galaxies
- The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
- The Concentration Dependence of the Galaxy-Halo Connection: Modeling Assembly Bias with Abundance Matching
- Semi-Analytic Galaxies - I. Synthesis of environmental and star-forming regulation mechanisms
- The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
- Phat ELVIS: The inevitable effect of the Milky Way's disk on its dark matter subhaloes
- Mergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster Virial Radii
- Beyond Assembly Bias: Exploring Secondary Halo Biases for Cluster-size Haloes
- A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations
- Forward Modeling of Large-Scale Structure: An open-source approach with Halotools
- MassiveNuS: Cosmological Massive Neutrino Simulations
- Astraeus I: The interplay between galaxy formation and reionization
- Proper Motions, Orbits, and Tidal Influences of Milky Way Dwarf Spheroidal Galaxies
- The clustering of galaxies at z~0.5 in the SDSS-III Data Release 9 BOSS-CMASS sample: a test for the LCDM cosmology
- Sussing Merger Trees: The Merger Trees Comparison Project
- The Caterpillar Project: A Large Suite of Milky Way Sized Halos
- The Topology of the Cosmic Web in Terms of Persistent Betti Numbers
- Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
- Beyond Halo Mass: Galactic Conformity as a Smoking Gun of Central Galaxy Assembly Bias
- The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
- Dark Matter Constraints from a Unified Analysis of Strong Gravitational Lenses and Milky Way Satellite Galaxies
- The Formation of Ultra-Diffuse Galaxies in the RomulusC Galaxy Cluster Simulation
- Satellite quenching timescales in clusters from projected phase space measurements matched to simulated orbits
- Satellite Dwarf Galaxies in a Hierarchical Universe: The Prevalence of Dwarf-Dwarf Major Mergers
- Satellites of LMC-Mass Dwarfs: Close Friendships Ruined by Milky Way Mass Halos
- A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
- The Dependence of Subhalo Abundance on Halo Concentration
- The Eating Habits of Milky Way Mass Halos: Destroyed Dwarf Satellites and the Metallicity Distribution of Accreted Stars
- On Detecting Halo Assembly Bias with Galaxy Populations
- The Growth of Black Holes from Population III Remnants in the Renaissance Simulations
- The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies
- HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
- Dissecting the properties of optically-thick hydrogen at the peak of cosmic star formation history
- The Dark Side of Galaxy Color: evidence from new SDSS measurements of galaxy clustering and lensing
- The Recent Burstiness of Star Formation in Galaxies at z~4.5 from H Measurements
- Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
- Understanding the Structural Scaling Relations of Early-Type Galaxies
- Assessing Colour-dependent Occupation Statistics Inferred from Galaxy Group Catalogues
- A survey of high- galaxies: SERRA simulations
- Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites
- Generating Merger Trees for Dark Matter Haloes: A Comparison of Methods
- Faint dwarfs as a test of DM models: WDM vs. CDM
- The splashback radius of halos from particle dynamics. I. The SPARTA algorithm
- A statistical investigation of the mass discrepancy-acceleration relation
- SHAM Beyond Clustering: New Tests of Galaxy-Halo Abundance Matching with Galaxy Groups
- Splashback Shells of Cold Dark Matter Halos
- Constraints on Assembly Bias from Galaxy Clustering
- UNIT project: Universe -body simulations for the Investigation of Theoretical models from galaxy surveys
- Connecting massive galaxies to dark matter halos in BOSS - I. Is galaxy color a stochastic process in high-mass halos?
- Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
- Coming of Age in the Dark Sector: How Dark Matter Haloes grow their Gravitational Potential Wells
- Modeling evolution of dark matter substructure and annihilation boost
- Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources
- The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
- Planes of satellites around Milky Way/M31-mass galaxies in the FIRE simulations and comparisons with the Local Group
- Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
- The Tully-Fisher and mass-size relations from halo abundance matching
- MultiDark-Galaxies: data release and first results
- Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
- The critical dark matter halo mass for Population III star formation: dependence on Lyman-Werner radiation, baryon-dark matter streaming velocity, and redshift
- Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
- Major Mergers Going Notts: Challenges for Modern Halo Finders
- Confronting Simulations of Optically Thick Gas in Massive Halos with Observations at z=2-3
- Cosmic web anisotropy is the primary indicator of halo assembly bias
- The clustering of ALFALFA galaxies: dependence on HI mass, relationship to optical samples & clues on host halo properties
- Dissecting the Evolution of Dark Matter Subhaloes in the Bolshoi Simulation
- Predicting the locations of possible long-lived low-mass first stars: Importance of satellite dwarf galaxies
- The clustering of luminous red galaxies at z 0.7 from eBOSS and BOSS data
- On the Physical Origin of Galactic Conformity
- Concentrations of Dark Haloes Emerge from Their Merger Histories
- Signatures of Velocity-Dependent Dark Matter Self-Interactions in Milky Way-mass Halos
- Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
- The intrinsic characteristics of galaxies on the SFR-stellar mass plane at 1.2<z<4: I. the correlation between stellar age, central density and position relative to the main sequence
- Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
- The CAMELS project: public data release
- Clustering properties of -selected galaxies at
- The Galaxy Clustering Crisis in Abundance Matching
- The Milky Way's Halo and Subhalos in Self-Interacting Dark Matter
- Reignition of Star Formation in Dwarf Galaxies
- Universal at last? The splashback mass function of dark matter halos
- Modeling the Impact of Baryons on Subhalo Populations with Machine Learning
- Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
- SURFS: Riding the waves with Synthetic UniveRses For Surveys
- Properties of Dark Matter Halos as a Function of Local Environment Density
- Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
- A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties
- The Edge of the Galaxy
- GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
- Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
- The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe
- Tracing the first stars and galaxies of the Milky Way
- Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization
- Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
- Extinguishing the FIRE: environmental quenching of satellite galaxies around Milky Way-mass hosts in simulations
- Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
- Forming massive seed black holes in high-redshift quasar host progenitors
- EMERGE: Empirical predictions of galaxy merger rates since
- Properties of Resonantly Produced Sterile Neutrino Dark Matter Subhalos
- On The History and Future of Cosmic Planet Formation
- On the Segregation of Dark Matter Substructure
- Empirical constraints on the formation of early-type galaxies
- Constraining the HI-Halo Mass Relation From Galaxy Clustering
- Interpreting Short Gamma Ray Burst Progenitor Kicks and Time Delays Using the Host Galaxy-Dark Matter Halo Connection
- A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
- Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
- Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way
- The impact of an evolving stellar initial mass function on early galaxies and reionisation
- The Scale-Dependence of Halo Assembly Bias
- An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
- Mock Lightcones and Theory Friendly Catalogs for the CANDELS Survey
- Halo Histories vs. Galaxy Properties at z=0 II: Large-Scale Galactic Conformity
- The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
- How Biased Are Halo Properties in Cosmological Simulations?
- Cosmological Constraint on and from Cluster Abundances using the Optical-Spectroscopic SDSS Catalog
- Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
- Assembly of filamentary void galaxy configurations
- YZiCS: Preprocessing of dark halos in the hydrodynamic zoom-in simulation of clusters
- Sussing Merger Trees: the influence of the halo finder
- Rhapsody. II. Subhalo Properties and the Impact of Tidal Stripping From a Statistical Sample of Cluster-Size Halos
- The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
- On the influence of halo mass accretion history on galaxy properties and assembly bias
- Motivations for a Large Self-Interacting Dark Matter Cross Section from Milky Way Satellites
- Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
- Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to M
- First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
- Evolution of star clusters in a cosmological tidal field
- Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
- Virial scaling of galaxies in clusters: bright to faint is cool to hot
- CLASH-VLT: Abell~S1063. Cluster assembly history and spectroscopic catalogue
- Dissipative Dark Matter on FIRE: I. Structural and kinematic properties of dwarf galaxies
- Self-consistent semi-analytic models of the first stars
- Predicting the density profiles of the first halos
- The Halos and Environments of Nearby Galaxies (HERON) I: Imaging, Sample Characteristics, and Envelope Diameters
- The Galaxy Progenitors of Stellar Streams around Milky Way-mass Galaxies in the FIRE Cosmological Simulations
- GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
- The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
- First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations
- How Accurately Can We Detect the Splashback Radius of Dark Matter Halos and its Correlation With Accretion Rate?
- Observing dynamical friction in galaxy clusters
- The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
- Flybys, orbits, splashback: subhalos and the importance of the halo boundary
- Formation of disk galaxies in preheated media: a preventative feedback model
- A Predicted Correlation Between Age Gradient and Star Formation History in FIRE Dwarf Galaxies
- The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
- Astraeus V: The emergence and evolution of metallicity scaling relations during the Epoch of Reionization
- : Learning Galaxy Properties from Merger Trees
- ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
- Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
- Mind the Gap: Tightening the Mass-Richness Relation with Magnitude Gaps
- Correlations between Triaxial Shapes and Formation History of Dark Matter Haloes
- Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
- Dynamical Evolution of Primordial Dark Matter Haloes through Mergers
- On the stark difference in satellite distributions around the Milky Way and Andromeda
- Uncertainties associated with the backward integration of dwarf satellites using simple parametric potentials
- Voronoi volume function: A new probe of cosmology and galaxy evolution
- Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
- Comprehensive Assessment of the Too-Big-to-Fail Problem
- Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
- Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
- The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
- Climbing Halo Merger Trees with TreeFrog
- The Secondary Spin Bias of Dark Matter Haloes
- Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
- Does the Galaxy-Halo Connection Vary with Environment?
- The ALMA Spectroscopic Survey in the HUDF: A model to explain observed 1.1 and 0.85 millimeter dust continuum number counts
- Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
- The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud
- On the stability of tidal streams in action space
- LCDM halo substructure properties revealed with high resolution and large volume cosmological simulations
- Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation
- Galaxy assembly bias of central galaxies in the Illustris simulation
- The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
- Dark Matter Halo Properties vs. Local Density and Cosmic Web Location
- The Phase Space Structure of Dark Matter Halos
- Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
- Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations
- Unbound Particles in Dark Matter Halos
- The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
- Formation of globular clusters in dwarf galaxies of the Local Group
- Semi-Analytic Galaxies - II. Revealing the role of environmental and mass quenching in galaxy formation
- Modeling Evolution of Galactic Bars at Cosmic Dawn
- Astraeus II: Quantifying the impact of cosmic variance during the Epoch of Reionization
- How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
- Cosmic CARNage I: on the calibration of galaxy formation models
- A cosmological context for compact massive galaxies
- A Parametric Model for Self-Interacting Dark Matter Halos
- The effects of LMC-mass environments on their dwarf satellite galaxies in the FIRE simulations
- The AGN-galaxy-halo connection: The distribution of AGN host halo masses to z=2.5
- Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
- CDM Predictions for the Satellite Population of M33
- A dynamics-based density profile for dark haloes -- II. Fitting function
- Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
- Globular cluster numbers in dark matter haloes in a dual formation scenario: an empirical model within EMERGE
- Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
- Surrogate modelling the Baryonic Universe I: The colour of star formation
- Violent starbursts and quiescence induced by FUV radiation feedback in metal-poor galaxies at high-redshift
- The importance of galaxy formation histories in models of reionization
- A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
- The Sheet of Giants: Unusual Properties of the Milky Way's Immediate Neighbourhood
- Probing the galaxy-halo connection with total satellite luminosity
- The Effects of Varying Cosmological Parameters on Halo Substructure
- Orbital dynamics and histories of satellite galaxies around Milky Way-mass galaxies in the FIRE simulations
- How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
- On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
- Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
- A New Method to Constrain the Appearance and Disappearance of Observed Jellyfish Galaxy Tails
- The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
- The observable properties of galaxy accretion events in Milky Way-like galaxies in the FIRE-2 cosmological simulations
- Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
- Identifying Direct Collapse Black Hole Seeds through their Small Host Galaxies
- The evolution of galaxy intrinsic alignments in the MassiveBlack II universe
- Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
- On the evolution of cluster scaling relations
- Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
- How long do high-redshift massive black hole seeds remain outliers in black hole vs. host galaxy relations?
- UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
- AstraeusIV : Quantifying the star formation histories of galaxies in the Epoch of Reionization
- Preprocessing, mass loss and mass segregation of galaxies in DM simulations
- Constructing high-fidelity halo merger trees in AbacusSummit
- Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
- Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
- Cosmic variance in the nanohertz gravitational wave background
- Generating Synthetic Cosmological Data with GalSampler
- Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
- Emission from the Ionized Gaseous Halos of Low Redshift Galaxies and Their Neighbors
- Observational Measures of Halo Properties Beyond Mass
- Milky Way-est: Cosmological Zoom-in Simulations with Large Magellanic Cloud and Gaia-Sausage-Enceladus Analogs
- What sets the splashback radius of dark matter haloes: accretion history or other properties?
- The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters
- The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
- Galaxy and Mass Assembly (GAMA): Formation and Growth of Elliptical Galaxies in the Group Environment
- Possibilities and Limitations of Kinematically Identifying Stars from Accreted Ultra-Faint Dwarf Galaxies
- The Clustering of X-ray Luminous Quasars
- Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
- The formation of the brightest cluster galaxy and intracluster light in cosmological N-body simulations with the Galaxy Replacement Technique
- DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
- The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
- A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to in the Hyper Suprime-Cam survey
- Understanding large-scale structure in the SSA22 protocluster region using cosmological simulations
- Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?
- Constraining Self-Interacting Dark Matter with Dwarf Spheroidal Galaxies and High-resolution Cosmological -body Simulations
- Comparison of Observed Galaxy Properties with Semianalytic Model Predictions using Machine Learning
- AGN-driven quenching of satellite galaxies
- Observing Merger Trees in a New Light
- The impact of filamentary accretion of subhaloes on the shape and orientation of haloes
- The assembly bias of emission line galaxies
- Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
- The dependence of subhalo abundance matching on galaxy photometry and selection criteria
- On the Prevalence of Super-Massive Black Holes over Cosmic Time
- ROGER: Reconstructing Orbits of Galaxies in Extreme Regions using machine learning techniques
- The dark side of FIRE: predicting the population of dark matter subhaloes around Milky Way-mass galaxies
- Astraeus VI: Hierarchical assembly of AGN and their large-scale effect during the Epoch of Reionization
- Insights into the origin of halo mass profiles from machine learning
- Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
- Turning Around along the Cosmic Web
- The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
- Assessing the accuracy of cosmological parameters estimated from velocity -- density comparisons via simulations
- Hierarchical structure of the cosmic web and galaxy properties
- External Enrichment of Minihalos by the First Supernovae
- Astraeus VIII: A new framework for Lyman- emitters applied to different reionisation scenarios
- First estimate of the local value of the baryonic streaming velocity
- Structure and dynamics in low density regions: galaxy-galaxy correlations inside cosmic voids
- The IllustrisTNG Simulations: Public Data Release
- The trajectories of galaxies in groups: mass loss and preprocessing
- Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
- Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
- Some observational tests of a minimal galaxy formation model
- Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
- The First Fall is the Hardest: The Importance of Peculiar Galaxy Dynamics at Infall Time for Tidal Stripping Acting at the Centers of Groups and Clusters
- The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
- Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
- Modeling Redshift-Space Clustering with Abundance Matching
- New empirical constraints on the cosmological evolution of gas and stars in galaxies
- Direct-collapse black hole formation induced by internal radiation of host halos
- Astraeus III: The environment and physical properties of reionization sources
- Spatial and orbital planes of the Milky Way satellites: unusual but consistent with CDM
- Emission line ratios for the Circumgalactic Medium and the "Bimodal" Nature of Galaxies
- A minimal empirical model for the cosmic far-infrared background anisotropies
- Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
- Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
- COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
- On the general nature of 21cm-Lyman- emitters cross-correlations during reionisation
- On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
- Differentiable Predictions for Large Scale Structure with SHAMNet
- Constraining the scatter in the galaxy-halo connection at Milky Way masses
- Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
- On The Effect of Environment on Line Emission from the Circumgalactic Medium
- Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
- A multi-tracer empirically-driven approach to line-intensity mapping lightcones
- Using Action Space Clustering to Constrain the Accretion History of Milky Way like Galaxies
- ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
- The Impact of Molecular Hydrogen Cooling on the Galaxy Formation Threshold
- The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
- Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
- OpenUniverse2024: A shared, simulated view of the sky for the next generation of cosmological surveys
- YZiCS: On the Mass Segregation of Galaxies in Clusters
- Multiply-imaged time-varying sources behind galaxy clusters - Comparing FRBs to QSOs, SNe, and GRBs
- Constraints On Duty Cycles Of Quasars At Z 6
- Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
- Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
- Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
- HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
- The Fabric of the Universe: Exploring the cosmic web in 3D prints and woven textiles
- Fragmentation in Population III Galaxies formed through Ionizing Radiation
- Investigating overdensities around z>6 galaxies through ALMA observations of [CII]
- SIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations
- Shaping the Milky Way: The interplay of mergers and cosmic filaments
- Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
- Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
- LMC-driven anisotropic boosts in stream--subhalo interactions
- Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
- Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
- The Past History of Galaxy Clusters told by their present neighbors
- The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
- Accurate Model of the Projected Velocity Distribution of Galaxies in Dark Matter Halos
- Tracking the orbit of unresolved subhalos for semi-analytic models
- Statistical properties of substructures around Milky Way-sized haloes and their implications for the formation of stellar streams
- Effect of interstellar objects on metallicity of low-mass first stars formed in a cosmological model
- Star formation histories of Coma Cluster galaxies matched to simulated orbits hint at quenching around first pericenter
- The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
- Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
- Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
- The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
- A semi-analytical perspective on massive galaxies at
- Extending Semi-numeric Reionisation Models to the First Stars and Galaxies
- The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
- Imprints of the cosmic void evolution on the baryon processes inside galaxy haloes
- Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
- Fast generation of mock galaxy catalogues with COLA
- Inferring dark matter halo properties for HI-selected galaxies
- Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
- MEGA: Merger graphs of structure formation
- Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
- Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
- An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
- An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
- Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses
- The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
- The Dark Matter Halos of HI Selected Galaxies
- Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
- The role of the elaphrocentre in void galaxy formation
- Observing the Effects of Galaxy Interactions on the Circumgalactic Medium
- Galaxy populations in haloes in high-density environments
- The dark matter halo concentration and stellar initial mass function of a CASSOWARY group
- Zooming in on the Circumgalactic Medium with GIBLE: Tracing the Origin and Evolution of Cold Clouds
- Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
- Universal dark halo scaling relation for the dwarf spheroidal satellites
- EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
- A deep learning approach to halo merger tree construction
- The Effects of Linear Matter Power Spectrum Enhancement on Dark Matter Substructure
- Beyond Mass: Detecting Secondary Halo Properties with Galaxy-Galaxy Lensing
- The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
- Halo Growth and Merger Rates as a Cosmological Test
- EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
- Effects of Neutrino Masses and Asymmetries on Dark Matter Halo Assembly
- Relative baryon-dark matter velocities in cosmological zoom simulations
- Astraeus VII: The environmental-dependent assembly of galaxies in the Epoch of Reionization
- Machine Learning the Fates of Dark Matter Subhalos: A Fuzzy Crystal Ball
- Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
- Semi-analytical frameworks for subhalos from the smallest to the largest scale
- Constraining cosmological parameters using void statistics from the SDSS survey
- NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
- COZMIC. II. Cosmological Zoom-in Simulations with Fractional non-CDM Initial Conditions
- Hungry or Not: How Stellar-Mass Black Holes Grow (or Don't) in Dark Matter Mini-Haloes at High-Resolution
- Topological data analysis reveals differences between simulated galaxies and dark matter haloes
- The PAU Survey: Close galaxy pairs identification and analysis
- Cluster Assembly Times as a Cosmological Test
- MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
- Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
- Signatures of reionization feedback in the near-infrared background
- "Observing" Unrelaxed Clusters in Dark Matter Simulations
- Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
- COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions
- Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
- Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
- Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters
- Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
- The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
- Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
- Environmental effects on associations of dwarf galaxies
- C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
- Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
- Accurate halo mass functions from the simplest excursion set theory
- The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
- The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
- Building Halo Merger Trees from the Q Continuum Simulation
- Observing Correlations Between Dark Matter Accretion and Galaxy Growth: II. Testing the Impact of Galaxy Mass, Star Formation Indicator, and Neighbour Colours
- Halo Properties from Observable Measures of Environment: I. Halo and Subhalo Masses
- FLORAH: A generative model for halo assembly histories
- New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing
- Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
- ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
- Densities and mass assembly histories of the Milky Way satellites are not a challenge to CDM
- Associations of dwarf galaxies in a CDM Universe
- Hermeian haloes: extreme objects with two interactions in the past
- The mass and galaxy distribution around SZ-selected clusters
- Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
- The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
- Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
- Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
- The evolution of the halo occupation distribution in cosmic voids
- A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
- Method for Determining AGN Accretion Phase in Field Galaxies
- Detecting cosmic voids via maps of geometric-optics parameters
- Machine Learning the Dark Matter Halo Mass of Milky Way-Like Systems
- On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster
- A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
- Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
- A Hierarchical Shock Model of Ultra-High-Energy Cosmic Rays
- Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses
- Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
- Halo Merger Tree Comparison: Impact on Galaxy Formation Models
- Rise of the forsaken relics: connecting present-day stellar streams and phase-mixed galaxies to the Epoch of Reionization
- DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
- The Formation of Dwarf Galaxy Disks
- Euclid preparation. L. Calibration of the linear halo bias in CDM cosmologies
- The multi-dimensional halo assembly bias can be preserved when enhancing halo properties with HALOSCOPE
- Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies
- Testing subhalo abundance matching with galaxy kinematics
- Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
- The life and times of dark matter haloes: what will I be when I grow up?
- A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
- Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
- Effect of the cosmological transition to metal-enriched star-formation on the hydrogen 21-cm signal
- Compact Groups in GDM Cosmological Simulations
- Correlation between Outlying Halo Abundance and Host Halo Properties
- Identification of Candidate Halos Hosting Massive Black Hole Seeds in the Simulations with Support Vector Machines
- Timing the last major merger of galaxy clusters with large halo sparsity
- A dynamics-based density profile for dark haloes. I. Algorithm and basic results
- Comparison of simulations and semi-analytical model for WDM subhalo mass functions
- DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
- Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
- Dynamical Properties and Velocity Dispersion-Mass Relation of Galaxy Clusters from the GOGREEN and GCLASS Surveys