Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time

Abstract

We employ high-resolution dissipationless simulations of the concordance LCDM cosmology to model the observed luminosity dependence and evolution of galaxy clustering through most of the age of the universe, from z~5 to z~0. We use a simple, non-parametric model which monotonically relates galaxy luminosities to the maximum circular velocity of dark matter halos (V_max) by preserving the observed galaxy luminosity function in order to match the halos in simulations with observed galaxies. The novel feature of the model is the use of the maximum circular velocity at the time of accretion, V_max,acc, for subhalos, the halos located within virial regions of larger halos. We argue that for subhalos in dissipationless simulations, V_max,acc reflects the luminosity and stellar mass of the associated galaxies better than the circular velocity at the epoch of observation, V_max,now. The simulations and our model L-V_max relation predict the shape, amplitude, and luminosity dependence of the two-point correlation function in excellent agreement with the observed galaxy clustering in the SDSS data at z~0 and in the DEEP2 samples at z~1 over the entire probed range of projected separations, 0.1<r_p/(Mpc/h)<10.0. In particular, the small-scale upturn of the correlation function from the power-law form in the SDSS and DEEP2 luminosity-selected samples is reproduced very well. At z~3-5, our predictions also match the observed shape and amplitude of the angular two-point correlation function of Lyman-break galaxies (LBGs) on both large and small scales, including the small-scale upturn.

16 pages 11 figures, ApJ in press

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• Sample variance in photometric redshift calibration: cosmological biases and survey requirements
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• Near-Field Limits on the Role of Faint Galaxies in Cosmic Reionization
• Constraints on the merging timescale of luminous red galaxies, or, where do all the halos go?
• Virial scaling of galaxies in clusters: bright to faint is cool to hot
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• Modelling the Transfer Function for the Dark Energy Survey
• Wide-Field Lensing Mass Maps from DES Science Verification Data
• Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• On the galaxy-halo connection in the EAGLE simulation
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Simulated ΛCDM analogues of the thin Plane of Satellites around the Andromeda galaxy are not kinematically coherent structures
• Galaxy properties and the cosmic web in simulations
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• The DEEP2 Galaxy Redshift Survey: The Voronoi-Delaunay Method catalog of galaxy groups
• The Halo Occupation Distribution of Active Galactic Nuclei
• Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
• The evolution of the stellar mass versus halo mass relationship
• Observing dynamical friction in galaxy clusters
• 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales
• A tale of two populations: the stellar mass of central and satellite galaxies
• The Faber-Jackson relation and Fundamental Plane from halo abundance matching
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
• Formation of disk galaxies in preheated media: a preventative feedback model
• Reconstructing the gravitational field of the local universe
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• Effects of Baryon Dissipation on the Dark Matter Virial Scaling Relation
• Cosmology with one galaxy?
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Modeling color-dependent galaxy clustering in cosmological simulations
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• Satellite Luminosities in Galaxy Groups
• Dark Energy Survey Year 1 results: Validation of weak lensing cluster member contamination estimates from P(z) decomposition
• Mind the Gap: Tightening the Mass-Richness Relation with Magnitude Gaps
• Properties of Submillimeter Galaxies in a Semi-analytic Model using the "Count Matching" Approach: Application to the ECDF-S
• Modelling Galaxy Merger Timescales and Tidal Destruction
• Are There Enough Ionizing Photons to Reionize the Universe by z=6?
• On stellar mass loss from galaxies in groups and clusters
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Large Scale Structure of the Universe
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• Spectroscopic failures in photometric redshift calibration: cosmological biases and survey requirements
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
• The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
• Combining FOF and halo-based algorithms for the identification of galaxy groups
• Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
• Scaling Relations for Galaxies Prior to Reionization
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• The Secondary Spin Bias of Dark Matter Haloes
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx 0.8$
• Mergers and Star Formation: The environment and Stellar Mass Growth of the Progenitors of Ultra-Massive Galaxies since z = 2
• Priors on Lagrangian bias parameters from galaxy formation modelling
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Multitracer technique for galaxy bispectrum - An application to constraints on non-local primordial non-Gaussianities -
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Degeneracies Between Self-interacting Dark Matter and Supernova Feedback as cusp-core transformation mechanisms
• Testing cold dark matter with the low mass Tully-Fisher relation
• Does the Galaxy-Halo Connection Vary with Environment?
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• Accounting for Cosmic Variance in Studies of Gravitationally-Lensed High-Redshift Galaxies in the Hubble Frontier Field Clusters
• A Method for Measuring the Bias of High-Redshift Galaxies from Cosmic Variance
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• Constraining modified theory of gravity with galaxy bispectrum
• Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog
• Disentangling correlated scatter in cluster mass measurements
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Small-scale galaxy clustering in the EAGLE simulation
• Galaxy subgroups in galaxy clusters
• The angular momentum of disc galaxies: implications for gas accretion, outflows, and dynamical friction
• Fifth force constraints from the separation of galaxy mass components
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The scatter in the galaxy-halo connection: a machine learning analysis
• Fifth force constraints from galaxy warps
• Brightest galaxies as halo centre tracers in SDSS DR7
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• Linking haloes to galaxies: how many halo properties are needed?
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• The evolution of the galaxy content of dark matter haloes
• Identification of galaxy cluster substructures with the Caustic method
• What determines large scale galaxy clustering: halo mass or local density?
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• The cosmological dependence of halo and galaxy assembly bias
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• Groups in the Millennium Simulation and in SDSS DR7
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Detecting neutral hydrogen in emission at redshift z ~ 1
• ELUCID V. Lighting dark matter halos with galaxies
• Galaxy groups in the 2MASS Redshift Survey
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Probing the galaxy-halo connection with total satellite luminosity
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• Hunting down systematics in baryon acoustic oscillations after cosmic high noon
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Understanding the non-linear clustering of high redshift galaxies
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Measures of galaxy environment -- II. Rank-ordered mark correlations
• The clustering of the first galaxy halos
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Spatial Clustering of High Redshift Lyman Break Galaxies
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• Suppressing cosmic variance with paired-and-fixed cosmological simulations: average properties and covariances of dark matter clustering statistics
• SHAM through the lens of a hydrodynamical simulation
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• The age dependence of galaxy clustering
• The statistics of voids as a tool to constrain cosmological parameters: sigma_8 and Omega_m h
• Generating Synthetic Cosmological Data with GalSampler
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
• Describing galaxy weak lensing measurements from tenths to tens of Mpc and up to z~0.6 with a single model
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Is the Universe Simpler than LCDM?
• Precision Cosmology: Successes and Challenges
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Scaling relations for globular cluster systems in early-type galaxies
• Astrophysical Tests of Dark Matter Self-Interactions
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• [OII] emitters in MultiDark-Galaxies and DEEP2
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• Clustering of star-forming galaxies detected in mid-infrared with the Spitzer wide-area survey
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• Constraints on galileons from the positions of supermassive black holes
• Bulk flow in the combined 2MTF and 6dFGSv surveys
• The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Passive Evolution of Galaxy Clustering
• Subhaloes gone Notts: Subhaloes as tracers of the dark matter halo shape
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Subhaloes gone Notts: the clustering properties of subhaloes
• Luminosity bias: from haloes to galaxies
• Galaxy Ecosystems: gas contents, inflows and outflows
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• Distortion of the luminosity function of high-redshift galaxies by gravitational lensing
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Tracing stars in Milky Way satellites with A-SLOTH
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• Cosmological Constraints from applying SHAM to rescaled cosmological simulations
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• The trajectories of galaxies in groups: mass loss and preprocessing
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• A tale of analogies: gravitomagnetic effects, rotating sources, observers and all that
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Constraints on the Evolution of the Galaxy Stellar Mass Function I: Role of Star Formation, Mergers and Stellar Stripping
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• Galaxy clustering with photometric surveys using PDF redshift information
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Density mapping with weak lensing and phase information
• Modeling Redshift-Space Clustering with Abundance Matching
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Connections between galaxy properties and halo formation time in the cosmic web
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Cosmological Probes of Structure Growth and Tests of Gravity
• Rosella: A mock catalogue from the P-Millennium simulation
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• We are not the 99 percent: quantifying asphericity in the distribution of Local Group satellites
• Cosmic Flow Measurement and Mock Sampling Algorithm of Cosmicflows-4 Tully-Fisher Catalogue
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• A minimal empirical model for the cosmic far-infrared background anisotropies
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• The Cosmic Evolution of Halo Pairs: I. Global Trends
• Good and Proper: Self-similarity of N-body Simulations with Proper Force Softening
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Testing galaxy formation models with galaxy stellar mass functions
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Constraining Dark Energy With Stacked Concave Lenses
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Ram pressure statistics for bent tail radio galaxies
• Dark Energy Survey Year 3 Results: Redshift Calibration of the MagLim Lens Sample from the combination of SOMPZ and clustering and its impact on Cosmology
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Dwarf satellites of high-z Lyman Break Galaxies: a free lunch for JWST
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• An empirical model to form and evolve galaxies in dark matter halos
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Spatial and Kinematic Clustering of Stars in the Galactic Disk
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Impact of tidal environment on galaxy clustering in GAMA
• Velocity Dispersions of Massive Quiescent Galaxies from Weak Lensing and Spectroscopy
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Relating galaxies across different redshift to study galaxy evolution
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Revealing the Galaxy-Halo Connection Through Machine Learning
• On the weak lensing masses of a new sample of galaxy groups
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• Extracting galaxy merger timescales I: Tracking haloes with WhereWolf and spinning orbits with OrbWeaver
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• A Two-Parameter Matching Scheme for Massive Galaxies and Dark Matter Haloes
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Rapid Simulations of Halo and Subhalo Clustering
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Inferring dark matter halo properties for HI-selected galaxies
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• Constraining galaxy-halo connection with high-order statistics
• Characterizing simulated galaxy stellar mass histories
• Close Galaxy Pairs at z = 3: A Challenge to UV Luminosity Abundance Matching
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• MAMBO -- An empirical galaxy and AGN mock catalogue for the exploitation of future surveys
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• A Candidate Brightest Proto-Cluster Galaxy at z = 3.03
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Subhalo abundance matching in $f(R)$ gravity
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Exploring the physical origins of halo assembly bias from early times
• DarkAI: Reconstructing the density, velocity and tidal field of dark matter from a DESI-like bright galaxy sample
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Galaxy-galaxy lensing in the VOICE deep survey
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• The information on halo properties contained in spectroscopic observations of late-type galaxies
• Probing Satellite Halos with Weak Gravitational Lensing
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• 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
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Clustering properties and halo masses for central galaxies in the local Universe
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• ELG$\times$LRG distribution through dark matter halo dynamics
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• Constraining galaxy properties with complete samples of lenses
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport
• The informativeness of [C II] line-intensity mapping as a probe of the H I content and metallicity of galaxies at the end of reionization
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Generalized local ansatz for scale-dependent primordial non-Gaussianities and future galaxy surveys
• A hierarchical clustering method for quantifying satellite abundance
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• The mass profile of NGC 3377 from a Bayesian approach
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• STRAWBERRY: Finding haloes in the gravitational potential
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Predicting halo occupation and galaxy assembly bias with machine learning
• Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• Testing subhalo abundance matching with galaxy kinematics
• Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• Euclid: Improving redshift distribution reconstruction using a deep-to-wide transfer function
• Dynamic Zoom Simulations of structure formation beyond standard cosmology
• Finding High-Redshift Galaxies with JWST
• Mimicking the halo-galaxy connection using machine learning
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG