A primer on hierarchical galaxy formation: the semi-analytical approach

Abstract

Recent observational and theoretical breakthroughs make this an exciting time to be working towards understanding the physics of galaxy formation. The goal of this review is to make the principles behind the hierarchical paradigm accessible to a wide audience by providing a pedagogical introduction to modern theories of galaxy formation. I outline the ingredients of the powerful approach called semi-analytical modelling and contrast this method with numerical simulations of the gas dynamics of baryons. Semi-analytical models have enjoyed many successes, but it is the observations which the models struggle to match which mark out areas where future progress is most likely to be made; these are also reviewed.

68 pages. Review article for Reports on Progress in Physics. A version with high resolution figures can be downloaded from http://star-www.dur.ac.uk/~cmb/rop_review.ps

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• MultiDark-Galaxies: data release and first results
• The host dark matter halos of [OII] emitters at 0.5< z< 1.5
• How robust are predictions of galaxy clustering?
• The evolution of Lyman-break galaxies in CDM
• The Evolution of Assembly Bias
• SPACE: the SPectroscopic All-sky Cosmic Explorer
• Galaxy Formation in WDM Cosmology
• Quenching star formation in cluster galaxies
• Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
• Halo model and halo properties in Galileon gravity cosmologies
• The angular momentum of cold dark matter haloes with and without baryons
• Faint Lyman-Break galaxies as a crucial test for galaxy formation models
• The velocity function of gas-rich galaxies
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• Predictions for Herschel from LambdaCDM: unveiling the cosmic star formation history
• Halo Shapes From Weak Lensing: The Impact of Galaxy--Halo Misalignment
• Can galactic outflows explain the properties of Ly-alpha emitters?
• The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way
• Evaluating and Improving Semi-analytic modelling of Dust in Galaxies based on Radiative Transfer Calculations
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• A semi-analytic model comparison - gas cooling and galaxy mergers
• The rest-frame $K$-band luminosity function of galaxies in clusters to $z=1.3$
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• A Lightcone Catalogue from the Millennium-XXL Simulation
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• The imprint of cosmic reionisation on the luminosity function of galaxies
• Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization
• The Hierarchical Origins of Observed Galaxy Morphology
• Star Clusters in Evolving Galaxies
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• Photo-heating and supernova feedback amplify each other's effect on the cosmic star formation rate
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• The evolution of the star forming sequence in hierarchical galaxy formation models
• The clustering of Ly-alpha emitters in a LambdaCDM Universe
• The sizes of mini-voids in the local universe: an argument in favor of a warm dark matter model?
• The role of submillimetre galaxies in hierarchical galaxy formation
• On the connection between the intergalactic medium and galaxies: The HI-galaxy cross-correlation at z < 1
• Empirical constraints on the formation of early-type galaxies
• Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
• The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
• Protocluster Discovery in Tomographic Ly$\alpha$ Forest Flux Maps
• Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
• Accurate mass and velocity functions of dark matter halos
• Terrestrial planets across space and time
• The effect of thermally pulsating asymptotic giant branch stars on the evolution of the rest-frame near-infrared galaxy luminosity function
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies
• The migration of nearby spirals from the blue to red sequence: AGN feedback or environmental effects?
• The Formation and Evolution of Virgo Cluster Galaxies - II. Stellar Populations
• A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations
• The structural and photometric properties of early-type galaxies in hierarchical models
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• Origin of the galaxy HI size-mass relation
• Galactic Chemical Evolution of Radioactive Isotopes
• A modified star formation law as a solution to open problems in galaxy evolution
• The UV colours and dust attenuation of Lyman-break galaxies
• The impact of TP-AGB stars on hierarchical galaxy formation models
• Stellar mass functions of galaxies at 4<z<7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies
• Creating mock catalogues of stellar haloes from cosmological simulations
• The HIX galaxy survey II: HI kinematics of HI eXtreme galaxies
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• Exploring the liminality: properties of haloes and subhaloes in borderline $f(R)$ gravity
• The evolution of the stellar mass versus halo mass relationship
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Supernovae and AGN driven galactic outflows
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• The MgII Cross-section of Luminous Red Galaxies
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Radio source feedback in galaxy evolution
• Evolution of galactic magnetic fields
• Marked clustering statistics in $f(R)$ gravity cosmologies
• The first Super Massive Black Holes: indications from models for future observations
• The galaxies that reionized the Universe
• Predictions for the intrinsic UV continuum properties of star forming galaxies and the implications for inferring dust extinction
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• Do model emission line galaxies live in filaments at z~1?
• Supermassive Black Holes and Their Environments
• Luminous Red Galaxies in hierarchical cosmologies
• Constraints on galaxy formation models from the galaxy stellar mass function and its evolution
• SINFONI/VLT 3D spectroscopy of massive galaxies: Evidence of rotational support at z~1.4
• The spatial distribution of cold gas in hierarchical galaxy formation models
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• Statistics of galaxy mergers: bridging the gap between theory and observation
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• Thick-disk evolution induced by the growth of an embedded thin disk
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• The HI Velocity Function: a test of cosmology or baryon physics?
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• The Molecular Gas Density in Galaxy Centers and How It Connects to Bulges
• Small-scale galaxy clustering in the EAGLE simulation
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• Regulation of Star Formation by a Hot Circumgalactic Medium
• Low-mass galaxy formation in cosmological AMR simulations: the effects of varying the sub-grid physics parameters
• The scatter in the galaxy-halo connection: a machine learning analysis
• Cosmic CARNage I: on the calibration of galaxy formation models
• Merger relics of cluster galaxies
• What determines large scale galaxy clustering: halo mass or local density?
• How does gas cool in DM halos?
• The dependence of AGN activity on stellar and halo mass in Semi-Analytic Models
• The evolution of the galaxy content of dark matter haloes
• Clustering properties of high redshift red galaxies in SA22 from the UKIDSS DXS
• The physical drivers of the atomic hydrogen-halo mass relation
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Remapping dark matter halo catalogues between cosmological simulations
• On the orbital and internal evolution of cluster galaxies
• On Physical Scales of Dark Matter Halos
• Massive, red galaxies in a hierarchical universe I. Counts of Extremely Red Objects and basic properties
• Galactic magnetic fields and hierarchical galaxy formation
• Gas cooling in semi-analytic models and SPH simulations: are results consistent?
• The accuracy of the UV continuum as an indicator of the star formation rate in galaxies
• S0 galaxies in the Coma cluster: Environmental dependence of the S0 offset from the Tully-Fisher relation
• Using Velocity Dispersion to Estimate Halo Mass: Is the Local Group in Tension with $\Lambda$CDM?
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• Probing the dark-matter halos of cluster galaxies with weak lensing
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• Statistical correlation between the distribution of Ly$\alpha$ emitters and IGM HI at $z\sim 2.2$ mapped by Subaru/Hyper Suprime-Cam
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Galaxy star formation in different environments
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• The effects of halo alignment and shape on the clustering of galaxies
• The halo light cone catalogues of \Abacus{AbacusSummit}
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• The PAU Survey: Spectral features and galaxy clustering using simulated narrow band photometry
• The Clustering Evolution of Dusty Star-Forming Galaxies
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• The segregation of baryons and dark matter during halo assembly
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Revisiting the role of the Thermally-Pulsating Asymptotic Giant Branch phase in high-redshift galaxies
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• Distinguishing `disks' from `mergers': tracing the kinematic asymmetries in local (U)LIRGs using `kinemetry'-based criteria
• The WIRCam Deep Survey II: Mass Selected Clustering
• Deviations from the Schmidt-Kennicutt relations during early galaxy evolution
• Extending the halo mass resolution of $N$-body simulations
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• HIghMass - High HI Mass, HI-rich Galaxies at z~0: High-Resolution VLA Imaging of UGC 9037 and UGC 12506
• Galaxy and Mass Assembly (GAMA): merging galaxies and their properties
• The Structure of Reionization in Hierarchical Galaxy Formation Models
• Lyα emitters in a cosmological volume I: the impact of radiative transfer
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Two phase galaxy formation: The Gas Content of Normal Galaxies
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• Observing Merger Trees in a New Light
• The assembly bias of emission line galaxies
• Luminosity bias: from haloes to galaxies
• The galaxy correlation function as a constraint on galaxy formation physics
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• Orbital distribution of infalling satellite halos across cosmic time
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• Robust constraints on dark energy and gravity from galaxy clustering data
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The HI mass function as a probe of photoionisation feedback on low mass galaxy formation
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Detection of Satellite Remnants in the Galactic Halo with Gaia - II. A modified Great Circle Cell Method
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
• Reignited star formation in dwarf galaxies quenched during reionization
• Hierarchical structure of the cosmic web and galaxy properties
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• Some observational tests of a minimal galaxy formation model
• The evolution of disc galaxies with and without classical bulges since z~1
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• The ages of stellar populations in a warm dark matter universe
• Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• A possible solution to the [alpha/Fe]-sigma problem in early type galaxies within a hierarchical galaxy formation model
• Modelling the dusty universe I: Introducing the artificial neural network and first applications to luminosity and colour distributions
• Milky Way type galaxies in a LCDM cosmology
• Rosella: A mock catalogue from the P-Millennium simulation
• The active and passive populations of Extremely Red Objects
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• Examining subgrid models of supermassive black holes in cosmological simulation
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Spectro-Imaging Forward Model of Red and Blue Galaxies
• Merger history trees of dark matter haloes in moving barrier models
• The effect of gas-dynamics on semi-analytic modeling of cluster galaxies
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Variations of the Initial Mass Function in Semi-Analytical models
• Particle tagging and its implications for stellar population dynamics
• Magnitude and size evolution of bulgeless galaxies
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmology
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• Galaxy formation with cold gas accretion and evolving stellar initial mass function
• A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• A new gas cooling model for semi-analytical galaxy formation models
• Variation in the escape fraction of ionising photons from galaxies and the redshifted 21-cm power spectrum during reionization
• The first spectral line surveys searching for signals from the Dark Ages
• Excursion Set Theory for Correlated Random Walks
• Using the Star Forming Main Sequence To Explore Quiescent Galaxies Across Cosmic Time
• Testing anthropic reasoning for the cosmological constant with a realistic galaxy formation model
• G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• An empirical model to form and evolve galaxies in dark matter halos
• Modelling emission lines in star forming galaxies
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Ram pressure profiles in galaxy groups and clusters
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• Ca II and Na I Quasar Absorption-Line Systems in an Emission-Selected Sample of SDSS DR7 Galaxy/Quasar Projections: I. Sample Selection
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Abundance matching for low mass galaxies in the CDM and FDM models
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Effective viscosity from cloud-cloud collisions in three-dimensional global SPH simulations
• Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
• Probing dark matter haloes of spiral galaxies at poorly explored distances using satellite kinematics
• Removal and mixing of the coronal gas from satellites in galaxy groups: cooling the intragoup gas
• Galactic Outflows and Evolution of the Interstellar Medium
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Evolution of the mass relation between supermassive black holes and dark matter halos across the cosmic time
• Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• The role of the elaphrocentre in void galaxy formation
• Co-evolution of supermassive black holes with galaxies from semi-analytic model: stochastic gravitational wave background and black hole clustering
• A fast and accurate method to compute the mass return from multiple stellar populations
• Growth of disc-like pseudo-bulges in SDSS DR7 since z = 0.1
• An efficient and robust method to estimate halo concentration
• An efficient hybrid method to produce high resolution large volume dark matter simulations for semi-analytic models of reionisation
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Galaxy luminosity function and its cosmological evolution: Testing a new feedback model depending on galaxy-scale dust opacity
• A hybrid multi resolution scheme to efficiently model the structure of reionization on the largest scales
• A Bayesian chemical evolution model of the DustPedia Galaxy M74
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• Sensitivity analysis of a galaxy formation model
• The Impact of Baryons on the Large-Scale Structure of the Universe
• The Environment of Lyman Break Analogues (ELBA) survey: Star-forming galaxies in small groups
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• A large change in the predicted number of small halos due to a small amplitude oscillating inflaton potential
• Evolution of dwarf galaxy observable parameters
• Extracting Galaxy Merger Timescales II: A new fitting formula
• The influence of superstructures on bright galaxy environments: clustering properties
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• Clustering of K-band selected local galaxies
• The AIDA-TNG project: 3D halo shapes
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• The invariance of group occupation across the cosmic web
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• The evolution of galaxy formation
• SDSS-IV MaNGA: Stellar rotational support in disk galaxies vs. central surface density and stellar population age
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• Covariances of Galaxy Stellar Mass Functions and Correlation Functions
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• On the Evidence for Violation of the Equivalence Principle in Disk Galaxies
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• A redshift distortion free correlation function at third order in the nonlinear regime
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl