Galacticus: A Semi-Analytic Model of Galaxy Formation
arXiv:1008.1786 · doi:10.1016/j.newast.2011.07.004
Abstract
We describe a new, free and open source semi-analytic model of galaxy formation, Galacticus. The Galacticus model was designed to be highly modular to facilitate expansion and the exploration of alternative descriptions of key physical ingredients. We detail the Galacticus engine for evolving galaxies through a merging hierarchy of dark matter halos and give details of the specific implementations of physics currently available in Galacticus. Finally, we show results from an example model that is in reasonably good agreement with several observational datasets. We use this model to explore numerical convergence and to demonstrate the types of information which can be extracted from Galacticus.
35 pages, submitted to New Astronomy
References in corpus (17)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
- A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
- The redshift dependence of the structure of massive LCDM halos
- The spin and shape of dark matter haloes in the Millennium simulation of a LambdaCDM universe
- Scaled solar tracks and isochrones in a large region of the Z-Y plane I. From the ZAMS to the TP-AGB end for 0.15 - 2.5 Mo stars
- Galaxy Formation Theory
- A fitting formula for the merger timescale of galaxies in hierarchical clustering
- The MORGANA model for the rise of galaxies and active nuclei
- On the final spin from the coalescence of two black holes
- The Tully-Fisher Relation and Its Residuals for a Broadly Selected Sample of Galaxies
- Feedback from central black holes in elliptical galaxies. I: models with either radiative or mechanical feedback but not both
- The Parameter Space of Galaxy Formation
- Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
- Disc instabilities and semi-analytic modelling of galaxy formation
- On the algorithms of radiative cooling in semi-analytic models
- Cold Mode Accretion in Galaxy Formation
Cited by in corpus (257)
- Simulating Galaxy Formation with the IllustrisTNG Model
- First results from the IllustrisTNG simulations: matter and galaxy clustering
- First results from the IllustrisTNG simulations: the galaxy color bimodality
- A model for cosmological simulations of galaxy formation physics
- Dusty Star-Forming Galaxies at High Redshift
- De Re Metallica: The cosmic chemical evolution of galaxies
- The Origin and Evolution of the Galaxy Mass-Metallicity Relation
- EMERGE - An empirical model for the formation of galaxies since
- A unified multi-wavelength model of galaxy formation
- The Connection between Galaxies and Dark Matter Structures in the Local Universe
- ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies
- The Current Status of Galaxy Formation
- Warm dark matter chills out: constraints on the halo mass function and the free-streaming length of dark matter with 8 quadruple-image strong gravitational lenses
- The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations
- Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results
- Shark: introducing an open source, free and flexible semi-analytic model of galaxy formation
- The Horizon-AGN simulation: evolution of galaxy properties over cosmic time
- The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications
- Formation of massive black holes in rapidly growing pre-galactic gas clouds
- Strong Constraints on Fuzzy Dark Matter from Ultrafaint Dwarf Galaxy Eridanus II
- Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
- Moving mesh cosmology: numerical techniques and global statistics
- Structure Finding in Cosmological Simulations: The State of Affairs
- Strong bimodality in the host halo mass of central galaxies from galaxy-galaxy lensing
- Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter
- An algorithm to build mock galaxy catalogues using MICE simulations
- The JWST Extragalactic Mock Catalog: Modeling galaxy populations from the UV through the near-IR over thirteen billion years of cosmic history
- Large-scale dark matter simulations
- The nature of the [CII] emission in dusty star-forming galaxies from the SPT survey
- Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100pc scales
- Essential physics of early galaxy formation
- Gravitational probes of dark matter physics
- Simulations of ram-pressure stripping in galaxy-cluster interactions
- Fundamental Mass-Spin-Morphology Relation of Spiral Galaxies
- The Dawes Review 1: Kinematic studies of star-forming galaxies across cosmic time
- Structure Formation and Microlensing with Axion Miniclusters
- The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
- Is the dark-matter halo spin a predictor of galaxy spin and size?
- Semi-Analytic Galaxies - I. Synthesis of environmental and star-forming regulation mechanisms
- Probing dark matter structure down to solar masses: flux ratio statistics in gravitational lenses with line of sight halos
- The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope
- Novel constraints on the particle nature of dark matter from stellar streams
- CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
- Dark Matter Constraints from a Unified Analysis of Strong Gravitational Lenses and Milky Way Satellite Galaxies
- The Subhalo Mass Function and Ultralight Bosonic Dark Matter
- A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
- Spatially resolved star formation and fuelling in galaxy interactions
- The Outer Rim Simulation: A Path to Many-Core Supercomputers
- Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
- Revealing the galaxy-halo connection in IllustrisTNG
- Elemental Abundances in Milky Way-like Galaxies from a Hierarchical Galaxy Formation Model
- Substructure of fuzzy dark matter haloes
- Connecting massive galaxies to dark matter halos in BOSS - I. Is galaxy color a stochastic process in high-mass halos?
- The LSST DESC DC2 Simulated Sky Survey
- Strong lensing signatures of self-interacting dark matter in low-mass halos
- \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
- Tidal disruption of fuzzy dark matter subhalo cores
- MultiDark-Galaxies: data release and first results
- PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics
- The Evolution of Assembly Bias
- Bayesian inference of galaxy formation from the K-band luminosity function of galaxies: tensions between theory and observation
- Inferring the star formation histories of the most massive and passive early-type galaxies at z<0.3
- The imprint of cosmic reionisation on the luminosity function of galaxies
- How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE
- Constraints on the mass-concentration relation of cold dark matter halos with 11 strong gravitational lenses
- Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
- EMERGE: Empirical predictions of galaxy merger rates since
- Gravothermal solutions of SIDM halos: mapping from constant to velocity-dependent cross section
- Nonlinear evolution of dark matter subhalos and applications to warm dark matter
- Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
- Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
- The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
- Quantum fluctuations masquerade as halos: Bounds on ultra-light dark matter from quadruply-imaged quasars
- Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
- Terrestrial planets across space and time
- The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
- The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
- Machine Learning and Cosmological Simulations I: Semi-Analytical Models
- The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
- The Dwarfs Beyond: The Stellar-to-Halo Mass Relation for a New Sample of Intermediate Redshift Low Mass Galaxies
- Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
- The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
- Core-halo mass relation of ultralight axion dark matter from merger history
- Characterizing the formation history of Milky Way-like stellar haloes with model emulators
- SPT 0538-50: Physical conditions in the ISM of a strongly lensed dusty star-forming galaxy at z=2.8
- Empirical Modeling of the Redshift Evolution of the [NII]/H-ratio for Galaxy Redshift Surveys
- Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the Stellar Mass Function
- Predicting Hα emission line galaxy counts for future galaxy redshift surveys
- The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
- The primordial matter power spectrum on sub-galactic scales
- Flybys, orbits, splashback: subhalos and the importance of the halo boundary
- New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
- TDCOSMO III: Dark matter substructure meets dark energy -- the effects of (sub)halos on strong-lensing measurements of
- ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
- Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
- : Learning Galaxy Properties from Merger Trees
- A semi-analytic study of self-interacting dark-matter haloes with baryons
- The first Super Massive Black Holes: indications from models for future observations
- The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
- Subhaloes gone Notts: Spin across subhaloes and finders
- On stellar mass loss from galaxies in groups and clusters
- Constraining the last 7 billion years of galaxy evolution in semi-analytic models
- WFIRST Science Investigation Team "Cosmology with the High Latitude Survey" Annual Report 2017
- Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
- Dark Matter Halo Environment for Primordial Star Formation
- nIFTy Cosmology: the clustering consistency of galaxy formation models
- Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
- Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
- The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
- Linear bias forecasts for emission line cosmological surveys
- Where are All the Gas-Bearing Local Dwarf Galaxies? Quantifying Possible Impacts of Reionization
- ZFIRE: The Evolution of the Stellar Mass Tully-Fisher Relation to Redshift 2.0 < Z < 2.5 with MOSFIRE
- Simulation-based inference of dynamical galaxy cluster masses with 3D convolutional neural networks
- The Three Hundred Project: the stellar and gas profiles
- Convergence of Galaxy Properties with Merger Tree Temporal Resolution
- Prediction of H and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
- The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
- A Parametric Model for Self-Interacting Dark Matter Halos
- Tidal Tracks and Artificial Disruption of Cold Dark Matter Halos
- J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
- ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
- A Joint Roman Space Telescope and Rubin Observatory Synthetic Wide-Field Imaging Survey
- Sensitivity of dark matter haloes to their accretion histories
- From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
- The MillenniumTNG Project: The large-scale clustering of galaxies
- Soliton Merger Rates and Enhanced Axion Dark Matter Decay
- Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
- Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
- Structure Formation and the Global 21-cm Signal in the Presence of Coulomb-like Dark Matter-Baryon Interactions
- The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
- HInet: Generating neutral hydrogen from dark matter with neural networks
- The halo light cone catalogues of \Abacus{AbacusSummit}
- Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
- Constructing high-fidelity halo merger trees in AbacusSummit
- The LSST-DESC 3x2pt Tomography Optimization Challenge
- Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
- A new calibration method of sub-halo orbital evolution for semi-analytic models
- Revisiting the Cosmic Star Formation History: Caution on the Uncertainties in Dust Correction and Star Formation Rate Conversion
- Studying Cosmic Dawn using redshifted HI 21-cm signal: A brief review
- HST Grism-derived Forecasts for Future Galaxy Redshift Surveys
- Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
- Generating Synthetic Cosmological Data with GalSampler
- The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
- Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
- Dark-ages Reionization and Galaxy Formation Simulation -- XVII. Sizes, angular momenta and morphologies of high redshift galaxies
- The clustering of galaxies: Predictions from the BLUETIDES simulation
- New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
- A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
- DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
- Tidal evolution of cored and cuspy dark matter halos
- [OII] emitters in MultiDark-Galaxies and DEEP2
- DSPS: Differentiable Stellar Population Synthesis
- The assembly bias of emission line galaxies
- Abell 2384: the galaxy population of a cluster post-merger
- Stellar angular momentum can be controlled from cosmological initial conditions
- A Composite Likelihood Approach for Inference under Photometric Redshift Uncertainty
- Structure and dynamics in low density regions: galaxy-galaxy correlations inside cosmic voids
- Dissecting galaxy formation models with Sensitivity Analysis -- A new approach to constrain the Milky Way formation history
- New empirical constraints on the cosmological evolution of gas and stars in galaxies
- The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
- Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
- Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
- Late Bloomer Galaxies: Growing Up in Cosmic Autumn
- Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
- A random-walk model for dark matter halo spins
- The evolutionary pathways of disk galaxies with different sizes
- The effects of peculiar velocities in SN Ia environments on the local measurement
- The time-scales of major mergers from simulations of isolated binary galaxy collisions
- Halo concentrations from extended Press-Schechter merger histories
- The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
- Bulge formation through disc instability -- I
- How feedback shapes galaxies: an analytic model
- Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
- Simulating image coaddition with the Nancy Grace Roman Space Telescope: I. Simulation methodology and general results
- The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
- On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
- A methodology to select galaxies just after the quenching of star formation
- GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
- Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
- Feedback in Galaxy Formation
- Clustering in the Simulated H Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
- The Clustering of Undetected High-redshift Black Holes and Their Signatures in Cosmic Backgrounds
- On the dark matter haloes inner structure and galaxy morphology
- Growing the First Galaxies' Merger Trees
- An empirical model to form and evolve galaxies in dark matter halos
- Tracking the orbit of unresolved subhalos for semi-analytic models
- Improving Photometric Redshift Estimates with Training Sample Augmentation
- Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
- G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
- A semi-analytical perspective on massive galaxies at
- Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation
- A consistent model for both the HI and stellar mass functions of galaxies
- Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
- Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector
- The features of the Cosmic Web unveiled by the flip-flop field
- The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
- Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
- Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
- Pushing the Limits of Detectability: Mixed Dark Matter from Strong Gravitational Lenses
- Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
- Probing the link between quenching and morphological evolution
- PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at
- The Grism Lens-Amplified Survey from Space (GLASS). XII. Spatially Resolved Galaxy Star Formation Histories and True Evolutionary Paths at z > 1
- Interlopers speak out: studying the dark universe using small-scale lensing anisotropies
- Chromatic Effects on the PSF and Shear Measurement for the Roman Space Telescope High-Latitude Wide Area Survey
- Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
- EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
- Trends in Dwarf Early-Type Kinematics with Cluster-centric Radius Driven By Tidal Stirring
- Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
- A deep learning approach to halo merger tree construction
- Anisotropic strong lensing as a probe of dark matter self-interactions
- The mass-size relation of LRGs from BOSS and DECaLS
- Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
- The Halo Masses of Galaxies to : A Hybrid Observational and Theoretical Approach
- Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
- A young galaxy cluster in the old Universe
- Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
- Protoclusters at z=5.7: A view from the MultiDark galaxies
- Non-Gaussian assembly bias from a semi-analytic galaxy formation model
- Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
- Sensitivity of the Global 21-cm Signal to Dark Matter-Baryon Scattering
- Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
- Statistics for dark matter subhalo searches in gamma rays from a kinematically constrained population model: Fermi-LAT-like telescopes
- YOLO-CL cluster detection in the Rubin/LSST DC2 simulation
- Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
- Cosmology with voids from the Nancy Grace Roman Space Telescope
- Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
- Solving the puzzle of subhalo spins
- A Galaxy-Halo Model for Multiple Cosmological Tracers
- The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
- Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
- Subhalos are Anisotropically Distributed and Aligned with the Smooth Matter Distribution of Their Host Halos
- Cluster density slopes from Dark Matter-Baryons Energy Transfer
- Constraining H0 Via Extragalactic Parallax
- Building Halo Merger Trees from the Q Continuum Simulation
- Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
- Phenomenological power spectrum models for H emission line galaxies from the Nancy Grace Roman Space Telescope
- Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
- Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
- UNITSIM-Galaxies: data release and clustering of emission-line galaxies
- Semianalytic model for decaying dark matter halos
- Visualization in Astrophysics: Developing New Methods, Discovering Our Universe, and Educating the Earth
- Extended Hernquist-Springel formalism for cosmic star formation
- Angular momentum and morphological sequence of massive galaxies through Dark Sage
- Halo Merger Tree Comparison: Impact on Galaxy Formation Models
- The progenitor galaxies of stellar haloes as "failed" Milky Ways
- The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
- Covariances of Galaxy Stellar Mass Functions and Correlation Functions
- The formation of blue cluster in local Universe
- Decomposition of stellar populations in CosmoDC2 galaxies using SCARLET and Deep Learning
- A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
- Prospects for measuring the Doppler magnification dipole with LSST and DESI
- Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
- Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation
- A Mass Dependent Density Profile from Dwarfs to Clusters
- An Estimate of the Impact of Reionization on Supermassive Black Hole Growth
- The Galaxy Evolution Probe