A unified multi-wavelength model of galaxy formation

Abstract

We present a new version of the GALFORM semi-analytical model of galaxy formation. This brings together several previous developments of GALFORM into a single unified model, including a different initial mass function (IMF) in quiescent star formation and in starbursts, feedback from active galactic nuclei supressing gas cooling in massive halos, and a new empirical star formation law in galaxy disks based on their molecular gas content. In addition, we have updated the cosmology, introduced a more accurate treatment of dynamical friction acting on satellite galaxies, and updated the stellar population model. The new model is able to simultaneously explain both the observed evolution of the K-band luminosity function and stellar mass function, and the number counts and redshift distribution of sub-mm galaxies selected at 850 mu. This was not previously achieved by a single physical model within the LambdaCDM framework, but requires having an IMF in starbursts that is somewhat top-heavy. The new model is tested against a wide variety of observational data covering wavelengths from the far-UV to sub-mm, and redshifts from z=0 to z=6, and is found to be generally successful. These observations include the optical and near-IR luminosity functions, HI mass function, fraction of early type galaxies, Tully-Fisher, metallicity-luminosity and size-luminosity relations at z=0, as well as far-IR number counts, and far-UV luminosity functions at z ~ 3-6. [abridged]

Accepted for publication in MNRAS. Revised in response to referee; minor changes only (including some figures), no change in results or conclusions. 62 pages (44 without appendices); 57 figures (32 without appendices)

References in corpus (56)

• Cosmic Star Formation History
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• 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
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• Physical Models of Galaxy Formation in a Cosmological Framework
• UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
• Gusty, gaseous flows of FIRE: galactic winds in cosmological simulations with explicit stellar feedback
• The Role of Pressure in GMC Formation II: The H_2 - Pressure Relation
• A systematic variation of the stellar initial mass function in early-type galaxies
• Massloss of galaxies due to a UV-background
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• A primer on hierarchical galaxy formation: the semi-analytical approach
• 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
• The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
• Evolutionary stellar population synthesis with MILES - II. Scaled-solar and α-enhanced models
• The Gemini Deep Deep Survey: III. The abundance of massive galaxies 3-6 billion years after the Big Bang
• Moving mesh cosmology: tracing cosmological gas accretion
• Bimodal gas accretion in the Horizon-MareNostrum galaxy formation simulation
• Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation
• Generating Dark Matter Halo Merger Trees
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source counts
• A fitting formula for the merger timescale of galaxies in hierarchical clustering
• The high redshift galaxy population in hierarchical galaxy formation models
• The MORGANA model for the rise of galaxies and active nuclei
• Effects of AGN feedback on LCDM galaxies
• The Atomic to Molecular Transition and its Relation to the Scaling Properties of Galaxy Disks in the Local Universe
• Black Hole Growth in Hierarchical Galaxy Formation
• The flip-side of galaxy formation: A combined model of Galaxy Formation and Cluster Heating
• Probing the submillimetre number counts at f(850um) < 2mJy
• HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
• Galaxy evolution in the infra-red: comparison of a hierarchical galaxy formation model with SPITZER data
• Variations in the initial mass function in early-type galaxies: A critical comparison between dynamical and spectroscopic results
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• Luminosity and stellar mass functions of disks and spheroids in the SDSS and the supermassive black hole mass function
• Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
• Orbital parameters of infalling satellite haloes in the hierarchical $\Lambda$CDM model
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• The origin of the atomic and molecular gas contents of early-type galaxies. I. A new test of galaxy formation physics
• The origin of the atomic and molecular gas contents of early-type galaxies. II. Misaligned gas accretion
• Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
• Reproducing the assembly of massive galaxies within the hierarchical cosmogony
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• The evolution of the star forming sequence in hierarchical galaxy formation models
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• The evolution of the stellar mass versus halo mass relationship
• The IMF-sensitive 1.14-micron Na I doublet in early-type galaxies
• The far infra-red SEDs of main sequence and starburst galaxies
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• The Clustering Evolution of Dusty Star-Forming Galaxies
• Variations of the Initial Mass Function in Semi-Analytical models
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model

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• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• "Dust Giant": Extended and Clumpy Star-Formation in a Massive Dusty Galaxy at $z=1.38$
• The north-south asymmetry of the ALFALFA HI velocity width function
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• Sensitivity analysis of a galaxy formation model
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Simulations of the accreted stellar halos of low-mass field galaxies
• Deep Submillimetre and Radio Observations in the SSA22 Field. II. Sub-millimetre source catalogue and number counts
• On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation
• Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals
• Joint inference on the redshift distribution of fast radio burst and on the intergalactic baryon content
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Dust contribution to the panchromatic galaxy emission
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• VEGA: Voids idEntification using Genetic Algorithm
• The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
• The progenitor galaxies of stellar haloes as "failed" Milky Ways
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Ultraviolet-to-far-infra-red self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Extended Hernquist-Springel formalism for cosmic star formation
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• New Insights into Uncertainties in the Relic Neutrino Background and Effects from the Nuclear Equation of State
• Dynamic Zoom Simulations of structure formation beyond standard cosmology
• 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
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES