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)

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• Chemical evolution of elliptical galaxies with a variable IMF -- A publicly available code
• Cosmic CARNage I: on the calibration of galaxy formation models
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^{\ast }$ Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
• The evolution of the galaxy content of dark matter haloes
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• Revisiting the classics: Is [Mg/Fe] a good proxy for galaxy formation time-scales?
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
• Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\mathbf{z}\sim 4$: hidden AGN and star formation activity
• Galactic conformity measured in semi-analytic models
• 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
• ZFIRE: Using H$\alpha$ equivalent widths to investigate the in situ initial mass function at z~2
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• The bright end of the infrared luminosity functions and the abundance of hyperluminous infrared galaxies
• Ionized Outflows in Nearby Quasars are Poorly Coupled to their Host Galaxies
• The far infra-red SEDs of main sequence and starburst galaxies
• The galaxy population in cold and warm dark matter cosmologies
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes
• The clustering of submillimeter galaxies detected with ALMA
• The PAU Survey: Spectral features and galaxy clustering using simulated narrow band photometry
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• The Clustering Evolution of Dusty Star-Forming Galaxies
• The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• The Missing Satellite Problem Outside of the Local Group: I -- Pilot Observation
• Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• Generating Synthetic Cosmological Data with GalSampler
• Predicting sub-millimeter flux densities from global galaxy properties
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• Comparing Models for IMF Variation Across Cosmological Time in Milky Way-like Galaxies
• The VANDELS survey: Discovery of massive overdensities of galaxies at z>2
• The ALMA Frontier Fields Survey - IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Lyα emitters in a cosmological volume I: the impact of radiative transfer
• The SCUBA-2 850 $\mu m$ follow-up of WISE-selected, luminous dust-obscured quasars
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• In pursuit of giants: II. Evolution of dusty quiescent galaxies over the last six billion years from the hCOSMOS survey
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• The UV luminosity functions of Bright z>8 Galaxies: Determination from ~0.41 deg2 of HST Observations along ~sim 300 independent sightlines
• Lyman-alpha emitters in a cosmological volume II: the impact of the intergalactic medium
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Halo models of HI selected galaxies
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• Candidate Massive Galaxies at $z\sim 4$ in the Dark Energy Survey
• An ALMA view of 11 Dusty Star Forming Galaxies at the peak of Cosmic Star Formation History
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• The $z\lesssim 1$ drop of cosmic dust abundance in a semi-analytic framework
• NIKA2 Cosmological Legacy Survey: Survey Description and Galaxy Number Counts
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• The cosmic spectral energy distribution in the EAGLE simulation
• G.A.S. II: Dust extinction in galaxies; Luminosity functions and InfraRed eXcess
• Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar halo
• Massive High-Redshift Quiescent Galaxies With JWST
• Compact Molecular Gas Distribution in Quasar Host Galaxies
• Reignited star formation in dwarf galaxies quenched during reionization
• The half mass radius of MaNGA galaxies: Effect of IMF gradients
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• Magnetic fields in elliptical galaxies: an observational probe of the fluctuation dynamo action
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• An ultra-deep multi-band VLA survey of the faint radio sky (COSMOS-XS): New constraints on the cosmic star formation history
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Influence of ~7 keV sterile neutrino dark matter on the process of reionization
• Redshift estimates for fast radio bursts and implications on intergalactic magnetic fields
• Rosella: A mock catalogue from the P-Millennium simulation
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright sub-millimetre galaxies
• Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
• Origins Space Telescope: predictions for far-IR spectroscopic surveys
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• How feedback shapes galaxies: an analytic model
• The dispersion measure and rotation measure from fast radio burst host galaxies based on the IllustrisTNG50 simulation
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy 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
• The cosmic atomic hydrogen mass density as a function of mass and galaxy hierarchy from spectral stacking
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• The Mass Growth and Stellar Ages of Galaxies: Observations versus Simulations
• Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning
• The environment of radio galaxies: A signature of AGN feedback at high redshifts
• AGNs at the cosmic dawn: predictions for future surveys from a $\Lambda$CDM cosmological model
• Maximising the power of deep extragalactic imaging surveys with the James Webb Space Telescope
• On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
• A new gas cooling model for semi-analytical galaxy formation models
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies
• The SCUBA-2 Large eXtragalactic Survey: 850um map, catalogue and the bright-end number counts of the XMM-LSS field
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Matching the mass function of Milky Way satellites in competing dark matter models
• NOEMA confirmation of an optically dark ALMA-AzTEC submillimetre galaxy at $z=5.24$. A late-stage starburst prior to quenching
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• Early Science with the Large Millimeter Telescope: a 1.1 mm AzTEC Survey of Red-$Herschel$ dusty star-forming galaxies
• Numerical simulations of bar formation in the Local Group
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• Modelling emission lines in star forming galaxies
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• High-z dusty star-forming galaxies: a top-heavy initial mass function?
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• ALMACAL VII: First Interferometric Number Counts at 650 $\mu$m
• Extragalactic Stellar Tidal Streams: Observations meet Simulation
• Diffuse neutrino supernova background as a cosmological test
• Measuring the BAO peak position with different galaxy selections
• Abundance matching for low mass galaxies in the CDM and FDM models
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Gravitational-wave event rates as a new probe for dark matter microphysics
• ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Recovering dark-matter clustering from galaxies with Gaussianization
• Halfway to the Peak: The JWST MIRI 5.6 micron number counts and source population
• Have we seen all the galaxies that comprise the cosmic infrared background at 250\,$\mu$m $\le \lambda \le$ 500\,$\mu$m?
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Recovery of the low- and high-mass end slopes of the IMF in massive early-type galaxies using detailed elemental abundances
• The faint end of the 250 micron luminosity function at z < 0.5
• Determining the systemic redshift of Lyman-alpha emitters with neural networks and improving the measured large-scale clustering
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• New constraints on red-spiral galaxies from their kinematics in clusters of galaxies
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Cosmic evolution of grain size distribution in galaxies using the ${\nu }^2$GC semi-analytic model
• SMART: spectral energy distributions Markov chain analysis with radiative transfer models
• The impact of the cosmological constant on past and future star formation
• How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 $\mu$m and Data Release for the COSMOS Field
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Multi-wavelength consensus of large-scale linear bias
• A comparison of ${\text{H}}_2$ formation models at high redshift
• A deep learning approach to halo merger tree construction
• Massive Molecular Gas as a Fuel Tank for Active Galactic Nuclei Feedback in Central Cluster Galaxies
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Measuring galaxy-galaxy-galaxy-lensing with higher precision and accuracy
• Infall Profiles for Supercluster-Scale Filaments
• Estimating the confusion noise for the Millimetron space telescope
• Cosmic happenstance: 24-$\mu$m selected, multi-component Herschel sources are line-of-sight projections
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• Are Lyα emitters segregated in protoclusters regions?
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• The history and mass content of cluster galaxies in the EAGLE simulation
• Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• 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