The EAGLE project: Simulating the evolution and assembly of galaxies and their environments

Abstract

We introduce the Virgo Consortium's EAGLE project, a suite of hydrodynamical simulations that follow the formation of galaxies and black holes in representative volumes. We discuss the limitations of such simulations in light of their finite resolution and poorly constrained subgrid physics, and how these affect their predictive power. One major improvement is our treatment of feedback from massive stars and AGN in which thermal energy is injected into the gas without the need to turn off cooling or hydrodynamical forces, allowing winds to develop without predetermined speed or mass loading factors. Because the feedback efficiencies cannot be predicted from first principles, we calibrate them to the z~0 galaxy stellar mass function and the amplitude of the galaxy-central black hole mass relation, also taking galaxy sizes into account. The observed galaxy mass function is reproduced to $\lesssim 0.2$ dex over the full mass range, $10^8<M_{\ast }/M_{\odot }\lesssim 10^{11}$, a level of agreement close to that attained by semi-analytic models, and unprecedented for hydrodynamical simulations. We compare our results to a representative set of low-redshift observables not considered in the calibration, and find good agreement with the observed galaxy specific star formation rates, passive fractions, Tully-Fisher relation, total stellar luminosities of galaxy clusters, and column density distributions of intergalactic CIV and OVI. While the mass-metallicity relations for gas and stars are consistent with observations for $M_{\ast }\gtrsim 10^9{M}_{\odot }$, they are insufficiently steep at lower masses. The gas fractions and temperatures are too high for clusters of galaxies, but for groups these discrepancies can be resolved by adopting a higher heating temperature in the subgrid prescription for AGN feedback. EAGLE constitutes a valuable new resource for studies of galaxy formation.

Accepted for publication in MNRAS. V2: Minor changes. For images and videos, see http://eagle.strw.leidenuniv.nl/ and http://icc.dur.ac.uk/Eagle/

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• Connecting the structure of dark matter haloes to the primordial power spectrum
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• The metallicity of galactic winds
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• The Gas-Star Formation Cycle in Nearby Star-forming Galaxies II. Resolved Distributions of CO and H$\alpha$ Emission for 49 PHANGS Galaxies
• The [α/Fe]-[Fe/H] relation in the E-MOSAICS simulations: its connection to the birth place of globular clusters and the fraction of globular cluster field stars in the bulge
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• A new direction for dark matter research: intermediate mass compact halo objects
• How Unusual is the Milky Way's Assembly History?
• Stellar Dynamics and Star-Formation Histories of z $\sim$ 1 Radio-loud Galaxies
• The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
• Galaxy and Mass Assembly (GAMA): Demonstrating the power of WISE in the study of Galaxy Groups to $z<0.1$
• From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Predicting star formation properties of galaxies using deep learning
• The effect of non-equilibrium metal cooling on the interstellar medium
• A Black Hole Mass Determination for the Compact Galaxy Mrk 1216
• High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
• On the Determination of Rotation Velocity and Dynamical Mass of Galaxies Based on Integrated H I Spectra
• Spectral Classification and Ionized Gas Outflows in $z\sim 2$ WISE-Selected Hot Dust-Obscured Galaxies
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• North Ecliptic Pole merging galaxy catalogue
• Simulating the effect of photoheating feedback during reionization
• Stellar and black hole assembly in z<0.3 infrared-luminous mergers: intermittent starbursts vs. super-Eddington accretion
• Quenching Timescales in the IllustrisTNG Simulation
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Does the Milky Way Obey Spiral Galaxy Scaling Relations?
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• Deciphering the imprint of AGN feedback in Seyfert galaxies: Nuclear-scale molecular gas deficits
• The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations
• The Origin of Exponential Star-forming Disks
• SDSS-IV MaNGA: drivers of stellar metallicity in nearby galaxies
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• Supernovae feedback propagation: the role of turbulence
• A population of galaxy-scale jets discovered using LOFAR
• UV to submillimetre luminosity functions of TNG50 galaxies
• Star formation quenching stages of active and non-active galaxies
• Deviations from tidal torque theory: evolution of the halo spin-filament alignment
• The physical drivers of the atomic hydrogen-halo mass relation
• A cosmological context for compact massive galaxies
• The Illustris Simulation: Supermassive Black Hole - Galaxy Connection Beyond the Bulge
• The angular momentum of disc galaxies at z=1
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• The impact of AGN-driven winds on physical and observable galaxy sizes
• Study of galaxies on large-scale filaments in simulations
• Stellar feedback strongly alters the amplification and morphology of galactic magnetic fields
• Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
• Linking globular cluster formation at low and high redshift through the age-metallicity relation in E-MOSAICS
• The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
• The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z~3
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• Galaxy populations in the Hydra I cluster from the VEGAS survey I. Optical properties of a large sample of dwarf galaxies
• Red quasars blow out molecular gas from galaxies during the peak of cosmic star formation
• A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate redshift galaxies with WEAVE
• Chemical evolution of disc galaxies from cosmological simulations
• VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
• Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• The ACCELERATION programme: I. Cosmology with the redshift drift
• Quantified diffuse light in compact groups of galaxies
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• A tight relation between the age distributions of stellar clusters and the properties of the interstellar medium in the host galaxy
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• On the detectability of visible-wavelength line emission from the local circumgalactic and intergalactic medium
• BAT AGN Spectroscopic Survey -- XVII: The Parsec-scale Jet Properties of the Ultra Hard X-ray Selected Local AGN
• Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
• A Multiwavelength Study of Active Galactic Nuclei in Post-Merger Remnants
• Reducing biases on $H_0$ measurements using strong lensing and galaxy dynamics: results from the EAGLE simulation
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI -- Stellar Populations
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• The bright end of the infrared luminosity functions and the abundance of hyperluminous infrared galaxies
• Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
• Ionized Outflows in Nearby Quasars are Poorly Coupled to their Host Galaxies
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• Direct measurement of the distribution of dark matter with strongly lensed gravitational waves
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Numerical modelling of the lobes of radio galaxies in cluster environments -- IV. Remnant radio galaxies
• Stacked star formation rate profiles of bursty galaxies exhibit 'coherent' star formation
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• Nonparametric galaxy morphology from UV to submm wavelengths
• Using the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre
• Stellar populations across the black hole mass - velocity dispersion relation
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• The fundamental metallicity relation emerges from the local anti-correlation between star formation rate and gas-phase metallicity existing in disk galaxies
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• Do we need soft cosmology?
• Predicting sub-millimeter flux densities from global galaxy properties
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• The cosmic build-up of dust and metals. Accurate abundances from GRB-selected star-forming galaxies at $1.7<z<6.3$
• Baryonic mass budgets for haloes in the EAGLE simulation, including ejected and prevented gas
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
• Star formation quenching imprinted on the internal structure of naked red nuggets
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Subaru Hyper Suprime-Cam View of Quasar Host Galaxies at z < 1
• Properties of brightest group galaxies in cosmic web filaments
• The Warm Circum-Galactic Medium: 10^5-6 K Gas Associated with a Single Galaxy Halo or with an Entire Group of Galaxies?
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• Simulation techniques for modified gravity
• ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Not a Copernican observer: biased peculiar velocity statistics in the local Universe
• The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
• Being WISE II: Reducing the Influence of Star Formation History on the Mass-to-Light Ratio of Quiescent Galaxies
• Coevolution of metallicity and star formation in galaxies to z=3.7: II. A theoretical model
• Impact of Baryonic Physics on Intrinsic Alignments
• Stellar feedback in M83 as observed with MUSE -- I. Overview, an unprecedented view of the stellar and gas kinematics and evidence of outflowing gas
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• Galaxy properties in the cosmic web of EAGLE simulation
• Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The Contribution of Quasar Absorption Outflows to AGN Feedback
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• Intermittent AGN episodes drive outflows with a large spread of observable loading factors
• Enhanced star formation in $z\sim 6$ quasar companions
• The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies
• First Light And Reionisation Epoch Simulations (FLARES) VI: The colour evolution of galaxies $z=5-15$
• Mass Metallicity Relationship of SDSS Star Forming Galaxies: Population Synthesis Analysis and Effects of Star Burst Length, Extinction Law, Initial Mass Function and Star Formation Rate
• MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Low-mass compact elliptical galaxies: spatially-resolved stellar populations and kinematics with the Keck Cosmic Web Imager
• Connecting cosmological accretion to strong Lyman-alpha absorbers
• Galaxies with monstrous black holes in galaxy cluster environments
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Hydrodynamical structure formation in Milgromian cosmology
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Merger histories of brightest group galaxies from MUSE stellar kinematics
• Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane
• Star formation in the nearby dwarf galaxy DDO 53: interplay between gas accretion and stellar feedback
• From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• Realistic HI scale heights of Milky Way-mass galaxies in the FIREbox cosmological volume
• The galaxy-galaxy strong lensing cross-sections of simulated LCDM galaxy clusters
• A 4% measurement of $H_0$ using the cumulative distribution of strong-lensing time delays in doubly-imaged quasars
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• Galaxy and Mass Assembly (GAMA): Small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Late-time cosmic evolution of dust: solving the puzzle
• The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
• Do galaxies die? Different views from simulations and observations in the Local Universe
• Some Die Filthy Rich: The Diverse Molecular Gas Contents of Post-starburst Galaxies Probed by Dust Absorption
• The cosmic spectral energy distribution in the EAGLE simulation
• The Hector Survey: integral field spectroscopy of 100,000 galaxies
• A new discovery space opened by eROSITA: Ionised AGN outflows from X-ray selected samples
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• The present-day gas content of simulated field dwarf galaxies
• Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• On the dearth of ultra-faint extremely metal poor galaxies
• The SAMI Galaxy Survey: The role of disc fading and progenitor bias in kinematic transitions
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Dissecting Nearby Galaxies with piXedfit: II. Spatially Resolved Scaling Relations Among Stars, Dust, and Gas
• Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Monte Carlo Physarum Machine: Characteristics of Pattern Formation in Continuous Stochastic Transport Networks
• Stellar dynamics in the strong-lensing central galaxy of Abell 1201: A low stellar mass-to-light ratio, a large central compact mass, and a standard dark matter halo
• The observed cosmic star formation rate density has an evolution which resembles a Γ(a, bt) distribution and can be described successfully by only 2 parameters
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• SUPER VII. Morphology and kinematics of H$\alpha$ emission in AGN host galaxies at Cosmic noon using SINFONI
• Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
• Mg II and Fe II fluxes of luminous quasars at z ~ 2.7 and evaluation of the Baldwin effect in the flux-to-abundance conversion method for quasars
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Simulating ionization feedback from young massive stars: impact of numerical resolution
• The impact of black hole seeding in cosmological simulations
• The Galactic Interstellar Object Population: A Framework for Prediction and Inference
• Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• Intracluster light in the core of z~2 galaxy proto-clusters
• The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments
• Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
• Gravitational lensing in LoTSS DR2 -- Extremely faint 144-MHz radio emission from two highly magnified quasars
• Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
• Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
• Nonparametric galaxy morphology from stellar and nebular emission with the CALIFA sample
• 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
• Simplified galaxy formation with mesh-less hydrodynamics
• The galaxy's gas content regulated by the dark matter halo mass results in a super-linear M${}_{\mathrm{BH}}$-M${}_{\star }$ relation
• The most luminous, merger-free AGN show only marginal correlation with bar presence
• Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• Where infall meets outflows: turbulent dissipation probed by CH${}^{+}$ and Ly$\alpha$ in the starburst/AGN galaxy group SMM J02399$-$0136 at z$\sim$2.8
• Cosmic gas highways in C-EAGLE simulations
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo Cluster
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• CMB-HD: Astro2020 RFI Response
• The growth of typical star-forming galaxies and their super massive black holes across cosmic time since z~2
• The impact of mass map truncation on strong lensing simulations
• 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
• Analysis of the galaxy size versus stellar mass relation
• Detection of the self-regulation of star formation in galaxy discs
• Testing galaxy formation models with galaxy stellar mass functions
• The Galaxy Stellar Mass Function and Low Surface Brightness Galaxies from Core-Collapse Supernovae
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• What has quenched the massive spiral galaxies?
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• WALLABY Pre-Pilot Survey: The effects of angular momentum and environment on the HI gas and star formation properties of galaxies in the Eridanus supergroup
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• Quantifying the cool ISM in radio AGNs: evidence for late-time re-triggering by galaxy mergers and interactions
• The Mass Growth and Stellar Ages of Galaxies: Observations versus Simulations
• Predicting the water content of interstellar objects from galactic star formation histories
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• The bar rotation rate as a diagnostic of dark matter content in the centre of disc galaxies
• Spatially resolved observations of outflows in the radio loud AGN of UGC 8782
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• The Velocity Dispersion Function for Massive Quiescent and Star-Forming Galaxies at 0.6 $<$ z $\le$ 1.0
• Detection capabilities of the Athena X-IFU for the warm-hot intergalactic medium using gamma-ray burst X-ray afterglows
• Morphology-assisted galaxy mass-to-light predictions using deep learning
• Galactic satellite systems in CDM, WDM and SIDM
• The kinematics of young and old stellar populations in nuclear rings of MUSE TIMER galaxies
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• An intergalactic medium temperature from a giant radio galaxy
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• CGM${}^2$ $+$ CASBaH: The Mass Dependence of H~I Ly$\alpha$-Galaxy Clustering and the Extent of the CGM
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
• Physical Conditions of Five O VI Absorption Systems Towards PG $1522+101$
• Abundance and group coalescence timescales of compact groups of galaxies in the EAGLE simulation
• VLT/SINFONI study of black hole growth in high redshift radio-loud quasars from the CARLA survey
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Young Massive Clusters: Their Population Properties, Formation and Evolution, and Their Relation to the Ancient Globular Clusters
• Cold molecular gas outflow encasing the ionised one in the Seyfert galaxy NGC 3281
• A Comparison of Star-Forming Clumps and Tidal Tails in Local Mergers and High Redshift Galaxies
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• LyMAS reloaded: improving the predictions of the large-scale Lyman-α forest statistics from dark matter density and velocity fields
• G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
• MARTINI: Mock Array Radio Telescope Interferometry of the Neutral ISM
• BUDHIES V: The baryonic Tully-Fisher relation at z=0.2 based on direct HI detections
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• Quenching in the Right Place at the Right Time: Tracing the Shared History of Starbursts, AGNs, and Post-starburst Galaxies Using Their Structures and Multiscale Environments
• Is Terzan 5 the remnant of a building block of the Galactic bulge? Evidence from APOGEE
• The OH Megamaser galaxy IRAS11506-3851: an AGN and starformation revealed by multiwavelength observations
• The Tail of Late-forming Dwarf Galaxies in $\Lambda$CDM
• The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• History of the gas fuelling star formation in eagle galaxies
• Probing Feedback in Galaxy Formation with Millimeter-wave Observations
• A Distinct Radial Acceleration Relation across Brightest Cluster Galaxies and Galaxy Clusters
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• Modelling Dark Matter Halo Spin using Observations and Simulations: application to UGC 5288
• A common origin for the Fundamental Plane of quiescent and star-forming galaxies in the EAGLE simulations
• A study of the HI gas fractions of galaxies at z ~ 1
• Quantifying the effect of black hole feedback from the central galaxy on the satellite populations of groups and clusters
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Testing the tidal stripping scenario of ultra-compact dwarf galaxy formation by using internal properties
• The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
• The physics governing the upper truncation mass of the globular cluster mass function
• Galaxy flows within 8,000 km/s from Numerical Action methods
• A modern view of galaxies and their stellar populations
• Stellar angular momentum distribution linked to galaxy morphology
• Early-type galaxies in low-density environments: NGC 6876 explored through its globular cluster system
• Formation and fate of low metallicity stars in IllustrisTNG50
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Projecting SPH Particles in Adaptive Environments
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• The faint end of the 250 micron luminosity function at z < 0.5
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• ASymba: HI global profile asymmetries in the Simba simulation
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Probing the physical properties of the intergalactic medium using gamma-ray bursts
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
• What is the real accretion rate onto a black hole for low angular momentum accretion?
• A counter-image to the gravitational arc in Abell 1201: Evidence for IMF variations, or a $10^{10}$M${}_{\odot }$ black hole?
• Can $\Lambda$CDM model reproduce MOND-like behavior?
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• The extragalactic $\gamma$-ray background: imprints from the physical properties and evolution of star-forming galaxy populations
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (I) Temporal dependency
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• Measuring the physical imprints of gas flows in galaxies I: Accretion rate histories
• Resolved star formation in TNG100 central and satellite galaxies
• SDSS-IV MaNGA: Unveiling Galaxy Interaction by Merger Stages with Machine Learning
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• The Ursa Major Association of Galaxies. VI: A relative dearth of gas-rich dwarf galaxies
• The SAMI Galaxy Survey: Detection of Environmental Dependence of Galaxy Spin in Observations and Simulations Using Marked Correlation Functions
• Probing the physical properties of the intergalactic medium using blazars
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
• A break in the high-redshift stellar mass Tully-Fisher relation
• A WHIM origin for the soft excess emission in the Coma cluster
• The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories
• Bursty star formation feedback and cooling outflows
• A deep learning approach to halo merger tree construction
• Old and New Major Mergers in the SOSIMPLE galaxy, NGC 7135
• The formation of compact massive relic galaxies in MOND
• Black Hole Feeding and Feedback in a Compact Galaxy
• A search for the missing baryons with X--ray absorption lines towards the blazar 1ES 1553+113
• Abundance matching tested on small scales with galaxy dynamics
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• Dipolar dark matter simulations on galaxy scales with the RAMSES code
• The MAGPI survey: The interdependence of the mass, star formation rate, and metallicity in galaxies at z~0.3
• Numerical Discreteness Errors in Multi-Species Cosmological N-body Simulations
• Dissociation of dark matter and gas in cosmic large-scale structure
• Local Two-Sample Testing: A New Tool for Analysing High-Dimensional Astronomical Data
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• Measurements of the angular momentum-mass relations in the Simba simulation
• An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
• Measuring Galaxy Asymmetries in 3D
• Disc-Halo Interactions in ΛCDM
• Simulating the dark matter decay signal from the Perseus galaxy cluster
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Tracing the Formation of Molecular Clouds in a Low-Metallicity Galaxy: A HI Narrow Self-Absorption Survey of the Large Magellanic Cloud
• The OTELO survey: the star formation rate evolution of low-mass galaxies
• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
• Domain adaptation techniques for improved cross-domain study of galaxy mergers
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• The case for two-dimensional galaxy-galaxy lensing
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• Does radiative feedback make faint z>6 galaxies look small?
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Galaxy-galaxy lensing in the VOICE deep survey
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• Efficiently estimating mean, uncertainty and unconstrained large scale fraction of local Universe simulations with paired fixed fields
• Galaxy formation from a timescale perspective
• Local variations of the Stellar Velocity Ellipsoid-I: the disc of galaxies in the Auriga simulations
• The Impact of Baryons on the Large-Scale Structure of the Universe
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• SEURAT: SPH scheme extended with ultraviolet line radiative transfer
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Evolution of thermal and nonthermal radio continuum emission on kpc scales--Predictions for SKA
• Dark matter haloes: a multistream view
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies
• Galaxy cluster photons alter the ionisation state of the nearby warm-hot intergalactic medium
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Digging deeper into NGC\,6868 I: stellar population
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Refueled and shielded - The early evolution of Tidal Dwarf Galaxies
• Evolution of dwarf galaxy observable parameters
• Using machine learning to study the kinematics of cold gas in galaxies
• Sensitivity analysis of a galaxy formation model
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (II) The inside-out growth of discs
• Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
• Probing the physical properties of the IGM using SRG/eROSITA spectra from blazars
• Local variations of the Stellar Velocity Ellipsoid-II: the effect of the bar in the inner regions of Auriga galaxies
• The "Building Blocks" of Stellar Halos
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
• The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories
• Eigenmode analysis of perurbations in the primordial medium at and before recombination
• Continuous Simulation Data Stream: A dynamical timescale-dependent output scheme for simulations
• Ionized gas kinematics of massive elliptical galaxies in CALIFA and in cosmological zoom-in simulations
• Distribution of Phantom Dark Matter in Dwarf Spheroidals
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• Following the crumbs: Statistical effects of Ram Pressure in Galaxies
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Study of Central Intensity Ratio of Seyfert Galaxies in nearby Universe
• Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• Study of dependence of ram pressure stripping on the orbital parameters of the galaxies
• Predicting far-infrared maps of galaxies via machine learning techniques
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• The Star Formation History of a Post-Starburst Galaxy Determined From Its Cluster Population
• Predicting halo occupation and galaxy assembly bias with machine learning
• The multi-component fitting to the star formation histories in the TNG simulation
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• Cluster environment quenches the star formation of low-mass satellite galaxies from the inside-out
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Supermassive black holes in a mass-limited galaxy sample
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Investigating the variability of Swift-BAT blazars with NICER
• A Halo Merger Tree Generation and Evaluation Framework
• The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra
• Debunking Generalization Error or: How I Learned to Stop Worrying and Love My Training Set
• Ultra-fast model emulation with PRISM; analyzing the Meraxes galaxy formation model
• Spatial disconnection between stellar and dust emissions: the test of the Antennae Galaxies (Arp 244)
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• Combining LOFAR and Apertif Data for Understanding the Life Cycle of Radio Galaxies
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• The Galaxy Evolution Probe
• The Metallicity Distribution Function in Outer Halo Fields of Simulated Elliptical Galaxies Compared to Observations of NGC 5128
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
• The MAGIC project. III. Radial and azimuthal Galactic abundance gradients using classical Cepheids
• Merger or Not: Accounting for Human Biases in Identifying Galactic Merger Signatures
• Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• The Scaling Relation between Galaxy Luminosity and WHIM Density from EAGLE Simulations with application to SDSS data
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• SDSS-IV MaNGA: Exploring the local scaling relations for N/O
• On the hosts of neutron star mergers in the nearby Universe
• The link between star formation and gas in nearby galaxies