The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations

Abstract

We present results from thirteen cosmological simulations that explore the parameter space of the "Evolution and Assembly of GaLaxies and their Environments" (EAGLE) simulation project. Four of the simulations follow the evolution of a periodic cube L = 50 cMpc on a side, and each employs a different subgrid model of the energetic feedback associated with star formation. The relevant parameters were adjusted so that the simulations each reproduce the observed galaxy stellar mass function at z = 0.1. Three of the simulations fail to form disc galaxies as extended as observed, and we show analytically that this is a consequence of numerical radiative losses that reduce the efficiency of stellar feedback in high-density gas. Such losses are greatly reduced in the fourth simulation - the EAGLE reference model - by injecting more energy in higher density gas. This model produces galaxies with the observed size distribution, and also reproduces many galaxy scaling relations. In the remaining nine simulations, a single parameter or process of the reference model was varied at a time. We find that the properties of galaxies with stellar mass <~ M* (the "knee" of the galaxy stellar mass function) are largely governed by feedback associated with star formation, while those of more massive galaxies are also controlled by feedback from accretion onto their central black holes. Both processes must be efficient in order to reproduce the observed galaxy population. In general, simulations that have been calibrated to reproduce the low-redshift galaxy stellar mass function will still not form realistic galaxies, but the additional requirement that galaxy sizes be acceptable leads to agreement with a large range of observables.

Accepted for publication by MNRAS. v2: minor changes from submitted manuscript

References in corpus (29)

• 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
• 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
• Cold streams in early massive hot haloes as the main mode of galaxy formation
• Properties of galaxies reproduced by a hydrodynamic simulation
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• The Origin of the Galaxy Mass-Metallicity Relation and Implications for Galactic Outflows
• Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH
• Inviscid SPH
• Turbulent Structure of a Stratified Supernova-Driven Interstellar Medium
• A Superbubble Feedback Model for Galaxy Simulations
• Cosmic ray feedback in hydrodynamical simulations of galaxy formation
• Feedback and the Structure of Simulated Galaxies at redshift z=2
• The Nature and Origin of Low-Redshift O VI Absorbers
• Gone With the Wind: Where is the Missing Stellar Wind Energy from Massive Star Clusters?
• On the baryonic, stellar, and luminous scaling relations of disk galaxies
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• Clues for the origin of the fundamental metallicity relations. I: The hierarchical building up of the structure
• The evolution of the star forming sequence in hierarchical galaxy formation models
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Monolithic or hierarchical star formation? A new statistical analysis
• The Main Sequence and the Fundamental Metallicity Relation in MaGICC Galaxies: Evolution and Scatter
• The metallicity of galactic winds
• Numerical simulations of shocks encountering clumpy regions

Cited by in corpus (639)

• xCOLD GASS: the complete IRAM-30m legacy survey of molecular gas for galaxy evolution studies
• The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end
• The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z~8
• The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
• A High Stellar Velocity Dispersion and ~100 Globular Clusters for the Ultra Diffuse Galaxy Dragonfly 44
• Cold gas stripping in satellite galaxies: from pairs to clusters
• Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra
• From dawn till disk: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
• An Atlas of Color-selected Quiescent Galaxies at $z>3$ in Public $JWST$ Fields
• COSMOS2020: The Galaxy Stellar Mass Function: the assembly and star formation cessation of galaxies at $0.2<z\le 7.5$
• A chronicle of galaxy mass assembly in the EAGLE simulation
• Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
• Large-scale dark matter simulations
• Angular momentum evolution of galaxies in EAGLE
• Reverse engineering the Milky Way
• The SAMI Galaxy Survey: Revisiting Galaxy Classification Through High-Order Stellar Kinematics
• Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep Survey
• The Initial Masses of the Red Supergiant Progenitors to Type-II Supernovae
• Dynamical properties of z $\sim 4.5$ dusty star-forming galaxies and their connection with local early type galaxies
• Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ΛCDM?
• The origin of fast molecular outflows in quasars: molecule formation in AGN-driven galactic winds
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• MUFASA: Galaxy star formation, gas, and metal properties across cosmic time
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• The E-MOSAICS project: tracing galaxy formation and assembly with the age-metallicity distribution of globular clusters
• The Structure of Multiphase Galactic Winds
• Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges
• Star clusters near and far; tracing star formation across cosmic time
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function to $z=0.1$ from the r-band selected equatorial regions
• Galaxy And Mass Assembly (GAMA): ${\mathcal{M}}_{\star }-R_{\mathrm{e}}$ relations of $z=0$ bulges, discs and spheroids
• First results from SMAUG: Characterization of Multiphase Galactic Outflows from a Suite of Local Star-Forming Galactic Disk Simulations
• Far-infrared and dust properties of present-day galaxies in the EAGLE simulations
• Shaken and Stirred: The Milky Way's Dark Substructures
• Galaxy groups in the low-redshift Universe
• Baryon Cycles in the Biggest Galaxies
• The local high velocity tail and the Galactic escape speed
• The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disk turbulence in z~0.9 star-forming galaxies
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Weighing the stellar constituents of the Galactic halo with APOGEE red giant stars
• Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• The Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• The effect of baryons on the inner density profiles of rich clusters
• The Chemo-Dynamical Groups of Galactic Globular Clusters
• The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies
• The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• The Science of the Einstein Telescope
• What Causes The Formation of Disks and End of Bursty Star Formation?
• Dark matters on the scale of galaxies
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• Has JWST already falsified dark-matter-driven galaxy formation?
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - II: Size-luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass
• Snap, Crackle, Pop: sub-grid supernova feedback in AMR simulations of disk galaxies
• Galaxy gas as obscurer: II. Separating the galaxy-scale and nuclear obscurers of Active Galactic Nuclei
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• The core-cusp problem: a matter of perspective
• Λ CDM is Consistent with SPARC Radial Acceleration Relation
• The oldest and most metal poor stars in the APOSTLE Local Group simulations
• JADES: A large population of obscured, narrow line AGN at high redshift
• Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• The environmental dependence of gas accretion onto galaxies: quenching satellites through starvation
• The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6
• The properties of "dark" ΛCDM halos in the Local Group
• The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z=3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
• Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Dynamical Friction Modeling of Massive Black Holes in Cosmological Simulations and Effects on Merger Rate Predictions
• The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation
• The evolution of the star formation rate function in the EAGLE simulations: A comparison with UV, IR and H$\alpha$ observations from z ~ 8 to z ~ 0
• Formation histories of stars, clusters and globular clusters in the E-MOSAICS simulations
• DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons
• First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier
• The Close AGN Reference Survey (CARS). A massive multi-phase outflow impacting the edge-on galaxy HE1353-1917
• Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions
• An EAGLE view of the missing baryons
• An EAGLE's View of Ex-situ Galaxy Growth
• Black-hole-regulated star formation in massive galaxies
• Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST
• Multi-wavelength properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
• The formation of hot gaseous haloes around galaxies
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE
• Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations
• Tidal dwarf galaxies in cosmological simulations
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• Systematic difference between ionized and molecular gas velocity dispersion in $z\sim 1-2$ disks and local analogues
• The importance of black hole repositioning for galaxy formation simulations
• Merger-induced galaxy transformations in the ARTEMIS simulations
• Alignments between galaxies, satellite systems and haloes
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• Expectations of the size evolution of massive galaxies at $3\le z\le 6$ from the TNG50 simulation: the CEERS/JWST view
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
• Witnessing galaxy assembly in an extended z~3 structure
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• The impact of pre-supernova feedback and its dependence on environment
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Galactic inflow and wind recycling rates in the EAGLE simulations
• How Gas Accretion Feeds Galactic Disks
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
• KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at $z$$\sim$$1.4$-$2.6$
• Characterization of Low Surface Brightness structures in annotated deep images
• SINFONI-HiZELS: The dynamics, merger rates & metallicity gradients of `typical' star-forming galaxies at $z$ = 0.8-2.2
• Sub one percent mass fractions of young stars in red massive galaxies
• The Low Redshift Circumgalactic Medium in Simba
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at $z\ge 5$
• Cold gas removal from the centre of a galaxy by a low-luminosity jet
• Evolution of galactic planes of satellites in the EAGLE simulation
• Recovering ${\lambda }_R$ and $V/\sigma$ from seeing-dominated IFS data
• The origin of the enhanced metallicity of satellite galaxies
• The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulations
• Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
• The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
• The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to $\sim$10${}^6$ L${}_{\odot }$ and Comparisons with Galaxy Formation Models
• Triggering Active Galactic Nuclei in galaxy clusters
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• Robust Field-level Likelihood-free Inference with Galaxies
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• The evolution of the oxygen abundance gradients in star-forming galaxies in the EAGLE simulations
• The diverse evolutionary pathways of post-starburst galaxies
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• The SAMI Galaxy Survey: Satellite galaxies undergo little structural change during their quenching phase
• BASS XXXI: Outflow scaling relations in low redshift X-ray AGN host galaxies with MUSE
• Color gradients and half-mass radii of galaxies out to $z=2$ in the CANDELS/3D-HST fields: further evidence for important differences in the evolution of mass-weighted and light-weighted sizes
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• The Morphology-Density relationship in 1<z<2 clusters
• Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
• Blandford-Znajek jets in galaxy formation simulations: exploring the diversity of outflows produced by spin-driven AGN jets in Seyfert galaxies
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• The Cluster-EAGLE project: velocity bias and the velocity dispersion - mass relation of cluster galaxies
• Survey of Water and Ammonia in Nearby galaxies (SWAN): Resolved Ammonia Thermometry, Water and Methanol Masers in the Nuclear Starburst of NGC 253
• VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• The first Super Massive Black Holes: indications from models for future observations
• Satellites Around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations Versus Simulations
• The abundance and physical properties of O VII and O VIII X-ray absorption systems in the EAGLE simulations
• The Physical Origins of the Identified and Still Missing Components of the Warm-Hot Intergalactic Medium: Insights from Deep Surveys in the Field of Blazar 1ES1553+113
• The diversity of rotation curves of simulated galaxies with cusps and cores
• Revealing the properties of void galaxies and their assembly using the EAGLE simulation
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• Stellar splashback: the edge of the intracluster light
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• Green Valley galaxies as a transition population in different environments
• A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time
• An evolving and mass dependent ${\sigma }_{\text{sSFR}}$-${\mathrm{M}}_{\star }$ relation for galaxies
• The Close AGN Reference Survey (CARS): IFU survey data and the BH mass dependence of long-term AGN variability
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• How Unusual is the Milky Way's Assembly History?
• 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
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• The evolution of the metallicity gradient and the star formation efficiency in disc galaxies
• A Black Hole Mass Determination for the Compact Galaxy Mrk 1216
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Seeing sharper and deeper: JWST's first glimpse of the photometric and spectroscopic properties of galaxies in the epoch of reionisation
• Exploring compact binary merger host galaxies and environments with $\mathrm{zELDA}$
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Regulation of Star Formation by a Hot Circumgalactic Medium
• The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations
• Cosmic filaments delay quenching inside clusters
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Quenching Timescales in the IllustrisTNG Simulation
• The Fornax3D project: discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• UV to submillimetre luminosity functions of TNG50 galaxies
• First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• Strong Lensing by Galaxies
• The impact of galactic feedback on the shapes of dark-matter haloes
• Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• The physical drivers of the atomic hydrogen-halo mass relation
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• The impact of AGN-driven winds on physical and observable galaxy sizes
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
• Study of galaxies on large-scale filaments in simulations
• The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• The Physical Origin of Galactic Conformity: From Theory to Observation
• The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
• Linking globular cluster formation at low and high redshift through the age-metallicity relation in E-MOSAICS
• The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA
• The evolution of barred galaxies in the EAGLE simulations
• The Intrinsic Scatter of Galaxy Scaling Relations
• The impact of ionised outflows from z$\sim$2.5 quasars is not through instantaneous in-situ quenching: the evidence from ALMA and VLT/SINFONI
• The impact of the Large Magellanic Cloud on dark matter direct detection signals
• Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
• SDSS-IV MaNGA: How Galaxy Interactions Influence Active Galactic Nuclei
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z=2-5 Ultra- and Hyperluminous Infrared Galaxies
• The physical drivers of gas turbulence in simulated disc galaxies
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Quantified diffuse light in compact groups of galaxies
• On the detectability of visible-wavelength line emission from the local circumgalactic and intergalactic medium
• The ACCELERATION programme: I. Cosmology with the redshift drift
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• Reducing biases on $H_0$ measurements using strong lensing and galaxy dynamics: results from the EAGLE simulation
• The bright end of the infrared luminosity functions and the abundance of hyperluminous infrared galaxies
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI -- Stellar Populations
• Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• The galaxy-halo size relation of low-mass galaxies in FIRE
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• Stellar populations across the black hole mass - velocity dispersion relation
• GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• Using the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre
• Panspermia in a Milky Way-like Galaxy
• Predicting sub-millimeter flux densities from global galaxy properties
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• 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
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
• Origin and evolution of dust-obscured galaxies in galaxy mergers
• The Ages and Metallicities of the Globular Clusters in the Sparkler
• Being WISE II: Reducing the Influence of Star Formation History on the Mass-to-Light Ratio of Quiescent Galaxies
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• Properties of brightest group galaxies in cosmic web filaments
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Star formation in galaxies hosting AGN: A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey
• Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
• First Light And Reionisation Epoch Simulations (FLARES) VI: The colour evolution of galaxies $z=5-15$
• The galaxy morphology-density relation in the EAGLE simulation
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5
• Massive galaxy formation caught in action at z~5 with JWST
• EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
• Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane
• Galaxies with monstrous black holes in galaxy cluster environments
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• Evidence of extended cold molecular gas and dust halos around $\mathbf{z}\sim 2.3$ Extremely Red Quasars with ALMA
• Study of gravitational fields and globular cluster systems of early-type galaxies
• How identifying circumgalactic gas by line-of-sight velocity instead of the location in 3D space affects O VI measurements
• Taking the Milky Way for a spin: disc formation in the ARTEMIS simulations
• The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
• BUDDI-MaNGA II: The Star-Formation Histories of Bulges and Discs of S0s
• Galaxy and Mass Assembly (GAMA): Small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Red Supergiant Candidates for Multimessenger Monitoring of the Next Galactic Supernova
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• 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
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
• The cosmic spectral energy distribution in the EAGLE simulation
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The present-day gas content of simulated field dwarf galaxies
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• First Light And Reionisation Epoch Simulations (FLARES) XIII: The Lyman-continuum emission of high-redshift galaxies
• 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
• There and back again: understanding the critical properties of backsplash galaxies
• Dissecting Nearby Galaxies with piXedfit: II. Spatially Resolved Scaling Relations Among Stars, Dust, and Gas
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
• Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations
• CLASH-VLT: The inner slope of the MACS J1206.2-0847 dark matter density profile
• Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• Cosmic gas highways in C-EAGLE simulations
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Multiple stellar population mass loss in massive Galactic globular clusters
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Milky Way and M31 rotation curves: $\Lambda$CDM vs. MOND
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo Cluster
• The impact of mass map truncation on strong lensing simulations
• Unravelling the physics of multiphase AGN winds through emission line tracers
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• First Light And Reionisation Epoch Simulations (FLARES) XI: [OIII] emitting galaxies at $5<z<10$
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• The Galaxy Stellar Mass Function and Low Surface Brightness Galaxies from Core-Collapse Supernovae
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• Globular cluster metallicity distributions in the E-MOSAICS simulations
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• 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
• What has quenched the massive spiral galaxies?
• Little Red Dots as Direct-collapse Black Hole Nurseries
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• Ram pressure stripping in the EAGLE simulation
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• On the absence of backsplash analogues to NGC 3109 in the $\Lambda$CDM framework
• The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
• The Physical Nature of Circumgalactic Medium Absorbers in Simba
• An intergalactic medium temperature from a giant radio galaxy
• Galactic satellite systems in CDM, WDM and SIDM
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Optical Properties of Peaked Spectrum Radio Sources
• The origin of star-gas misalignments in simulated galaxies
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Do current X-ray observations capture most of the black-hole accretion at high redshifts?
• Detection capabilities of the Athena X-IFU for the warm-hot intergalactic medium using gamma-ray burst X-ray afterglows
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• The first GLIMPSE of the faint galaxy population at Cosmic Dawn with JWST: The evolution of the ultraviolet luminosity function across z~9-15
• Discovery of a multiphase OVI and OVII absorber in the circumgalactic/intergalactic transition region
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• Formation of disc galaxies around z~2
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Abundance and group coalescence timescales of compact groups of galaxies in the EAGLE simulation
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• A common origin for the Fundamental Plane of quiescent and star-forming galaxies in the EAGLE simulations
• An environment-dependent halo mass function as a driver for the early quenching of $z\ge 1.5$ cluster galaxies
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
• A Distinct Radial Acceleration Relation across Brightest Cluster Galaxies and Galaxy Clusters
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• History of the gas fuelling star formation in eagle galaxies
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• The local dark matter distribution in self-interacting dark matter halos
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• JCMT/SCUBA-2 uncovers an excess of $850\mu$m counts on megaparsec scales around high-redshift quasars. Characterization of the overdensities and their alignment with the quasars' Ly$\alpha$ nebulae
• Is Terzan 5 the remnant of a building block of the Galactic bulge? Evidence from APOGEE
• Maximal X-ray feedback in the pre-reionization universe
• The SAMI Galaxy Survey: The contribution of different kinematic classes to the stellar mass function of nearby galaxies
• 3D Detection and Characterisation of ALMA Sources through Deep Learning
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
• 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
• Constraints on galactic outflows from the metallicity-stellar mass-SFR relation of EAGLE simulation and SDSS galaxies
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• Determining Satellite Infall Times Using Machine Learning
• ASymba: HI global profile asymmetries in the Simba simulation
• A field-level emulator for modeling baryonic effects across hydrodynamic simulations
• SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
• The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• Early-type galaxies in low-density environments: NGC 6876 explored through its globular cluster system
• Using EAGLE simulations to study the effect of observational constraints on the determination of HI asymmetries in galaxies
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• Can $\Lambda$CDM model reproduce MOND-like behavior?
• Black hole feedback and the evolution of massive early-type galaxies
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• The Close AGN Reference Survey (CARS). A parsec scale multi-phase outflow in the super-Eddington NLS1 Mrk 1044
• A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• The Dark Matter Halos of HI Selected Galaxies
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• Resolved star formation in TNG100 central and satellite galaxies
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• The extragalactic $\gamma$-ray background: imprints from the physical properties and evolution of star-forming galaxy populations
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Insights on Metal Enrichment and Environmental Effect at $z\approx 5-7$ with JWST ASPIRE/EIGER and Chemical Evolution Model
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• Gravitational Waves from Massive Black Hole Mergers in ASTRID: Predictions for LISA
• SQuIGG$\vec{L}$E: Observational Evidence of Low Ongoing Star Formation Rates in Gas-Rich Post-Starburst Galaxies
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Globular cluster ages and their relation to high-redshift stellar cluster formation times from different globular cluster models
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• Simulated [CII] in high-z galaxies
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• A search for the missing baryons with X--ray absorption lines towards the blazar 1ES 1553+113
• A deep learning approach to halo merger tree construction
• Spin speed correlations and the evolution of galaxy-halo systems
• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
• Old and New Major Mergers in the SOSIMPLE galaxy, NGC 7135
• Initial sizes of star clusters: implications for cluster dissolution during galaxy evolution
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• A Simple Sub-Grid Model For Cosmic Ray Effects on Galactic Scales
• A comprehensive study on the relation between the metal enrichment of ionised and atomic gas in star-forming galaxies
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Measuring Galaxy Asymmetries in 3D
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• The history and mass content of cluster galaxies in the EAGLE simulation
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• On the application of dimensionality reduction and clustering algorithms for the classification of kinematic morphologies of galaxies
• Gamma rays from dark matter spikes in EAGLE simulations
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• Velocity-dependent J-factors for Milky Way dwarf spheroidal analogues in cosmological simulations
• Red riding on hood: Exploring how galaxy colour depends on environment
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• An HI story of galaxies in Abell 2626 and beyond
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• The formation and disruption of globular cluster populations in simulations of present-day $L^{\ast }$ galaxies with controlled assembly histories
• Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• The case for two-dimensional galaxy-galaxy lensing
• Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
• From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Sensitivity analysis of a galaxy formation model
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies
• Multiphase gas in elliptical galaxies: the role of Type Ia supernovae
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• Detection of an orthogonal alignment between parsec scale AGN jets and their host galaxies
• Rapid, out of equilibrium metal enrichment indicated by a flat mass-metallicity relation at z~6 from NIRCam grism spectroscopy
• syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Robust machine learning model of inferring the ex-situ stellar fraction of galaxies from photometric data
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Simulations of the accreted stellar halos of low-mass field galaxies
• Untangling Stellar Components of Galaxies: Evaluation of Dynamical Decomposition Methods in Simulated Galaxies with GalaxyChop
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• Unveiling galaxy pair alignment in cosmic filaments: A 3D exploration using EAGLE simulation
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
• The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
• The Star Formation Reference Survey. IV. Stellar mass distribution of local star-forming galaxies
• Using machine learning to study the kinematics of cold gas in galaxies
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• A correlation between accreted stellar kinematics and dark matter halo spin in the ARTEMIS simulations
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• The "Building Blocks" of Stellar Halos
• Fast radio bursts as probes of feedback from active galactic nuclei
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• The Type Ia Supernova and Asymptotic Giant Branch Stellar Ejecta-regulated Interstellar Medium of Massive Galaxies
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
• The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories
• A new strategy for matching observed and simulated lensing galaxies
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Are there any extragalactic high speed dark matter particles in the Solar neighborhood?
• The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies
• Identification and Quenching of Nugget Galaxies in the RESOLVE Survey at z = 0
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type galaxies
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• Using dust to constrain dark matter models
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Following the crumbs: Statistical effects of Ram Pressure in Galaxies
• Spatial field reconstruction with INLA: Application to simulated galaxies
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• Investigating chemical variations between interstellar gas clouds in the Solar neighbourhood
• The dynamical evolution of the stellar clumps in the Sparkler galaxy
• The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
• Exploring the outskirts of the EAGLE disc galaxies
• The FLAMINGO simulations data release
• NEW-MUSIC: The Next-generation Extended-Wavelength Multiband Sub/millimeter Inductance Camera
• Study of dependence of ram pressure stripping on the orbital parameters of the galaxies
• Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• No dependence of radio properties of brightest group galaxies on the luminosity gap
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• The intragroup light in KiDS+GAMA groups: A stacking analysis
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• The haloes that reionized the Universe
• The multi-component fitting to the star formation histories in the TNG simulation
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• A Halo Merger Tree Generation and Evaluation Framework
• Deciphering galaxy images using machine vision -- Combining variational autoencoder and principal component analysis for feature extraction
• One latent to fit them all: a unified representation of baryonic feedback on matter distribution
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
• On the signature of black holes on the quenched stellar mass function
• Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
• Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
• The intracluster light as an estimator of the cluster mass profile
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Reduced Gas Accretion onto Galaxies due to Effects of External Giant Radio Lobes
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
• Baryon-driven decontraction in Milky Way mass haloes
• Assessment of Dark Matter Models Using Dark Matter Correlations across Dwarf Spheroidal Galaxies
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• The long road to the Green Valley: Tracing the evolution of the Green Valley galaxies in the EAGLE simulation
• Predicting large scale cosmological structure evolution with generative adversarial network-based autoencoders
• Ergodicity of FIRE: star formation variations within and between simulated galaxies
• Mainly on the Plane: Observing the Extended, Ionized Disks of Milky Way Analogs in IllustrisTNG
• Numerical Study of Bar Suppression in Galaxy Models Due to Disc Heating
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation
• Reconciling concentration to virial mass relations
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?
• From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
• The Scaling Relation between Galaxy Luminosity and WHIM Density from EAGLE Simulations with application to SDSS data
• The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra
• 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
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• Can AI Dream of Unseen Galaxies? Conditional Diffusion Model for Galaxy Morphology Augmentation
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• A Tilt in the Dark Matter Halo of the Galaxy
• Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation
• Modeling Multiphase Galactic Outflows: A Multifluid Moving Mesh Approach
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Now you see it, now you don't: Star formation truncation precedes the loss of molecular gas by ~100 Myr in massive post-starburst galaxies at z~0.6
• Detection of HI filament: Pair Stacking vs. Filament Stacking
• Estimating Transient Rates from Cosmological Simulations and BPASS
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Determining the Dark Matter distribution in galaxies with Deep Learning
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Molecular gas content of gravitational-lensed quasars at cosmic noon
• SDSS-IV MaNGA: Exploring the local scaling relations for N/O
• Stellar halos of bright central galaxies II: Scaling relations, colors and metallicity evolution with redshift
• The stellar population of a $z\sim 3.25$ Ly$\alpha$ emitting group associated with a damped Ly$\alpha$ absorber
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Aligned and misaligned metallicity gradients in young stars and star-forming regions in the EAGLE discs
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• Imladris: a detailed and flexible model for galaxy simulations with individual stars