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.

arXiv commentAccepted 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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• Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ΛCDM?
• A Model for the Origin of Bursty Star Formation in Galaxies
• Jellyfish galaxies with the IllustrisTNG simulations: I. Gas-stripping phenomena in the full cosmological context
• Cosmic evolution of stellar quenching by AGN feedback: clues from the Horizon-AGN simulation
• Vlasov methods in space physics and astrophysics
• Hydrodynamical Coupling of Mass and Momentum in Multiphase Galactic Winds
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• Formation of In Situ Stellar Haloes in Milky Way-Mass Galaxies
• Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback
• The FABLE simulations: A feedback model for galaxies, groups and clusters
• How do central and satellite galaxies quench? -- Insights from spatially resolved spectroscopy in the MaNGA survey
• MUFASA: Galaxy star formation, gas, and metal properties across cosmic time
• The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation
• The ASTRID simulation: the evolution of Supermassive Black Holes
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• The role of cosmic ray pressure in accelerating galactic outflows
• The E-MOSAICS project: tracing galaxy formation and assembly with the age-metallicity distribution of globular clusters
• Simulating the interstellar medium and stellar feedback on a moving mesh: Implementation and isolated galaxies
• Globular Cluster Formation and Evolution in the Context of Cosmological Galaxy Assembly: Open Questions
• Non-circular motions and the diversity of dwarf galaxy rotation curves
• The Extraordinary Amount of Substructure in the Hubble Frontier Fields Cluster Abell 2744
• The alignment and shape of dark matter, stellar, and hot gas distributions in the EAGLE and cosmo-OWLS simulations
• The origin of galactic metal-rich stellar halo components with highly eccentric orbits
• First Light And Reionisation Epoch Simulations (FLARES) I: Environmental Dependence of High-Redshift Galaxy Evolution
• Are galactic star formation and quenching governed by local, global or environmental phenomena?
• The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
• Galaxy metallicity scaling relations in the EAGLE simulations
• Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges
• The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes
• Metal-enriched galactic outflows shape the mass-metallicity relationship
• The role of mergers in driving morphological transformation over cosmic time
• Star clusters near and far; tracing star formation across cosmic time
• Active Galactic Nuclei Feedback in an Elliptical Galaxy with the Most Updated AGN Physics (I): Low-angular Momentum Case
• The total satellite population of the Milky Way
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function to $z=0.1$ from the r-band selected equatorial regions
• The erratic dynamical life of black hole seeds in high-redshift galaxies
• The formation and evolution of low-surface-brightness galaxies
• Galactic outflow rates in the EAGLE simulations
• Origin and properties of dual and offset active galactic nuclei in a cosmological simulation at z=2
• The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
• Galaxy Simulation with Dust Formation and Destruction
• Dark-ages reionization and galaxy formation simulation - III. Modelling galaxy formation and the epoch of reionization
• The Dawes Review 8: Measuring the Stellar Initial Mass Function
• The Concentration Dependence of the Galaxy-Halo Connection: Modeling Assembly Bias with Abundance Matching
• Virialization of the inner CGM in the FIRE simulations and implications for galaxy discs, star formation and feedback
• The Formation of Ultra-Diffuse Galaxies in Clusters
• Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons
• The Atacama Cosmology Telescope: Modeling the Gas Thermodynamics in BOSS CMASS galaxies from Kinematic and Thermal Sunyaev-Zel'dovich Measurements
• Feedback from Active Galactic Nuclei in Galaxy Groups
• The mass of our Milky Way
• Galaxy And Mass Assembly (GAMA): ${\mathcal{M}}_{\star }-R_{\mathrm{e}}$ relations of $z=0$ bulges, discs and spheroids
• Baryonic impact on the dark matter distribution in Milky Way-size galaxies and their satellites
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• Introducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution
• Red & Dead CANDELS: massive passive galaxies at the dawn of the Universe
• It's not easy being green: The evolution of galaxy colour in the EAGLE simulation
• The impact of stellar feedback on the structure, size and morphology of galaxies in Milky Way size dark matter haloes
• Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations
• Testing Feedback-Modified Dark Matter Haloes with Galaxy Rotation Curves: Estimation of Halo Parameters and Consistency with $\Lambda$CDM
• Revisiting the Integrated Star Formation Law. II. Starbursts and the Combined Global Schmidt Law
• Stochastic modelling of star-formation histories II: star-formation variability from molecular clouds and gas inflow
• Simulations of extragalactic magnetic fields and of their observables
• Evidence for a change in the dominant satellite galaxy quenching mechanism at z=1
• Far-infrared and dust properties of present-day galaxies in the EAGLE simulations
• The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
• The ASTRID Simulation: Galaxy Formation and Reionization
• Quenching star formation with quasar outflows launched by trapped IR radiation
• Supermassive black holes in the EAGLE Universe. Revealing the observables of their growth
• AutoLens: Automated Modeling of a Strong Lens's Light, Mass and Source
• Shaken and Stirred: The Milky Way's Dark Substructures
• Planes of satellite galaxies and the cosmic web
• ALMA and Herschel reveal that X-ray selected AGN and main-sequence galaxies have different star formation rate distributions
• Galaxy groups in the low-redshift Universe
• Lyman-alpha emitters gone missing: evidence for late reionization?
• Baryon-induced dark matter cores in the EAGLE simulations
• The main sequence of star forming galaxies I. The local relation and its bending
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• Early results from GLASS-JWST. XIV: A spectroscopically confirmed protocluster 650 million years after the Big Bang
• Slicing COSMOS with SC4K: the evolution of typical Lya emitters and the Lya escape fraction from z~2 to z~6
• Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations
• The Southern Stellar Stream Spectroscopic Survey ($S^5$): Overview, Target Selection, Data Reduction, Validation, and Early Science
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).I. Introduction to the Survey
• L-GALAXIES 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs
• KMOS^3D: Dynamical constraints on the mass budget in early star-forming disks
• Galaxies that Shine: radiation-hydrodynamical simulations of disk galaxies
• Simulating an Isolated Dwarf Galaxy with Multi-Channel Feedback and Chemical Yields from Individual Stars
• MusE GAs FLOw and Wind (MEGAFLOW) III: galactic wind properties using background quasars
• SDSS-IV MaNGA: Evidence of the importance of AGN feedback in low-mass galaxies
• The diverse evolutionary paths of simulated high-z massive, compact galaxies to z=0
• The equilibrium view on dust and metals in galaxies: Galactic outflows drive low dust-to-metal ratios in dwarf galaxies
• Atomic and molecular gas in IllustrisTNG galaxies at low redshift
• The Topology of the Cosmic Web in Terms of Persistent Betti Numbers
• The Next Generation Fornax Survey (NGFS): II. The Central Dwarf Galaxy Population
• The Caterpillar Project: A Large Suite of Milky Way Sized Halos
• A consistent measure of the merger histories of massive galaxies using close-pair statistics I: Major mergers at $z<3.5$
• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• The Cosmic Ballet: spin and shape alignments of haloes in the cosmic web
• Deep Extragalactic VIsible Legacy Survey (DEVILS): SED Fitting in the D10-COSMOS Field and the Evolution of the Stellar Mass Function and SFR-$M_{\star }$ relation
• The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes
• ProFit: Bayesian Profile Fitting of Galaxy Images
• The impact of assembly bias on the halo occupation in hydrodynamical simulations
• The origin of scatter in the star formation rate - stellar mass relation
• The Mass-Discrepancy Acceleration Relation: a Natural Outcome of Galaxy Formation in Cold Dark Matter halos
• The Impact of Star Formation and Gamma-Ray Burst Rates at High Redshift on Cosmic Chemical Evolution and Reionization
• The KMOS Deep Survey (KDS) I: dynamical measurements of typical star-forming galaxies at z $\simeq$ 3.5
• The local high velocity tail and the Galactic escape speed
• Solving the small-scale structure puzzles with dissipative dark matter
• Deep learning predictions of galaxy merger stage and the importance of observational realism
• AREPO-RT: Radiation hydrodynamics on a moving mesh
• The SINFONI Nearby Elliptical Lens Locator Survey: Discovery of two new low-redshift strong lenses and implications for the initial mass function in giant early-type galaxies
• Angular momentum properties of haloes and their baryon content in the Illustris simulation
• Mergers, Starbursts, and Quenching in the Simba Simulation
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• Modeling baryonic physics in future weak lensing surveys
• Simulating galactic dust grain evolution on a moving mesh
• The Formation of Ultra-Diffuse Galaxies in the RomulusC Galaxy Cluster Simulation
• Old and young stellar populations in DustPedia galaxies and their role in dust heating
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• Zooming in on accretion - I. The structure of halo gas
• Individual Stellar Halos of Massive Galaxies Measured to 100 kpc at $0.3<z<0.5$ using Hyper Suprime-Cam
• The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disk turbulence in z~0.9 star-forming galaxies
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target Catalogue
• The GHOSTS survey. II. The diversity of Halo Color and Metallicity Profiles of Massive Disk Galaxies
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
• The modelling of feedback in star formation simulations
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Baryonic clues to the puzzling diversity of dwarf galaxy rotation curves
• The link between the assembly of the inner dark matter halo and the angular momentum evolution of galaxies in the EAGLE simulation
• On the Progenitor of Binary Neutron Star Merger GW170817
• Tidal stripping and the structure of dwarf galaxies in the Local Group
• Supernova-driven winds in simulated dwarf galaxies
• Barred galaxies in the EAGLE cosmological hydrodynamical simulation
• Inspiraling Halo Accretion Mapped in Lyman-$\alpha$ Emission around a $z\sim 3$ Quasar
• The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces
• Weighing the stellar constituents of the Galactic halo with APOGEE red giant stars
• Zooming in on major mergers: dense, starbursting gas in cosmological simulations
• Modelling galaxy clustering: halo occupation distribution versus subhalo matching
• Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
• Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
• A Stellar Feedback Origin for Neutral Hydrogen in High-Redshift Quasar-Mass Halos
• The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
• Stochastic modeling of star-formation histories I: the scatter of the star-forming main sequence
• The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
• Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies
• Tidally induced bars in Illustris galaxies
• Massive black hole merger rates: the effect of kpc separation wandering and supernova feedback
• The origin of diverse $\alpha$-element abundances in galaxy discs
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• The Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• Cosmic distribution of highly ionized metals and their physical conditions in the EAGLE simulations
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• The Massive Ancient Galaxies At $z>3$ NEar-infrared (MAGAZ3NE) Survey: Confirmation of Extremely Rapid Star-Formation and Quenching Timescales for Massive Galaxies in the Early Universe
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• Numerical Convergence in Smoothed Particle Hydrodynamics
• The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
• Cosmological simulation with dust formation and destruction
• The link between galaxy and black hole growth in the EAGLE simulation
• The X-ray Halo Scaling Relations of Supermassive Black Holes
• The Formation of Isolated Ultra-Diffuse Galaxies in Romulus25
• SDSS IV MaNGA - The spatially resolved transition from star formation to quiescence
• Spatially resolved star formation and fuelling in galaxy interactions
• Galaxy And Mass Assembly (GAMA): A forensic SED reconstruction of the cosmic star formation history and metallicity evolution by galaxy type
• The environmental dependence of HI in galaxies in the EAGLE simulations
• Black Hole Mass Scaling Relations for Spiral Galaxies. I. $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{sph}}$
• The fundamental plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
• A Lonely Giant: The Sparse Satellite Population of M94 Challenges Galaxy Formation
• Can tides disrupt cold dark matter subhaloes?
• A census of cool core galaxy clusters in IllustrisTNG
• Simulated Milky Way analogues: implications for dark matter direct searches
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies
• NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
• The effect of baryons on the inner density profiles of rich clusters
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• The origin of most massive black holes at high-z: BLUETIDES and the next quasar frontier
• Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• Dancing to ChaNGa: A Self-Consistent Prediction For Close SMBH Pair Formation Timescales Following Galaxy Mergers
• The low-end of the black hole mass function at cosmic dawn
• Quiescence correlates strongly with directly-measured black hole mass in central galaxies
• The Chemo-Dynamical Groups of Galactic Globular Clusters
• Revealing the galaxy-halo connection in IllustrisTNG
• The effect of magnetic fields on properties of the circumgalactic medium
• The MUSE Hubble Ultra Deep Field Survey XI. Constraining the low-mass end of the stellar mass - star formation rate relation at $z<1$
• The relation between galaxy morphology and colour in the EAGLE simulation
• Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
• The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies
• Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations
• Efficient early stellar feedback can suppress galactic outflows by reducing supernova clustering
• MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
• Synthetic nebular emission from massive galaxies I: origin of the cosmic evolution of optical emission-line ratios
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• Gas Accretion via Condensation and Fountains
• Simulations of the star-forming molecular gas in an interacting M51-like galaxy
• Flickering AGN can explain the strong circumgalactic O VI observed by COS-Halos
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Colours, Star formation Rates, and Environments of Star forming and Quiescent Galaxies at the Cosmic Noon
• The masses and metallicities of stellar haloes reflect galactic merger histories
• The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
• The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
• Trident: a universal tool for generating synthetic absorption spectra from astrophysical simulations
• The Origin and Evolution of Fast and Slow Rotators in the Illustris Simulation
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• Supermassive black holes as the regulators of star formation in central galaxies
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Galaxies hosting an AGN: a view from the CALIFA survey
• The SAMI Galaxy Survey: mass as the driver of the kinematic morphology - density relation in clusters
• The Science of the Einstein Telescope
• Taking the Universe's Temperature with Spectral Distortions of the Cosmic Microwave Background
• Black Hole - Galaxy Scaling Relationships for Active Galactic Nuclei with Reverberation Masses
• From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation
• A statistical investigation of the mass discrepancy-acceleration relation
• MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey
• The connection between mass, environment and slow rotation in simulated galaxies
• The asymptotic tidal remnants of cold dark matter subhalos
• Gas-phase metallicity gradients of TNG50 star-forming galaxies
• Dark matters on the scale of galaxies
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• Powering galactic super-winds with small-scale AGN winds
• How to constrain warm dark matter with the Lyman $\alpha$ forest
• Massive Close Pairs Measure Rapid Galaxy Assembly in Mergers at High Redshift
• The multiphase circumgalactic medium traced by low metal ions in EAGLE zoom simulations
• Has JWST already falsified dark-matter-driven galaxy formation?
• Advanced LIGO Constraints on Neutron Star Mergers and R-Process Sites
• The diverse density profiles of galaxy clusters with self-interacting dark matter plus baryons
• Galaxy gas as obscurer: II. Separating the galaxy-scale and nuclear obscurers of Active Galactic Nuclei
• Snap, Crackle, Pop: sub-grid supernova feedback in AMR simulations of disk galaxies
• 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
• The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent galaxies at z < 0.7
• The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• The low-mass end of the baryonic Tully-Fisher relation
• The core-cusp problem: a matter of perspective
• The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM
• The Hubble Sequence at $z\sim 0$ in the IllustrisTNG simulation with deep learning
• A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 Quasar
• First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
• Galaxy Zoo: Morphological Classifications for 120,000 Galaxies in HST Legacy Imaging
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• The brighter galaxies reionised the Universe
• Fast galaxy bars continue to challenge standard cosmology
• The three phases of galaxy formation
• NIHAO XIV: Reproducing the observed diversity of dwarf galaxy rotation curve shapes in LCDM
• Galaxy Merger Rates up to z $\sim$ 3 using a Bayesian Deep Learning Model $-$ A Major-Merger classifier using IllustrisTNG Simulation data
• The oldest and most metal poor stars in the APOSTLE Local Group simulations
• Λ CDM is Consistent with SPARC Radial Acceleration Relation
• No massive black holes in the Milky Way halo
• The Fornax Deep Survey (FDS) with VST. VI. Optical properties of the dwarf galaxies in the Fornax cluster
• Black Hole -- Galaxy Correlations in Simba
• The Black Hole -- Bulge Mass Relation including Dwarf Galaxies Hosting Active Galactic Nuclei
• The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE
• Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7
• Large-scale mass distribution in the Illustris simulation
• Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
• Constraints on the identity of the dark matter from strong gravitational lenses
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• Missing dark matter in dwarf galaxies?
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• AGN-Driven Outflows in Dwarf Galaxies
• Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering
• The rapid growth phase of supermassive black holes
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter
• Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
• What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses
• Large-scale outflows in luminous QSOs revisited: The impact of beam smearing on AGN feedback efficiencies
• The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales
• Log-normal star formation histories in simulated and observed galaxies
• Semi-analytic forecasts for JWST -- IV. Implications for cosmic reionization and LyC escape fraction
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• Intrinsic alignments of galaxies in the EAGLE and cosmo-OWLS simulations
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• Storm in a "Teacup": a radio-quiet quasar with ~10kpc radio-emitting bubbles and extreme gas kinematics
• Ultra-diffuse galaxies in the Auriga simulations
• The Multi-Wavelength Tully-Fisher relation with spatially resolved HI kinematics
• Merger-Induced Metallicity Dilution in Cosmological Galaxy Formation Simulations
• Convolutional neural network identification of galaxy post-mergers in UNIONS using IllustrisTNG
• The environmental dependence of gas accretion onto galaxies: quenching satellites through starvation
• Simulated Milky Way analogues: implications for dark matter indirect searches
• The MOSDEF survey: a census of AGN-driven ionized outflows at $z=1.4-3.8$
• Project AMIGA: The Circumgalactic Medium of Andromeda
• AGNIFS survey of local AGN: GMOS-IFU data and outflows in 30 sources
• The Aurora radiation-hydrodynamical simulations of reionization: calibration and first results
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• And yet it flips: connecting galactic spin and the cosmic web
• The properties of the first galaxies in the BLUETIDES simulation
• Populations of filaments from the distribution of galaxies in numerical simulations
• The Metal Abundances across Cosmic Time ($\mathcal{M}\mathcal{A}\mathcal{C}\mathcal{T}$) Survey. II. Evolution of the Mass-Metallicity Relation over 8 Billion Years, using [OIII]$\lambda$4363Å-based Metallicities
• On the persistence of two small-scale problems in ΛCDM
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• ALMA 200-parsec Resolution Imaging of Smooth Cold Dusty Disks in Typical $z\sim 3$ Star-Forming Galaxies
• The unorthodox evolution of major merger remnants into star-forming spiral galaxies
• Properties of gas phases around cosmic filaments at z=0 in the Illustris-TNG simulation
• An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations
• The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• The inner structure of early-type galaxies in the Illustris simulation
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• Origins and Demographics of Wandering Black Holes
• Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
• Column Density Profiles of Multi-Phase Gaseous Halos
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• Formation channels of single and binary stellar-mass black holes
• Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
• Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
• The Tully-Fisher and mass-size relations from halo abundance matching
• Magnetising the circumgalactic medium of disk galaxies
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• The link between accretion mode and environment in radio-loud active galaxies
• The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products
• MultiDark-Galaxies: data release and first results
• The properties of "dark" ΛCDM halos in the Local Group
• Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE project
• Galaxy mergers in EAGLE do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN
• Revisiting the tension between fast bars and the $\Lambda$CDM paradigm
• Quasar Feedback Survey: Multi-phase outflows, turbulence and evidence for feedback caused by low power radio jets inclined into the galaxy disk
• Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
• Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• Deviations from hydrostatic equilibrium in the circumgalactic medium: spinning hot haloes and accelerating flows
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Properties of HI discs in the Auriga cosmological simulations
• Dynamical Friction Modeling of Massive Black Holes in Cosmological Simulations and Effects on Merger Rate Predictions
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation
• The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
• A comparison of observed and simulated absorption from HI, CIV, and SiIV around $z\approx 2$ star-forming galaxies suggests redshift-space distortions are due to inflows
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• Star cluster formation in cosmological simulations. III. Dynamical and chemical evolution
• Feedback from massive stars at low metallicities: MUSE observations of N44 and N180 in the Large Magellanic Cloud
• High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers
• Quenching timescales of galaxies in the EAGLE simulations
• A tale of two populations: surviving and destroyed dwarf galaxies and the build up of the Milky Way's stellar halo
• ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
• 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
• Molecular Gas Contents and Scaling Relations for Massive Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
• Formation histories of stars, clusters and globular clusters in the E-MOSAICS simulations
• Reionization in Technicolor
• Galaxy evolution across environments as probed by the ages, stellar metallicities and [alpha/Fe] of central and satellite galaxies
• Fade to grey: systematic variation of the galaxy attenuation curves with galaxy properties in EAGLE
• The separate and combined effects of baryon physics and neutrino free-streaming on large-scale structure
• Spurious heating of stellar motions in simulated galactic disks by dark matter halo particles
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Dark-ages Reionization and Galaxy Formation Simulation - X. The small contribution of quasars to reionization
• From 'bathtub' galaxy evolution models to metallicity gradients
• The Cosmic Ultraviolet Baryon Survey (CUBS) I. Overview and the diverse environments of Lyman limit systems at z<1
• The fate of disk galaxies in IllustrisTNG clusters
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• Primordial power spectrum in light of JWST observations of high redshift galaxies
• Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
• The buildup of strongly barred galaxies in the TNG100 simulation
• Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
• The THESAN project: predictions for multi-tracer line intensity mapping in the epoch of reionization
• Shaken, not blown: the gentle baryonic feedback of nearby starburst dwarf galaxies
• The Lyman-$\alpha$ forest as a diagnostic of the nature of the dark matter
• DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons
• Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
• Horizon-AGN virtual observatory - 1. SED-fitting performance and forecasts for future imaging surveys
• Supernova-blast waves in wind-blown bubbles, turbulent, and power-law ambient media
• First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier
• Galaxy-halo alignments in the Horizon-AGN cosmological hydrodynamical simulation
• Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions
• The intra-cluster light as a tracer of the total matter density distribution: a view from simulations
• Black-hole-regulated star formation in massive galaxies
• An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• The multiplicity and anisotropy of galactic satellite accretion
• Painting galaxies into dark matter halos using machine learning
• An EAGLE's View of Ex-situ Galaxy Growth
• An EAGLE view of the missing baryons
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• Supermassive black holes and their host spheroids I. Disassembling galaxies
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• Dark-matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions
• LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars
• Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST
• Black hole feeding and feedback: the physics inside the "subgrid"
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• Subhalo destruction in the Apostle and Auriga simulations
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• Multi-wavelength properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
• SHARP - IV. An apparent flux ratio anomaly resolved by the edge-on disc in B0712+472
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• NIHAO VI. The hidden discs of simulated galaxies
• Music from the heavens - Gravitational waves from supermassive black hole mergers in the EAGLE simulations
• Lessons from the Auriga discs: The hunt for the Milky Way's ex-situ disc is not yet over
• The VLT SINFONI Mg ii Program for Line Emitters (SIMPLE) II: background quasars probing z $\sim$ 1 galactic winds
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• The influence of environment on satellite galaxies in the GAEA semi-analytic model
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
• Multi-phase feedback processes in the Sy2 galaxy NGC 5643
• Dancing in the Dark: Uncertainty in ultra-faint dwarf galaxy predictions from cosmological simulations
• On the evolution of galaxy spin in a cosmological hydrodynamic simulation of galaxy clusters
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Evolution of galaxy size--stellar mass relation from the Kilo Degree Survey
• The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view
• The oxygen abundance gradients in the gas discs of galaxies in the EAGLE simulation
• The formation of hot gaseous haloes around galaxies
• The Galaxy Clustering Crisis in Abundance Matching
• The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
• Higher-order initial conditions for mixed baryon-CDM simulations
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters
• Galaxy and Mass Assembly (GAMA): halo formation times and halo assembly bias on the cosmic web
• The origin of dust in galaxies across cosmic time
• Physical properties and evolution of (Sub-)millimeter selected galaxies in the galaxy formation simulation Shark
• Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations
• Quasar outflows at $z\ge 6$: the impact on the host galaxies
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• Automated Distant Galaxy Merger Classifications from Space Telescope Images using the Illustris Simulation
• Future constraints on halo thermodynamics from combined Sunyaev-Zel'dovich measurements
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• The Initial Mass Function in the Nearest Strong Lenses from SNELLS: Assessing the Consistency of Lensing, Dynamical, and Spectroscopic Constraints
• Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses
• The origin of low-surface-brightness galaxies in the dwarf regime
• A flexible modelling of galaxy assembly bias
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• Systematic search for tidal features around nearby galaxies: I. Enhanced SDSS imaging of the Local Volume
• Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
• Cosmological constraints from galaxy-lensing cross correlations using BOSS galaxies with SDSS and CMB lensing
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• Statistical properties of paired fixed fields
• Spatially resolved cold molecular outflows in ULIRGs
• The Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma
• Blandford-Znajek jets in galaxy formation simulations: method and implementation
• Studying galaxy troughs and ridges using Weak Gravitational Lensing with the Kilo-Degree Survey
• SDSS-IV MaNGA: The Spatial Distribution of Star Formation and its Dependence on Mass, Structure and Environment
• The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies
• ZFIRE: Galaxy Cluster Kinematics, H$\alpha$ Star Formation Rates, and Gas-Phase Metallicities of XMM-LSS J02182-05102 at z=1.6233
• Unveiling Galaxy Bias via the Halo Model, KiDS and GAMA
• Extraterrestrial Axion Search with the Breakthrough Listen Galactic Center Survey
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies
• How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE
• RAiSE II: resolved spectral evolution in radio AGN
• Genetically modified halos: towards controlled experiments in $\Lambda$CDM galaxy formation
• The Edge of the Galaxy
• Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• Probing 3D Structure with a Large MUSE Mosaic: Extending the Mass Model of Frontier Field Abell 370
• Intrinsic alignments of disk and elliptical galaxies in the MassiveBlack-II and Illustris simulations
• Tidal dwarf galaxies in cosmological simulations
• Systematic difference between ionized and molecular gas velocity dispersion in $z\sim 1-2$ disks and local analogues
• Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z~1
• Flux-ratio anomalies from discs and other baryonic structures in the Illustris simulation
• The prevalence of pseudo-bulges in the Auriga simulations
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• Evolution of the Mass-Metallicity Relation from Redshift $z\approx 8$ to the Local Universe
• nIFTy galaxy cluster simulations II: radiative models
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• The importance of black hole repositioning for galaxy formation simulations
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching
• BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes
• The distribution of mass components in simulated disc galaxies
• Hydrogen Reionization in the Illustris universe
• A Characteristic Mass Scale in the Mass-Metallicity Relation of Galaxies
• Alignments between galaxies, satellite systems and haloes
• Galaxy merger histories and the role of merging in driving star formation at z>1
• The SLUGGS Survey: Dark matter fractions at large radii and assembly epochs of early-type galaxies from globular cluster kinematics
• The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5
• The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations
• The role of atomic hydrogen in regulating the scatter of the mass-metallicity relation
• A Gaia-Enceladus Analog in the EAGLE Simulation: Insights into the Early Evolution of the Milky Way
• The stellar halos of ETGs in the IllustrisTNG simulations: the photometric and kinematic diversity of galaxies at large radii
• Merger-induced galaxy transformations in the ARTEMIS simulations
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• Star Formation in Luminous Quasars at 2<z<3
• The impact of quenching on galaxy profiles in the Simba simulation
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• The Frequency of Dwarf Galaxy Multiples at Low Redshift in SDSS vs. Cosmological Expectations
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
• Simulations of Jet Heating in Galaxy Clusters: Successes and Challenges
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• Introducing a new, robust galaxy finder algorithm for simulations
• The Redshift Evolution of the $M_{\bullet }-M_{\star }$ Relation for JWST's Supermassive Black Holes at $z>4$
• Anatomy of Eddington-like inversion methods in the context of dark matter searches
• Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
• Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies
• Expectations of the size evolution of massive galaxies at $3\le z\le 6$ from the TNG50 simulation: the CEERS/JWST view
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Constraining the Milky Way Mass Profile with Phase-Space Distribution of Satellite Galaxies
• Barred Galaxies in the IllustrisTNG Simulation
• Constraints on the Lyman continuum escape fraction for faint star forming galaxies
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Normal black holes in bulge-less galaxies: the largely quiescent, merger-free growth of black holes over cosmic time
• The origin of the $\alpha$-enhancement of massive galaxies
• The mass, colour, and structural evolution of today's massive galaxies since z~5
• Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• The origin and properties of massive prolate galaxies in the Illustris simulation
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Extensions to models of the galaxy-halo connection
• Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations
• Witnessing galaxy assembly in an extended z~3 structure
• Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
• The COS CGM Compendium. III: Metallicity and Physical Properties of the Cool Circumgalactic Medium at z<1
• The Three Hundred Project: Ram pressure and gas content of haloes and subhaloes in the phase-space plane
• From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• A Foreground Masking Strategy for [CII] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift
• A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
• Fitting the nonlinear matter bispectrum by the Halofit approach
• On the model of the circumgalactic mist: the implications of cloud sizes in galactic winds and halos
• The Metallicity and Elemental Abundance Gradients of Simulated Galaxies, and their Environmental Dependence
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• Supernova feedback and the energy deposition in molecular clouds
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last $\approx$10 Gyr
• Observational signatures of a warped disk associated with cold-flow accretion
• Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
• The abundances and properties of Dual AGN and their host galaxies in the EAGLE simulations
• Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
• Dark matter halo shapes in the Auriga simulations
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
• A Versatile Family of Galactic Wind Models
• The Impact of Star Formation Histories on Stellar Mass Estimation: Implications from the Local Group Dwarf Galaxies
• On the Appearance of Thresholds in the Dynamical Model of Star Formation
• Tracing the Quenching History in Galaxy Clusters in the EAGLE Simulation
• Realistic simulations of galaxy formation in f(R) modified gravity
• Constraints on Quenching of $z\lesssim 2$ Massive Galaxies from the Evolution of the average Sizes of Star-Forming and Quenched Populations in COSMOS
• Kinematic scaling relations of CALIFA galaxies: A dynamical mass proxy for galaxies across the Hubble sequence
• Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probe
• Galactic inflow and wind recycling rates in the EAGLE simulations
• The KMOS Redshift One Spectroscopic Survey (KROSS): The Tully-Fisher Relation at z ~ 1
• Bulge plus disc and Sérsic decomposition catalogues for 16,908 galaxies in the SDSS Stripe 82 co-adds: A detailed study of the $ugriz$ structural measurements
• Detailed HI kinematics of Tully-Fisher calibrator galaxies
• The ALMA-ALPAKA survey I: high-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Halo ellipticity of GAMA galaxy groups from KiDS weak lensing
• How Gas Accretion Feeds Galactic Disks
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• On the Origin of Diffuse Ionized Gas in the Antennae Galaxy
• The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
• Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• On the origin of gas-poor galaxies in galaxy clusters using cosmological hydrodynamic simulations
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• SDSS IV MaNGA: Visual Morphological and Statistical Characterization of the DR15 sample
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• To beta or not to beta: can higher-order Jeans analysis break the mass-anisotropy degeneracy in simulated dwarfs?
• Stellar Feedback and Resolved Stellar IFU Spectroscopy in the nearby Spiral Galaxy NGC 300
• Constraining baryonic feedback and cosmology with weak-lensing, X-ray, and kinematic Sunyaev-Zeldovich observations
• Rapid early coeval star formation and assembly of the most massive galaxies in the universe
• EAGLE and Illustris-TNG predictions for resolved eROSITA X-ray observations of the circumgalactic medium around normal galaxies
• Metallicity gradients in small and nearby spiral galaxies
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• The effects of host galaxy properties on merging compact binaries detectable by LIGO
• Following the Cosmic Evolution of Pristine Gas II: The search for Pop III-Bright Galaxies
• Characterization of Low Surface Brightness structures in annotated deep images
• The splashback boundary of haloes in hydrodynamic simulations
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Cosmology with the Wide-Field Infrared Survey Telescope -- Synergies with the Rubin Observatory Legacy Survey of Space and Time
• Gas-phase metallicity gradients in galaxies at $z\sim 6-8$
• MUSE Analysis of Gas around Galaxies (MAGG) -- IV: The gaseous environment of $z\sim$ 3-4 Lyman-alpha emitting galaxies
• Intermediate-Mass Black Hole Growth and Feedback in Dwarf Galaxies at High Redshifts
• The SLUGGS Survey: Measuring globular cluster ages using both photometry and spectroscopy
• The SLUGGS Survey: A comparison of total-mass profiles of early-type galaxies from observations and cosmological simulations, to $\sim$4 effective radii
• Sub one percent mass fractions of young stars in red massive galaxies
• A quartet of black holes and a missing duo: probing the low-end of the Mbh - sigma relation with the adaptive optics assisted integral-field spectroscopy
• Introducing CGOLS: The Cholla Galactic OutfLow Simulation Suite
• Red Supergiants as Cosmic Abundance Probes: massive star clusters in M83, and the mass-metallicity relation of nearby galaxies
• The diverse nature and formation paths of slow rotator galaxies in the EAGLE simulations
• The COS CGM Compendium. II: Metallicities of the Partial and Lyman Limit Systems at z<1
• A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies
• Baryonic effects on the matter bispectrum
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• SWIFT: Using task-based parallelism, fully asynchronous communication, and graph partition-based domain decomposition for strong scaling on more than 100,000 cores
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• Simple Yet Powerful: Hot Galactic Outflows Driven by Supernovae
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• The gas metallicity gradient and the star formation activity of disc galaxies
• FOREVER22: galaxy formation in protocluster regions
• MUFASA: The assembly of the red sequence
• Galaxy And Mass Assembly (GAMA): The sSFR-M* relation part I - ${\sigma }_{\mathrm{sSFR}}$-M* as a function of sample, SFR indicator and environment
• The Low Redshift Circumgalactic Medium in Simba
• Morphological decomposition of TNG50 galaxies: methodology and catalogue
• On CMB B-Mode Non-Gaussianity
• Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• Composite Spectral Energy Distributions and Infrared-Optical Colors of Type 1 and Type 2 Quasars
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• How Do Supernovae Impact the Circumgalactic Medium? I. Large-Scale Fountains Around a Milky Way-Like Galaxy
• No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
• Inhomogeneous Reionization Models in Cosmological Hydrodynamical Simulations
• The Effect of AGN on the Global HI Content of Isolated Low-Mass Galaxies
• The rise and fall of stellar discs across the peak of cosmic star formation history: mergers versus smooth accretion
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• The contribution of N-rich stars to the Galactic stellar halo using APOGEE red giants
• YZiCS: Preprocessing of dark halos in the hydrodynamic zoom-in simulation of clusters
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• Sustained super-Eddington accretion in high-redshift quasars
• Cold gas removal from the centre of a galaxy by a low-luminosity jet
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies
• Relative distribution of dark matter, gas, and stars around cosmic filaments in the IllustrisTNG simulation
• A detection of wobbling Brightest Cluster Galaxies within massive galaxy clusters
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Dust evolution in zoom-in cosmological simulations of galaxy formation
• The Imprint of Cosmic Web Quenching on Central Galaxies
• Duty cycle of the radio galaxy B2 0258+35
• First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at $z\ge 5$
• On the origin of star-gas counterrotation in low-mass galaxies
• The AGNIFS survey: spatially resolved observations of hot molecular and ionised outflows in nearby active galaxies
• The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulations
• Climbing to the top of the galactic mass ladder: evidence for frequent prolate-like rotation among the most massive galaxies
• Fossil stellar streams and their globular cluster populations in the E-MOSAICS simulations
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
• Characterizing the local relation between star formation rate and gas-phase metallicity in MaNGA spiral galaxies
• Evolution of galactic planes of satellites in the EAGLE simulation
• The origin of the enhanced metallicity of satellite galaxies
• Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to $10^8$M${}_{\odot }$
• A Link Between Ram Pressure Stripping and Active Galactic Nuclei
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• The turbulent destruction of clouds - III. Three dimensional adiabatic shock-cloud simulations
• Solitons in the dark: non-linear structure formation with fuzzy dark matter
• Following The Cosmic Evolution Of Pristine Gas I: Implications For Milky Way Halo Stars
• Recovering ${\lambda }_R$ and $V/\sigma$ from seeing-dominated IFS data
• On the origin of the mass-metallicity gradient relation in the local Universe
• DeepMerge II: Building Robust Deep Learning Algorithms for Merging Galaxy Identification Across Domains
• Cosmological baryon transfer in the SIMBA simulations
• The origin of the 'blue tilt' of globular cluster populations in the E-MOSAICS simulations
• Evolution of Galactic Outflows at $z\sim 0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra
• On the galaxy-halo connection in the EAGLE simulation
• Realistic galaxy image simulation via score-based generative models
• Evolution of the cold gas properties of simulated post-starburst galaxies
• WISDOM project - IV. A molecular gas dynamical measurement of the supermassive black hole mass in NGC 524
• The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
• AGN All the Way Down? AGN-like Line Ratios are Common In the Lowest-Mass Isolated Quiescent Galaxies
• Gas Content Regulates the Lifecycle of Star Formation and Black Hole Accretion in Galaxies
• First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5<z<2$ from KMOS
• Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
• A Multi-wavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population
• Implications of hydrodynamical simulations for the interpretation of direct dark matter searches
• Weak Lensing Minima and Peaks: Cosmological Constraints and the Impact of Baryons
• Hyper-Eddington accretion flows onto black holes accompanied by powerful outflows
• The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to $\sim$10${}^6$ L${}_{\odot }$ and Comparisons with Galaxy Formation Models
• Winds of change: reionization by starburst galaxies
• GAMA/DEVILS: Constraining the cosmic star-formation history from improved measurements of the 0.3-2.2 micron Extragalactic Background Light
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Dynamical cluster disruption and its implications for multiple population models in the E-MOSAICS simulations
• The KMOS${}^{3D}$ Survey: rotating compact star forming galaxies and the decomposition of integrated line widths
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• The SAMI Galaxy Survey: a statistical approach to an optimal classification of stellar kinematics in galaxy surveys
• The emergence of passive galaxies in the early Universe
• Caustic Skeleton & Cosmic Web
• Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation
• FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
• Constraining the Baryonic Feedback with Cosmic Shear Using the DES Year-3 Small-Scale Measurements
• Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• Beyond halo mass: quenching galaxy mass assembly at the edge of filaments
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• Are star formation rates of galaxies bimodal?
• Robust Field-level Likelihood-free Inference with Galaxies
• Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
• The Growth and Enrichment of the Intragroup Gas
• Revealing the Dark Threads of the Cosmic Web
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• The evolution of the stellar mass versus halo mass relationship
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The decline of cosmic star formation: quenching, mass, and environment connections
• Early growth of typical high redshift black holes seeded by direct collapse
• The Faber-Jackson relation and Fundamental Plane from halo abundance matching
• The hot circumgalactic medium of the Milky Way: evidence for super-virial, virial, and sub-virial temperature, non-solar chemical composition, and non-thermal line broadening
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Modelling the cosmic spectral energy distribution and extragalactic background light over all time
• The nature of H-alpha star-forming galaxies at z~0.4 in and around Cl 0939+4713: the environment matters
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Stellar mass functions of galaxies, disks and spheroids at z~0.1
• Efficacy of early stellar feedback in low gas surface density environments
• Black Hole Growth and Feedback in Isolated Romulus25 Dwarf Galaxies
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• The evolution of the oxygen abundance gradients in star-forming galaxies in the EAGLE simulations
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• Energy wrinkles and phase-space folds of the last major merger
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• Barred galaxies in the Illustris-1 and TNG100 simulations
• Black Hole Starvation and Bulge Evolution in a Milky Way-like Galaxy
• The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars
• From Stellar Halos to Intracluster Light: the physics of the Intra-Halo Stellar Component in cosmological hydrodynamical simulations
• Nature and statistical properties of quasar associated absorption systems in the XQ-100 Legacy Survey
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Ly$\alpha$ nebulae associated with a bright $z\approx 3.23$ quasar pair
• Identifying kinematic structures in simulated galaxies using unsupervised machine learning
• A Break in Spiral Galaxy Scaling Relations at the Upper Limit of Galaxy Mass
• Equilibrium model prediction for the scatter in the star-forming main sequence
• The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
• Characterizing hydrostatic mass bias with Mock-X
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• Young and turbulent: the early life of massive galaxy progenitors
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• RAMSES-RTZ: Non-Equilibrium Metal Chemistry and Cooling Coupled to On-The-Fly Radiation Hydrodynamics
• Dark matter annihilation radiation in hydrodynamic simulations of Milky Way haloes
• Physical origin of the large-scale conformity in the specific star formation rates of galaxies
• Determining star-formation rates in Active Galactic Nuclei hosts via stellar population synthesis
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• 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
• Great Balls of FIRE I: The formation of star clusters across cosmic time in a Milky Way-mass galaxy
• The limited role of galaxy mergers in driving stellar mass growth over cosmic time
• The diverse evolutionary pathways of post-starburst galaxies
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters
• KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since $z\approx 1$
• The Cluster-EAGLE project: velocity bias and the velocity dispersion - mass relation of cluster galaxies
• The SAMI Galaxy Survey: Satellite galaxies undergo little structural change during their quenching phase
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• $\text{Mangrove}$: Learning Galaxy Properties from Merger Trees
• The Morphology-Density relationship in 1<z<2 clusters
• HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
• The Mass and Absorption Columns of Galactic Gaseous Halos
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• The origin of the red sequence galaxy population in the EAGLE simulation
• HST/COS Observations of Quasar Outflows in the 500-1050 Å Rest Frame: I. The Most Energetic Outflows in the Universe and Other Discoveries
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• The impact of AGN feedback on the 1D power spectra from the Ly$\alpha$ forest using the Horizon-AGN suite of simulations
• The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS
• Effective photon mass and (dark) photon conversion in the inhomogeneous Universe
• Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
• Evolution of the galaxy stellar mass function: evidence for an increasing $M^{\ast }$ from $z=2$ to the present day
• 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
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• The abundance and physical properties of O VII and O VIII X-ray absorption systems in the EAGLE simulations
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• The velocity anisotropy of the Milky Way satellite system
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• Baryon effects on void statistics in the EAGLE simulation
• The origin of compact galaxies with anomalously high black hole masses
• The Dearth of Difference between Central and Satellite Galaxies I. Perspectives on star formation quenching and AGN activities
• Young star cluster populations in the E-MOSAICS simulations
• The first Super Massive Black Holes: indications from models for future observations
• The Radio Galaxy Population in the SIMBA SImulations
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• Satellites Around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations Versus Simulations
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Is there enough star formation in simulated protoclusters?
• Connecting and dissecting galaxies' angular momenta and neutral gas in a hierarchical universe: cue DARK SAGE
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• Jet Feedback and the Photon Underproduction Crisis in Simba
• Kinematics and Dynamics of Multiphase Outflows in Simulations of the Star-Forming Galactic ISM
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• H$\alpha$ Morphologies of Star Clusters in 16 LEGUS Galaxies: Constraints on HII region evolution timescales
• Evolution of LMC/M33-mass dwarf galaxies in the EAGLE simulation
• ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
• The rocky road to quiescence: compaction and quenching of quasar host galaxies at z~2
• Galactic angular momentum in cosmological zoom-in simulations. I. Disk and bulge components and the galaxy--halo connection
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• 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
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• Discovery of massive star formation quenching by nonthermal effects in the center of NGC 1097
• 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
• Connecting the dots: a correlation between ionising radiation and cloud mass-loss rate traced by optical integral field spectroscopy
• nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes
• The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
• A Deep Search For Faint Galaxies Associated With Very Low-redshift C IV Absorbers: II. Program Design, Absorption-line Measurements, and Absorber Statistics
• The aftermath of the Great Collision between our Galaxy and the Large Magellanic Cloud
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• An alternate approach to measure specific star formation rates at 2<z<7
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• The star formation histories of dwarf galaxies in Local Group cosmological simulations
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part I. Methodology and code description
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.5 in HSC-SSP PDR1
• Climbing Halo Merger Trees with TreeFrog
• MUSEQuBES: Characterizing the circumgalactic medium of redshift $\approx 3.3$ Ly$\alpha$ emitters
• The offsets between galaxies and their dark matter in Lambda-CDM
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• Microwave Spectro-Polarimetry of Matter and Radiation across Space and Time
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Empirically Constrained Predictions for Metal-Line Emission from the Circumgalactic Medium
• Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'
• The Three-Phase Evolution of the Milky Way
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• The impact of spurious collisional heating on the morphological evolution of simulated galactic discs
• Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample
• Stellar splashback: the edge of the intracluster light
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• The MBHBM* Project -- I: Measurement of the Central Black Hole Mass in Dwarf Galaxy NGC 3504 Using Molecular Gas Kinematics
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• The stellar metallicity gradients in galaxy discs in a cosmological scenario
• Local SDSS galaxies in the Herschel Stripe82 survey: A critical assessment of optically-derived star-formation rates
• The history of the dark and luminous side of Milky Way-like progenitors
• The Radial Acceleration Relation in Disk Galaxies in the MassiveBlack-II Simulation
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• Green Valley galaxies as a transition population in different environments
• Large and small-scale structures and the dust energy balance problem in spiral galaxies
• Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars
• Cooling in a Dissipative Dark Sector
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• The mass assembly of high-redshift black holes
• Dust Obscured Star Forming Galaxies in the Early Universe
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• Priors on Lagrangian bias parameters from galaxy formation modelling
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• Total density profile of massive early-type galaxies in Horizon-AGN simulation: impact of AGN feedback and comparison with observations
• Probing Dark Matter Self-interaction with Ultra-faint Dwarf Galaxies
• The chemical composition of globular clusters in the Local Group
• Statistical modelling of the cosmological dispersion measure
• The e-MERLIN Galaxy Evolution Survey (e-MERGE): Overview and Survey Description
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• Towards a general parametrization of the warm dark matter halo mass function
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time
• A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• The role of gas infall in the evolution of disc galaxies
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• Intrinsic alignment of redMaPPer clusters: cluster shape - matter density correlation
• Gas-phase Metallicity as a Diagnostic of the Drivers of Star-formation on Different Spatial Scales
• Taking snapshots of the jet-ISM interplay: The case of PKS0023-26
• The Impact of Dust on the Sizes of Galaxies in the Epoch of Reionization
• Fountains and storms: The role of AGN and mergers in disrupting the cool-core in the RomulusC simulation
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Galaxy formation in the brane world I: overview and first results
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• Statistics of galaxy mergers: bridging the gap between theory and observation
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• The First Large Absorption Survey in HI (FLASH): I. Science Goals and Survey Design
• The metallicity of galactic winds
• The MUSE eXtremely Deep Field: Individual detections of Lyα haloes around rest-frame UV-selected galaxies at z~2.9-4.4
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Observations of metals in the $z\approx 3.5$ intergalactic medium and comparison to the EAGLE simulations
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• An evolving and mass dependent ${\sigma }_{\text{sSFR}}$-${\mathrm{M}}_{\star }$ relation for galaxies
• Dark matter dynamics in Abell 3827: new data consistent with standard Cold Dark Matter
• On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
• Connecting the structure of dark matter haloes to the primordial power spectrum
• GA-NIFS: High number of dual active galactic nuclei at z~3
• The Gas-Star Formation Cycle in Nearby Star-forming Galaxies II. Resolved Distributions of CO and H$\alpha$ Emission for 49 PHANGS Galaxies
• A new direction for dark matter research: intermediate mass compact halo objects
• 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
• Statistical strong lensing. I. Constraints on the inner structure of galaxies from samples of a thousand lenses
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
• Stellar Dynamics and Star-Formation Histories of z $\sim$ 1 Radio-loud Galaxies
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Bayesian Inference of Spreading Processes on Networks
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• Gauging the effect of Supermassive Black Holes feedback on Quasar host galaxies
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Predicting star formation properties of galaxies using deep learning
• 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
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• LoTSS Jellyfish Galaxies IV: Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• The Pristine Dwarf-Galaxy survey -- III. Revealing the nature of the Milky Way globular cluster Sagittarius II
• A spectral stacking analysis to search for faint outflow signatures in z~6 quasars
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Radiative properties of the first galaxies: rapid transition between blue and red
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• Correlations in the three-dimensional Lyman-alpha forest contaminated by high column density absorbers
• The effect of non-equilibrium metal cooling on the interstellar medium
• Properties and Origin of Galaxy Velocity Bias in the Illustris Simulation
• On the effect of galactic outflows in cosmological simulations of disc galaxies
• Metals in the circumgalactic medium are out of ionization equilibrium due to fluctuating active galactic nuclei
• Theoretical Accuracy in Cosmological Growth Estimation
• A Black Hole Mass Determination for the Compact Galaxy Mrk 1216
• The resolution bias: low resolution feedback simulations are better at destroying galaxies
• Seeing sharper and deeper: JWST's first glimpse of the photometric and spectroscopic properties of galaxies in the epoch of reionisation
• Monsters in the Dark: Predictions for Luminous Galaxies in the Early Universe from the BlueTides Simulation
• Probing sub-galactic mass structure with the power spectrum of surface-brightness anomalies in high-resolution observations of galaxy-galaxy strong gravitational lenses. II.Observational constraints on the sub-galactic matter power spectrum
• The HI Velocity Function: a test of cosmology or baryon physics?
• Spectral Classification and Ionized Gas Outflows in $z\sim 2$ WISE-Selected Hot Dust-Obscured Galaxies
• North Ecliptic Pole merging galaxy catalogue
• Formation of Globular Cluster Systems II: Impact of the Cutoff of the Cluster Initial Mass Function
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Exploring compact binary merger host galaxies and environments with $\mathrm{zELDA}$
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04
• Prospects for dark matter detection with inelastic transitions of xenon
• Determination of the escape velocity of the Milky Way using a proper motion selected halo sample
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN
• On the Determination of Rotation Velocity and Dynamical Mass of Galaxies Based on Integrated H I Spectra
• Massive Black Hole Mergers with Orbital Information: Predictions from the ASTRID Simulation
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• 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
• Formation and Morphology of the First Galaxies in the Cosmic Morning
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• Group quenching and galactic conformity at low redshift
• Revealing the physical properties of gas accreting to haloes in the EAGLE simulations
• Constraining self-interacting dark matter with scaling laws of observed halo surface densities
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
• Deciphering the imprint of AGN feedback in Seyfert galaxies: Nuclear-scale molecular gas deficits
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• Constraining AGN Feedback in Massive Ellipticals with South Pole Telescope Measurements of the Thermal Sunyaev-Zel'dovich Effect
• Simulating the effect of photoheating feedback during reionization
• Quenching Timescales in the IllustrisTNG Simulation
• Fifth force constraints from the separation of galaxy mass components
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Unequal-Time Correlators for Cosmology
• The Origin of Exponential Star-forming Disks
• Cosmic filaments delay quenching inside clusters
• Stellar and black hole assembly in z<0.3 infrared-luminous mergers: intermittent starbursts vs. super-Eddington accretion
• Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate and α-enhancement
• The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Satellites of Satellites: The Case for Carina and Fornax
• Osaka Feedback Model II: Modeling Supernova Feedback Based on High-Resolution Simulations
• The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations
• Testing strong lensing subhalo detection with a cosmological simulation
• Regulation of Star Formation by a Hot Circumgalactic Medium
• Does the Milky Way Obey Spiral Galaxy Scaling Relations?
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history
• SDSS-IV MaNGA: drivers of stellar metallicity in nearby galaxies
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• The innate origin of radial and vertical gradients in a simulated galaxy disc
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Small-scale galaxy clustering in the EAGLE simulation
• AGN evolution from galaxy evolution viewpoint - II
• An observational test for star formation prescriptions in cosmological hydrodynamical simulations
• The Fornax3D project: discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427
• Exploring a new definition of the green valley and its implications
• The different baryonic Tully-Fisher relations at low masses
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• UV to submillimetre luminosity functions of TNG50 galaxies
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Constraining SIDM with halo shapes: revisited predictions from realistic simulations of early-type galaxies
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation
• Massive Low Surface Brightness Galaxies in the EAGLE Simulation
• A population of galaxy-scale jets discovered using LOFAR
• Modeling Evolution of Galactic Bars at Cosmic Dawn
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• Direct Detection of Mirror Matter in Twin Higgs Models
• Star formation quenching stages of active and non-active galaxies
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
• The dark matter component of the Gaia radially anisotropic substructure
• A new strong-lensing galaxy at z=0.066: Another elliptical galaxy with a lightweight IMF
• Supernovae feedback propagation: the role of turbulence
• Deviations from tidal torque theory: evolution of the halo spin-filament alignment
• Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting
• The impact of AGN-driven winds on physical and observable galaxy sizes
• Gas outflows from the z= 7.54 quasar : predictions from the BlueTides Simulation
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• The twisted dark matter halo of the Milky Way
• The physical drivers of the atomic hydrogen-halo mass relation
• The abundance of compact quiescent galaxies since z ~ 0.6
• The Illustris Simulation: Supermassive Black Hole - Galaxy Connection Beyond the Bulge
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^{\ast }$ Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• The distinct stellar metallicity populations of simulated Local Group dwarfs
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• A cosmological context for compact massive galaxies
• Mixing matters
• The angular momentum of disc galaxies at z=1
• Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• Barred galaxies in cosmological zoom-in simulations: the importance of feedback
• LYRA III: The smallest Reionization survivors
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: host galaxy properties and accretion rates of radio galaxies
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio correlation for High-redshift Dusty Star-forming Galaxies
• Observability of intermittent radio sources in galaxy groups and clusters
• Constraining the inner density slope of massive galaxy clusters
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model
• Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• 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
• Global Simulations of Galactic Discs: Violent Feedback from Clustered Supernovae during Bursts of Star Formation
• NIHAO III: The constant disc gas mass conspiracy
• Chemo-Dynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-$s$ and CEMP-no Stars
• Study of galaxies on large-scale filaments in simulations
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• An HST/COS legacy survey of intervening SiIII absorption in the extended gaseous halos of low-redshift galaxies
• The Physical Origin of Galactic Conformity: From Theory to Observation
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• A new sample of southern radio galaxies: Host galaxy masses and star-formation rates
• The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
• The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
• Stellar halos from The Dragonfly Edge-on Galaxies Survey
• Stellar feedback strongly alters the amplification and morphology of galactic magnetic fields
• RHAPSODY-G simulations II - Baryonic growth and metal enrichment in massive galaxy clusters
• The evolution of barred galaxies in the EAGLE simulations
• The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z~3
• The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation I: Introducing the Physically Evolved Winds (PhEW) Model
• Linking globular cluster formation at low and high redshift through the age-metallicity relation in E-MOSAICS
• On the Environments of Giant Radio Galaxies
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
• Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
• The Interaction between AGN and Starburst Activity in the Circumnuclear Region of NGC 7469 as Viewed with JWST
• Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias
• Chemical evolution of disc galaxies from cosmological simulations
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• The impact of the Large Magellanic Cloud on dark matter direct detection signals
• The impact of AGN on stellar kinematics and orbits in simulated massive galaxies
• 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
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• 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
• The importance of galaxy formation histories in models of reionization
• Revisiting the stellar mass -- angular momentum -- morphology relation: extension to higher bulge fraction, and the effect of bulge type
• Galaxy populations in the Hydra I cluster from the VEGAS survey I. Optical properties of a large sample of dwarf galaxies
• SDSS-IV MaNGA: How Galaxy Interactions Influence Active Galactic Nuclei
• VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift
• How AGN feedback drives the size growth of the first quasars
• History and destiny of an emerging early-type galaxy: New IFU insights on the major-merger remnant NGC7252
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• The shape of galaxy dark matter halos in massive galaxy clusters: Insights from strong gravitational lensing
• Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
• Modelling the M*-SFR relation at high redshift: untangling factors driving biases in the intrinsic scatter measurement
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• Linking the brightest stellar streams with the accretion history of Milky Way-like galaxies
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• The physical drivers of gas turbulence in simulated disc galaxies
• The missing dwarf galaxies of the Local Group
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• The MillenniumTNG Project: The large-scale clustering of galaxies
• The ACCELERATION programme: I. Cosmology with the redshift drift
• What to expect from dynamical modelling of galactic haloes II: the spherical Jeans equation
• The Geometry of the Infrared and X-ray Obscurer in a Dusty Hyperluminous Quasar
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Projected alignment of non-sphericities of stellar, gas, and dark matter distributions in galaxy clusters: analysis of the Horizon-AGN simulation
• Bars in dark matter-dominated dwarf galaxy discs
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• 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
• On the detectability of visible-wavelength line emission from the local circumgalactic and intergalactic medium
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Quantified diffuse light in compact groups of galaxies
• Generative deep fields: arbitrarily sized, random synthetic astronomical images through deep learning
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Galaxy clusters in local Universe simulations without density constraints: a long uphill struggle
• Cosmic evolution of radio-AGN feedback: confronting models with data
• Towards an improved model of self-interacting dark matter haloes
• The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• AGN feedback and the origin and fate of the hot gas in early-type galaxies
• The bright end of the infrared luminosity functions and the abundance of hyperluminous infrared galaxies
• The origin of the relation between metallicity and size in star-forming galaxies
• Reducing biases on $H_0$ measurements using strong lensing and galaxy dynamics: results from the EAGLE simulation
• The Compact Structures of Massive $z\sim 0.7$ Post-Starburst Galaxies in the SQuIGG$\vec{L}$E Sample
• VIS3COS: I. survey overview and the role of environment and stellar mass on star formation
• Rise and fall of post-starburst galaxies in Magneticum Pathfinder
• A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation
• A Candidate Kiloparsec-scale Quasar Pair at $z=5.66$
• Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
• Biases and systematics in the observational derivation of galaxy properties: comparing different techniques on synthetic observations of simulated galaxies
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI -- Stellar Populations
• Implications of a variable IMF for the interpretation of observations of galaxy populations
• BAT AGN Spectroscopic Survey -- XVII: The Parsec-scale Jet Properties of the Ultra Hard X-ray Selected Local AGN
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• A Multiwavelength Study of Active Galactic Nuclei in Post-Merger Remnants
• Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
• Strategies for Detecting the Missing Hot Baryons in the Universe
• Ionized Outflows in Nearby Quasars are Poorly Coupled to their Host Galaxies
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• The nature of damped HI absorbers probed by cosmological simulations: satellite accretion and outflows
• The COS-AGN survey: Revealing the nature of circum-galactic gas around hosts of active galactic nuclei
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• The stellar halo in Local Group Hestia simulations II. The accreted component
• Tidal disruption events from massive black hole binaries: predictions for ongoing and future surveys
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• The relation between star formation rate and stellar mass of galaxies at z $\sim$ 1-4
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Effects of Inner Halo Angular Momentum on the Peanut/X-shapes of Bars
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• Stacked star formation rate profiles of bursty galaxies exhibit 'coherent' star formation
• Modeling the kinematics of globular cluster systems
• The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
• The evolution of galaxy intrinsic alignments in the MassiveBlack II universe
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• Explaining the scatter in the galaxy mass-metallicity relation with gas flows
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• Enhanced Star Formation Efficiency in the Central Regions of Nearby Quasars Hosts
• Numerical modelling of the lobes of radio galaxies in cluster environments -- IV. Remnant radio galaxies
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data
• Baryons Shaping Dark Matter Haloes
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• Direct measurement of the distribution of dark matter with strongly lensed gravitational waves
• MAMMOTH: Confirmation of Two Massive Galaxy Overdensities at $z=2.24$ with H$\alpha$ Emitters
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• The clustering of submillimeter galaxies detected with ALMA
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• Spiral Arms are Metal Freeways: Azimuthal Gas-Phase Metallicity Variations in Simulated Cosmological Zoom-in Flocculent Disks
• The formation and evolution of star clusters in interacting galaxies
• Using the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• Dark-matter-deficient galaxies in hydrodynamical simulations
• Velocity-dependent J-factors for annihilation radiation from cosmological simulations
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• On the Role of Hot Feedback Mode in Active Galactic Nuclei Feedback in an Elliptical Galaxy
• An FMOS Survey of moderate-luminosity broad-line AGN in COSMOS, SXDS and E-CDF-S
• The impact of baryonic physics and massive neutrinos on weak lensing peak statistics
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• The fundamental metallicity relation emerges from the local anti-correlation between star formation rate and gas-phase metallicity existing in disk galaxies
• Panspermia in a Milky Way-like Galaxy
• The orbital phase space of contracted dark matter halos
• Stellar populations across the black hole mass - velocity dispersion relation
• The Type II AGN-host galaxy connection: insights from the VVDS and VIPERS surveys
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Merging galaxies produce outliers from the Fundamental Metallicity Relation
• Nonparametric galaxy morphology from UV to submm wavelengths
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• Measuring the Density Fields around Bright Quasars at $z\sim 6$ with XQR-30 Spectra
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• A first estimate of the Milky Way dark matter halo spin
• Constraining dark photons and their connection to 21 cm cosmology with CMB data
• The Clustering Evolution of Dusty Star-Forming Galaxies
• 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
• A General Precipitation-Limited L_X-T-R Relation Among Early-Type Galaxies
• Do we need soft cosmology?
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• The CGM${}^2$ Survey: Quenching and the Transformation of the Circumgalactic Medium
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• 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 $1.7<z<6.3$
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• Predicting sub-millimeter flux densities from global galaxy properties
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• The inner structure of dwarf sized halos in Warm and Cold Dark Matter cosmologies
• Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
• Baryonic mass budgets for haloes in the EAGLE simulation, including ejected and prevented gas
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Strongly lensed cluster substructures are not in tension with $\Lambda$CDM
• The Quasar Feedback Survey: Revealing the Interplay of Jets, Winds & Emission Line Gas in Type 2 Quasars with Radio Polarization
• The FLAMINGO project: Baryon effects on the matter power spectrum
• Star formation quenching imprinted on the internal structure of naked red nuggets
• Deep ALMA photometry of distant X-ray AGN: improvements in star formation rate constraints, and AGN identification
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Cosmic Reionization On Computers: Numerical and Physical Convergence
• The Variability of Star Formation Rate in Galaxies: II. Power Spectrum Distribution on the Main Sequence
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• Detection of thermal Sunyaev-Zel'dovich Effect in the circumgalactic medium of low-mass galaxies -- a surprising pattern in self-similarity and baryon sufficiency
• A numerical twist on the observational spin parameter, ${\lambda }_R$
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• The Velocity Dispersion Function for Quiescent Galaxies in the Local Universe
• The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• The Ages and Metallicities of the Globular Clusters in the Sparkler
• Not a Copernican observer: biased peculiar velocity statistics in the local Universe
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Properties of brightest group galaxies in cosmic web filaments
• High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair
• The Supersonic Project: rotational effects of supersonic motions on the first structures in the Universe
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Being WISE II: Reducing the Influence of Star Formation History on the Mass-to-Light Ratio of Quiescent Galaxies
• Subaru Hyper Suprime-Cam View of Quasar Host Galaxies at z < 1
• Star Formation and AGN Feedback in the Local Universe: Combining LOFAR and MaNGA
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• Simulation techniques for modified gravity
• Coevolution of metallicity and star formation in galaxies to z=3.7: II. A theoretical model
• A galaxy's accretion history unveiled from its integrated spectrum
• The Warm Circum-Galactic Medium: 10^5-6 K Gas Associated with a Single Galaxy Halo or with an Entire Group of Galaxies?
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• Exploring the Dust Content of Galactic Winds With Herschel. II. Nearby Dwarf Galaxies
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• Impact of Baryonic Physics on Intrinsic Alignments
• The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
• Searching for Environmental Effects on Galaxy Kinematics in Groups and Clusters at z~1 from the ORELSE Survey
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Into the Lyα jungle: exploring the circumgalactic medium of galaxies at z ~ 4-5 with MUSE
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• SOAP: A Python Package for Calculating the Properties of Galaxies and Halos Formed in Cosmological Simulations
• The metallicity distribution of HI systems in the EAGLE cosmological simulation
• Inferring galaxy dark halo properties from visible matter with Machine Learning
• Dark Matter Candidates and Searches
• Origins of carbon-enhanced metal-poor stars
• The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• Stellar feedback in M83 as observed with MUSE -- I. Overview, an unprecedented view of the stellar and gas kinematics and evidence of outflowing gas
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• The assembly of spheroid-dominated galaxies in the EAGLE simulation
• Distance, Energy, and Variability of Quasar Outflows: Two HST/COS epochs of LBQS 1206+1052
• 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
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• The galaxy morphology-density relation in the EAGLE simulation
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Galaxy properties in the cosmic web of EAGLE simulation
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• The hot circumgalactic medium of the Milky-Way: new insights from XMM-Newton observations
• RAiSE: simulation-based analytical model of AGN jets and lobes
• AGN Feedback in Groups and Clusters of Galaxies
• Low-mass compact elliptical galaxies: spatially-resolved stellar populations and kinematics with the Keck Cosmic Web Imager
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$). Mass budget, satellites spin alignment and gas infall in a massive $z\sim 3$ quasar host halo
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• Clustering of Gravitational Wave and Supernovae events: a multitracer analysis in Luminosity Distance Space
• The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• Chemical evolution of giant molecular clouds in simulations of galaxies
• The moving mesh code Shadowfax
• Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• Halo uncertainties in electron recoil events at direct detection experiments
• Enhanced star formation in $z\sim 6$ quasar companions
• Constraints on galileons from the positions of supermassive black holes
• The Effect of Galactic Feedback on Gas Accretion and Wind Recycling
• MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues
• The origin of X-ray coronae around simulated disc galaxies
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• First Light And Reionisation Epoch Simulations (FLARES) VI: The colour evolution of galaxies $z=5-15$
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• 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
• The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies
• Is There a Fundamental Upper Limit to the Mass of a Star Cluster?
• Bayesian Calibration of Force-fields from Experimental Data: TIP4P Water
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• The Contribution of Quasar Absorption Outflows to AGN Feedback
• Kinematics of the OVI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
• Calibrated, cosmological hydrodynamical simulations with variable IMFs III: Spatially-resolved properties and evolution
• Realistic HI scale heights of Milky Way-mass galaxies in the FIREbox cosmological volume
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
• To be or not to be: hot WHIM absorption in the blazar PKS 2155-304 sight line?
• Voyage through the Hidden Physics of the Cosmic Web
• Taking the Milky Way for a spin: disc formation in the ARTEMIS simulations
• Galaxies with monstrous black holes in galaxy cluster environments
• Gas around galaxy haloes - II: hydrogen absorption signatures from the environments of galaxies at redshifts 2 < z < 3
• Fast Multipole Method for Gravitational Lensing. Application to High Magnification Quasar Microlensing
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• How identifying circumgalactic gas by line-of-sight velocity instead of the location in 3D space affects O VI measurements
• Dynamical History of the Local Group in $\Lambda$CDM
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• The low abundance and insignificance of dark discs in simulated Milky Way galaxies
• Hydrodynamical structure formation in Milgromian cosmology
• Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• What to expect from dynamical modelling of galactic haloes
• The assembly bias of emission line galaxies
• 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
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• Dynamical evolution of massive black holes in galactic-scale N-body simulations - introducing the regularized tree code "rVINE"
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Quantifying substructures in {\it Hubble Frontier Field} clusters: comparison with $\Lambda CDM$ simulations
• Searching For Fossil Evidence of AGN Feedback in WISE-Selected Stripe-82 Galaxies By Measuring the Thermal Sunyaev-Zel'dovich Effect With the Atacama Cosmology Telescope
• The survival of globular clusters in a cuspy Fornax
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• Baryonic Distributions in Galaxy Dark Matter Haloes I: New Observations of Neutral and Ionized Gas Kinematics
• Star-Gas Misalignment in Galaxies: II. Origins Found from the Horizon-AGN Simulation
• From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass
• Connecting cosmological accretion to strong Lyman-alpha absorbers
• On the correlation between the local dark matter and stellar velocities
• Star-gas misalignment in galaxies: I. The properties of galaxies from the Horizon-AGN simulation and comparisons to SAMI
• Massive galaxy formation caught in action at z~5 with JWST
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• The Cosmic Dispersion Measure in the EAGLE Simulations
• The galaxy correlation function as a constraint on galaxy formation physics
• A new model framework for circumgalactic Ly$\alpha$ radiative transfer constrained by galaxy-Ly$\alpha$ forest clustering
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Merger histories of brightest group galaxies from MUSE stellar kinematics
• H2 chemistry in galaxy simulations: an improved supernova feedback model
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• Predictions for the detection of Tidal Streams with Gaia using Great Circle Methods
• Simulating the Carbon Footprint of Galactic Halos
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
• A large difference in the progenitor masses of active and passive galaxies in the EAGLE simulation
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• The galaxy-galaxy strong lensing cross-sections of simulated LCDM galaxy clusters
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• A 4% measurement of $H_0$ using the cumulative distribution of strong-lensing time delays in doubly-imaged quasars
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Does jackknife scale really matter for accurate large-scale structure covariances?
• The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
• Star-formation quenching of cluster galaxies as traced by metallicity, presence of active galactic nuclei, and galactic conformity
• Exploring Relations Between BCG \& Cluster Properties in the SPectroscopic IDentification of eROSITA Sources Survey from $0.05<z<0.3$
• BUDDI-MaNGA II: The Star-Formation Histories of Bulges and Discs of S0s
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• Late-time cosmic evolution of dust: solving the puzzle
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Galaxy and Mass Assembly (GAMA): Small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies
• A high-resolution cosmological simulation of a strong gravitational lens
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• The mass-size plane of EAGLE galaxies
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• The present-day gas content of simulated field dwarf galaxies
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• Local photoionization feedback effects on galaxies
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Some Die Filthy Rich: The Diverse Molecular Gas Contents of Post-starburst Galaxies Probed by Dust Absorption
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• The IllustrisTNG Simulations: Public Data Release
• A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
• The cosmic spectral energy distribution in the EAGLE simulation
• Reignited star formation in dwarf galaxies quenched during reionization
• Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Tidal features of classical Milky Way satellites in a $\Lambda$CDM universe
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• The Hector Survey: integral field spectroscopy of 100,000 galaxies
• On the dearth of ultra-faint extremely metal poor galaxies
• The volume density of giant low surface brightness galaxies
• Informing dark matter direct detection limits with the ARTEMIS simulations
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• Through a Smoother Lens: An expected absence of LCDM substructure detections from hydrodynamic and dark matter only simulations
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• Groups and protocluster candidates in the CLAUDS and HSC-SSP joint deep surveys
• Non-isotropic feedback from accreting spinning black holes
• A new discovery space opened by eROSITA: Ionised AGN outflows from X-ray selected samples
• The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
• Compact Molecular Gas Distribution in Quasar Host Galaxies
• Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar halo
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• Push it to the limit: Local Group constraints on high-redshift stellar mass functions for Mstar > 10^5 Msun
• The SAMI Galaxy Survey: The role of disc fading and progenitor bias in kinematic transitions
• Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
• Dissecting Nearby Galaxies with piXedfit: II. Spatially Resolved Scaling Relations Among Stars, Dust, and Gas
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Forensic reconstruction of galaxy colour evolution and population characterisation
• 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
• What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• Monte Carlo Physarum Machine: Characteristics of Pattern Formation in Continuous Stochastic Transport Networks
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?
• The Obsidian model: Three regimes of black hole feedback
• 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
• TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
• Outflow densities and ionisation mechanisms in the NLRs of the prototypical Seyfert galaxies NGC 1068 and NGC 4151
• Faint Satellite Population of the NGC-3175 Group - a Local Group Analogue
• Gas Accretion and Galactic Chemical Evolution: Theory and Observations
• First Light And Reionisation Epoch Simulations (FLARES) XIII: The Lyman-continuum emission of high-redshift galaxies
• The abundance of dark matter haloes down to Earth mass
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Spatially offset black holes in the Horizon-AGN simulation and comparison to observations
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• A multiwavelength survey of HI-excess galaxies with surprisingly inefficient star formation
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions
• On the relevance of chaos for halo stars in the solar neighbourhood II
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• QSOFEED: The relationship between star formation and AGN Feedback
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• There and back again: understanding the critical properties of backsplash galaxies
• Intracluster light in the core of z~2 galaxy proto-clusters
• Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies
• CLASH-VLT: The inner slope of the MACS J1206.2-0847 dark matter density profile
• Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• The complex interplay of AGN jet-inflated bubbles and the intracluster medium
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• 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
• Simulating ionization feedback from young massive stars: impact of numerical resolution
• The impact of black hole seeding in cosmological simulations
• Properties of Fast and Slow Bars Classified by Epicyclic Frequency Curves from Photometry of Barred Galaxies
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Nonparametric galaxy morphology from stellar and nebular emission with the CALIFA sample
• The Galactic Interstellar Object Population: A Framework for Prediction and Inference
• Effective Dark Matter Halo catalog in $f(R)$ gravity
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• 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
• The Cluster-EAGLE project: a comparison of dynamical mass estimators using simulated clusters
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Attack of the Flying Snakes : Formation of Isolated HI Clouds By Fragmentation of Long Streams
• Gravitational lensing in LoTSS DR2 -- Extremely faint 144-MHz radio emission from two highly magnified quasars
• Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
• 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
• SUPER VII. Morphology and kinematics of H$\alpha$ emission in AGN host galaxies at Cosmic noon using SINFONI
• The Ultraviolet Detection of Diffuse Gas in Galaxy Groups
• Teaching neural networks to generate Fast Sunyaev Zel'dovich Maps
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Candidate star clusters toward the inner Milky Way discovered on deep-stacked Ks-band images from the VVV Survey
• Star formation in mergers with cosmologically motivated initial conditions
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• The galaxy's gas content regulated by the dark matter halo mass results in a super-linear M${}_{\mathrm{BH}}$-M${}_{\star }$ relation
• The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
• Spectro-Imaging Forward Model of Red and Blue Galaxies
• The whole picture of the large-scale structure of the CL1604 supercluster at z$\sim$0.9
• Where infall meets outflows: turbulent dissipation probed by CH${}^{+}$ and Ly$\alpha$ in the starburst/AGN galaxy group SMM J02399$-$0136 at z$\sim$2.8
• An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation
• ABCpy: A High-Performance Computing Perspective to Approximate Bayesian Computation
• The Mass and Absorption Columns of Galactic Gaseous Halos II -- The High Ionization State Ions
• Dynamical modelling and origin of gas turbulence in z $\sim$ 4.5 galaxies
• Milky Way and M31 rotation curves: $\Lambda$CDM vs. MOND
• Simplified galaxy formation with mesh-less hydrodynamics
• Revisiting the fundamental metallicity relation with observation and simulation
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• Oxygen yields as a constraint on feedback processes in galaxies
• Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
• Cosmic gas highways in C-EAGLE simulations
• Excitation and acceleration of molecular outflows in LIRGs: The extended ESO 320-G030 outflow on 200-pc scales
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• How feedback shapes galaxies: an analytic model
• The role of AGN on the structure, kinematics and evolution of ETGs in the Horizon simulations
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• A Big Red Dot: Scattered light, host galaxy signatures and multi-phase gas flows in a luminous, heavily reddened quasar at cosmic noon
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• The MOSDEF Survey: Differences in SFR and Metallicity for Morphologically-Selected Mergers at z~2
• The most luminous, merger-free AGN show only marginal correlation with bar presence
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Micro galaxies in LCDM
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Detection of the self-regulation of star formation in galaxy discs
• The large-scale structure around the Fornax-Eridanus Complex
• Signatures of dark and baryonic structures on weakly lensed gravitational waves
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• CMB-HD: Astro2020 RFI Response
• Evaluating hydrodynamical simulations with green valley galaxies
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Local and global gas metallicity versus stellar age relation in MaNGA galaxies
• 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
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• The Galaxy Stellar Mass Function and Low Surface Brightness Galaxies from Core-Collapse Supernovae
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• Stellar populations and origin of thick disks in AURIGA simulations
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• Correlation function: biasing and fractal properties of the cosmic web
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• On the small scale clustering of quasars: constraints from the MassiveBlack II simulation
• Analysis of the galaxy size versus stellar mass relation
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Detecting the neutral IGM in filaments with the SKA
• A Nitrogen-Enhanced Metal-Poor star discovered in the globular cluster ESO280-SC06
• Massive spheroids can form in single minor mergers
• Gaia Data Release 3: Surface brightness profiles of galaxies and host galaxies of quasars
• The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
• Galaxy Structural Analysis with the Curvature of the Brightness Profile
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• Globular cluster metallicity distributions in the E-MOSAICS simulations
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Calibrated, cosmological hydrodynamical simulations with variable IMFs II: Correlations between the IMF and global galaxy properties
• First Light And Reionisation Epoch Simulations (FLARES) XI: [OIII] emitting galaxies at $5<z<10$
• AGN must be very efficient at powering outflows
• Intrinsic and observed dual AGN fractions from major mergers
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• Testing galaxy formation models with galaxy stellar mass functions
• Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo Cluster
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• 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
• Quantifying the cool ISM in radio AGNs: evidence for late-time re-triggering by galaxy mergers and interactions
• The distribution and properties of DLAs at z $\le$ 2 in the EAGLE simulations
• Gas Accretion and Star Formation Rates
• MHONGOOSE discovery of a gas-rich low-surface brightness galaxy in the Dorado Group
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• What has quenched the massive spiral galaxies?
• The Mass Growth and Stellar Ages of Galaxies: Observations versus Simulations
• 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
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• The bar rotation rate as a diagnostic of dark matter content in the centre of disc galaxies
• 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
• Spatially resolved observations of outflows in the radio loud AGN of UGC 8782
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• Luminosity function of [OII] emission-line galaxies in the MassiveBlack-II simulation
• Little Red Dots as Direct-collapse Black Hole Nurseries
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• Ram pressure stripping in the EAGLE simulation
• A too-many dwarf satellite galaxies problem in the MATLAS low-to-moderate density fields
• The CGM-GRB Study. I. Uncovering The CircumGalactic Medium around GRB hosts at redshifts 2-6
• Predicting the water content of interstellar objects from galactic star formation histories
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• Stellar migration in the Auriga simulations
• Baryonic feedback measurement from KV450 cosmic shear analysis
• Column Density Profiles of Cold Clouds Driven by Galactic Outflows
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• The Velocity Dispersion Function for Massive Quiescent and Star-Forming Galaxies at 0.6 $<$ z $\le$ 1.0
• The origin of star-gas misalignments in simulated galaxies
• Evolution of Dust-Obscured Star Formation and Gas to z=2.2 from HiZELS
• Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure
• The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
• The Physical Nature of Circumgalactic Medium Absorbers in Simba
• Unveiling the warm molecular outflow component of type-2 quasars with SINFONI
• Galactic satellite systems in CDM, WDM and SIDM
• Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
• MusE GAs FLOw and Wind (MEGAFLOW) IX. The impact of gas flows on the relations between the mass, star formation rate and metallicity of galaxies
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• New constraints on the evolution of the MHI-M* scaling relation combining CHILES and MIGHTEE-HI data
• Morphology-assisted galaxy mass-to-light predictions using deep learning
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• Translators of galaxy morphology indicators between observation and simulation
• The kinematics of young and old stellar populations in nuclear rings of MUSE TIMER galaxies
• Testing the fidelity of simulations of black hole - galaxy co-evolution at z ~ 1.5 with observations
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• An intergalactic medium temperature from a giant radio galaxy
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• On the absence of backsplash analogues to NGC 3109 in the $\Lambda$CDM framework
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• Photoevaporation of Molecular Clouds in Regions of Massive Star Formation as Revealed Through H${}_2$ and Br$\gamma$ Emission
• A simple way to improve AGN feedback prescription in SPH simulations
• Detection capabilities of the Athena X-IFU for the warm-hot intergalactic medium using gamma-ray burst X-ray afterglows
• Progenitor-mass-dependent yields amplify intrinsic scatter in dwarf-galaxy elemental abundance ratios
• Inconsistencies arising from the coupling of galaxy formation sub-grid models to Pressure-Smoothed Particle Hydrodynamics
• Toward a Physical Understanding of Galaxy-Halo Alignment
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• The Fornax Cluster VLT Spectroscopic Survey IV -- Cold kinematical substructures in the Fornax core from COSTA
• The SFR-radius connection: data and implications for wind strength and halo concentration
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• Do current X-ray observations capture most of the black-hole accretion at high redshifts?
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• Young Massive Clusters: Their Population Properties, Formation and Evolution, and Their Relation to the Ancient Globular Clusters
• Galaxy stellar and total mass estimation using machine learning
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
• The mass-size relation of galaxy clusters
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• A Comparison of Star-Forming Clumps and Tidal Tails in Local Mergers and High Redshift Galaxies
• Angular momentum-related probe of cold gas deficiencies
• Cold molecular gas outflow encasing the ionised one in the Seyfert galaxy NGC 3281
• G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
• The ALPINE-ALMA [CII] Survey: CGM pollution and gas mixing by tidal stripping in a merging system at z~4.57
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations I: Unique Galaxy Morphologies in Imaging
• BUDHIES V: The baryonic Tully-Fisher relation at z=0.2 based on direct HI detections
• Angular momentum evolution of bulge stars in disc galaxies in NIHAO
• Abundance and group coalescence timescales of compact groups of galaxies in the EAGLE simulation
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
• MARTINI: Mock Array Radio Telescope Interferometry of the Neutral ISM
• Tracking the orbit of unresolved subhalos for semi-analytic models
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• CGM${}^2$ $+$ CASBaH: The Mass Dependence of H~I Ly$\alpha$-Galaxy Clustering and the Extent of the CGM
• VLT/SINFONI study of black hole growth in high redshift radio-loud quasars from the CARLA survey
• Discovery of a multiphase OVI and OVII absorber in the circumgalactic/intergalactic transition region
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H${}_2$ in the radio galaxy 3C 326 N
• Evolution of CIV Absorbers. II. Where does CIV live?
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
• The Host Galaxies of Radio AGN: New Views from Combining LoTSS and MaNGA Observations
• Testing the Impact of Satellite Anisotropy on Large and Small Scale Intrinsic Alignments using Hydrodynamical Simulations
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Physical Conditions of Five O VI Absorption Systems Towards PG $1522+101$
• Testing the Breathing Mode in Intermediate Mass Galaxies and its Predicted Star Formation Rate-Size Anti-Correlation
• Imprint of baryons and massive neutrinos on velocity statistics
• LyMAS reloaded: improving the predictions of the large-scale Lyman-α forest statistics from dark matter density and velocity fields
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Molecular gas excitation and outflow properties of obscured quasars at z$\sim$0.1
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• The local dark matter distribution in self-interacting dark matter halos
• History of the gas fuelling star formation in eagle galaxies
• Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters
• Great Balls of FIRE III: Modeling Black Hole Mergers from Massive Star Clusters in Simulations of Galaxies
• Lack of Correlations between Cold Molecular Gas and AGN Properties in Type 1 AGNs at $z\lesssim 0.5$
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• Carbon envelopes around merging galaxies at z ~ 4.5
• The OH Megamaser galaxy IRAS11506-3851: an AGN and starformation revealed by multiwavelength observations
• Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
• The signal of decaying dark matter with hydrodynamical simulations
• 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
• Measuring the temperature and profiles of Lyman-$\alpha$ absorbers
• Can Stellar Discs in a Cosmological Setting Avoid Forming Strong Bars?
• Extending Semi-numeric Reionisation Models to the First Stars and Galaxies
• Testing the tidal stripping scenario of ultra-compact dwarf galaxy formation by using internal properties
• Quantifying the effect of black hole feedback from the central galaxy on the satellite populations of groups and clusters
• Populating The Milky Way: Characterising Planet Demographics by Combining Galaxy Formation Simulations and Planet Population Synthesis Models
• The Quasar Feedback Survey: zooming into the origin of radio emission with e-MERLIN
• Probing Feedback in Galaxy Formation with Millimeter-wave Observations
• A Distinct Radial Acceleration Relation across Brightest Cluster Galaxies and Galaxy Clusters
• 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
• Setting the Stage: Structures from Gaussian Random Fields
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• Is Terzan 5 the remnant of a building block of the Galactic bulge? Evidence from APOGEE
• An environment-dependent halo mass function as a driver for the early quenching of $z\ge 1.5$ cluster galaxies
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• A common origin for the Fundamental Plane of quiescent and star-forming galaxies in the EAGLE simulations
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• An HSC view of the CMASS galaxy sample. Halo mass as a function of stellar mass, size and Sérsic index
• Revealing the Galaxy-Halo Connection Through Machine Learning
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Star Formation and Chemical Enrichment in Protoclusters
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• A study of the HI gas fractions of galaxies at z ~ 1
• Extragalactic Stellar Tidal Streams: Observations meet Simulation
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Merge and strip: dark matter-free dwarf galaxies in clusters can be formed by galaxy mergers
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• Colour-magnitude diagram in simulations of galaxy formation
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16
• Relating galaxies across different redshift to study galaxy evolution
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• The Tail of Late-forming Dwarf Galaxies in $\Lambda$CDM
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
• Modelling Dark Matter Halo Spin using Observations and Simulations: application to UGC 5288
• Radial stellar populations of AGN-host dwarf galaxies in SDSS-IV MaNGA survey
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Constraints on galactic outflows from the metallicity-stellar mass-SFR relation of EAGLE simulation and SDSS galaxies
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• Determining Satellite Infall Times Using Machine Learning
• Surveying the onset and evolution of supermassive black holes at high-z with AXIS
• Sensitivity of non-radiative cloud-wind interactions to the hydrodynamics solver
• Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
• SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
• Black hole virial masses from single-epoch photometry: the miniJPAS test case
• A field-level emulator for modeling baryonic effects across hydrodynamic simulations
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• QSO MUSEUM II: Search for extended Ly$\alpha$ emission around eight $z\sim 3$ quasar pairs
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• Using angular momentum maps to detect kinematically distinct galactic components
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• GABE: Galaxy Assembly with Binary Evolution
• Numerical simulations of AGN wind feedback on black hole accretion: probing down to scales within the sphere of influence
• Searching for HI around MHONGOOSE Galaxies via Spectral Stacking
• Early-type galaxies in low-density environments: NGC 6876 explored through its globular cluster system
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• A modern view of galaxies and their stellar populations
• The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
• 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
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• The physics governing the upper truncation mass of the globular cluster mass function
• Outskirts of Nearby Disk Galaxies: Star Formation and Stellar Populations
• Galaxy flows within 8,000 km/s from Numerical Action methods
• Formation and fate of low metallicity stars in IllustrisTNG50
• The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation
• The faint end of the 250 micron luminosity function at z < 0.5
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• Projecting SPH Particles in Adaptive Environments
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Probing the physical properties of the intergalactic medium using gamma-ray bursts
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• Stellar angular momentum distribution linked to galaxy morphology
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• 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
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Using EAGLE simulations to study the effect of observational constraints on the determination of HI asymmetries in galaxies
• Can $\Lambda$CDM model reproduce MOND-like behavior?
• Resolved star formation in TNG100 central and satellite galaxies
• Measuring the physical imprints of gas flows in galaxies I: Accretion rate histories
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• A Local Universe model for constrained simulations
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• Constraining galaxy-halo connection with high-order statistics
• On the connection between AGN radiative feedback and massive black hole spin
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• The extragalactic $\gamma$-ray background: imprints from the physical properties and evolution of star-forming galaxy populations
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• SDSS-IV MaNGA: Unveiling Galaxy Interaction by Merger Stages with Machine Learning
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• The impact of HII regions on Giant Molecular Cloud properties in nearby galaxies sampled by PHANGS ALMA and MUSE
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Black Hole Weather Forecasting with Deep Learning: A Pilot Study
• What is the real accretion rate onto a black hole for low angular momentum accretion?
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (I) Temporal dependency
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• Mitigating baryonic effects with a theoretical error covariance
• The parametrization of gas flows in discs in the Auriga simulations
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• A counter-image to the gravitational arc in Abell 1201: Evidence for IMF variations, or a $10^{10}$M${}_{\odot }$ black hole?
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• On the detectability of massive black hole merger eventsby LISA
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• New constraints on red-spiral galaxies from their kinematics in clusters of galaxies
• The Close AGN Reference Survey (CARS): No evidence of galaxy-scale hot outflows in two nearby AGN
• The Dark Matter Halos of HI Selected Galaxies
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Galaxy And Mass Assembly (GAMA) Survey: The Merging Potential of Brightest Group Galaxies
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• The chemical imprint of the bursty nature of Milky Way's progenitors
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• Connection Between Galaxies and HI in the Circumgalactic and Intergalactic Media: Variation According to Galaxy Stellar Mass and Star-formation Activity
• Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
• A robust two-parameter description of the stellar profile of elliptical galaxies
• X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
• 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
• The formation of compact massive relic galaxies in MOND
• Abundance matching tested on small scales with galaxy dynamics
• VALES V: A kinematic analysis of the molecular gas content in $H$-ATLAS galaxies at $z\sim 0.03-0.35$ using ALMA
• 2mm Observations and the Search for High-Redshift Dusty Star-forming Galaxies
• A break in the high-redshift stellar mass Tully-Fisher relation
• Spin speed correlations and the evolution of galaxy-halo systems
• Old and New Major Mergers in the SOSIMPLE galaxy, NGC 7135
• Properties of Galaxies in the Disc Central Surface Brightness Gap
• The impact of the cosmological constant on past and future star formation
• Assembly bias evidence in close galaxy pairs
• Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
• El Gordo needs El Anzuelo: Probing the structure of cluster members with multi-band extended arcs in JWST data
• DIISC-I: The Discovery of Kinematically Anomalous HI Clouds in M 100
• The impact of filaments on dwarf galaxy properties in the Auriga simulations
• Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars
• Probing the physical properties of the intergalactic medium using blazars
• Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
• Ubiquity of density slope oscillations in the central regions of galaxy and cluster-sized systems
• The SAMI Galaxy Survey: Detection of Environmental Dependence of Galaxy Spin in Observations and Simulations Using Marked Correlation Functions
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Multi-wavelength consensus of large-scale linear bias
• Subhalo abundance matching in $f(R)$ gravity
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• Radial X-ray profiles of simulated galaxies: Contributions from hot gas and XRBs
• A search for the missing baryons with X--ray absorption lines towards the blazar 1ES 1553+113
• Bursty star formation feedback and cooling outflows
• Lessons from a blind study of simulated lenses: image reconstructions do not always reproduce true convergence
• Black Hole Feeding and Feedback in a Compact Galaxy
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• Probing satellite galaxies in the Local Group by using FAST
• Simulated [CII] in high-z galaxies
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Cosmic Web & Caustic Skeleton: non-linear Constrained Realizations -- 2D case studies
• A deep learning approach to halo merger tree construction
• A WHIM origin for the soft excess emission in the Coma cluster
• Correlations between mass, stellar kinematics and gas metallicity in EAGLE galaxies
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• On the Tremaine-Weinberg method: how much can we trust gas tracers to measure pattern speeds?
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• Globular cluster ages and their relation to high-redshift stellar cluster formation times from different globular cluster models
• Setting the scene for BUFFALO: A study of the matter distribution in the HFF galaxy cluster MACS J0416.1-2403 and its parallel field
• Initial sizes of star clusters: implications for cluster dissolution during galaxy evolution
• The perils of stacking optically selected groups in eROSITA data. The Magneticum perspective
• Studying galaxy cluster morphological metrics with Mock-X
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• Local Two-Sample Testing: A New Tool for Analysing High-Dimensional Astronomical Data
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• Can tides explain the low dark matter density in Fornax?
• Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• Measuring Galaxy Asymmetries in 3D
• An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• Astrophysics with the Laser Interferometer Space Antenna
• GalaxyFlow: Upsampling Hydrodynamical Simulations for Realistic Mock Stellar Catalogs
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• Numerical Discreteness Errors in Multi-Species Cosmological N-body Simulations
• The MAGPI survey: The interdependence of the mass, star formation rate, and metallicity in galaxies at z~0.3
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• The history and mass content of cluster galaxies in the EAGLE simulation
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• NIHAO XXVII: Crossing the green valley
• What is the origin of the JWST SMBHs?
• The effect of hydrodynamical simulation inspired dark matter velocity profile on directional detection of dark matter
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Gamma rays from dark matter spikes in EAGLE simulations
• A rising tide: Intrinsic alignments since the turn of the millennium
• Controlling systematics in ground-based CMB surveys with partial boresight rotation
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
• Dipolar dark matter simulations on galaxy scales with the RAMSES code
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• A comprehensive study on the relation between the metal enrichment of ionised and atomic gas in star-forming galaxies
• Indirect searches of Galactic diffuse dark matter in INO-MagICAL detector
• The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• Explaining the formation of bulges with MOND
• Dissociation of dark matter and gas in cosmic large-scale structure
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• Disc-Halo Interactions in ΛCDM
• ALPINE: A Large Survey to Understand Teenage Galaxies
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
• Multidimensional upwind hydrodynamics on unstructured meshes using Graphics Processing Units I. Two-dimensional uniform meshes
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• On the application of dimensionality reduction and clustering algorithms for the classification of kinematic morphologies of galaxies
• Dwarf Galaxies as Cosmological Probes
• Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model
• Measurements of the angular momentum-mass relations in the Simba simulation
• Domain adaptation techniques for improved cross-domain study of galaxy mergers
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Tracing the Formation of Molecular Clouds in a Low-Metallicity Galaxy: A HI Narrow Self-Absorption Survey of the Large Magellanic Cloud
• Can Cooling and Heating Functions be Modeled with Homogeneous Radiation Fields?
• The case for two-dimensional galaxy-galaxy lensing
• CMB-HD: An Ultra-Deep, High-Resolution Millimeter-Wave Survey Over Half the Sky
• Simulating the dark matter decay signal from the Perseus galaxy cluster
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Velocity-dependent J-factors for Milky Way dwarf spheroidal analogues in cosmological simulations
• Magnesium isotope ratios in Milky Way and dwarf galaxy stars
• Efficiently estimating mean, uncertainty and unconstrained large scale fraction of local Universe simulations with paired fixed fields
• The formation and disruption of globular cluster populations in simulations of present-day $L^{\ast }$ galaxies with controlled assembly histories
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• Local variations of the Stellar Velocity Ellipsoid-I: the disc of galaxies in the Auriga simulations
• Red riding on hood: Exploring how galaxy colour depends on environment
• SWIFT: Maintaining weak-scalability with a dynamic range of $10^4$ in time-step size to harness extreme adaptivity
• Searching for dark matter subhalos in the Fermi-LAT catalog with Bayesian neural networks
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Does radiative feedback make faint z>6 galaxies look small?
• Degeneracies between Modified Gravity and Baryonic Physics
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• An HI story of galaxies in Abell 2626 and beyond
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• A young galaxy cluster in the old Universe
• The OTELO survey: the star formation rate evolution of low-mass galaxies
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• 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
• Galaxy-galaxy lensing in the VOICE deep survey
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
• First Light and Reionisation Epoch Simulations (FLARES) X: Environmental Galaxy Bias and Survey Variance at High Redshift
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• The High Mass X-ray Binaries in star-forming galaxies
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
• CEMPlifying reionization
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• The global energetics of radio AGN kinetic feedback in the local universe
• Galaxy formation from a timescale perspective
• Kinematic Lensing with the Roman Space Telescope
• Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• SWIFT: task-based hydrodynamics and gravity for cosmological simulations
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• Recent Observations of the Rotation of Distant Galaxies and the Implication for Dark Matter
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
• Precision Pollution - The effects of enrichment yields and timing on galactic chemical evolution
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• Jet-mode feedback in NGC 5972: insights from resolved MUSE, GMRT and VLA observations
• Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Probing the physical properties of the IGM using SRG/eROSITA spectra from blazars
• A systematic study of AGN feedback in a disk galaxy I: global overview
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (II) The inside-out growth of discs
• Dark matter haloes: a multistream view
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Rapid, out of equilibrium metal enrichment indicated by a flat mass-metallicity relation at z~6 from NIRCam grism spectroscopy
• Alignment between Satellite and Central Galaxies in the EAGLE Simulation: Dependence on the Large-Scale Environments
• A census of quiescent galaxies across $0.5<z<8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• An H$\alpha$ kinematic survey of the $Herschel$ Reference Survey -- I. Fabry-Perot observations with the 1.93m telescope at OHP
• Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
• Digging deeper into NGC\,6868 I: stellar population
• The Impact of Baryons on the Large-Scale Structure of the Universe
• The "Building Blocks" of Stellar Halos
• Panchromatic SED fitting codes and modelling techniques
• 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
• Modelling the selection of galaxy groups with end to end simulations
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Galaxy cluster photons alter the ionisation state of the nearby warm-hot intergalactic medium
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies
• Sensitivity analysis of a galaxy formation model
• Recovering the pattern speeds of edge-on barred galaxies via an orbit-superposition method
• Detection of the Intrinsic Spin Alignments in Isolated Spiral Pairs
• The building blocks of the Milky Way halo using APOGEE and Gaia -- or -- Is the Galaxy a typical galaxy?
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• The average structural evolution of massive galaxies can be reliably estimated using cumulative galaxy number densities
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• A Hybrid MPI+Threads Approach to Particle Group Finding Using Union-Find
• Cosmic filament spin -- I: a comparative study in observation
• 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
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Probing large-scale structures with the two-point function and the power spectrum: insights into cosmic clustering evolution
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• The effect of environment on the mass assembly history of the Milky Way and M31
• Resummed Kinetic Field Theory: a model of coupled baryonic and dark matter
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• A Global Census of Metals in the Universe
• Reconstructing the LISA massive black hole binary population via iterative kernel density estimation
• SEURAT: SPH scheme extended with ultraviolet line radiative transfer
• Refueled and shielded - The early evolution of Tidal Dwarf Galaxies
• Untangling Stellar Components of Galaxies: Evaluation of Dynamical Decomposition Methods in Simulated Galaxies with GalaxyChop
• Local variations of the Stellar Velocity Ellipsoid-II: the effect of the bar in the inner regions of Auriga galaxies
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• Evolution of thermal and nonthermal radio continuum emission on kpc scales--Predictions for SKA
• Massive Black Hole Mergers
• 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
• First resolved stellar halo kinematics of a MW-mass galaxy outside the Local Group: A flat counter-rotating halo in NGC 4945
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• Measuring the Substructure Mass Power Spectrum of 23 SLACS Strong Galaxy-Galaxy Lenses with Convolutional Neural Networks
• The influence of baryons on low-mass haloes
• Fast radio bursts as probes of feedback from active galactic nuclei
• Evolution of dwarf galaxy observable parameters
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Evolution of X-ray galaxy Cluster Properties in a Representative Sample (EXCPReS). Optimal binning for temperature profile extraction
• Spherical accretion of collisional gas in modified gravity I: self-similar solutions and a new cosmological hydrodynamical code
• The Dawn of Black Holes
• Total mass slopes and enclosed mass constrained by globular cluster system dynamics
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Using machine learning to study the kinematics of cold gas in galaxies
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• Exploring the Dependence of Gas Cooling and Heating Functions on the Incident Radiation Field with Machine Learning
• A correlation between accreted stellar kinematics and dark matter halo spin in the ARTEMIS simulations
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
• A new framework for understanding the evolution of early-type galaxies
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• Detection of an orthogonal alignment between parsec scale AGN jets and their host galaxies
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Ionized gas kinematics of massive elliptical galaxies in CALIFA and in cosmological zoom-in simulations
• The evolution of the barred galaxy population in the TNG50 simulation
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• Eigenmode analysis of perurbations in the primordial medium at and before recombination
• The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
• Constraining dark matter halo profiles with symbolic regression
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• A new strategy for matching observed and simulated lensing galaxies
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies
• Strong Evidence for Cosmic Ray-Supported $\sim$L${}^{\ast }$ Galaxy Halos via X-ray \& tSZ Constraints
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• Do AGN really suppress star formation?
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• The imprint of dark subhaloes on the circumgalactic medium
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• The Type Ia Supernova and Asymptotic Giant Branch Stellar Ejecta-regulated Interstellar Medium of Massive Galaxies
• Growth and Feedback from the First Black Holes
• Continuous Simulation Data Stream: A dynamical timescale-dependent output scheme for simulations
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• Impact of supermassive black hole growth on star formation
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• The role of magnetic fields in ram pressure stripping of satellite galaxies in the circumgalactic medium around massive galaxies
• Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Born to be Starless: Revisiting the Missing Satellite Problem
• Are there any extragalactic high speed dark matter particles in the Solar neighborhood?
• Distribution of Phantom Dark Matter in Dwarf Spheroidals
• The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• Following the crumbs: Statistical effects of Ram Pressure in Galaxies
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type galaxies
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Self-generated ultraviolet radiation in molecular shock waves I. Effects of Lyman $\alpha$, Lyman $\beta$, and two-photon continuum
• Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• A jet-driven bipolar outflow in NGC 1125
• MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z$\sim$2
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Spatial field reconstruction with INLA: Application to simulated galaxies
• The MeerKAT Fornax Survey VI. The collapse of the galaxy HI Mass Function in Fornax
• Dynamics of Companion Galaxies of Early-Type Galaxies
• A multi-ion non-equilibrium solver for ionised astrophysical plasmas with arbitrary elemental abundances
• The dynamical evolution of the stellar clumps in the Sparkler galaxy
• A MeerKAT study of a neutral hydrogen rich grouping of galaxies with megaparsec-scale filamentary-like structure
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• ALMA survey of a massive node of the Cosmic Web at $z\sim 3$. II. A dynamically cold and massive disk galaxy in the proximity of a hyperluminous quasar
• Environment matters: stronger magnetic fields in satellite galaxies
• Dust contribution to the panchromatic galaxy emission
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Dispersion Measures of Fast Radio Bursts through the Epoch of Reionization
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• Mapping Large-Scale-Structure Evolution over Cosmic Times
• The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
• Photometric and Kinematic Misalignments and Their Evolution Among Fast and Slow Rotators in the Illustris Simulation
• No dependence of radio properties of brightest group galaxies on the luminosity gap
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• Study of Central Intensity Ratio of Seyfert Galaxies in nearby Universe
• The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations
• Predicting far-infrared maps of galaxies via machine learning techniques
• Information divergences to parametrize astrophysical uncertainties in dark matter direct detection
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
• Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
• Shockingly Effective: Cluster Winds as Engines of Feedback in Starburst Galaxy VV 114
• Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
• Exploring the outskirts of the EAGLE disc galaxies
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Unsupervised Domain Adaptation for Constraining Star Formation Histories
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• The FLAMINGO simulations data release
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• The origin of galaxy scaling laws in LCDM
• HI asymmetries in spatially resolved SIMBA galaxies
• Bulgeless Evolution And the Rise of Discs (BEARD) II. The role of mergers in shaping the Milky Way analogues in TNG50
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Study of dependence of ram pressure stripping on the orbital parameters of the galaxies
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• The galaxy-environment connection revealed by constrained simulations
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Investigating chemical variations between interstellar gas clouds in the Solar neighbourhood
• Investigating the variability of Swift-BAT blazars with NICER
• Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
• Observed versus Simulated Halo c-Mvir Relations
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• The NewHorizon Simulation -- To Bar Or Not To Bar
• Low-luminosity galaxies in the early universe have observed sizes similar to star cluster complexes
• DESI Mg II Absorbers: Extinction Characteristics & Quasar Redshift Accuracy
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Baryon-driven decontraction in Milky Way mass haloes
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• The haloes that reionized the Universe
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
• Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
• Extended Hernquist-Springel formalism for cosmic star formation
• Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties
• The nature of the variable millimetre-selected AGN in the Brightest Cluster Galaxy of Abell 851
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• The multi-component fitting to the star formation histories in the TNG simulation
• Deciphering galaxy images using machine vision -- Combining variational autoencoder and principal component analysis for feature extraction
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
• Supermassive black holes in a mass-limited galaxy sample
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• Cosmological evolution of gas and supermassive black holes in idealized isolated halos
• Establishing the impact of powerful AGN on their host galaxies
• The intragroup light in KiDS+GAMA groups: A stacking analysis
• The long road to the Green Valley: Tracing the evolution of the Green Valley galaxies in the EAGLE simulation
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• Beyond mirkwood: Enhancing SED Modeling with Conformal Predictions
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• Constraining Galaxy-Halo Connection Using Machine Learning
• Assessment of Dark Matter Models Using Dark Matter Correlations across Dwarf Spheroidal Galaxies
• Search for Slow Bars in Two Barred Galaxies with Nuclear Structures: NGC 6951 and NGC 7716
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• On the signature of black holes on the quenched stellar mass function
• The physical properties and impact of AGN outflows from high to low redshift
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Environmental Invariance of the Galaxy Size-Mass Relation
• Testing the role of AGN on the star formation and metal enrichment of "twin galaxies"
• Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability
• Efficiency of parallel computations of gravitational forces by TreeCode method in N-body models
• Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Scaling relations of early-type galaxies in MOND
• Dipole Distortions in the Intergalactic Medium
• A Halo Merger Tree Generation and Evaluation Framework
• The APOSTLE simulations: Rotation curves derived from synthetic 21-cm observations
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• The Tremaine-Weinberg method at high redshifts
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• The intracluster light as an estimator of the cluster mass profile
• PHIBSS: Searching for Molecular Gas Outflows in Star-Forming Galaxies at $z=$ 0.5-2.6
• Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies
• MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Cluster environment quenches the star formation of low-mass satellite galaxies from the inside-out
• Gaia GraL: Gaia gravitational lens systems IX. Using XGBoost to explore the Gaia Focused Product Release GravLens catalogue
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• The Star Formation History of a Post-Starburst Galaxy Determined From Its Cluster Population
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Absorption systems at $z\sim 2$ as a probe of the circum galactic medium: a probabilistic approach
• Predicting halo occupation and galaxy assembly bias with machine learning
• Reduced Gas Accretion onto Galaxies due to Effects of External Giant Radio Lobes
• Resolved Neutral Outflow from a Lensed Dusty Star Forming Galaxy at z=2.09
• Hot accretion onto spiral galaxies: the origin of extended and warped HI discs
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Detection of HI filament: Pair Stacking vs. Filament Stacking
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Intermediate-mass black holes and contribution to extragalactic background light from Population III stars in Milky Way-like galaxies
• Mainly on the Plane: Observing the Extended, Ionized Disks of Milky Way Analogs in IllustrisTNG
• A Tilt in the Dark Matter Halo of the Galaxy
• 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
• Implication of a galaxy-scale negative feedback by one of the most powerful multi-phase outflows in a hyper-luminous infrared galaxy at the intermediate redshift
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Sensitivity to Axion-like Particle dark matter with very-high-energy gamma-ray observations of Active Galactic Nuclei located behind Galaxy Clusters
• The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra
• FEASTS and MHONGOOSE: HI Column Density Distribution at $z=0$ for $N_{\mathrm{HI}}>10^{17.8}{\mathrm{cm}}^{-2}$
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• Chemical evolution history of MaNGA galaxies
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Time-Dependent Cosmic Ray Halos from Bursty Star Formation and Active Galactic Nuclei: Semi-Analytic Formalism and Galaxy Formation Implications
• SDSS-IV MaNGA: Exploring the local scaling relations for N/O
• Relativistic Angular Redshift Fluctuations embedded in Large Scale Varying Gravitational Potentials
• The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Galaxies in the central regions of simulated galaxy clusters
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Bound or blown: the fate of hot gas in galaxy groups
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• Mocking IFU observations and metallicity diagnostics from cosmological simulations
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• The Scaling Relation between Galaxy Luminosity and WHIM Density from EAGLE Simulations with application to SDSS data
• The halo finding problem revisited: a deep revision of the ASOHF code
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• The MAGIC project. III. Radial and azimuthal Galactic abundance gradients using classical Cepheids
• Intrinsic alignments of galaxies in multiple projections
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• 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
• Baryon-photon interactions in Resummed Kinetic Field Theory
• Stellar halos of bright central galaxies II: Scaling relations, colors and metallicity evolution with redshift
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• The Galaxy Evolution Probe
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation
• Simulated X-ray Emission in Galaxy Clusters with Feedback from Active Galactic Nuclei
• X-ray Emission from the Interstellar and Circumgalactic Medium of Elliptical Galaxies based on MACER simulations
• Spatial disconnection between stellar and dust emissions: the test of the Antennae Galaxies (Arp 244)
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• Merger or Not: Accounting for Human Biases in Identifying Galactic Merger Signatures
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events
• Black Holes and Baryon Number Violation: Unveiling the Origins of Early Galaxies and the Low-Mass Gap
• On the hosts of neutron star mergers in the nearby Universe
• Combining LOFAR and Apertif Data for Understanding the Life Cycle of Radio Galaxies
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Deep Learning for Galaxy Mergers in the Galaxy Main Sequence
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• The stellar population of a $z\sim 3.25$ Ly$\alpha$ emitting group associated with a damped Ly$\alpha$ absorber
• The Metallicity Distribution Function in Outer Halo Fields of Simulated Elliptical Galaxies Compared to Observations of NGC 5128
• Ultra-fast model emulation with PRISM; analyzing the Meraxes galaxy formation model
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Insights into the structure and kinematics of a Milky Way-like galaxy
• Reconciling concentration to virial mass relations
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Modelling the outskirts of galaxies in a cosmological context
• Tidal Structures Around Edge-On Galaxies in Deep Imaging Surveys
• Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams
• Massive black holes and their galaxies
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Numerical Study of Bar Suppression in Galaxy Models Due to Disc Heating
• Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies
• Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation
• Determining the Dark Matter distribution in galaxies with Deep Learning
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Estimating Transient Rates from Cosmological Simulations and BPASS
• 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
• Debunking Generalization Error or: How I Learned to Stop Worrying and Love My Training Set
• Dark Matter profiles of "in silico" galaxies: deep learning inference
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
• Testing subhalo abundance matching with galaxy kinematics
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• The link between star formation and gas in nearby galaxies
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• Beyond single tracers: CNN-based inference of galaxy mass profiles from combined gas and stellar kinematics
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• Understanding the Galaxy
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• The miniJPAS survey quasar selection I: Mock catalogues for classification
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window