Cosmological SPH simulations: A hybrid multi-phase model for star formation

Abstract

We present a model for star formation and supernova feedback that describes the multi-phase structure of star forming gas on scales that are typically not resolved in cosmological simulations. Our approach includes radiative heating and cooling, the growth of cold clouds embedded in an ambient hot medium, star formation in these clouds, feedback from supernovae in the form of thermal heating and cloud evaporation, galactic winds and outflows, and metal enrichment. Implemented using SPH, our scheme is a significantly modified and extended version of the grid-based method of Yepes et al. (1997), and enables us to achieve high dynamic range in simulations of structure formation. We discuss properties of the feedback model in detail and show that it predicts a self-regulated, quiescent mode of star formation, which, in particular, stabilises the star forming gaseous layers of disk galaxies. The parameterisation of this mode can be reduced to a single free quantity which determines the overall timescale for star formation. We fix this parameter to match the observed rates of star formation in local disk galaxies. When normalised in this manner, cosmological simulations nevertheless overproduce the observed cosmic abundance of stellar material. We are thus motivated to extend our feedback model to include galactic winds associated with star formation. Using small-scale simulations of individual star-forming disk galaxies, we show that these winds produce either galactic fountains or outflows, depending on the depth of the gravitational potential. Moreover, outflows from galaxies in these simulations drive chemical enrichment of the intergalactic medium, in principle accounting for the presence of metals in the Lyman alpha forest. (abridged)

submitted to MNRAS, 25 pages, version with high-resolution figures available at http://www.mpa-garching.mpg.de/~volker/paper_multiphase/

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• The interplay between chemical and mechanical feedback from the first generation of stars
• A Detailed Study of Feedback from a Massive Star
• The Growth of Massive Black Holes in Galaxy Merger Simulations with Feedback by Radiation Pressure
• How to distinguish starbursts and quiescently star-forming galaxies: The `bimodal' submillimetre galaxy population as a case study
• Molecular Star Formation Rate Indicators in Galaxies
• Forming disk galaxies in wet major mergers. I. Three fiducial examples
• Orbital structure of merger remnants: Trends with gas fraction in 1:1 mergers
• Shape of Dark Matter Haloes in the Illustris Simulation: Effects of Baryons
• Galaxy-Scale Outflows Driven by Active Galactic Nuclei
• Should we believe the results of UV-mm galaxy SED modelling?
• The diverse evolutionary paths of simulated high-z massive, compact galaxies to z=0
• Dwarf galaxy formation with H2-regulated star formation
• Moving Mesh Cosmology: Properties of Gas Disks
• Atomic and molecular gas in IllustrisTNG galaxies at low redshift
• Investigating the velocity structure and X-ray observable properties of simulated galaxy clusters with PHOX
• The Evolution in the Faint-End Slope of the Quasar Luminosity Function
• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• High-J CO Versus Far-Infrared Relations in Normal and Starburst Galaxies
• The History of Cosmological Star Formation: Three Independent Approaches and a Critical Test Using the Extragalactic Background Light
• The MUSIC of Galaxy Clusters I: Baryon properties and Scaling Relations of the thermal Sunyaev-Zel'dovich Effect
• Can Gas prevent the Destruction of Thin Stellar Discs by Minor Mergers?
• Hydrogen and Metal Line Absorption Around Low-Redshift Galaxies in Cosmological Hydrodynamic Simulations
• Characterizing Diffused Stellar Light in simulated galaxy clusters
• Galactic and Circumgalactic OVI and its Impact on the Cosmological Metal and Baryon Budgets at 2<z<3.5
• AREPO-RT: Radiation hydrodynamics on a moving mesh
• Simulating galactic dust grain evolution on a moving mesh
• Simulating Star Formation and Feedback in Galactic Disk Models
• Radiative Stellar Feedback in Galaxy Formation: Methods and Physics
• Ionizing radiation fluctuations and large-scale structure in the Lyman-alpha forest
• Modeling baryonic physics in future weak lensing surveys
• A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations
• The Origins of AGN Obscuration: The 'Torus' as a Dynamical, Unstable Driver of Accretion
• Simulations of cosmic ray feedback by AGN in galaxy clusters
• On the formation of dwarf galaxies and stellar halos
• Zooming in on accretion - I. The structure of halo gas
• Black Hole-Galaxy Correlations without Self-Regulation
• AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
• ACCESS - V. Dissecting ram-pressure stripping through integral-field spectroscopy and multi-band imaging
• The universal distribution of halo interlopers in projected phase space. Bias in galaxy cluster concentration and velocity anisotropy?
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• Hot gas in massive halos drives both mass quenching and environment quenching
• The influence of non-uniform reionization on the CMB
• The effects of baryons on the halo mass function
• The stellar accretion origin of stellar population gradients in massive galaxies at large radii
• From Starburst to Quiescence: Testing AGN feedback in Rapidly Quenching Post-Starburst Galaxies
• The modelling of feedback in star formation simulations
• Cosmic ray-driven galactic winds: streaming or diffusion?
• Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution
• Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: cosmological implications
• Galaxy Shapes and Intrinsic Alignments in The MassiveBlack-II Simulation
• Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution
• The photoheating of the intergalactic medium in synthesis models of the UV background
• The baryon fraction in hydrodynamical simulations of galaxy clusters
• Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
• An observer's view of simulated galaxies: disc-to-total ratios, bars, and (pseudo-)bulges
• Zooming in on major mergers: dense, starbursting gas in cosmological simulations
• A Constrained-Gradient Method to Control Divergence Errors in Numerical MHD
• Thermal conduction in cosmological SPH simulations
• The Physical and Photometric Properties of High-Redshift Galaxies in Cosmological Hydrodynamic Simulations
• Recovering Stellar Population Properties and Redshifts from Broad-Band Photometry of Simulated Galaxies: Lessons for SED Modeling
• Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
• The Impact of Galactic Feedback on the Circumgalactic Medium
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys III: Measurement Biases and Cosmological Evolution of Gas and Stellar Mass Fractions
• Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies
• The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
• The assembly of dusty galaxies at $z\ge 4$: statistical properties
• The Collision Between The Milky Way And Andromeda
• A Deep Search For Faint Galaxies Associated With Very Low-redshift C IV Absorbers: III. The Mass- and Environment-dependent Circumgalactic Medium
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• Heart of Darkness: the influence of galactic dynamics on quenching star formation in galaxy spheroids
• In a hot bubble: why does superbubble feedback work, but isolated supernovae do not?
• Star Formation in Isolated Disk Galaxies. I. Models and Characteristics of Nonlinear Gravitational Collapse
• The effect of AGN feedback on the halo mass function
• Double-peaked Narrow-Line Signatures of Dual Supermassive Black Holes in Galaxy Merger Simulations
• Simulated X-ray galaxy clusters at the virial radius: slopes of the gas density, temperature and surface brightness profiles
• X-ray mass proxies from hydrodynamic simulations of galaxy clusters (paper I)
• X-ray Emission from Hot Gas in Galaxy Mergers
• The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization
• Spatially resolved star formation and fuelling in galaxy interactions
• How is Star Formation Quenched in Massive Galaxies?
• Dissipation and the Fundamental Plane: Observational Tests
• The Enrichment History of Baryons in the Universe
• The origin of most massive black holes at high-z: BLUETIDES and the next quasar frontier
• The physics of multiphase gas flows: fragmentation of a radiatively cooling gas cloud in a hot wind
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• The Dependence of the Occupation of Galaxies on the Halo Formation Time
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• Tracing the Reionization-Epoch Intergalactic Medium with Metal Absorption Lines
• Self-Regulated Black Hole Growth via Momentum Deposition in Galaxy Merger Simulations
• The simulated 21 cm signal during the epoch of reionization : full modeling of the Ly-alpha pumping
• Pressure of the hot gas in simulations of galaxy clusters
• How galaxies form stars: the connection between local and global star formation in galaxy simulations
• Chemical evolution of galaxies. I. A composition-dependent SPH model for chemical evolution and cooling
• A survey of dual active galactic nuclei in simulations of galaxy mergers: frequency and properties
• Galaxy mergers on a moving mesh: a comparison with smoothed-particle hydrodynamics
• Gone after one orbit: How cluster environments quench galaxies
• The effect of magnetic fields on properties of the circumgalactic medium
• The Nature of Sub-millimetre Galaxies in Cosmological Hydrodynamic Simulations
• Abundance of damped Lyman-alpha absorbers in cosmological SPH simulations
• Efficient early stellar feedback can suppress galactic outflows by reducing supernova clustering
• The evolution of Black Hole scaling relations in galaxy mergers
• Scaling Relations of Dwarf Galaxies without Supernova-Driven Winds
• The imprints of local superclusters on the Sunyaev-Zel'dovich signals and their detectability with Planck
• Entropy amplification from energy feedback in simulated galaxy groups and clusters
• MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
• The imprint of neutrinos on clustering in redshift-space
• Observing the Reionization Epoch Through 21 Centimeter Radiation
• When did Population III star formation end?
• The Dark Halo - Spheroid Conspiracy and the Origin of Elliptical Galaxies
• Interpreting the Evolution of the Size - Luminosity Relation for Disk Galaxies from Redshift 1 to the Present
• The history of chemical enrichment in the intracluster medium from cosmological simulations
• Satellite Systems around Galaxies in Hydrodynamic Simulations
• The Origin and Evolution of Fast and Slow Rotators in the Illustris Simulation
• The Star-Forming Molecular Gas in High Redshift Submillimeter Galaxies
• Simulation techniques for cosmological simulations
• Kinematics of Simulated Galaxies I: Connecting Dynamical and Morphological Properties of Early-Type Galaxies at Different Redshifts
• Gas-phase metallicity gradients of TNG50 star-forming galaxies
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• Powering galactic super-winds with small-scale AGN winds
• Chaos and Variance in Galaxy Formation
• The Growth of Red Sequence Galaxies in a Cosmological Hydrodynamic Simulation
• Star formation rate and metallicity of damped Lyman-alpha absorbers in cosmological SPH simulations
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• How Much Mass do Supermassive Black Holes Eat in their Old Age?
• 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
• Constrained simulations of the Local Group: on the radial distribution of substructures
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• Connecting stellar mass and star-formation rate to dark matter halo mass out to z ~ 2
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations
• Disassembling the Galaxy with angle-action coordinates
• Large-scale inhomogeneities of the intracluster medium: improving mass estimates using the observed azimuthal scatter
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• The Self-Regulated Growth of Supermassive Black Holes
• The Dynamical and Chemical Evolution of Dwarf Spheroidal Galaxies with GEAR
• High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM
• The MillenniumTNG Project: The galaxy population at $z\ge 8$
• The impact of radio feedback from active galactic nuclei in cosmological simulations: Formation of disk galaxies
• Outflows and complex stellar kinematics in SDSS star forming galaxies
• Signatures of Galactic Superwinds: Inhomogeneous Metal Enrichment of the Lyman Alpha Forest
• The formation and evolution of bars in low surface brightness galaxies with cold dark matter halos
• The Azimuthal Dependence of Outflows and Accretion Detected Using OVI Absorption
• What is the (Dark) Matter with Dwarf Galaxies?
• Formation history, structure and dynamics of discs and spheroids in simulated Milky Way mass galaxies
• Torque-Limited Growth of Massive Black Holes in Galaxies Across Cosmic Time
• The Physical Properties and Detectability of Reionization-Epoch Galaxies
• Star Formation Feedback and Metal Enrichment History Of The Intergalactic Medium
• The Effect of the Interstellar Model on Star Formation Properties in Galactic Disks
• Legacy of star formation in the pre-reionization universe
• The Outer Stellar Halos of Galaxies: how Radial Merger Mass Deposition, Shells and Streams depend on Infall-Orbit Configurations
• On the Assembly of Dwarf Galaxies in Clusters and their Efficient Formation of Globular Clusters
• The effect of feedback and reionization on star formation in low-mass dwarf galaxy haloes
• On the nature of the ring-like structure in the outer Galactic disk
• Origin of strong magnetic fields in Milky-Way like galactic haloes
• Fashionably Late? Building up the Milky Way's Inner Halo
• The effects of a hot gaseous halo in galaxy major mergers
• The impact of supernovae driven winds on stream-fed protogalaxies
• Large-scale mass distribution in the Illustris simulation
• High-Redshift Galaxy Kinematics: Constraints on Models of Disk Formation
• The impact of gas physics on strong cluster lensing
• nIFTy galaxy cluster simulations I: dark matter & non-radiative models
• The Tau of Galaxy Clusters
• The dependence of cosmic ray driven galactic winds on halo mass
• A Systematic Look at the Effects of Radiative Feedback on Disc Galaxy Formation
• Resolving the high redshift Lyman-alpha forest in smoothed particle hydrodynamics simulations
• The Kinematic Sunyaev-Zel'dovich Effect with Projected Fields II: prospects, challenges, and comparison with simulations
• Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes. I: Feedback-regulated Star Formation and Black Hole Growth
• On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• Preheating by Previrialization and its Impact on Galaxy Formation
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• X-ray bubbles in the circumgalactic medium of TNG50 Milky Way- and M31-like galaxies: signposts of supermassive black hole activity
• Fast cold gas in hot AGN outflows
• Intrinsic alignments of galaxies in the MassiveBlack-II simulation: analysis of two-point statistics
• On the nature of the barlens component in barred galaxies: what do boxy/peanut bulges look like when viewed face-on?
• Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Constraints on Physical Properties of z~6 Galaxies Using Cosmological Hydrodynamic Simulations
• Log-normal star formation histories in simulated and observed galaxies
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• Physical viscosity in smoothed particle hydrodynamics simulations of galaxy clusters
• Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies
• Merger-Induced Metallicity Dilution in Cosmological Galaxy Formation Simulations
• Fully compressive tides in galaxy mergers
• Star Formation in Isolated Disk Galaxies. II. Schmidt Laws and Efficiency of Gravitational Collapse
• Temperature Structure of the Intra-Cluster Medium from SPH and AMR simulations
• Periodic bursts of Star Formation in Irregular Galaxies
• A dynamical model of supernova feedback: gas outflows from the interstellar medium
• Quenching Massive Galaxies with On-the-fly Feedback in Cosmological Hydrodynamic Simulations
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• Buried AGNs in Advanced Mergers:Mid-infrared color selection as a dual AGN finder
• Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
• Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies II: The Effects of Star Formation Feedback
• Baryon Cycling in the Low-Redshift Circumgalactic Medium: A Comparison of Simulations to the COS-Halos Survey
• Consequences of Mechanical and Radiative Feedback from Black Holes in Disc Galaxy Mergers
• QSO Absorption Systems Detected in Ne VIII: High-Metallicity Clouds with a Large Effective Cross Section
• X-MAS2: Study Systematics on the ICM Metallicity Measurements
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• Damped Lyman-alpha systems in high-resolution hydrodynamical simulations
• 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
• Mergers and the outside-in formation of dwarf spheroidals
• The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• A first direct measurement of the intergalactic medium temperature around a quasar at z=6
• Population III stars and the Long Gamma Ray Burst rate
• Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
• Magnetising the circumgalactic medium of disk galaxies
• The physics of gas phase metallicity gradients in galaxies
• Interacting galaxies in the IllustrisTNG simulations -- II: Star formation in the post-merger stage
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• Luminosity-Dependent Quasar Lifetimes: Reconciling the Optical and X-ray Quasar Luminosity Functions
• The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data
• The GalMer database: Galaxy Mergers in the Virtual Observatory
• Steep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 and the Implications for Reionisation
• Early Structure Formation and Reionization in a Cosmological Model with a Running Primordial Power Spectrum
• Star formation in shocked cluster spirals and their tails
• CLASSY III: The Properties of Starburst-Driven Warm Ionized Outflows
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• Dynamical difference between the cD galaxy and the stellar diffuse component in simulated galaxy clusters
• An Extreme Metallicity, Large-Scale Outflow from a Star-Forming Galaxy at z ~ 0.4
• The THESAN project: ionizing escape fractions of reionization-era galaxies
• Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
• An N-body/SPH Study of Isolated Galaxy Mass Density Profiles
• Properties of HI discs in the Auriga cosmological simulations
• Galaxy morphology, kinematics and clustering in a hydrodynamic simulation of a LambdaCDM universe
• The Last Eight-Billion Years of Intergalactic CIV Evolution
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• Dynamical Friction Modeling of Massive Black Holes in Cosmological Simulations and Effects on Merger Rate Predictions
• Enrichment and Pre-Heating in Intragroup Gas from Galactic Outflows
• Reionization in Technicolor
• Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at $z$$\sim$2
• Properties of the galaxy population in hydrodynamical simulations of clusters
• Non-linear evolution of the cosmic neutrino background
• One moment in time - modeling star formation in the Antennae
• The evolution of the star formation rate function in the EAGLE simulations: A comparison with UV, IR and H$\alpha$ observations from z ~ 8 to z ~ 0
• Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
• Hot and Cooled baryons in SPH simulations of galaxy clusters: physics and numerics
• NGC6240: Merger-Induced Star Formation & Gas Dynamics
• Evolution at z>0.5 of the X-ray properties of simulated galaxy clusters: comparison with the observational constraints
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• The Lyman-alpha forest in a blazar-heated Universe
• Lyman-alpha Emitters and Lyman-break Galaxies at z=3-6 in Cosmological SPH Simulations
• Cosmic ray feedback from supernovae in dwarf galaxies
• Faint Submillimeter Galaxies Revealed by Multifield Deep ALMA Observations: Number Counts, Spatial Clustering, and A Dark Submillimeter Line Emitter
• $R$-process enhancements of Gaia-Enceladus in GALAH DR3
• The evolution of galaxies from primeval irregulars to present-day ellipticals
• X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations
• SZE Observables, Pressure Profiles and Center Offsets in Magneticum Simulation Galaxy Clusters
• The buildup of strongly barred galaxies in the TNG100 simulation
• The THESAN project: predictions for multi-tracer line intensity mapping in the epoch of reionization
• Stellar Halo Constraints on Simulated Late Type Galaxies
• Escape of Lyman-alpha and continuum photons from star-forming galaxies
• A Total Molecular Gas Mass Census in z~2-3 Star-forming Galaxies: Low-J CO Excitation Probes of Galaxies' Evolutionary States
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• A Comparative Study of AGN Feedback Algorithms
• On the linearity of tracer bias around voids
• GMASS Ultradeep Spectroscopy of Galaxies at redshift z~2. I. The stellar metallicity
• Constraining Cosmic Rays and Magnetic Fields in the Perseus Galaxy Cluster with TeV observations by the MAGIC telescopes
• SPHRAY: A Smoothed Particle Hydrodynamics Ray Tracer for Radiative Transfer
• On the morphologies, gas fractions, and star formation rates of small galaxies
• Simulations of Dust in Interacting Galaxies I: Dust Attenuation
• Gravitational waves from Population III binary black holes formed by dynamical capture
• A Fluid-Dynamical Subgrid Scale Model for Highly Compressible Astrophysical Turbulence
• The angular momentum of cold dark matter haloes with and without baryons
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• Modeling the Dust Properties of z ~ 6 Quasars with ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree
• Metal enrichment processes
• Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN
• Active Galactic Nucleus Pairs from the Sloan Digital Sky Survey. II. Evidence for Tidally Enhanced Star Formation and Black Hole Accretion
• Semi-implicit anisotropic cosmic ray transport on an unstructured moving mesh
• LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars
• Constraints on the CMB Temperature Evolution using Multi-Band Measurements of the Sunyaev Zel'dovich Effect with the South Pole Telescope
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• Interpreting the observed UV continuum slopes of high-redshift galaxies
• Star formation rates and mass distributions in interacting galaxies
• Gamma-ray burst rate: high-redshift excess and its possible origins
• SAURON's Challenge for the Major Merger Scenario of Elliptical Galaxy Formation
• Why Are AGN and Host Galaxies Misaligned?
• Momentum transfer across shear flows in Smoothed Particle Hydrodynamic simulations of galaxy formation
• Distribution of Damped Lyman-alpha Absorbers in a Lambda Cold Dark Matter Universe
• Massive galaxies & EROs at z=1-3 in cosmological hydrodynamic simulations: near-IR properties
• Lyman Alpha Emitter Evolution in the Reionization Epoch
• Simulating the assembly of galaxies at redshifts z = 6 - 12
• A sub-resolution multiphase interstellar medium model of star formation and SNe energy feedback
• QSO obscuration at high redshift ($z\gtrsim 7$): Predictions from the BlueTides simulation
• Clues for the origin of the fundamental metallicity relations. I: The hierarchical building up of the structure
• Linking bar- and interaction-driven molecular gas concentration with centrally-enhanced star formation in EDGE-CALIFA galaxies
• Simulating Chandra observations of galaxy clusters
• The Three Hundred Project: correcting for the hydrostatic-equilibrium mass bias in X-ray and SZ surveys
• On the influence of ram-pressure stripping on interacting galaxies in clusters
• Lyman Alpha Emitters and Lyman Break Galaxies: dichotomous twins?
• Cosmological HII Bubble Growth During Reionization
• ART^2 : Coupling Lyman-alpha Line and Multi-wavelength Continuum Radiative Transfer
• The CAMELS project: public data release
• Multi-wavelength Cosmological Simulations of Elliptical Galaxies
• Weighing neutrinos with cosmic neutral hydrogen
• The impact of feedback on the low redshift Intergalactic Medium
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Tracing Outflowing Metals in Simulations of Dwarf and Spiral Galaxies
• Faraday rotation maps of disk galaxies
• The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
• Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations
• The DIANOGA simulations of galaxy clusters: characterizing star formation in proto-clusters
• The origin of pseudobulges in cosmological simulations of galaxy formation
• Galaxy shapes and alignments in the MassiveBlack-II hydrodynamic and dark matter-only simulations
• Quasar outflows at $z\ge 6$: the impact on the host galaxies
• Galactic Winds and Extended Lya Emission from the Host Galaxies of High Column Density QSO Absorption Systems
• The impact of AGN feedback and baryonic cooling on galaxy clusters as gravitational lenses
• Cosmological Feedback from High-Redshift Dwarf Galaxies
• Simulating Gamma-ray Emission in Star-forming Galaxies
• Inhomogeneous extragalactic magnetic fields and the second knee in the cosmic ray spectrum
• Is There a Missing Galaxy Problem at High Redshift?
• Galactic Simulations of r-process Elemental Abundances
• The chemical enrichment of the ICM from hydrodynamical simulations
• Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• The Simulated HI Sky at low redshift
• Remodeling the evolution of grain size distribution in galaxies
• Comprehensive Broadband X-ray and Multiwavelength Study of Active Galactic Nuclei in Local 57 Ultra/luminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT
• The Epoch of IGM heating by early sources of X-rays
• Magnetised winds in dwarf galaxies
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- I: Halo Gas Properties and the Role of SMBH Feedback
• The baryonic Tully-Fisher relation and galactic outflows
• How AGN feedback and metal cooling shape cluster entropy profiles
• Resolving The Generation of Starburst Winds in Galaxy Mergers
• How the super-Eddington regime regulates black hole growth in high-redshift galaxies
• Intrinsic alignments of disk and elliptical galaxies in the MassiveBlack-II and Illustris simulations
• Numerical resolution limits on subhalo abundance matching
• Local Group Dwarf Galaxies: Nature And Nurture
• Physics of Galactic Metals: Evolutionary Effects due to Production, Distribution, Feedback & Interaction with Black Holes
• Confronting cosmological simulations with observations of intergalactic metals
• Gravitational recoils of supermassive black holes in hydrodynamical simulations of gas rich galaxies
• A Framework for Multiphase Galactic Wind Launching using TIGRESS
• The prevalence of pseudo-bulges in the Auriga simulations
• Seeding Black Holes in Cosmological Simulations
• Simulating high-z Gamma-ray Burst host galaxies
• The Clustering of AGN in the Sloan Digital Sky Survey
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• The Impact of Galactic Winds on the Angular Momentum of Disk Galaxies in the Illustris Simulation
• AGN contamination of galaxy-cluster thermal X-ray emission: predictions for eRosita from cosmological simulations
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• On the Origin of Dynamically Cold Rings Around the Milky Way
• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
• A new population of recently quenched elliptical galaxies in the SDSS
• nIFTy galaxy cluster simulations II: radiative models
• BCG Mass Evolution in Cosmological Hydro-Simulations
• A Characteristic Mass Scale in the Mass-Metallicity Relation of Galaxies
• The Small Scatter in BH-Host Correlations & The Case for Self-Regulated BH Growth
• Kinetic AGN Feedback Effects on Cluster Cool Cores Simulated using SPH
• The luminosities of backsplash galaxies in constrained simulations of the Local Group
• Joint analysis of anisotropic power spectrum, bispectrum and trispectrum: application to N-body simulations
• Accurate Identification of Galaxy Mergers with Imaging
• Shapley Supercluster Survey: Ram-Pressure Stripping vs. Tidal Interactions in the Shapley Supercluster
• The Magellanic Corona and the formation of the Magellanic Stream
• A three-phase amplification of the cosmic magnetic field in galaxies
• Evaluating Galactic Habitability Using High Resolution Cosmological Simulations of Galaxy Formation
• The Baryons in the Milky Way Satellites
• The impact of baryonic physics on the shape and radial alignment of substructures in cosmological dark matter haloes
• The Magellanic Stream at 20 kpc: A New Orbital History for the Magellanic Clouds
• Intensity mapping with SDSS/BOSS Lyman-alpha emission, quasars and their Lyman-alpha forest
• Observing simulated galaxy clusters with PHOX: a novel X-ray photon simulator
• The resolved star-formation relation in nearby active galactic nuclei
• Massive galaxies in cosmological simulations: UV-selected sample at redshift z=2
• Physical regimes for feedback in galaxy formation
• Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• Interpreting the evolution of galaxy colours from $z=8$ to $z=5$
• Photometric Properties of Lyman-break Galaxies at z=3 in Cosmological SPH Simulations
• Simulating the 21-cm signal from reionisation including non-linear ionisations and inhomogeneous recombinations
• Galaxy Mergers with Adaptive Mesh Refinement: Star Formation and Hot Gas Outflow
• Moving mesh cosmology: properties of neutral hydrogen in absorption
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• The Three Hundred Project: The evolution of galaxy cluster density profiles
• Assessing the Jeans Anisotropic Multi-Gaussian Expansion method with the Illustris simulation
• XMM-Newton study of 0.012<z<0.024 groups. I: Overview of the IGM thermodynamics
• Metal enrichment of the intra-cluster medium over a Hubble time for merging and relaxed galaxy clusters
• Warm dark matter signatures on the 21cm power spectrum: Intensity mapping forecasts for SKA
• The effect of variations in the input physics on the cosmic distribution of metals predicted by simulations
• The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations
• Cosmological Zoom Simulations of z = 2 Galaxies: The Impact of Galactic Outflows
• Cosmic rays and non-thermal emission in simulated galaxies: III. probing cosmic ray calorimetry with radio spectra and the FIR-radio correlation
• Testing Subhalo Abundance Matching in Cosmological Smoothed Particle Hydrodynamics Simulations
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• Relationship between the Metallicity of the Circumgalactic Medium and Galaxy Orientation
• Metallicity-dependendent kinematics and morphology of the Milky Way bulge
• Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
• The Three Hundred Project: Ram pressure and gas content of haloes and subhaloes in the phase-space plane
• Inflow velocities of cold flows streaming into massive galaxies at high redshifts
• Systematic study of outflows in the Local Universe using CALIFA: I. Sample selection and main properties
• Impact of H_2-based star formation model on the z>=6 luminosity function and the ionizing photon budget for reionization
• Dust Evolution in Galaxy Cluster Simulations
• Exploring the magnetized cosmic web through low frequency radio emission
• Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
• Kinetic or thermal AGN feedback in simulations of isolated and merging disk galaxies calibrated by the M-sigma relation
• On the Dynamical Origin of the ICM Metallicity Evolution
• Effects of simulated cosmological magnetic fields on the galaxy population
• Stellar Halos in Illustris- Probing the Histories of Milky Way-Mass Galaxies
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far infrared-radio correlation
• The structure of gravitationally unstable gas-rich disk galaxies
• Models of Tidally Induced Gas Filaments in the Magellanic Stream
• The merger-driven evolution of warm infrared luminous galaxies
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Kinetic energy from supernova feedback in high-resolution galaxy simulations
• Properties of simulated galaxies and supermassive black holes in cosmic voids
• Vast planes of satellites in a high resolution simulation of the Local Group: comparison to Andromeda
• Strong magnetic fields and large rotation measures in protogalaxies by supernova seeding
• The cool side of Lyman Alpha Emitters
• Joint deprojection of Sunyaev-Zeldovich and X-ray images of galaxy clusters
• Accurate mass and velocity functions of dark matter halos
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• How well do cosmological simulations reproduce individual-halo properties?
• Weak-Lensing Mass Calibration of the Atacama Cosmology Telescope Equatorial Sunyaev-Zeldovich Cluster Sample with the Canada-France-Hawaii Telescope Stripe 82 Survey
• Reconstructing mass profiles of simulated galaxy clusters by combining Sunyaev-Zeldovich and X-ray images
• Merger induced scatter and bias in the cluster mass - Sunyaev-Zeldovich effect scaling relation
• Planck intermediate results. VIII. Filaments between interacting clusters
• The splashback boundary of haloes in hydrodynamic simulations
• Galaxy Pairs in the Sloan Digital Sky Survey - X: Does gas content alter star formation rate enhancement in galaxy interactions?
• A fundamental test for stellar feedback recipes in galaxy simulations
• The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
• Galaxies undergoing ram-pressure stripping: the influence of the bulge on morphology and star formation rate
• Baryonic effects on the matter bispectrum
• Origin and evolution of ultra-diffuse galaxies in different environments
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• Intermediate-Mass Black Hole Growth and Feedback in Dwarf Galaxies at High Redshifts
• Cosmic rays and non-thermal emission in simulated galaxies. II. $\gamma$-ray maps, spectra and the far infrared-$\gamma$-ray relation
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
• Lyman Break Galaxies at z = 4 - 6 in cosmological SPH Simulations
• Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies
• Galactic Winds in Cosmological Simulations of the Circumgalactic Medium
• Gravitational Lensing Statistics in Universes Dominated by Dark Energy
• Alignment between filaments and galaxy spins from the MaNGA integral-field survey
• Duty Cycle and the Increasing Star Formation History of z>=6 Galaxies
• Formation of an extended stellar halo around an ultra-faint dwarf galaxy following one of the earliest mergers from galactic building blocks
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• The impact of galaxy formation on X-ray groups
• Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
• Strong Calcium Emission Indicates that the Ultraviolet-Flashing Type Ia SN 2019yvq was the Result of a Sub-Chandrasekhar Mass Double-Detonation Explosion
• Matter trispectrum: theoretical modelling and comparison to N-body simulations
• Cosmic evolution of the CIV in high-resolution hydrodynamic simulations
• nIFTy Galaxy Cluster simulations IV: Quantifying the Influence of Baryons on Halo Properties
• Forced turbulence in thermally bistable gas: A parameter study
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• High redshift supermassive blackholes: accretion through cold flows
• Searching for Star Formation Beyond Reionization
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• The assembly of dusty galaxies at $z\ge 4$: the build-up of stellar mass and its scaling relations with hints from early JWST data
• Effect of radiative transfer on damped Lyman-alpha and Lyman limit systems in cosmological SPH simulations
• Probing the star formation history using the redshift evolution of luminosity functions
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts
• Disk settling and dynamical heating: histories of Milky Way-mass stellar disks across cosmic time in the FIRE simulations
• Resolving flows around black holes: numerical technique and applications
• Color Distributions, Number and Mass Densities of Massive Galaxies at 1.5 < z < 3: Comparing Observations with Merger Simulations
• Dust evolution in zoom-in cosmological simulations of galaxy formation
• The Late Reionization of Filaments
• On the origin of star-gas counterrotation in low-mass galaxies
• The Reionization of Carbon
• The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
• On the origin of the mass-metallicity gradient relation in the local Universe
• AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
• The MUSIC of Galaxy Clusters II: X-ray global properties and scaling relations
• Modelling the Transfer Function for the Dark Energy Survey
• Imprints of temperature fluctuations on the $z\sim 5$ Lyman-$\alpha$ forest: a view from radiation-hydrodynamic simulations of reionization
• Fully cosmological virtual massive galaxies at z=0: kinematical, morphological, and stellar population characterisation
• The origin of the enhanced metallicity of satellite galaxies
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• Cosmological baryon transfer in the SIMBA simulations
• Star formation from dense shocked regions in supersonic isothermal magneto-turbulence
• A simple model linking galaxy and dark matter evolution
• Galaxies going MAD: The Galaxy-Finder Comparison Project
• Too small to succeed? Lighting up massive dark matter subhaloes of the Milky Way
• Investigating Galaxy-Filament Alignments in Hydrodynamic Simulations using Density Ridges
• The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
• Size matters: the non-universal density profile of subhaloes in SPH simulations and implications for the Milky Way's dSphs
• Large scale simulations of H and He reionization and heating driven by stars and more energetic sources
• Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping
• Signatures of the M31-M32 Galactic Collision
• SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• The imprint of dissipation on the shapes of merger remnant LOSVDs
• Evolution of Galactic Outflows at $z\sim 0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra
• Momentum feedback from marginally-resolved HII regions in isolated disc galaxies
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• An Evolutionary Model For Submillimeter Galaxies
• Hot Galactic Winds Constrained by the X-Ray Luminosities of Galaxies
• Star-formation efficiency and metal enrichment of the intracluster medium in local massive clusters of galaxies
• The Nature of CO Emission From z~6 Quasars
• Enrichment of the hot intracluster medium: numerical simulations
• The Formation of Galaxies Hosting z~6 Quasars
• Thermodynamical properties of the ICM from hydrodynamical simulations
• Cosmological Implications of a Stellar Initial Mass Function that Varies with the Jeans Mass in Galaxies
• On the Discrepancy between Theoretical and X-Ray Concentration-Mass Relations for Galaxy Clusters
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• New multi-zoom method for N-body simulations: application to galaxy growth by accretion
• The effect of baryons in the cosmological lensing PDFs
• The Growth and Enrichment of the Intragroup Gas
• Robust Field-level Likelihood-free Inference with Galaxies
• Cosmic rays and non-thermal emission in simulated galaxies. I. Electron and proton spectra compared to Voyager-1 data
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• Efficacy of early stellar feedback in low gas surface density environments
• Stellar orbits in cosmological galaxy simulations: the connection to formation history and line-of-sight kinematics
• Studying the WHIM with Gamma Ray Bursts
• The cold circumgalactic medium in emission: MgII halos in TNG50
• The visibility of Lyman Alpha Emitters: constraining reionization, ionizing photons and dust
• Properties of the diffuse X-ray background in a high-resolution hydrodynamical simulation
• Using dwarf satellite proper motions to determine their origin
• Great Balls of FIRE I: The formation of star clusters across cosmic time in a Milky Way-mass galaxy
• Metals in the z~3 intergalactic medium: results from an ultra-high signal-to-noise ratio UVES quasar spectrum
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• Satellite dwarf galaxies: Stripped but not quenched
• Simulating magnetic fields in the Antennae galaxies
• Exploring 21cm - Lyman Alpha emitter synergies for SKA
• Effects of Ultraviolet Background and Local Stellar Radiation on the H_I Column Density Distribution
• The Mice at play in the CALIFA survey: A case study of a gas-rich major merger between first passage and coalescence
• The structure of cosmic voids in a LCDM Universe
• The Host Halos of OI Absorbers in the Reionization Epoch
• An Investigation of intra-cluster light evolution using cosmological hydro-dynamical simulations
• Multicomponent and Variable Velocity Galactic Outflow in Cosmological Hydrodynamic Simulations
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• Faint-end Quasar Luminosity Functions from Cosmological Hydrodynamic Simulations
• A Simple Model for the Relationship Between Star Formation and Surface Density
• The scatter in the radial profiles of X-ray luminous galaxy clusters as diagnostic of the thermodynamical state of the ICM
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
• The onset of star formation in primordial haloes
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Observational Properties of Simulated Galaxies in Overdense and Average Regions at High Redshifts z= 6-12
• The bispectrum of the Lyman-alpha forest at z~2-2.4 from a Large sample of UVES QSO Absorption Spectra (LUQAS)
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• Satellites Around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations Versus Simulations
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• Were progenitors of local L* galaxies Lyman-alpha emitters at high redshift?
• The velocity anisotropy of the Milky Way satellite system
• Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South
• The probability of galaxy-galaxy strong lensing events in hydrodynamical simulations of galaxy clusters
• The High-Ion Content and Kinematics of Low-Redshift Lyman Limit Systems
• The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
• Colour gradients within SDSS DR7 galaxies: hints of recent evolution
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• Dark Matter in the Local Universe
• The Non-Linear Matter Power Spectrum in Warm Dark Matter Cosmologies
• Feedback-Driven Evolution of the Far-Infrared Spectral Energy Distributions of Luminous and Ultraluminous Infrared Galaxies
• Galactic ménage à trois: Simulating magnetic fields in colliding galaxies
• From Discs to Bulges: effect of mergers on the morphology of galaxies
• Is there enough star formation in simulated protoclusters?
• The Three Hundred project: shapes and radial alignment of satellite, infalling, and backsplash galaxies
• Pericentric passage-driven star formation in satellite galaxies and their hosts: CLUES from Local Group simulations
• Theoretical predictions for the effect of nebular emission on the broad band photometry of high-redshift galaxies
• Simulations of galaxy formation with radiative transfer: Hydrogen reionization and radiative feedback
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Impact of Supernova feedback on the Tully-Fisher relation
• Tidally induced warps of spiral galaxies in IllustrisTNG
• Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe
• Catastrophic Cooling in Superwinds: Line Emission and Non-equilibrium Ionization
• Panchromatic SED modelling of spatially-resolved galaxies
• Properties and Evolution of Dual and Offset AGN in the ASTRID Simulation at $z\sim 2$
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN
• Sub-millimetre galaxies in cosmological hydrodynamic simulations: Source number counts and the spatial clustering
• The descendants of the first quasars in the BlueTides simulation
• nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• Simulating Supersonic Turbulence in Galaxy Outflows
• Radial profile and log-normal fluctuations of intra-cluster medium as an origin of systematic bias of spectroscopic temperature
• The Radial Acceleration Relation in Disk Galaxies in the MassiveBlack-II Simulation
• Constraints on the Nature of CID-42: Recoil Kick or Supermassive Black Hole Pair?
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Effects of metal enrichment and metal cooling in galaxy growth and cosmic star formation history
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• Simulations of XUV Disks with a Star Formation Density Threshold
• Active galactic nucleus jet feedback in hydrostatic halos
• The global stability of M33: still a puzzle
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• The Impact of Dust on the Sizes of Galaxies in the Epoch of Reionization
• Deconstructing Thermal Sunyaev-Zel'dovich - Gravitational Lensing Cross-Correlations: Implications for the Intracluster Medium
• Evidence for Black Hole Growth in Local Analogs to Lyman Break Galaxies
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Tidally Induced Offset Disks in Magellanic Spiral Galaxies
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Spiral-Induced Star Formation in the Outer Disks of Galaxies
• Loops formed by tidal tails as fossil records of a major merger
• The DUVET Survey: Resolved Maps of Star Formation Driven Outflows in a Compact, Starbursting Disk Galaxy
• The metallicity of galactic winds
• Galaxy cluster mergers
• Magnetic buoyancy in simulated galactic discs with a realistic circum galactic medium
• Conservation Laws in Smooth Particle Hydrodynamics: the DEVA Code
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• Nonparametric 3D map of the IGM using the Lyman-alpha forest
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
• Dark Matter Halo Environment for Primordial Star Formation
• AGN Feedback models: Correlations with star formation and observational implications of time evolution
• Numerical Simulations of Bubble-Induced Star Formation in Dwarf Irregular Galaxies with a Novel Stellar Feedback Scheme
• The Complex Structure of the Multi-Phase Galactic Wind in a Starburst Merger
• Effects of Quasar Feedback in Galaxy Groups
• Merger Signatures in the Dynamics of Star-forming Gas
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• "Grandeur in this view of life": N-body simulation models of the Galactic habitable zone
• The Angular Momentum of Gas in Proto-Galaxies: II -- The Impact of Preheating
• Kinematics of Simulated Galaxies II: Probing the Stellar Kinematics of Galaxies out to Large Radii
• Hydrodynamical simulations of galaxy clusters in dark energy cosmologies: I. general properties
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Formation of massive disk galaxies in the IllustrisTNG simulation
• Lyalpha versus X-ray heating in the high-z IGM
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• The eROSITA view of the Abell 3391/95 field: a case study from the Magneticum cosmological simulation
• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• The impact of environment and mergers on the HI content of galaxies in hydrodynamic simulations
• The resolution bias: low resolution feedback simulations are better at destroying galaxies
• Formation and evolution of early-type galaxies. II. Models with quasi-cosmological initial conditions
• The cross-correlation between 21cm intensity mapping maps and the Lyman-alpha forest in the post-reionization era
• The Cosmological Simulation Code OpenGadget3 -- Implementation of Meshless Finite Mass
• Keck OSIRIS AO LIRG Analysis: Feedback in the Nuclei of Luminous Infrared Galaxies
• Radiative properties of the first galaxies: rapid transition between blue and red
• Magnetic Fields on FIRE: Comparing B-fields in the multiphase ISM and CGM of Simulated L${}_{\ast }$ Galaxies to Observations
• The Effect Of AGN Heating On The Low-Redshift Lyα Forest
• The IRX-$\beta$ relation: Insights from simulations
• Testing the accuracy of the Hydro-PM approximation in numerical simulations of the Lyman-alpha forest
• Effects of cosmological parameters and star formation models on the cosmic star formation history in LambdaCDM cosmological simulations
• Finding Dwarf Galaxies From Their Tidal Imprints
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• On the effect of galactic outflows in cosmological simulations of disc galaxies
• Massive Black Hole Mergers with Orbital Information: Predictions from the ASTRID Simulation
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• On the accretion history of galaxy clusters: temporal and spatial distribution
• The evolution of the star formation rate function and cosmic star formation rate density of galaxies at $z\sim 1-4$
• Dust-Enshrouded AGN can Dominate Host-Galaxy-Scale Cold-Dust Emission
• High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions
• Probing the large and massive CGM of a galaxy at z ~ 0.2 using a pair of quasars
• The effects of a hot gaseous halo on disc thickening in galaxy minor mergers
• Ultraviolet Line Emission from Metals in the Low-Redshift Intergalactic Medium
• An ever-present $Gaia$ snail shell triggered by a dark matter wake
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• Osaka Feedback Model II: Modeling Supernova Feedback Based on High-Resolution Simulations
• Panchromatic Spectral Energy Distributions of Dusty Galaxies with RADISHE. I. Predictions for Herschel: Correlating Colors with Galactic Energy Sources
• The First Quiescent Galaxies in TNG300
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
• Galactic winds and the Lya forest
• Simulation of Soft X-ray Emission Lines from the Missing Baryons
• How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
• Characterising the Circum-Galactic Medium of Damped Lyman-$\alpha$ Absorbing Galaxies
• Baryon history and cosmic star formation in non-Gaussian cosmological models: numerical simulations
• Eavesdropping on Radio Broadcasts from Galactic Civilizations with Upcoming Observatories for Redshifted 21cm Radiation
• Bulge-driven Fueling of Seed Black Holes
• Satellites of Satellites: The Case for Carina and Fornax
• WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
• Physical properties of simulated galaxy populations at z=2 - II. Effects of cosmology, reionization and ISM physics
• Scaling Rrelation in two situations of extreme mergers
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• On the origin of magnetic driven winds and the structure of the galactic dynamo in isolated galaxies
• Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin
• Robust PCA and MIC statistics of baryons in early mini-haloes
• Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters
• 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
• Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs
• Tidal Imprints of a Dark Sub-Halo on the Outskirts of the Milky Way II. Perturber Azimuth
• Simulating the effect of photoheating feedback during reionization
• Low-mass galaxy formation in cosmological AMR simulations: the effects of varying the sub-grid physics parameters
• Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes
• Simulating the formation of a proto-cluster at z~2
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• The Three Hundred Project: the stellar and gas profiles
• Empirical Constraints for the Magnitude and Composition of Galactic Winds
• Self-regulated AGN feedback of light jets in cool-core galaxy clusters
• The Minimum Halo Mass for Star Formation at z = 6 - 8
• R-process enrichment in ultrafaint dwarf galaxies
• The scatter in the galaxy-halo connection: a machine learning analysis
• UV to submillimetre luminosity functions of TNG50 galaxies
• Modeling Evolution of Galactic Bars at Cosmic Dawn
• The baryonic Tully-Fisher relation in the Simba simulation
• The effect of feedback on the emission properties of the Warm-Hot Intergalactic Medium
• Flow-Driven Cloud Formation and Fragmentation: Results From Eulerian and Lagrangian Simulations
• The Gentle Growth of Galaxies at High Redshifts in Overdense Environments
• Discriminating Topology in Galaxy Distributions using Network Analysis
• The Kennicutt-Schmidt Star Formation Relation at z~2
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• Powerful quasar outflow in a massive disc galaxy at $z\sim 5$
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• Lyman Alpha and MgII as Probes of Galaxies and their Environments
• More accurate simulations with separate initial conditions for baryons and dark matter
• Gas outflows from the z= 7.54 quasar : predictions from the BlueTides Simulation
• Stellar population gradients in the cores of nearby field E+A galaxies
• Black hole clustering and duty cycles in the Illustris simulation
• Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• Towards a self-consistent numerical model of late-type galaxies: Calibrating the effects of sub-grid physics on galactic models
• Simulating the formation and evolution of galaxies: Multi-phase description of the interstellar medium, star formation, and energy feedback
• Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
• Multi-Fidelity Emulation for the Matter Power Spectrum using Gaussian Processes
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys IV: Characterizing Density and Pressure Clumping due to Infalling Substructures
• Stellar feedback strongly alters the amplification and morphology of galactic magnetic fields
• Extended Lyman-alpha emission from interacting galaxies at high redshifts
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• Tomographic weak lensing shear spectra from large N-body and hydrodynamical simulations
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• Mapping the Cosmic Web with Ly-alpha Emission
• Characterising the intra-cluster light in The Three Hundred simulations
• Distribution of streaming rates into high-redshift galaxies
• Gas Accretion Can Drive Turbulence in Galaxies
• Galaxy Formation in Heavily Overdense Regions at z~10: the Prevalence of Disks in Massive Halos
• A semi-analytic model of the turbulent multi-phase interstellar medium
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• The host galaxies of z=7 quasars: predictions from the BlueTides simulation
• How AGN feedback drives the size growth of the first quasars
• Chemical evolution of disc galaxies from cosmological simulations
• Super massive black holes in star forming gaseous circumnuclear discs
• On the algorithms of radiative cooling in semi-analytic models
• Cosmological insights into the assembly of the radial and compact stellar halo of the Milky Way
• Molecular cloud regulated star formation in galaxies
• Future Evolution of the Intergalactic Medium in a Universe Dominated by a Cosmological Constant
• Cosmological DCBH formation sites hostile for their growth
• Populating H${}_2$ and CO in galaxy simulation with dust evolution
• The evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10)
• Cosmological shock waves: clues to the formation history of haloes
• Counts of high-redshift GRBs as probe of primordial non-Gaussianities
• Cosmology dependence of galaxy cluster scaling relations
• Simulating the Soft X-ray excess in clusters of galaxies
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases
• A model for the metallicity evolution of damped Lyman-alpha systems
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• What Can the Distribution of Intergalactic Metals Tell us About the History of Cosmological Enrichment?
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• Linking the brightest stellar streams with the accretion history of Milky Way-like galaxies
• Where are the Cosmic Metals at z~3?
• Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
• Relative velocity of dark matter and barions in clusters of galaxies and measurements of their peculiar velocities
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations II: Resolution Effects
• Resolving flows around black holes: the impact of gas angular momentum
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• Probing Feedback via IGM tomography and Ly$\alpha$ forest with Subaru PFS, TMT/ELT, and JWST
• Rise and fall of post-starburst galaxies in Magneticum Pathfinder
• Evolution of the metal content of the intra-cluster medium with hydrodynamical simulations
• Can gravitational infall energy lead to the observed velocity dispersion in DLAs?
• The impact of natal kicks on galactic r-process enrichment by neutron star mergers
• The VLT LBG Redshift Survey - VI. Mapping HI in the proximity of $z\sim 3$ LBGs with X-Shooter
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• Statistical properties of mass, star formation, chemical content and rotational patterns in early z > 9 structures
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Baryons Shaping Dark Matter Haloes
• Radiative feedback and cosmic molecular gas: the role of different radiative sources
• The Accretion and Cooling of Preheated Gas in Dark Matter Halos
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• Detectability of [CII] 158 micron emission from high-redshift galaxies: predictions for ALMA and SPICA
• Disruption of Star Clusters in the Interacting Antennae Galaxies
• Is ram-pressure stripping an efficient mechanism to remove gas in galaxies?
• Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
• The Role of Star-Formation and AGN in Dust Heating of z=0.3-2.8 Galaxies - II. Informing IR AGN fraction estimates through simulations
• The formation and evolution of star clusters in interacting galaxies
• The reionization of galactic satellite populations
• KETJU -- resolving small-scale supermassive black hole dynamics in GADGET-4
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• The relation between star formation rate and stellar mass of galaxies at z $\sim$ 1-4
• Stellar Velocity Dispersion in Dissipative Galaxy Mergers with Star Formation
• Predictions of the causal entropic principle for environmental conditions of the universe
• Accurate Identification of Galaxy Mergers with Stellar Kinematics
• Interaction between dark matter sub-halos & galactic gaseous disk
• An Observational Estimate for the Mean Secular Evolution Rate in Spiral Galaxies
• The cosmological evolution of metal enrichment in quasar host galaxies
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• High resolution simulations of the reionization of an isolated Milky Way - M31 galaxy pair
• A New Discrete Dynamical Friction Estimator Based on $N$-body Simulations
• The association between gas and galaxies II: The 2-point correlation function
• The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite
• Studying the Warm-Hot Intergalactic Medium in Emission
• Clustering and lifetime of Lyman Alpha Emitters in the Epoch of Reionization
• Velocity Structure Diagnostics of Simulated Galaxy Clusters
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Gravitational lensing magnification without multiple imaging
• Influence of baryonic physics on the merger time-scale of galaxies in N-body/hydrodynamical simulations
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Troubled cosmic flows: turbulence, enstrophy and helicity from the assembly history of the intracluster medium
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
• Large-scale 3D mapping of the intergalactic medium using the Lyman Alpha Forest
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• SimSpin -- Constructing mock IFS kinematic data cubes
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Redshift evolution of the dark matter haloes shapes
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• The VLT LBG Redshift Survey - IV. Gas and galaxies at z ~ 3 in observations and simulations
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• Galaxy Lookback Evolution Models -- a Comparison with Magneticum Cosmological Simulations and Observations
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• The complementary roles of feedback and mergers in building the gaseous halo and the X-ray corona of Milky Way-sized galaxies
• Deviations from the Schmidt-Kennicutt relations during early galaxy evolution
• The seeds of supermassive black holes and the role of local radiation and metal spreading
• Magnetic field amplification and X-ray emission in galaxy minor mergers
• Modelling the fraction of Lyman Break Galaxies with strong Lyman alpha emission at 5 < z < 7
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Gas distribution, metal enrichment, and baryon fraction in Gaussian and non-Gaussian universes
• Impact of Baryonic Physics on Intrinsic Alignments
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• X-ray measured metallicities of the intra-cluster medium: a good measure for the metal mass?
• Constraining the intrinsic population of Long Gamma-Ray Bursts: implications for spectral correlations, cosmic evolution and their use as tracers of star formation
• A high baryon fraction in massive haloes at z~3
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• Recovering the Physical Properties of Molecular Gas in Galaxies from CO SLED Modeling
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
• Growth of Early Supermassive Black Holes and the High-Redshift Eddington Ratio Distribution
• The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• A Local Leaky-box Model for the Local Stellar Surface Density - Gas Surface Density - Gas Phase Metallicity Relation
• What shapes the far-infrared spectral energy distributions of galaxies?
• Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
• Enhanced star formation in $z\sim 6$ quasar companions
• Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs
• Modeling multi-phase gases in cosmological simulations using compressible multi-fluid hydrodynamics
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• The stellar mass function and star formation rate-stellar mass relation of galaxies at z ~ 4 - 7
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Weak lensing calibration of mass bias in the REFLEX+BCS X-ray galaxy cluster catalogue
• Collapse and fragmentation of molecular clouds under pressure
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• Incidence Rate of GRB-host-DLAs at High Redshift
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• X-Ray Absorption by the Warm-Hot Intergalactic Medium in the Hercules Supercluster
• Coevolution of the galactic cores and spiral galaxies
• Cold accretion in early galaxy formation and its Lyman-alpha signatures
• Termination of star formation by BH feedback in equal- and unequal-mass mergers of disk and elliptical galaxies
• Thermal state of the intergalactic medium at $z\sim 2-4$
• The Three Hundred project: A Machine Learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• Gas around galaxy haloes - II: hydrogen absorption signatures from the environments of galaxies at redshifts 2 < z < 3
• On the inconsistency between the estimates of cosmic star formation rate and stellar mass density of high redshift galaxies
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• The cosmic web in Lyman-alpha emission
• Satellite galaxies in groups in the CIELO Project I. Gas removal from galaxies and its re-distribution in the intragroup medium
• A study of simulated histories of reionization with merger trees of HII regions
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• A tiny host galaxy for the first giant black hole: $z=7.5$ quasar in BlueTides
• Cold versus Warm Dark Matter simulations of a galaxy group
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• Correlation between SFR surface density and thermal pressure of ionized gas in local analogs of high-redshift galaxies
• Constraining quasar host halo masses with the strength of nearby Lyman-alpha forest absorption
• Evolution of Late-type Galaxies in a Cluster Environment: Effects of High-speed Multiple Encounters with Early-type Galaxies
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• Lensing reconstruction of cluster-mass cross-correlation with cosmic microwave background polarization
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations
• Simulated metal and HI absorption lines at the conclusion of Reionization
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• Radiative Transfer Distortions of Lyman-$\alpha$ Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space
• The NGC 4013 tale: a pseudo-bulged, late-type spiral shaped by a major merger
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• The globular cluster system of the Auriga simulations
• Schmidt-Kennicutt relations in SPH simulations of disc galaxies with effective thermal feedback from supernovae
• Simulating the Carbon Footprint of Galactic Halos
• Effect of the Metallicity on the X-ray Emission from the Warm-Hot Intergalactic Medium
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• The baryon cycle of Seven Dwarfs with superbubble feedback
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• Simulations Find Our Accounting of Dust-Obscured Star Formation May Be Incomplete
• Impact of ICM disturbances on the mean pressure profile of galaxy clusters: a prospective study of the NIKA2 SZ large program with MUSIC synthetic clusters
• The IllustrisTNG Simulations: Public Data Release
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Tidally induced bars in gas-rich dwarf galaxies orbiting the Milky Way
• Survey parameters for detecting 21cm - Ly$\alpha$ emitter cross correlations with the Square Kilometre Array
• Atomic and molecular gas as traced by [C II] emission
• On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters
• SImulator of GAlaxy Millimetre/submillimetre Emission (SIGAME): CO emission from massive z=2 main-sequence galaxies
• Galactic winds - How to launch galactic outflows in typical Lyman-break galaxies
• The Three Hundred Project: the evolution of physical baryon profiles
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• The complexity that the first stars brought to the Universe: Fragility of metal enriched gas in a radiation field
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The dust attenuation law in $z\sim 6$ quasars
• Mass accretion toward black holes in the final phase of galaxy mergers
• Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
• Photometric Properties of the Most Massive High-Redshift Galaxies
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
• The Dispersion Measure Contributions of the Cosmic Web
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Cosmological Simulations of Massive Compact High-z Galaxies
• Velocity dispersion of the brightest cluster galaxies in cosmological simulations
• Ram pressure stripping of the multiphase ISM: a detailed view from TIGRESS simulations
• Morphology of galaxies with quiescent recent assembly history in a Lambda-CDM universe
• 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
• The Mystery of the $\sigma$-Bump -- A new Signature for Major Mergers in Early-type Galaxies?
• Galaxy Evolution: Modeling the Role of Non-thermal Pressure in the Interstellar medium
• There and back again: understanding the critical properties of backsplash galaxies
• Global dynamic scaling relations of HI-rich ultra-diffuse galaxies
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• Simulating extremely metal-poor gas and DLA metal content at redshift z=7
• Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
• Cross-correlation between the 21-cm signal and [OIII] emitters during early cosmic reionization
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• Hunting for Metals Using XQ-100 Legacy Survey Composite Spectra
• Fingerprints of the hierarchical building up of the structure on the gas kinematics of galaxies
• Information field dynamics for simulation scheme construction
• The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Forming disc galaxies in major mergers: III. The effect of angular momentum on the radial density profiles of disc galaxies
• Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• The THESAN project: Lyman-alpha emitter luminosity function calibration
• The role of gas kinematics in setting metallicity gradients at high redshift
• Constraints on ${\Omega }_{\mathrm{m}}$ and ${\sigma }_8$ from the potential-based cluster temperature function
• Constraints on the velocity profiles of galaxies from strong lensing statistics and semi-analytical modelling of galaxy formation
• The imprint of cosmological non-Gaussianities on primordial structure formation
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Cosmic Star Formation: a simple model of the SFRD(z)
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• The effect of gravitational tides on dwarf spheroidal galaxies
• Testing Feedback from Star Clusters in Simulations of the Milky Way Formation
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Properties of the Magellanic Corona
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• Star formation in mergers with cosmologically motivated initial conditions
• Pointing to the minimum scatter: the generalized scaling relations for galaxy clusters
• Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogs
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• Tracing early structure formation with massive starburst galaxies and their implications for reionization
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• A warm mode of gas accretion on forming galaxies
• Gamma-ray emission from spectrally resolved cosmic rays in galaxies
• Probing the Metal Enrichment of the Intergalactic Medium at $z=5-6$ Using the Hubble Space Telescope
• The impact of galactic winds from LBGs on the Intergalactic Medium
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Role of ionizing background on the statistics of metal absorbers in hydrodynamical simulations
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• The magnetised and thermally unstable tails of jellyfish galaxies
• Expected properties of the Two-Point Autocorrelation Function of the IGM
• Is the star formation rate in $z\sim 6$ quasars overestimated?
• Towards 1% accurate galaxy cluster masses: Including baryons in weak-lensing mass inference
• Bimodal Behavior and Convergence Requirement in Macroscopic Properties of the Multiphase Interstellar Medium Formed by Atomic Converging Flows
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• Metal Enrichment in the Reionization Epoch
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• Prospects of detecting soft X-ray emission from typical WHIM filaments around massive clusters and the Coma cluster soft excess
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• Heating and enriching the intracluster medium
• s-process Enirchment of Ultrafaint Dwarf Galaxies
• Luminosity Distribution of Gamma-Ray Burst Host Galaxies at redshift z=1 in Cosmological Smoothed Particle Hydrodynamic Simulations: Implications for the Metallicity Dependence of GRBs
• Disentangling the multi-phase circumgalactic medium shared between a dwarf and a massive star-forming galaxy at z~0.4
• Star Formation and Gas Phase History of the Cosmic Web
• Statistical properties of SZ and X-ray cluster detections
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• The dispersion measure and rotation measure from fast radio burst host galaxies based on the IllustrisTNG50 simulation
• ColdSIM predictions of [C II] emission in primordial galaxies
• Chemo-dynamical simulations of dwarf galaxy evolution
• On the small scale clustering of quasars: constraints from the MassiveBlack II simulation
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• The effects of binary stars on galaxies and metal-enriched gas during reionization
• Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey
• Luminosity function of [OII] emission-line galaxies in the MassiveBlack-II simulation
• Stellar migration in the Auriga simulations
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• Toward an Improved Analytical Description of Lagrangian Bias
• The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
• Constrained simulations of the Antennae Galaxies: Comparison with Herschel-PACS observations
• Cosmic magnetic fields with MASCLET: an application to galaxy clusters
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• Little Red Dots as Direct-collapse Black Hole Nurseries
• The impact of magnetic fields on cosmological galaxy mergers -- II. Modified angular momentum transport and feedback
• Host galaxies of long gamma-ray bursts in the Millennium Simulation
• Effects of hot halo gas on the star formation and mass transfer during distant galaxy-galaxy encounters
• Testing Galaxy Formation Simulations with Damped Lyman-$\alpha$ Abundance and Metallicity Evolution
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts
• Gas dynamics and star formation in NGC 6822
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
• Testing the fidelity of simulations of black hole - galaxy co-evolution at z ~ 1.5 with observations
• Satellite Alignment: III. Satellite Galaxies Spatial Distribution and their Dependence on Redshift with A Novel Galaxy Finder
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Star formation and bar instability in cosmological haloes
• Deep Forest: Neural Network reconstruction of the Lyman-alpha forest
• Dust grain size evolution in local galaxies: a comparison between observations and simulations
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Suppression of Dwarf Galaxy Formation by Cosmic Shocks
• A Multi-Fidelity Emulator for the Lyman-$\alpha$ Forest Flux Power Spectrum
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• Evolution of Starburst Galaxies in the Illustris Simulation
• Column Density Profiles of Cold Clouds Driven by Galactic Outflows
• Storm fronts over galaxy discs: Models of how waves generate extraplanar gas and its anomalous kinematics
• Gas stripping and mixing in galaxy clusters: A numerical comparison study
• The Importance of Being Interpretable: Toward An Understandable Machine Learning Encoder for Galaxy Cluster Cosmology
• Numerical simulations of bar formation in the Local Group
• Identification of a Fundamental Transition in a Turbulently-Supported Interstellar Medium
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Signatures of very massive stars: supercollapsars and their cosmological rate
• Star Formation Variability as a Probe for the Baryon Cycle within Galaxies
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• The cooler past of the intracluster medium in TNG-Cluster
• Angular diameter distance estimates from the Sunyaev-Zel'dovich effect in hydrodynamical cluster simulations
• The CO universe: Modelling CO emission and H${}_2$ abundance in cosmological galaxy formation simulations
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Distinguishing Dirac vs. Majorana Neutrinos: a Cosmological Probe
• Revealing the Nature of a Lyman-$\alpha$ Halo in a Strongly Lensed Interacting System at $z=2.92$
• Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• Orbital and Radiative Properties of Wandering Intermediate-Mass Black Holes in the ASTRID Simulation
• Synthetic X-ray and radio maps for two different models of Stephan's Quintet
• Narrow C IV absorption doublets on quasar spectra of the Baryon Oscillation Spectroscopic Survey
• Is There a Fundamental Line for Disk Galaxies?
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• A VLT/FORS2 Narrowband Imaging Search for MgII Emission Around z ~ 0.7 Galaxies
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
• Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies
• Colour-magnitude diagram in simulations of galaxy formation
• Field spheroid-dominated galaxies in a Λ-CDM Universe
• Gas Cooling in Hydrodynamic Simulations with An Exact Time Integration Scheme
• The BlueTides Mock Image Catalogue: Simulated observations of high-redshift galaxies and predictions for JWST imaging surveys
• Merge and strip: dark matter-free dwarf galaxies in clusters can be formed by galaxy mergers
• The circumgalactic medium in Lyman-alpha: a new constraint on galactic outflow models
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Carbon envelopes around merging galaxies at z ~ 4.5
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Imprints of the cosmic void evolution on the baryon processes inside galaxy haloes
• Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters
• Coupled map lattice for the spiral pattern formation in astronomical objects
• The relation between Lyman-alpha absorbers and gas--rich galaxies in the local universe
• The Anatomy of a Star-Forming Galaxy II: the role of FUV heating via dust
• Self-gravitating equilibrium models of dwarf galaxies and the minimum mass for star formation
• Detecting the Cosmic Web: Lyα Emission from Simulated Filaments at z=3
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches
• The influence of mergers on the cluster temperature function and cosmological parameters derived from it
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• Not all peaks are created equal: the early growth of Supermassive Black Holes
• Formation and fate of low metallicity stars in IllustrisTNG50
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Constraints on galactic wind models
• On the phase-space structure of galaxy clusters from cosmological simulations
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• Properties of the circumgalactic medium in simulations compared to observations
• Accretion onto supermassive and intermediate mass black holes in cosmological simulations
• The environments and hosts of metal absorption at z>5
• The Population of Galaxies that Contribute to The HI Mass Function
• Implications of galaxy buildup for putative IMF variations in massive galaxies
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• The Interstellar Medium and Star Formation in Local Galaxies: Variations of the Star Formation Law in Simulations
• Multiplicity functions of quasars: Predictions from the MassiveBlackII simulation
• Addressing via N-body simulations the distribution of the satellite tidal debris in the Milky Way environment
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• The parametrization of gas flows in discs in the Auriga simulations
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• Entropy-Conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations
• Simulated vs. observed UV emission at high redshift: a hint for a clumpy ISM?
• Extensions and applications of the iterative method
• On the detectability of massive black hole merger eventsby LISA
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Magnetically Regulated Gas Accretion in High-Redshift Galactic Disks
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• On the connection between AGN radiative feedback and massive black hole spin
• The Dark Matter Halos of HI Selected Galaxies
• Numerical dependencies of the galactic dynamo in isolated galaxies with SPH
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• Hydrodynamical Simulations of the Triggering of Nuclear Activities by Minor Mergers of Galaxies
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Molecular Disk Properties in Early-Type Galaxies
• Triple-ionised carbon associated with the low-density neutral hydrogen gas at 1.7 < z < 3.3: the integrated N(HI)-N(CIV) relation
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (I) Temporal dependency
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Towards an accurate model for the Antennae Galaxies
• The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies
• Mass-morphology relation of TNG50 galaxies
• Growth and anisotropy of ionization fronts near high redshift quasars in the MassiveBlack simulation
• ΛCDM with baryons vs. MOND: the time evolution of the universal acceleration scale in the Magneticum simulations
• Galaxy Formation and Dark Matter
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Lux ex tenebris: The imprint of annihilating dark matter on the intergalactic medium during Cosmic Dawn
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• Response of the LMC's Bar to a Recent SMC Collision and Implications for the SMC's Dark Matter Profile
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• Galaxy populations of ProtoClusters in cosmological hydrodynamical simulations
• Evolution and instabilities of disks harboring super massive black holes
• The perils of stacking optically selected groups in eROSITA data. The Magneticum perspective
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• Star Formation during Galaxy Formation
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• Simulated [CII] in high-z galaxies
• Radial X-ray profiles of simulated galaxies: Contributions from hot gas and XRBs
• DLA kinematics and outflows from starburst galaxies
• VALES V: A kinematic analysis of the molecular gas content in $H$-ATLAS galaxies at $z\sim 0.03-0.35$ using ALMA
• Lyman alpha Properties of Simulated Galaxies in Overdense Regions: Effects of Galactic Winds at z > 6
• The impact of the cosmological constant on past and future star formation
• Dynamically Produced Moving Groups in Interacting Simulations
• Viscous time lags between starburst and AGN activity
• Positive and negative feedback by AGN jets in high-redshift galaxies
• Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• Forming disc galaxies in major mergers II. The central mass concentration problem and a comparison of GADGET3 with GIZMO
• Confronting predictions of the galaxy stellar mass function with observations at high-redshift
• Triple and Quadruple Black Holes in the ASTRID Simulation at $z\sim 2$
• Kinematic signatures of impulsive supernova feedback in dwarf galaxies
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• A simple numerical experiment on the dust temperature bias for Lyman break galaxies at $z\gtrsim 5$
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• Chemical abundances and spatial distribution of Long Gamma-Ray Bursts
• Boosting Line Intensity Map Signal-to-Noise with the Ly-$\alpha$ Forest Cross-Correlation
• Gas Inflow and Outflow Histories in Disk Galaxies as Revealed from Observations of Distant Star-Forming Galaxies
• On the star formation efficiency in high redshift Lyman-α emitters
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• MF-Box: Multi-fidelity and multi-scale emulation for the matter power spectrum
• Embedded AGN and star formation in the central 80 pc of IC 3639
• Cloud angular momentum and effective viscosity in global SPH simulations with feedback
• Dark Matter-Induced Baryonic Feedback in Galaxies
• Influence of mergers on LyC escape of high redshift galaxies
• The Glow of Axion Quark Nugget Dark Matter: (I) Large Scale Structures
• Stacking Redshifted 21cm Images of HII Regions Around High Redshift Galaxies as a Probe of Early Reionization
• Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
• The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies
• Disc-Halo Interactions in ΛCDM
• Understanding Galaxy Formation and Evolution
• The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
• Multi-scale simulations of black hole accretion in barred galaxies: Self-gravitating disk models
• High Velocity-dispersion Cold Gas in ULIRG Outflows. I: Direct Simulations
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Comparing the interstellar and circumgalactic origin of gas in the tails of jellyfish galaxies
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies
• Gravitational Lensing as Signal and Noise in Lyman-alpha Forest Measurements
• Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence
• Cross-Correlation between Damped Ly-alpha Systems and Ly-break Galaxies in Cosmological SPH Simulations
• Differentiable Cosmological Hydrodynamics for Field-Level Inference and High Dimensional Parameter Constraints
• The eROSITA view on the halo mass-temperature relation: From low-mass groups to massive clusters
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Large scale environmental bias of the QSO line of sight proximity effect
• A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• The collaborative effect of ram pressure and merging on star formation and stripping fraction
• Hydrodynamical chemistry simulations of the SZ effect and the impacts from primordial non-Gaussianities
• Negative feedback effects on star formation history and cosmic reionization
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Simulation-based marginal likelihood for cluster strong lensing cosmology
• Self-gravitating barotropic equilibrium configurations of rotating bodies with SPH
• Assuming Ionization Equilibrium and the Impact on the Lyman-$\alpha$ Forest Power Spectrum during the End of Reionization at $8\ge z\ge 5$
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (II) The inside-out growth of discs
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• CLUES to the past: Local Group progenitors amongst high-redshift Lyman Break Galaxies
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• The neutron-capture and alpha-elements abundance ratios scatter in old stellar populations. Cosmological simulations of the stellar halo
• Recovering the pattern speeds of edge-on barred galaxies via an orbit-superposition method
• Modelling the selection of galaxy groups with end to end simulations
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• Feedback Factory: Multiple faint radio-jets detected in a cluster at z=2
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Kinematics of the Local Group gas and galaxies in the Hestia simulations
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• The role of magnetic fields in ram pressure stripping of satellite galaxies in the circumgalactic medium around massive galaxies
• Using dust to constrain dark matter models
• The Sunyaev-Zel'dovich effect due to hyper-starburst galaxy winds
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• Stellar populations with MEGARA: the inner regions of NGC 7025
• Modelling Galaxies with a Multi-Phase ISM in 3d
• SISSI: Supernovae in a stratified, shearing interstellar medium -- I. The geometry of supernova remnants
• Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
• The physical properties and the evolution of the interacting system AM1204-292
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• Physically motivated modeling of LyC escape fraction during reionization
• Exploring the evolution of a dwarf spheroidal galaxy with SPH simulations: I. Stellar feedback
• High-redshift AGN population in radiation-hydrodynamics simulations
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• The Three Hundred: The existence of massive dark matter-deficient satellite galaxies in cosmological simulations
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• Exploring the evolution of a dwarf spheroidal galaxy with SPH simulations: II. AGN feedback
• Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Wind of Change: Faraday Rotation in a Simulated Large Magellanic Cloud
• Formation and evolution of boxy/peanut bulges in the Auriga cosmological simulations
• Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics
• Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• An attractor for the dynamical state of the intracluster medium
• The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z=3.55$
• Comparing energy and entropy formulations for cosmic ray hydrodynamics
• Large, fast and accurate HI intensity maps with latent overlap diffusion
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Evolution of the degree of substructures in simulated galaxy clusters
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Environment matters: stronger magnetic fields in satellite galaxies
• Entropy generation in merging galaxy clusters
• SubDLe: identification of substructures in cosmological simulations with deep learning
• Modelling the chemical evolution of the Milky Way
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Intermediate-Mass Black Hole Feedback in Dwarf Galaxies: a View from Cosmological Simulations
• High$-z$ [OI] emission lines: ColdSIM simulations and ALMA observations
• Tracing the environmental history of observed galaxies via extended fast action minimization method
• Dipole Distortions in the Intergalactic Medium
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• Absorption systems at $z\sim 2$ as a probe of the circum galactic medium: a probabilistic approach
• Go with the Flow: The Self-Similar and Non-Linear Behaviour of Large-Scale In- and Outflows and the Impact of Accretion Shocks from Galaxies to Galaxy Clusters
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• The large-scale distribution of ionized metals in IllustrisTNG
• "Observing and Analyzing" Images From a Simulated High Redshift Universe
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability
• Extended Hernquist-Springel formalism for cosmic star formation
• Damped Lyman-alpha Absorbers in Cosmological SPH Simulations: the "metallicity problem"
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Simulating the galactic system in interaction AM 2229-735 and the formation of its polar structure
• The role of AGN feedback and gas viscosity in hydrodynamical simulations of galaxy clusters
• Dark Energy Simulations
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• OpenGadget3 GPU solver tests
• The origin of the intra-cluster light in The Three Hundred simulations
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• Evolution of the spin of late-type galaxies caused by galaxy-galaxy interactions
• Inferring the mass of the circumgalactic medium using X-ray resonant scattering
• DLAs and Galaxy Formation
• A thick-disk galaxy model and simulations of equal-mass galaxy pair collisions
• A supernova scenario for magnetic fields and rotation measures in galaxies
• Numerical approaches to star formation and SuperNovae energy feedback in simulations of galaxy clusters
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• A general framework for unbiased tests of gravity using galaxy clusters
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• Substructures in Minor Mergers' Tidal Streams
• Feedback and the Initial Mass function
• Mainly on the Plane: Observing the Extended, Ionized Disks of Milky Way Analogs in IllustrisTNG
• Quenching Star Formation: Can AGN Do the Trick?
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• Simulations of Early Galaxy Formation
• Can UVB variations reconcile simulated quasar absorption lines at high redshift?
• The Galaxy Evolution Probe
• The Challenge of Modelling Galactic Disks
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• The origin of ionized gas in retired galaxies: dynamical clues
• Measuring Scaling Relationships: Fitting Technique Matters
• Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Modeling Multiphase Galactic Outflows: A Multifluid Moving Mesh Approach
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Spectrally resolved cosmic rays: II -- Momentum-dependent cosmic ray diffusion drives powerful galactic winds
• Effects of Supernova Feedback on the Formation of Galaxies