Simulating galaxy formation with black hole driven thermal and kinetic feedback

Abstract

The inefficiency of star formation in massive elliptical galaxies is widely believed to be caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas. Achieving a sufficiently rapid reddening of moderately massive galaxies without expelling too many baryons has however proven difficult for hydrodynamical simulations of galaxy formation, prompting us to explore a new model for the accretion and feedback effects of supermassive black holes. For high accretion rates relative to the Eddington limit, we assume that a fraction of the accreted rest mass energy heats the surrounding gas thermally, similar to the `quasar mode' in previous work. For low accretion rates, we invoke a new, pure kinetic feedback model which imparts momentum into the surrounding gas in a stochastic manner. These two modes of feedback are motivated both by theoretical conjectures for the existence of different types of accretion flows as well as recent observational evidence for the importance of kinetic AGN winds in quenching galaxies. We find that a large fraction of the injected kinetic energy in this mode thermalises via shocks in the surrounding gas, thereby providing a distributed heating channel. In cosmological simulations, the resulting model produces red, non star-forming massive elliptical galaxies, and achieves realistic gas fractions, black hole growth histories and thermodynamic profiles in large haloes.

19 pages, 15 figures

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• AGN Feedback and Multi-phase Gas in Giant Elliptical Galaxies
• Tidally induced warps of spiral galaxies in IllustrisTNG
• Decoupling the rotation of stars and gas -- I: the relationship with morphology and halo spin
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• An alternate approach to measure specific star formation rates at 2<z<7
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• Suppression of AGN-Driven Turbulence by Magnetic Fields in a Magnetohydrodynamic Model of the Intracluster Medium
• Taking snapshots of the jet-ISM interplay: The case of PKS0023-26
• The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• AGN Feedback in SDSS-IV MaNGA: AGNs have Suppressed Central Star Formation Rates
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Active galactic nucleus jet feedback in hydrostatic halos
• Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Fountains and storms: The role of AGN and mergers in disrupting the cool-core in the RomulusC simulation
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• The Close AGN Reference Survey (CARS): IFU survey data and the BH mass dependence of long-term AGN variability
• Galaxy formation in the brane world I: overview and first results
• The Galaxy Activity, Torus, and Outflow Survey (GATOS). (IV): Exploring Ionized Gas Outflows in Central Kiloparsec Regions of GATOS Seyferts
• The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• An evolving and mass dependent ${\sigma }_{\text{sSFR}}$-${\mathrm{M}}_{\star }$ relation for galaxies
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• The Effect Of AGN Heating On The Low-Redshift Lyα Forest
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Finding universal relations in subhalo properties with artificial intelligence
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• A quasar-galaxy merger at $z\sim 6.2$: black hole mass and quasar properties from the NIRSpec spectrum
• From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Formation of massive disk galaxies in the IllustrisTNG simulation
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Breaking baryon-cosmology degeneracy with the electron density power spectrum
• Spectral Classification and Ionized Gas Outflows in $z\sim 2$ WISE-Selected Hot Dust-Obscured Galaxies
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• 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
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Deciphering the imprint of AGN feedback in Seyfert galaxies: Nuclear-scale molecular gas deficits
• The First Quiescent Galaxies in TNG300
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Simulating the effect of photoheating feedback during reionization
• Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data
• Quenching Timescales in the IllustrisTNG Simulation
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• The impact of galactic feedback on the shapes of dark-matter haloes
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• Constraining SIDM with halo shapes: revisited predictions from realistic simulations of early-type galaxies
• UV to submillimetre luminosity functions of TNG50 galaxies
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• The scatter in the galaxy-halo connection: a machine learning analysis
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• SDSS-IV MaNGA: The Roles of AGNs and Dynamical Processes in Star Formation Quenching in Nearby Disk Galaxies
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• Radiative heating in the kinetic mode of AGN feedback
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• The impact of AGN-driven winds on physical and observable galaxy sizes
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• Identifying Galaxy Mergers in Simulated CEERS NIRCam Images using Random Forests
• Revealing impacts of stellar mass and environment on galaxy quenching
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• The Physical Origin of Galactic Conformity: From Theory to Observation
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems
• Gas Accretion Can Drive Turbulence in Galaxies
• The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
• Probing the Circum-Galactic Medium with Fast Radio Bursts: Insights from the CAMELS Simulations
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• The jet/wind outflow in Centaurus A: a local laboratory for AGN feedback
• How AGN feedback drives the size growth of the first quasars
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• Surrogate modelling the Baryonic Universe I: The colour of star formation
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Red quasars blow out molecular gas from galaxies during the peak of cosmic star formation
• The Interaction between AGN and Starburst Activity in the Circumnuclear Region of NGC 7469 as Viewed with JWST
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• A NOEMA molecular line scan of the Hubble Deep Field North: Improved constraints on the CO luminosity functions and cosmic density of molecular gas
• The Interplay of Kinetic and Radiative Feedback in Galaxy Clusters
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Decoupling the rotation of stars and gas -- II: the link between black hole activity and MaNGA kinematics in TNG
• Evidence that Shocks Destroy Small PAH Molecules in Low-luminosity Active Galactic Nuclei
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
• HIFlow: Generating Diverse HI Maps and Inferring Cosmology while Marginalizing over Astrophysics using Normalizing Flows
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• HInet: Generating neutral hydrogen from dark matter with neural networks
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• An AGN with an ionized gas outflow in a massive quiescent galaxy in a protocluster at $\mathbf{z}=3.09$
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• Towards robust determination of non-parametric morphologies in marginal astronomical data: resolving uncertainties with cosmological hydrodynamical simulations
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• SHAM through the lens of a hydrodynamical simulation
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Large-scale dynamics of winds originated from black hole accretion flows: (II) Magnetohydrodynamics
• The CGM${}^2$ Survey: Quenching and the Transformation of the Circumgalactic Medium
• On the Role of Hot Feedback Mode in Active Galactic Nuclei Feedback in an Elliptical Galaxy
• A hidden population of massive black holes in simulated dwarf galaxies
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• The impact of AGN feedback on galaxy intrinsic alignments in the Horizon simulations
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
• Redshift evolution of the dark matter haloes shapes
• Characterizing Protoclusters and Protogroups at z $\sim$ 2.5 Using Ly$\alpha$ Tomography
• Predicting sub-millimeter flux densities from global galaxy properties
• Star formation quenching imprinted on the internal structure of naked red nuggets
• Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• The (black hole mass)-(color) relations for early- and late-type galaxies: red and blue sequences
• Inferring galaxy dark halo properties from visible matter with Machine Learning
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Neural networks as optimal estimators to marginalize over baryonic effects
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
• Evidence for A Hot Wind from High-resolution X-ray Spectroscopic Observation of the Low-luminosity Active Galactic Nucleus in NGC 7213
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• A high baryon fraction in massive haloes at z~3
• The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• Detecting low-mass haloes with strong gravitational lensing II: constraints on the density profiles of two detected subhaloes
• Galaxies with monstrous black holes in galaxy cluster environments
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth
• The cosmic web in Lyman-alpha emission
• The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Multifield Cosmology with Artificial Intelligence
• Redshift space distortions of the {\rm HI} 21-cm intensity mapping signal due to the internal motions within galaxies
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Cooling flows around cold clouds in the circumgalactic medium: steady-state models & comparison with TNG50
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• Young stellar population gradients in central cluster galaxies from NUV and optical spectroscopy
• Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• The Spiderweb proto-cluster is being magnetized by its central radio jet
• Compact Molecular Gas Distribution in Quasar Host Galaxies
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• A general framework to test gravity using galaxy clusters III: Observable-mass scaling relations in $f(R)$ gravity
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• A multi-wavelength study of a massive, active galaxy at $z\sim 2$: coupling the kinematics of the ionized and molecular gas
• The IllustrisTNG Simulations: Public Data Release
• Large-scale dynamics of winds originated from black hole accretion flows: (I) Hydrodynamics
• Observational Evidence for Large-Scale Gas Heating in a Galaxy Protocluster at z=2.30
• The Obsidian model: Three regimes of black hole feedback
• QSOFEED: The relationship between star formation and AGN Feedback
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• A merging pair of massive quiescent galaxies at $z=3.44$ in the Cosmic Vine
• RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries
• Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Spatially offset black holes in the Horizon-AGN simulation and comparison to observations
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• The Stellar Mass - Black Hole Mass Relation at $z\sim 2$ Down to ${\mathcal{M}}_{\mathrm{BH}}\sim 10^7{M}_{\odot }$ Determined by HETDEX
• WALLABY pre-pilot survey: Two dark clouds in the vicinity of NGC 1395
• There and back again: understanding the critical properties of backsplash galaxies
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• Detecting the halo heating from AGN feedback with ALMA
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Teaching neural networks to generate Fast Sunyaev Zel'dovich Maps
• Evidence for non-merger co-evolution of galaxies and their supermassive black holes
• Hunting for Metals Using XQ-100 Legacy Survey Composite Spectra
• The impact of black hole seeding in cosmological simulations
• The evolutionary pathways of disk galaxies with different sizes
• The THESAN project: Lyman-alpha emitter luminosity function calibration
• Cosmological Probes of Structure Growth and Tests of Gravity
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• Using Real and Simulated Measurements of the Thermal Sunyaev-Zel'dovich Effect to Constrain Models of AGN Feedback
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• Pattern speed evolution of barred galaxies in TNG50
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
• Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• The dispersion measure and rotation measure from fast radio burst host galaxies based on the IllustrisTNG50 simulation
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4
• Evaluating hydrodynamical simulations with green valley galaxies
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• Spatially resolved observations of outflows in the radio loud AGN of UGC 8782
• The environment of radio galaxies: A signature of AGN feedback at high redshifts
• Evolution of central galaxy alignments in simulations
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Planting a Lyman alpha forest on AbacusSummit
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• Zooming in on the Circumgalactic Medium with GIBLE: the Topology and Draping of Magnetic Fields around Cold Clouds
• Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
• Discovery of a strong ionized-gas outflow in an AKARI-selected Ultra-luminous Infrared Galaxy at z = 0.5
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• SIEGE IV: compact star clusters in cosmological simulations with high star formation efficiency and sub-parsec resolution
• Clustering of MgII absorption line systems around massive galaxies: an important constraint on feedback processes in galaxy formation
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• Toward a Physical Understanding of Galaxy-Halo Alignment
• Formation of a barred galaxy in a major merger: The role of AGN feedback
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Do current X-ray observations capture most of the black-hole accretion at high redshifts?
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Radiation-driven outflows in AGNs: Revisiting feedback effects of scattered and reprocessed photons
• Imprint of baryons and massive neutrinos on velocity statistics
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• The CO universe: Modelling CO emission and H${}_2$ abundance in cosmological galaxy formation simulations
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• A Catalog of High-Velocity CIV Mini-BALs in the VLT-UVES and Keck-HIRES Archives
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• The Host Galaxies of Radio AGN: New Views from Combining LoTSS and MaNGA Observations
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• The cooler past of the intracluster medium in TNG-Cluster
• Anisotropic Satellite Galaxy Quenching: A Unique Signature of Energetic Feedback by Supermassive Black Holes?
• Cosmic evolution of radio-excess AGNs in quiescent and star-forming galaxies across $0<z<4$
• Differential rotation of the halo traced by the K-giant stars
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• Radiation-pressure Waves and Multiphase Quasar Outflows
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Detecting the Cosmic Web: Lyα Emission from Simulated Filaments at z=3
• Formation of super-thin galaxies in Illustris-TNG
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16
• Extragalactic Stellar Tidal Streams: Observations meet Simulation
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• Large-scale Dynamics of Winds Driven by Line Force from a Thin Accretion Disk
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• Classification of cosmic structures for galaxies with deep learning: connecting cosmological simulations with observations
• JCMT/SCUBA-2 uncovers an excess of $850\mu$m counts on megaparsec scales around high-redshift quasars. Characterization of the overdensities and their alignment with the quasars' Ly$\alpha$ nebulae
• Gas Cooling in Hydrodynamic Simulations with An Exact Time Integration Scheme
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Relating galaxies across different redshift to study galaxy evolution
• Searching for HI around MHONGOOSE Galaxies via Spectral Stacking
• Cosmology with Galaxy Cluster Properties using Machine Learning
• High-order Discontinuous Galerkin hydrodynamics with sub-cell shock capturing on GPUs
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- I. Constraining physical processes in local star-forming galaxies
• Galaxy shapes in Magneticum. I. Connecting stellar and dark matter shapes to dynamical and morphological galaxy properties and the large-scale structure
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• Maximal X-ray feedback in the pre-reionization universe
• Black hole virial masses from single-epoch photometry: the miniJPAS test case
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• ASymba: HI global profile asymmetries in the Simba simulation
• Accretion onto supermassive and intermediate mass black holes in cosmological simulations
• Formation and fate of low metallicity stars in IllustrisTNG50
• Probabilistic model for dynamic galaxy decomposition
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Implications of galaxy buildup for putative IMF variations in massive galaxies
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• NOEMA spatially resolved view of the multi-phase outflow in IRAS17020+4544: a shocked wind in action?
• Off-centre supermassive black holes in bright central galaxies
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• Where binary neutron stars merge: predictions from IllustrisTNG
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• On the connection between AGN radiative feedback and massive black hole spin
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• What is the real accretion rate onto a black hole for low angular momentum accretion?
• The Close AGN Reference Survey (CARS). A parsec scale multi-phase outflow in the super-Eddington NLS1 Mrk 1044
• On the Origin of High-velocity Clouds in the Galaxy
• What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Early formation of supermassive black holes from the collapse of strongly self-interacting dark matter
• The four cosmic tidal web elements from the $\beta$-skeleton
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Measuring the thermal and ionization state of the low-$z$ IGM using likelihood free inference
• Resolved star formation in TNG100 central and satellite galaxies
• Zooming in on the Circumgalactic Medium with GIBLE: Tracing the Origin and Evolution of Cold Clouds
• The Direct-Method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High-Noon
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• Mass-morphology relation of TNG50 galaxies
• The origin and properties of red spirals: Insights from cosmological simulations
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• MIRACLE I.: Unveiling the Multi-Phase, Multi-Scale physical properties of the Active Galaxy NGC 424 with MIRI, MUSE, and ALMA
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• The impact of the cosmological constant on past and future star formation
• Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
• The diverse physical origins of stars in the dynamically hot bulge: CALIFA vs. IllustrisTNG
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators
• Gravitational Waves from Massive Black Hole Mergers in ASTRID: Predictions for LISA
• Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
• Simulated [CII] in high-z galaxies
• Critical Stellar Central Densities Drive Galaxy Quenching in the Nearby Universe
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• Mass accretion rates of the HectoMAP clusters of galaxies
• Studying galaxy cluster morphological metrics with Mock-X
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Galaxy populations in protoclusters at cosmic noon
• Matter power spectrum induced by primordial magnetic fields: from the linear to the non-linear regime
• Euclid preparation. Simulations and nonlinearities beyond $\Lambda$CDM. 1. Numerical methods and validation
• Inpainting hydrodynamical maps with deep learning
• CAHA/PPAK Integral-field Spectroscopic Observations of M81 -- I. Circumnuclear ionized gas
• Absorption-line Environments of High-redshift BOSS Quasars
• Influence of mergers on LyC escape of high redshift galaxies
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Astrophysics with the Laser Interferometer Space Antenna
• NOEMA${}^{3D}$: A first kpc resolution study of a $z\sim 1.5$ main sequence barred galaxy channeling gas into a growing bulge
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Extreme High-velocity Outflows from High-redshift BOSS Quasars
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• SDSS-IV/MaNGA: Can impulsive gaseous inflows explain steep oxygen abundance profiles \& anomalously-low-metallicity regions?
• Differentiable Cosmological Hydrodynamics for Field-Level Inference and High Dimensional Parameter Constraints
• Prospects for detecting cosmic filaments in Lyman-alpha emission across redshifts $z=2-5$
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Hot Gas Flows on Parsec Scale in the Low-Luminosity Active Galactic Nucleus NGC 3115
• A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
• Total and dark mass from observations of galaxy centers with Machine Learning
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Constraint on magnetized galactic outflows from LOFAR rotation measure data
• The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• Mock Observations: Three Different Types of Galaxy Alignment in TNG100 Simulations
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Global structure and dynamics of slowly rotating accretion flows
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• A systematic study of AGN feedback in a disk galaxy I: global overview
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
• LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• Tracing the origins of galaxy lopsidedness across cosmic time
• Searching for Radio Outflows from M31* with VLBI Observations
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• Impact of supermassive black hole growth on star formation
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• A graph model for the clustering of dark matter halos
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• Probing neutral outflows in z ~ 2 galaxies using JWST observations of Ca II H and K absorption lines
• Tests of AGN Feedback Kernels in Simulated Galaxy Clusters
• The Compressed 3D Lyman-Alpha Forest Bispectrum
• Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering
• Field-Level Comparison and Robustness Analysis of Cosmological N-body Simulations
• High-redshift AGN population in radiation-hydrodynamics simulations
• Physically motivated modeling of LyC escape fraction during reionization
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
• Active galactic nuclei feedback at parsec scale
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• Challenges in Cosmic Magnification Reconstruction by Magnification Response
• Densified pupil spectrograph as high-precision radial velocimetry: From direct measurement of the Universe's expansion history to characterization of nearby habitable planet candidates
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• A jet-driven bipolar outflow in NGC 1125
• The evolution of the barred galaxy population in the TNG50 simulation
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type galaxies
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• A Spatially Resolved Evolutionary Sequence of Multi-wavelength AGN Host Galaxies
• The THESAN project: environmental drivers of Local Group reionization
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• LeMMINGs. V. Nuclear activity and bulge properties: a detailed multi-component decomposition of $e$-MERLIN Palomar galaxies with $HST$
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• You Are What You Eat: The Circumgalactic Medium Around BreakBRD Galaxies has Low Mass and Angular Momentum
• On the effects of parameters on galaxy properties in CAMELS and the predictability of ${\Omega }_{\mathrm{m}}$
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• ZFIRE -- The Gas Inflow Inequality for Satellite Galaxies in Cluster and Field Halos at z = 2
• Study of Central Intensity Ratio of Seyfert Galaxies in nearby Universe
• Cosmology with Topological Deep Learning
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• Study of central intensity ratio of early-type galaxies from low density environment
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• The AIDA-TNG project: 3D halo shapes
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Inferring halo masses with Graph Neural Networks
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• Spatial field reconstruction with INLA: Application to simulated galaxies
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• AVISM: Algorithm for Void Identification in coSMology
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Galaxy-halo internal alignments across cosmic time
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster
• ReveaLLAGN 1: JWST Emission-Line Spectra Reveal Low-Luminosity AGN with UV-Deficient SEDs and Warm Molecular Gas
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• Quadrupole signature as a kinematic diagnostic to constrain bar properties : implications for the Milky Way
• Tracing black hole and galaxy growth across environments since cosmic noon
• dm2gal: Mapping Dark Matter to Galaxies with Neural Networks
• The Origin of the Gas and Its Low Star Formation Efficiency in Quiescent Galaxies
• The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
• The large-scale distribution of ionized metals in IllustrisTNG
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Extended Hernquist-Springel formalism for cosmic star formation
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• The assembly history of NGC 1365 through chemical archaeology
• Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• The multi-component fitting to the star formation histories in the TNG simulation
• Morphology of dark matter haloes beyond triaxiality
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level
• The PARADIGM project II: The lifetimes and quenching of satellites in Milky Way-mass haloes
• Bound or blown: the fate of hot gas in galaxy groups
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• X-ray Emission from the Interstellar and Circumgalactic Medium of Elliptical Galaxies based on MACER simulations
• Combining LOFAR and Apertif Data for Understanding the Life Cycle of Radio Galaxies
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• Inferring the mass of the circumgalactic medium using X-ray resonant scattering
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Simulated X-ray Emission in Galaxy Clusters with Feedback from Active Galactic Nuclei
• Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Estimating Transient Rates from Cosmological Simulations and BPASS
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies
• Now you see it, now you don't: Star formation truncation precedes the loss of molecular gas by ~100 Myr in massive post-starburst galaxies at z~0.6
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• The dynamical lineage of ultra-diffuse galaxies from TNG50-1
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• How supermassive black holes shape central entropies in galaxy clusters
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
• Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
• The History of Galaxy Mergers in IllustrisTNG
• The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Massive black holes and their galaxies
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• Unravelling the role of merger histories in the population of In situ stars: linking IllustrisTNG cosmological simulation to H3 survey
• An Energetic Hot Wind from the Low-luminosity Active Galactic Nucleus M81*
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• From simulations to observations. Methodology and data release of mock TNG50 galaxies at 0.3 < z < 0.7 for WEAVE-StePS
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations