First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Abstract

We introduce the IllustrisTNG project, a new suite of cosmological magnetohydrodynamical simulations performed with the moving-mesh code AREPO employing an updated Illustris galaxy formation model. Here we focus on the general properties of magnetic fields and the diffuse radio emission in galaxy clusters. Magnetic fields are prevalent in galaxies, and their build-up is closely linked to structure formation. We find that structure formation amplifies the initial seed fields ($10^{-14}$ comoving Gauss) to the values observed in low-redshift galaxies ($1-10\mu \mathrm{G}$). The magnetic field topology is closely connected to galaxy morphology such that irregular fields are hosted by early-type galaxies, while large-scale, ordered fields are present in disc galaxies. Using two simple models for the energy distribution of relativistic electrons we predict the diffuse radio emission of $280$ clusters with a baryonic mass resolution of $1.1\times 10^7{\mathrm{M}}_{\odot }$, and generate mock observations for VLA, LOFAR, ASKAP and SKA. Our simulated clusters show extended radio emission, whose detectability correlates with their virial mass. We reproduce the observed scaling relations between total radio power and X-ray emission, $M_{500}$, and the Sunyaev-Zel'dovich $Y_{500}$ parameter. The radio emission surface brightness profiles of our most massive clusters are in reasonable agreement with VLA measurements of Coma and Perseus. Finally, we discuss the fraction of detected extended radio haloes as a function of virial mass and source count functions for different instruments. Overall our results agree encouragingly well with observations, but a refined analysis requires a more sophisticated treatment of relativistic particles in large-scale galaxy formation simulations.

arXiv comment28 pages, 18 figures, 2 tables, 3 appendices. Added a new relativistic electron energy parametrization and text modifications to match the accepted version for publication in MNRAS. More information, images and movies of the IllustrisTNG project can be found at http://www.tng-project.org

References in corpus (76)

• Planck 2015 results. XIII. Cosmological parameters
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Simulating Galaxy Formation with the IllustrisTNG Model
• First results from the IllustrisTNG simulations: matter and galaxy clustering
• First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
• First results from the IllustrisTNG simulations: the galaxy color bimodality
• Properties of galaxies reproduced by a hydrodynamic simulation
• First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• A model for cosmological simulations of galaxy formation physics
• A unified model for AGN feedback in cosmological simulations of structure formation
• Multi-scale initial conditions for cosmological simulations
• The LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release
• The Illustris simulation: the evolving population of black holes across cosmic time
• Clusters of galaxies : observational properties of the diffuse radio emission
• A New Radio - X-Ray Probe of Galaxy Cluster Magnetic Fields
• Constrained Simulations of the Magnetic Field in the Local Universe and the Propagation of UHECRs
• On the connection between giant radio halos and cluster mergers
• Simulations of magnetic fields in isolated disk galaxies
• The Energy Spectrum of Primary Cosmic Ray Electrons in Clusters of Galaxies and Inverse Compton Emission
• Radio Halo and Relic Candidates from the NRAO VLA Sky Survey
• Magnetohydrodynamics on an unstructured moving grid
• Cosmic Rays, Radio Halos and Non-Thermal X-ray Emission in Clusters of Galaxies
• Magnetic Fields and Faraday Rotation in Clusters of Galaxies
• Radio and X-ray diffuse emission in six clusters of galaxies
• Revisiting scaling relations for giant radio halos in galaxy clusters
• SZ effects in the Magneticum Pathfinder Simulation: Comparison with the Planck, SPT, and ACT results
• Do Hot Haloes Around Galaxies Contain the Missing Baryons?
• GMRT Radio Halo Survey in galaxy clusters at z = 0.2 -- 0.4. II.The eBCS clusters and analysis of the complete sample
• GMRT Radio Halo Survey in galaxy clusters at z = 0.2 -- 0.4 I.The REFLEX sub--sample
• Simulating cosmic ray physics on a moving mesh
• Magnetic field formation in the Milky Way-like disk galaxies of the Auriga project
• Cosmic ray transport in galaxy clusters: implications for radio halos, gamma-ray signatures, and cool core heating
• Giant radio relics in galaxy clusters: reacceleration of fossil relativistic electrons?
• Mechanical AGN Feedback: Controlling the Thermodynamical Evolution of Elliptical Galaxies
• Simulating cosmic rays in clusters of galaxies - II. A unified scheme for radio halos and relics with predictions of the gamma-ray emission
• Cosmic rays and Radio Halos in galaxy clusters : new constraints from radio observations
• Resolved magnetic dynamo action in the simulated intracluster medium
• The intracluster magnetic field power spectrum in Abell 2255
• Rise and Fall of Radio Halos in Simulated Merging Galaxy Clusters
• On the amplification of magnetic fields in cosmic filaments and galaxy clusters
• The intracluster magnetic field power spectrum in Abell 2382
• Cosmic Ray Streaming in Clusters of Galaxies
• Search for gamma-ray emission from the Coma Cluster with six years of Fermi-LAT data
• Simulating the gamma-ray emission from galaxy clusters: a universal cosmic ray spectrum and spatial distribution
• Zooming in on accretion - I. The structure of halo gas
• Constraints on Cosmic Rays, Magnetic Fields, and Dark Matter from Gamma-Ray Observations of the Coma Cluster of Galaxies with VERITAS and Fermi
• Turbulence and Particle Acceleration in Giant Radio Haloes: the Origin of Seed Electrons
• Occurrence of radio minihalos in a mass-limited sample of galaxy clusters
• Relativistic protons in the Coma galaxy cluster: first gamma-ray constraints ever on turbulent reacceleration
• The Extended GMRT Radio Halo Survey II: Further results and analysis of the full sample
• Radio Continuum Surveys with Square Kilometre Array Pathfinders
• Do radio relics challenge diffusive shock acceleration?
• Constraining the efficiency of cosmic ray acceleration by cluster shocks
• The large-scale properties of simulated cosmological magnetic fields
• On the Physics of Radio Halos in Galaxy Clusters: Scaling Relations and Luminosity Functions
• Semi-implicit anisotropic cosmic ray transport on an unstructured moving mesh
• A small-scale dynamo in feedback-dominated galaxies - II. The saturation phase and the final magnetic configuration
• Magnetic fields in nearby normal galaxies: Energy equipartition
• LOFAR and APERTIF surveys of the radio sky: probing shocks and magnetic fields in galaxy clusters
• Effects of simulated cosmological magnetic fields on the galaxy population
• A morphological comparison between giant radio halos and radio mini--halos in galaxy clusters
• Do radio mini-halos and gas heating in cool-core clusters have a common origin?
• Discovery of diffuse emission in the galaxy cluster A1689
• Accurately simulating anisotropic thermal conduction on a moving mesh
• Comparisons of Cosmological MHD Galaxy Cluster Simulations to Radio Observations
• Detection of diffuse radio emission in the galaxy clusters A800, A910, A1550, and CL1446+26
• Simulations of cosmic rays in large-scale structures: numerical and physical effects
• Estimates of relativistic electron and proton energy densities in starburst galactic nuclei from radio measurements
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• Cluster Radio Halos at the crossroads between astrophysics and cosmology in the SKA era
• Faraday Rotation Measures through the Cores of Southern Galaxy Clusters
• Cosmic rays in magnetized intracluster plasma
• MHD Turbulence Simulation in a Cosmic Structure Context

Cited by in corpus (717)

• First results from the IllustrisTNG simulations: matter and galaxy clustering
• First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
• First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time
• Supermassive black holes and their feedback effects in the IllustrisTNG simulation
• The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
• The Arepo public code release
• Simulating cosmic structure formation with the GADGET-4 code
• The star-formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
• The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z~8
• Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization
• The evolution of the mass-metallicity relation in IllustrisTNG
• The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
• Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors
• Baryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids
• Ingredients for 21cm intensity mapping
• Open Questions in Cosmic-Ray Research at Ultrahigh Energies
• The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
• Ejective and preventative: the IllustrisTNG black hole feedback and its effects on the thermodynamics of the gas within and around galaxies
• Resolving small-scale cold circumgalactic gas in TNG50
• Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
• Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
• Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
• Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
• Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
• The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters
• Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep Survey
• CEERS Key Paper III: The Diversity of Galaxy Structure and Morphology at z=3-9 with JWST
• High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
• The redshift evolution of the binary black hole merger rate: a weighty matter
• The fraction of dark matter within galaxies from the IllustrisTNG simulations
• Jellyfish galaxies with the IllustrisTNG simulations: I. Gas-stripping phenomena in the full cosmological context
• Magnetic Field Amplification in Galaxy Clusters and its Simulation
• The Formation of Ultra-Diffuse Galaxies in Clusters
• Introducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution
• Interaction of a cold cloud with a hot wind: the regimes of cloud growth and destruction and the impact of magnetic fields
• Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations
• The ASTRID Simulation: Galaxy Formation and Reionization
• The THESAN project: properties of the intergalactic medium and its connection to Reionization-era galaxies
• Atomic and molecular gas in IllustrisTNG galaxies at low redshift
• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• The Milky Way's Disk of Classical Satellite Galaxies in Light of Gaia DR2
• The Zwicky Transient Facility Census of the Local Universe I: Systematic search for Calcium rich gap transients reveal three related spectroscopic sub-classes
• A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• Limitations to the "basic'' HOD model and beyond
• Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
• The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization
• A census of cool core galaxy clusters in IllustrisTNG
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• An Extremely Massive Quiescent Galaxy at $z=3.493$: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models
• Revealing the galaxy-halo connection in IllustrisTNG
• The effect of magnetic fields on properties of the circumgalactic medium
• 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
• Has JWST already falsified dark-matter-driven galaxy formation?
• The Hubble Sequence at $z\sim 0$ in the IllustrisTNG simulation with deep learning
• First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
• The MillenniumTNG Project: The galaxy population at $z\ge 8$
• A Deep Learning Approach to Galaxy Cluster X-ray Masses
• Fast galaxy bars continue to challenge standard cosmology
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales
• X-ray bubbles in the circumgalactic medium of TNG50 Milky Way- and M31-like galaxies: signposts of supermassive black hole activity
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• Probing Dark Low-mass Halos and Primordial Black Holes with Frequency-dependent Gravitational Lensing Dispersions of Gravitational Waves
• Convolutional neural network identification of galaxy post-mergers in UNIONS using IllustrisTNG
• The Three Hundred Project: Dynamical state of galaxy clusters and morphology from multi-wavelength synthetic maps
• The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
• Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
• 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
• Intergalactic medium dispersion measures of fast radio bursts estimated from IllustrisTNG simulation and their cosmological applications
• An unexpected high concentration for the dark substructure in the gravitational lens SDSSJ0946+1006
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• The THESAN project: ionizing escape fractions of reionization-era galaxies
• Dynamical evolution of magnetic fields in the intracluster medium
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• The fate of disk galaxies in IllustrisTNG clusters
• X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations
• The THESAN project: predictions for multi-tracer line intensity mapping in the epoch of reionization
• The buildup of strongly barred galaxies in the TNG100 simulation
• First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier
• First results from SMAUG: Uncovering the Origin of the Multiphase Circumgalactic Medium with a Comparative Analysis of Idealized and Cosmological Simulations
• Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST
• Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
• The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• A flexible modelling of galaxy assembly bias
• Statistical properties of paired fixed fields
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• Introducing SPHINX-MHD: The Impact of Primordial Magnetic Fields on the First Galaxies, Reionization, and the Global 21cm Signal
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
• Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
• Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
• Barred Galaxies in the IllustrisTNG Simulation
• How primordial magnetic fields shrink galaxies
• Expectations of the size evolution of massive galaxies at $3\le z\le 6$ from the TNG50 simulation: the CEERS/JWST view
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• Extensions to models of the galaxy-halo connection
• Fitting the nonlinear matter bispectrum by the Halofit approach
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Introducing piXedfit -- a Spectral Energy Distribution Fitting Code Designed for Resolved Sources
• The BACCO simulation project: biased tracers in real space
• Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• Is diffuse intracluster light a good tracer of the galaxy cluster matter distribution?
• Realistic simulations of galaxy formation in f(R) modified gravity
• The merger fraction of post-starburst galaxies in UNIONS
• Predictions for local PNG bias in the galaxy power spectrum and bispectrum and the consequences for $f_{\mathrm{NL}}$ constraints
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• Galaxy Evolution in all Five CANDELS Fields and IllustrisTNG: Morphological, Structural, and the Major Merger Evolution to $z\sim 3$
• The splashback boundary of haloes in hydrodynamic simulations
• How Biased Are Halo Properties in Cosmological Simulations?
• Origin and evolution of ultra-diffuse galaxies in different environments
• Baryonic effects on the matter bispectrum
• Morphological decomposition of TNG50 galaxies: methodology and catalogue
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• Direct Measurement of the HI-Halo Mass Relation through Stacking
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• The impact of magnetic fields on cold streams feeding galaxies
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• On the origin of star-gas counterrotation in low-mass galaxies
• Origin of the galaxy HI size-mass relation
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• Radial Distributions of Dwarf Satellite Systems in the Local Volume
• AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
• Seed magnetic fields in turbulent small-scale dynamos
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• Interacting galaxies in the IllustrisTNG simulations -- IV: Enhanced Supermassive Black Hole Accretion Rates in Post-Merger Galaxies
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
• Tidal evolution of galaxies in the most massive cluster of IllustrisTNG-100
• Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation
• Beyond halo mass: quenching galaxy mass assembly at the edge of filaments
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• An Excess of Globular Clusters in UDGs Formed Through Tidal Heating
• Robust Field-level Likelihood-free Inference with Galaxies
• The Progenitors of Calcium-Strong Transients
• Efficacy of early stellar feedback in low gas surface density environments
• The cold circumgalactic medium in emission: MgII halos in TNG50
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• Identifying kinematic structures in simulated galaxies using unsupervised machine learning
• A survey of the thermal and non-thermal properties of cosmic filaments
• Learning effective physical laws for generating cosmological hydrodynamics with Lagrangian Deep Learning
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• Cosmology with one galaxy?
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• Rapid Quenching of Galaxies at Cosmic Noon
• Characterizing hydrostatic mass bias with Mock-X
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relics
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• The two formation pathways of S0 galaxies
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster
• Magnetization of the intergalactic medium in the IllustrisTNG simulations: the importance of extended, outflow-driven bubbles
• Color gradients and half-mass radii of galaxies out to $z=2$ in the CANDELS/3D-HST fields: further evidence for important differences in the evolution of mass-weighted and light-weighted sizes
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• Evolution of galactic magnetic fields
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
• Is there enough star formation in simulated protoclusters?
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• Decoupling the rotation of stars and gas -- I: the relationship with morphology and halo spin
• Tidally induced warps of spiral galaxies in IllustrisTNG
• Star formation characteristics of CNN-identified post-mergers in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Constraining Magnetic Fields in the Circumgalactic Medium
• Priors on Lagrangian bias parameters from galaxy formation modelling
• Statistical modelling of the cosmological dispersion measure
• Reconstructing the Assembly of Massive Galaxies. I: The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at $z\approx 2$
• Deep Synoptic Array science: Two fast radio burst sources in massive galaxy clusters
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
• Active galactic nucleus jet feedback in hydrostatic halos
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• Galaxy formation in the brane world I: overview and first results
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754
• Magnetic buoyancy in simulated galactic discs with a realistic circum galactic medium
• Box/peanut-shaped bulges in action space
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• Evolution of primordial magnetic fields during large-scale structure formation
• 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
• Massive Black Hole Binaries from the TNG50-3 Simulation: I. Coalescence and LISA Detection Rates
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• Finding universal relations in subhalo properties with artificial intelligence
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• Formation of massive disk galaxies in the IllustrisTNG simulation
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• From large-scale environment to CGM angular momentum to star forming activities -- I: star-forming galaxies
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Deep Learning-Based Super-Resolution and De-Noising for XMM-Newton Images
• The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
• The First Quiescent Galaxies in TNG300
• 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
• Quenching Timescales in the IllustrisTNG Simulation
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• Simulating the effect of photoheating feedback during reionization
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• The connection between the escape of ionizing radiation and galaxy properties at z~3 in the Keck Lyman Continuum Spectroscopic Survey
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• The impact of galactic feedback on the shapes of dark-matter haloes
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• UV to submillimetre luminosity functions of TNG50 galaxies
• The scatter in the galaxy-halo connection: a machine learning analysis
• A deep learning view of the census of galaxy clusters in IllustrisTNG
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• Fundamental scales in the kinematic phase of the turbulent dynamo
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• Gas Accretion Can Drive Turbulence in Galaxies
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• Identifying Galaxy Mergers in Simulated CEERS NIRCam Images using Random Forests
• The cosmological dependence of halo and galaxy assembly bias
• The Physical Origin of Galactic Conformity: From Theory to Observation
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• How cosmological merger histories shape the diversity of stellar haloes
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Surrogate modelling the Baryonic Universe I: The colour of star formation
• An Intensity Mapping Constraint on the CO-Galaxy Cross Power Spectrum at Redshift ~ 3
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Bar-like galaxies in IllustrisTNG
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• Probing the cold magnetized Universe with SPICA-POL (B-BOP)
• Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Towards an Understanding of the Massive Red Spiral Galaxy Formation
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• Decoupling the rotation of stars and gas -- II: the link between black hole activity and MaNGA kinematics in TNG
• AGN in post-mergers from the Ultraviolet Near Infrared Optical Northern Survey
• Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
• Nonlinear turbulent dynamo during gravitational collapse
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• Modeling HI at the field level
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• INSPIRE: INvestigating Stellar Population In RElics II. First Data Release (DR1)
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• Towards robust determination of non-parametric morphologies in marginal astronomical data: resolving uncertainties with cosmological hydrodynamical simulations
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• SHAM through the lens of a hydrodynamical simulation
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• SDSS-IV MaNGA : spatial resolved properties of kinematically misaligned galaxies
• Strongly lensed cluster substructures are not in tension with $\Lambda$CDM
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• Conditional HI mass functions and the HI-to-halo mass relation in the local Universe
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• Characterizing Protoclusters and Protogroups at z $\sim$ 2.5 Using Ly$\alpha$ Tomography
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• 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
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• Dynamics of Intermediate-Mass Black Holes Wandering in the Milky Way Galaxy Using the Illustris TNG50 Simulation
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• Baryonic effects on CMB lensing and neutrino mass constraints
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• Weak-Lensing Detection of Intracluster Filaments in the Coma Cluster
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• The cosmic web in Lyman-alpha emission
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• A Parameter Space Exploration of Galaxy Cluster Mergers II: Effects of Magnetic Fields
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• Continuous wavelet analysis of matter clustering using the Gaussian-derived wavelet
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• The Magnetic Field Across the Molecular Warped Disk of Centaurus A
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• Non-ideal magnetohydrodynamics on a moving mesh
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
• Local Group timing argument and virial theorem mass estimators from cosmological simulations
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Do galaxies die? Different views from simulations and observations in the Local Universe
• KLLR: A scale-dependent, multivariate model class for regression analysis
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• The IllustrisTNG Simulations: Public Data Release
• The lopsided distribution of satellites of isolated central galaxies
• Lopsided galactic bars
• 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 interaction between rising bubbles and cold fronts in cool core clusters
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• Modeling Redshift-Space Clustering with Abundance Matching
• There and back again: understanding the critical properties of backsplash galaxies
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Magnetogenesis at Cosmic Dawn: Tracing the Origins of Cosmic Magnetic Fields
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath$z\gtrsim 1$
• Realistic galaxy images and improved robustness in machine learning tasks from generative modelling
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• The THESAN project: Lyman-alpha emitter luminosity function calibration
• Teaching neural networks to generate Fast Sunyaev Zel'dovich Maps
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• Understanding the early stages of galaxy formation using very metal-poor stars from the Hamburg/ESO survey
• Decaying turbulence and magnetic fields in galaxy clusters
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• Unveiling the origins of galactic bars: insights from barred and unbarred galaxies
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• The formation pathways of compact elliptical galaxies
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• Evaluating hydrodynamical simulations with green valley galaxies
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• Sensitivity reach of gamma-ray measurements for strong cosmological magnetic fields
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• The outermost edges of the Milky Way halo from galaxy kinematics
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• Planting a Lyman alpha forest on AbacusSummit
• Mock HUBS observations of hot gas with IllustrisTNG
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim 4$ gas-rich halo
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• Toward a Physical Understanding of Galaxy-Halo Alignment
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• Deep Synoptic Array Science: Implications of Faraday Rotation Measures of Localized Fast Radio Bursts
• An intergalactic medium temperature from a giant radio galaxy
• Evolution of Starburst Galaxies in the Illustris Simulation
• Disk flaring with TNG50: diversity across Milky Way and M31 analogs
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Limit on intergalactic magnetic field from ultra-high-energy cosmic ray hotspot in Perseus-Pisces region
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe
• Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation
• The cooler past of the intracluster medium in TNG-Cluster
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Lopsided Satellite Distributions around Isolated Host Galaxies in a LCDM Universe
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Intrinsic alignments of bulges and discs
• Debiased Galaxy Cluster Pressure Profiles from X-ray Observations and Simulations
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Differential rotation of the halo traced by the K-giant stars
• Three-point intrinsic alignments of dark matter halos in the IllustrisTNG simulation
• Galaxy stellar and total mass estimation using machine learning
• Mass Dependence of Galaxy-Halo Alignment in LOWZ and CMASS
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Anisotropic Satellite Galaxy Quenching: A Unique Signature of Energetic Feedback by Supermassive Black Holes?
• SDSS-IV MaNGA: Stellar population correlates with stellar root-mean-square velocity $V_{\mathrm{rms}}$ gradients or total-density-profile slopes at fixed effective velocity dispersion ${\sigma }_{\mathrm{e}}$
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
• The effect of selection -- a tale of cluster mass measurement bias induced by correlation and projection
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• The continuous wavelet derived by smoothing function and its application in cosmology
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• Off-centre supermassive black holes in bright central galaxies
• Probabilistic model for dynamic galaxy decomposition
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Intrinsic shapes of Brightest Cluster Galaxies
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• An off-centred bulge or a satellite? Hydrodynamical $N$-body simulations of the disc galaxy NGC 5474
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Formation and fate of low metallicity stars in IllustrisTNG50
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• MOSEL and IllustrisTNG: Massive Extended Galaxies at z=2 Quench Later Than Normal-size Galaxies
• Cosmology from one galaxy in a void?
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• Where binary neutron stars merge: predictions from IllustrisTNG
• Resolved star formation in TNG100 central and satellite galaxies
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• The four cosmic tidal web elements from the $\beta$-skeleton
• Baryonic Effects on Lagrangian Clustering and Angular Momentum Reconstruction
• Inflationary and phase-transitional primordial magnetic fields in galaxy clusters
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Galaxy populations in haloes in high-density environments
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• The Alcock Paczynski test with 21cm intensity field
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Metallicity beats sSFR: The connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Fingerprints of modified gravity on galaxies in voids
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• Spin speed correlations and the evolution of galaxy-halo systems
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• Role of magnetic pressure forces in fluctuation dynamo saturation
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• The contribution of magnetized galactic outflows to extragalactic Faraday rotation
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• Studying galaxy cluster morphological metrics with Mock-X
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• Measuring Galaxy Asymmetries in 3D
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• Polarised radiative transfer, rotation measure fluctuations and large-scale magnetic fields
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium III: Effects of Co-rotation and Magnetic Fields
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Living with Neighbors. IV. Dissecting the Spin$-$Orbit Alignment of Dark Matter Halos: Interacting Neighbors and the Local Large-scale Structure
• Jet interaction with galaxy cluster mergers
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Clash of Titans: a MUSE dynamical study of the extreme cluster merger SPT-CL J0307-6225
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
• The spatial distribution deviation and the power suppression of baryons from dark matter
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• Meshless Methods for Magnetohydrodynamics with Vector Potential
• Spin alignment around TNG300-1 voids
• Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• Searching for photon-ALPs mixing effects in AGN gamma-ray energy spectra
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Reoriented Memory of Galaxy Spins for the Early Universe
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Turbulence revealed by wavelet transform: power spectrum and intermittency for the velocity field of the cosmic baryonic fluid
• The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• FRB cosmology with the RM-PRS Luminosity Correlation
• 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
• 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
• A census of quiescent galaxies across $0.5<z<8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• 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
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Challenges in Cosmic Magnification Reconstruction by Magnification Response
• High-redshift AGN population in radiation-hydrodynamics simulations
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• Reorientation Rates of Structural and Kinematic Axes in Simulated Massive Galaxies and the Origins of Prolate Rotation
• Turbulence, Thermal Pressure, and Their Dynamical Effects on Cosmic Baryonic Fluid
• IFUM Integrated Field Spectroscopy of Ten M104 Satellite Galaxy Candidates
• A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5<z<2.5$
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• Densified pupil spectrograph as high-precision radial velocimetry: From direct measurement of the Universe's expansion history to characterization of nearby habitable planet candidates
• Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
• The evolution of the barred galaxy population in the TNG50 simulation
• Negligible Effects of Baryons on the Angular Momentum Scaling Relations of Galactic Dark Matter Halos
• Effects of large-scale magnetic fields on the observed composition of ultra high-energy cosmic rays
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
• How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• You Are What You Eat: The Circumgalactic Medium Around BreakBRD Galaxies has Low Mass and Angular Momentum
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• Upper limit on the axion-photon coupling from magnetic white dwarf polarization
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• Inferring halo masses with Graph Neural Networks
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• On the effects of parameters on galaxy properties in CAMELS and the predictability of ${\Omega }_{\mathrm{m}}$
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• ZFIRE -- The Gas Inflow Inequality for Satellite Galaxies in Cluster and Field Halos at z = 2
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Intergalactic magnetic field lower limits up to the redshift $z\approx 3$
• A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• The mass and redshift dependence of halo star clustering
• The Milky Way and M31 Orbital History: Did the Local Group evolve in isolation?
• On the signature of black holes on the quenched stellar mass function
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• The large-scale distribution of ionized metals in IllustrisTNG
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• The impact of cosmic filaments on the abundance of satellite galaxies
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• The Formation of Dwarf Galaxy Disks
• Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy
• Tracing black hole and galaxy growth across environments since cosmic noon
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• 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
• Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535
• Testing the role of AGN on the star formation and metal enrichment of "twin galaxies"
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
• Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
• Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
• Estimating Transient Rates from Cosmological Simulations and BPASS
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Dark Matter profiles of "in silico" galaxies: deep learning inference
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• Cavendish experiment with fast radio bursts on cosmological scales
• A Simulation Driven Deep Learning Approach for Separating Mergers and Star Forming Galaxies: The Formation Histories of Clumpy Galaxies in all the CANDELS Fields
• Stealing galaxies from galaxy clusters
• Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events
• Determining the Dark Matter distribution in galaxies with Deep Learning
• Modeling the imprints of large-scale magnetized structures on $\gamma$-rays from extragalactic transients
• Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
• DeepVoid: A Deep Learning Void Detector
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Measuring Scaling Relationships: Fitting Technique Matters
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Mesoscopic Energy Ranking Constraints in the IllustrisTNG Simulations
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• Scaling Relations in the Phase-Space Structure of Dark Matter Haloes
• Mimicking the halo-galaxy connection using machine learning
• Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
• Hydromagnetic waves in an expanding universe -- cosmological MHD code tests using analytic solutions
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
• 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
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• Identification of Compact Groups of Galaxies in IllustrisTNG300
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• The History of Galaxy Mergers in IllustrisTNG
• Spatially non-parametric recovery of intrinsic kinematic maps in pre- to post-merger galaxies
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• Inferring the mass of the circumgalactic medium using X-ray resonant scattering
• Fluctuation dynamos in supersonic turbulence at $\mathrm{Pm}\gtrsim 1$
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50