First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium

Abstract

The distribution of elements in galaxies provides a wealth of information about their production sites and their subsequent mixing into the interstellar medium. Here we investigate the distribution of elements within stars in the IllustrisTNG simulations. In particular, we analyze the abundance ratios of magnesium and europium in Milky Way-like galaxies from the TNG100 simulation (stellar masses $\log (M_{\star }/{\mathrm{M}}_{\odot })\sim 9.7-11.2$). As abundances of magnesium and europium for individual stars in the Milky Way are observed across a variety of spatial locations and metallicities, comparison with the stellar abundances in our more than $850$ Milky Way-like galaxies provides stringent constraints on our chemical evolutionary methods. To this end we use the magnesium to iron ratio as a proxy for the effects of our SNII and SNIa metal return prescription, and a means to compare our simulated abundances to a wide variety of galactic observations. The europium to iron ratio tracks the rare ejecta from neutron star -- neutron star mergers, the assumed primary site of europium production in our models, which in turn is a sensitive probe of the effects of metal diffusion within the gas in our simulations. We find that europium abundances in Milky Way-like galaxies show no correlation with assembly history, present day galactic properties, and average galactic stellar population age. In general, we reproduce the europium to iron spread at low metallicities observed in the Milky Way, with the level of enhancement being sensitive to gas properties during redshifts $z\approx 2-4$. We show that while the overall normalization of [Eu/Fe] is susceptible to resolution and post-processing assumptions, the relatively large spread of [Eu/Fe] at low [Fe/H] when compared to that at high [Fe/H] is very robust.

18 pages, 14 figures, accepted to MNRAS

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• Gas Accretion Can Drive Turbulence in Galaxies
• The cosmological dependence of halo and galaxy assembly bias
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances
• Identifying Galaxy Mergers in Simulated CEERS NIRCam Images using Random Forests
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Radiogenic Heating and its Influence on Rocky Planet Dynamos and Habitability
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• An Intensity Mapping Constraint on the CO-Galaxy Cross Power Spectrum at Redshift ~ 3
• How cosmological merger histories shape the diversity of stellar haloes
• Elemental Abundances in M31: Gradients in the Giant Stellar Stream
• Turbulent mixing of r-process elements in the Milky Way
• Surrogate modelling the Baryonic Universe I: The colour of star formation
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Bar-like galaxies in IllustrisTNG
• The MillenniumTNG Project: The large-scale clustering of galaxies
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• 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
• On Neutron Star Mergers as the Source of r-process Enhanced Metal Poor Stars in the Milky Way
• Highly r-process enhanced stars in ultra-faint dwarf galaxies
• Towards an Understanding of the Massive Red Spiral Galaxy Formation
• AGN in post-mergers from the Ultraviolet Near Infrared Optical Northern Survey
• No Tension: JWST Galaxies at $z>10$ Consistent with Cosmological Simulations
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
• Decoupling the rotation of stars and gas -- II: the link between black hole activity and MaNGA kinematics in TNG
• The impact of natal kicks on galactic r-process enrichment by neutron star mergers
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Modeling HI at the field level
• Milky Way globular clusters on cosmological timescales. I. Evolution of the orbital parameters in time-varying potentials
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• Variations of Observed Lyman-α Spectra Shapes due to the Intergalactic Absorption
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• 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
• INSPIRE: INvestigating Stellar Population In RElics II. First Data Release (DR1)
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• SHAM through the lens of a hydrodynamical simulation
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• Strongly lensed cluster substructures are not in tension with $\Lambda$CDM
• The R-Process Alliance: Fifth Data Release from the Search for R-Process-Enhanced Metal-poor Stars in the Galactic Halo with the GTC
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• 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
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Characterizing Protoclusters and Protogroups at z $\sim$ 2.5 Using Ly$\alpha$ Tomography
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• SDSS-IV MaNGA : spatial resolved properties of kinematically misaligned galaxies
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• 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
• 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
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• Weak-Lensing Detection of Intracluster Filaments in the Coma Cluster
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• Dynamics of Intermediate-Mass Black Holes Wandering in the Milky Way Galaxy Using the Illustris TNG50 Simulation
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• Baryonic effects on CMB lensing and neutrino mass constraints
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Continuous wavelet analysis of matter clustering using the Gaussian-derived wavelet
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• The cosmic web in Lyman-alpha emission
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Effects of Baryonic Feedback on the Cosmic Web
• Neutron-capture elements in dwarf galaxies I: Chemical clocks & the short timescale of the r-process
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• Local Group timing argument and virial theorem mass estimators from cosmological simulations
• The Stars in M15 Were Born with the r-process
• Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields
• The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
• A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
• 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
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• The Gaia-ESO Survey: Oxygen abundance in the Galactic thin and thick disks
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• KLLR: A scale-dependent, multivariate model class for regression analysis
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The IllustrisTNG Simulations: Public Data Release
• Lopsided galactic bars
• The lopsided distribution of satellites of isolated central galaxies
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• The Dispersion Measure Contributions of the Cosmic Web
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• Modeling Redshift-Space Clustering with Abundance Matching
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• There and back again: understanding the critical properties of backsplash galaxies
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Constraining Delay Time Distribution of Binary Neutron Star Mergers from Host Galaxy Properties
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• 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
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Realistic galaxy images and improved robustness in machine learning tasks from generative modelling
• Rosella: A mock catalogue from the P-Millennium simulation
• 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
• BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• The evolutionary pathways of disk galaxies with different sizes
• Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• 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
• When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath$z\gtrsim 1$
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• The THESAN project: Lyman-alpha emitter luminosity function calibration
• Teaching neural networks to generate Fast Sunyaev Zel'dovich Maps
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• The role of AGN on the structure, kinematics and evolution of ETGs in the Horizon simulations
• The mass-metallicity and fundamental metallicity relations in non-AGN and AGN-host galaxies
• Lopsided galactic disks in IllustrisTNG
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
• Understanding the early stages of galaxy formation using very metal-poor stars from the Hamburg/ESO survey
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• Unveiling the origins of galactic bars: insights from barred and unbarred galaxies
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• Merging galaxy clusters in IllustrisTNG
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Evaluating hydrodynamical simulations with green valley galaxies
• The outermost edges of the Milky Way halo from galaxy kinematics
• The formation pathways of compact elliptical galaxies
• s-process Enirchment of Ultrafaint Dwarf Galaxies
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• The Gaia-ESO survey: placing constraints on the origin of r-process elements
• Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
• Evolution of central galaxy alignments in simulations
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• Planting a Lyman alpha forest on AbacusSummit
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim 4$ gas-rich halo
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Mock HUBS observations of hot gas with IllustrisTNG
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• Disk flaring with TNG50: diversity across Milky Way and M31 analogs
• Supernova-driven turbulent metal mixing in high redshift galactic disks: metallicity fluctuations in the interstellar medium and its imprints on metal poor stars in the Milky Way
• Formation of a barred galaxy in a major merger: The role of AGN feedback
• An intergalactic medium temperature from a giant radio galaxy
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• Toward a Physical Understanding of Galaxy-Halo Alignment
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Evolution of Starburst Galaxies in the Illustris Simulation
• Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• The cooler past of the intracluster medium in TNG-Cluster
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• 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
• Galaxy stellar and total mass estimation using machine learning
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Mass Dependence of Galaxy-Halo Alignment in LOWZ and CMASS
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Anisotropic Satellite Galaxy Quenching: A Unique Signature of Energetic Feedback by Supermassive Black Holes?
• Lopsided Satellite Distributions around Isolated Host Galaxies in a LCDM Universe
• Debiased Galaxy Cluster Pressure Profiles from X-ray Observations and Simulations
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Differential rotation of the halo traced by the K-giant stars
• MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe
• The CO universe: Modelling CO emission and H${}_2$ abundance in cosmological galaxy formation simulations
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Three-point intrinsic alignments of dark matter halos in the IllustrisTNG simulation
• Merger Effects on the Spin and Shape Alignments of Galaxy Stellar, Cold and Hot Gas, and Dark Matter Components
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Intrinsic alignments of bulges and discs
• Imprint of baryons and massive neutrinos on velocity statistics
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• 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
• MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation
• Formation of super-thin galaxies in Illustris-TNG
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• 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 ${\sigma }_{\mathrm{e}}$
• The continuous wavelet derived by smoothing function and its application in cosmology
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Milky Way globular clusters on cosmological timescales. III. Interaction rates
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Milky Way globular clusters on cosmological timescales. II. Interaction with the Galactic centre
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Intrinsic shapes of Brightest Cluster Galaxies
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Off-centre supermassive black holes in bright central galaxies
• An off-centred bulge or a satellite? Hydrodynamical $N$-body simulations of the disc galaxy NGC 5474
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Probabilistic model for dynamic galaxy decomposition
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Formation and fate of low metallicity stars in IllustrisTNG50
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• Constraints on the frequency and mass content of r-process events derived from turbulent mixing in galactic disks
• Europium enrichment and hierarchical formation of the Galactic halo
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• 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
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• MusE GAs FLOw and Wind (MEGAFLOW) XIII. Cool gas traced by MgII around isolated galaxies
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• Where binary neutron stars merge: predictions from IllustrisTNG
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Mass-morphology relation of TNG50 galaxies
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• The Alcock Paczynski test with 21cm intensity field
• Enrichment of the Galactic disc with neutron-capture elements: Gd, Dy, and Th
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• Galaxy populations in haloes in high-density environments
• The origin and properties of red spirals: Insights from cosmological simulations
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• The four cosmic tidal web elements from the $\beta$-skeleton
• What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
• Cosmology from one galaxy in a void?
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• Chemodynamic evolution of Sun-like stars in nearby moving groups
• MOSEL and IllustrisTNG: Massive Extended Galaxies at z=2 Quench Later Than Normal-size Galaxies
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Resolved star formation in TNG100 central and satellite galaxies
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• The diverse physical origins of stars in the dynamically hot bulge: CALIFA vs. IllustrisTNG
• Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
• Galaxy populations in protoclusters at cosmic noon
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• 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
• The formation of compact massive relic galaxies in MOND
• Metallicity beats sSFR: The connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
• MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
• 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
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• Measuring Galaxy Asymmetries in 3D
• Realistic consecutive galaxy mergers form eccentric PTA sources
• The effects of the orbital configurations of mergers on reshaping galaxy structures
• Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Determining the time before or after a galaxy merger event
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Exploring the physical origins of halo assembly bias from early times
• Preprocessing in small groups: Three simulated galaxies interacting prior to cluster infall
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• A new long gamma-ray burst formation pathway at solar metallicity
• An interesting case of the formation and evolution of a barred galaxy in the cosmological context
• FIRST J1419+3940 as the First Observed Radio Flare from a Neutron Star Merger
• The spatial distribution deviation and the power suppression of baryons from dark matter
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• 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
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• 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
• Polynomial expansion of the star formation history in galaxies
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• A Sagittarius-like simulated dwarf spheroidal galaxy from TNG50
• Stellar Migration and Chemical Enrichment in the Milky Way Disc: A Hybrid Model
• Living with Neighbors. IV. Dissecting the Spin$-$Orbit Alignment of Dark Matter Halos: Interacting Neighbors and the Local Large-scale Structure
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• The galaxy bias profile of cosmic voids
• Clash of Titans: a MUSE dynamical study of the extreme cluster merger SPT-CL J0307-6225
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• The VANDELS Survey: Star formation and quenching in two over-densities at 3 < z < 4
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Spin alignment around TNG300-1 voids
• 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
• 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
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• Reoriented Memory of Galaxy Spins for the Early Universe
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation
• Robust machine learning model of inferring the ex-situ stellar fraction of galaxies from photometric data
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Constraint on magnetized galactic outflows from LOFAR rotation measure data
• 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
• 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
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
• Untangling Stellar Components of Galaxies: Evaluation of Dynamical Decomposition Methods in Simulated Galaxies with GalaxyChop
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• The neutron-capture and alpha-elements abundance ratios scatter in old stellar populations. Cosmological simulations of the stellar halo
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Challenges in Cosmic Magnification Reconstruction by Magnification Response
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Effects of large-scale magnetic fields on the observed composition of ultra high-energy cosmic rays
• Reorientation Rates of Structural and Kinematic Axes in Simulated Massive Galaxies and the Origins of Prolate Rotation
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• Turbulence, Thermal Pressure, and Their Dynamical Effects on Cosmic Baryonic Fluid
• Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
• 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
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type galaxies
• The evolution of the barred galaxy population in the TNG50 simulation
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament 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
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• Negligible Effects of Baryons on the Angular Momentum Scaling Relations of Galactic Dark Matter Halos
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• IFUM Integrated Field Spectroscopy of Ten M104 Satellite Galaxy Candidates
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?
• Physically motivated modeling of LyC escape fraction during reionization
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• The oldest tidally induced bar-like galaxy in the IllustrisTNG cluster
• Gaussian Lagrangian Galaxy Bias
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Tidally induced bar-like galaxies in simulated clusters
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Major merger fraction along the massive galaxy quenching channel at 0.2$<z<$0.7
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• zELDA II: reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z$\sim$2
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Estimating infall times of galaxies around clusters: how accurately can it be done with observational data?
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• You Are What You Eat: The Circumgalactic Medium Around BreakBRD Galaxies has Low Mass and Angular Momentum
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
• Assessing the connection between galactic conformity and assembly-type bias
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• ZFIRE -- The Gas Inflow Inequality for Satellite Galaxies in Cluster and Field Halos at z = 2
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Exploring the halo-galaxy connection with probabilistic approaches
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Inferring halo masses with Graph Neural Networks
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• The Milky Way and M31 Orbital History: Did the Local Group evolve in isolation?
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• On the signature of black holes on the quenched stellar mass function
• The large-scale distribution of ionized metals in IllustrisTNG
• The mass and redshift dependence of halo star clustering
• All the Massive Galaxy Overdensities during Reionization: JWST Rest-Frame Optical Selection Reveals Young, Chemically Evolved Galaxies Embedded in Dense, Neutral Gas at z > 5
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• The Formation of Dwarf Galaxy Disks
• The Tremaine-Weinberg method at high redshifts
• Tracing black hole and galaxy growth across environments since cosmic noon
• Distribution of Europium in The Milky Way Disk; Its Connection to Planetary Habitability and The Source of The R-Process
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• The merger-driven evolution of massive early-type galaxies
• The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
• The major merger-active galactic nucleus connection up to the cosmic noon
• The multi-component fitting to the star formation histories in the TNG simulation
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• Galaxy-halo internal alignments across cosmic time
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• The impact of cosmic filaments on the abundance of satellite galaxies
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• A statistical method for the identification of stars enriched in neutron-capture elements from medium-resolution spectra
• The assembly history of NGC 1365 through chemical archaeology
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ~ 0.8 with BOSS and DESI
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Determining the Dark Matter distribution in galaxies with Deep Learning
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• The dynamical lineage of ultra-diffuse galaxies from TNG50-1
• Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• Stealing galaxies from galaxy clusters
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• Identification of Compact Groups of Galaxies in IllustrisTNG300
• 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
• DeepVoid: A Deep Learning Void Detector
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• Measuring Scaling Relationships: Fitting Technique Matters
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Cavendish experiment with fast radio bursts on cosmological scales
• Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• The Fornax Deep Survey (FDS) with the VST: III. Low Surface Brightness (LSB) dwarfs and Ultra Diffuse Galaxies (UDGs) in the center of the Fornax cluster
• Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
• Stellar Abundances at the Center of Early Type Galaxies with Fine Structure
• A Simulation Driven Deep Learning Approach for Separating Mergers and Star Forming Galaxies: The Formation Histories of Clumpy Galaxies in all the CANDELS Fields
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• Quasar clustering at redshift 6
• The History of Galaxy Mergers in IllustrisTNG
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
• Inferring the mass of the circumgalactic medium using X-ray resonant scattering
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Mimicking the halo-galaxy connection using machine learning
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• Mesoscopic Energy Ranking Constraints in the IllustrisTNG Simulations
• Spatially non-parametric recovery of intrinsic kinematic maps in pre- to post-merger galaxies
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Scaling Relations in the Phase-Space Structure of Dark Matter Haloes
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Dark Matter profiles of "in silico" galaxies: deep learning inference