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

References in corpus (132)

• Planck 2015 results. XIII. Cosmological parameters
• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• The Global Schmidt Law in Star Forming Galaxies
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Simulating Galaxy Formation with the IllustrisTNG Model
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• Cosmological Results from High-z Supernovae
• Properties of galaxies reproduced by a hydrodynamic simulation
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• Progenitors of core-collapse supernovae
• Star Formation Histories, Abundances and Kinematics of Dwarf Galaxies in the Local Group
• Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei
• First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
• Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood
• The mass distribution and gravitational potential of the Milky Way
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• Cosmological Simulations with TreeSPH
• A model for cosmological simulations of galaxy formation physics
• Elemental Abundance Survey of The Galactic Thick Disk
• Galactic chemical evolution: Carbon through Zinc
• Stellar Chemical Signatures And Hierarchical Galaxy Formation
• The Chemical Compositions of Galactic Disk F and G Dwarfs
• ASPCAP: The Apogee Stellar Parameter and Chemical Abundances Pipeline
• Updated stellar yields from Asymptotic Giant Branch models
• A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• The Illustris simulation: the evolving population of black holes across cosmic time
• alpha-, r-, and s-process element trends in the Galactic thin and thick disks
• Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers
• Systematics of dynamical mass ejection, nucleosynthesis, and radioactively powered electromagnetic signals from neutron-star mergers
• Nearby Supernova Rates from the Lick Observatory Supernova Search. III. The Rate-Size Relation, and the Rates as a Function of Galaxy Hubble Type and Colour
• Forming Realistic Late-Type Spirals in a LCDM Universe: The Eris Simulation
• The Hamburg/ESO R-process Enhanced Star survey (HERES) II. Spectroscopic analysis of the survey sample
• A Search for Stars of Very Low Metal Abundance. VI. Detailed Abundances of 313 Metal-Poor Stars
• Formation Rates of Black Hole Accretion Disk Gamma-Ray Bursts
• The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
• Energy Input and Mass Redistribution by Supernovae in the Interstellar Medium
• R-process enrichment from a single event in an ancient dwarf galaxy
• Detailed Abundances for 28 Metal-poor Stars: Stellar Relics in the Milky Way
• The formation of disc galaxies in high resolution moving-mesh cosmological simulations
• Abundances for metal-poor stars with accurate parallaxes I. Basic data
• The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars With [Fe/H] < -3.5
• Electromagnetic Transients Powered by Nuclear Decay in the Tidal Tails of Coalescing Compact Binaries
• A physical model for cosmological simulations of galaxy formation: multi-epoch validation
• Environment and self-regulation in galaxy formation
• Nucleosynthesis in Type Ia Supernovae
• The Remarkable Deaths of 9 - 11 Solar Mass Stars
• A Study of Compact Object Mergers as Short Gamma-ray Burst Progenitors
• The delay-time distribution of type-Ia supernovae from Sloan II
• Stellar Abundances in the Solar Neighborhood: The Hypatia Catalog
• Supernova Feedback in an Inhomogeneous Interstellar Medium
• The Electromagnetic Signals of Compact Binary Mergers
• Early-Type Galaxy Archeology: Ages, Abundance Ratios, and Effective Temperatures from Full-Spectrum Fitting
• Oxygen Abundances in Nearby FGK Stars and the Galactic Chemical Evolution of the Local Disk and Halo
• Compact Binary Merger Rates: Comparison with LIGO/Virgo Upper Limits
• The long-term evolution of neutron star merger remnants - II. Radioactively powered transients
• First stars XII. Abundances in extremely metal-poor turnoff stars,and comparison with the giants
• The Metallicity Evolution of Interacting Galaxies
• Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence
• Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] < -2
• The Spatial Distribution of Coalescing Neutron Star Binaries: Implications for Gamma-Ray Bursts
• Super and Massive AGB Stars: II - Nucleosynthesis and Yields - Z=0.02, 0.008 and 0.004
• Galaxy assembly, stellar feedback and metal enrichment: the view from the GAEA model
• Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe
• Galactic r-process enrichment by neutron star mergers in cosmological simulations of a Milky Way-mass galaxy
• Type-Ia Supernova Rates to Redshift 2.4 from CLASH: the Cluster Lensing And Supernova survey with Hubble
• Abundances In Very Metal Poor Dwarf Stars
• Evolution and nucleosynthesis of asymptotic giant branch stellar models of low metallicity
• The History of R-Process Enrichment in the Milky Way
• Silver and palladium help unveil the nature of a second r-process
• The Coalescence Rate of Double Neutron Star Systems
• The origin and evolution of r- and s-process elements in the Milky Way stellar disk
• Supernova rates from the Southern inTermediate Redshift ESO Supernova Search (STRESS)
• Stellar Archaeology -- Exploring the Universe with Metal-Poor Stars
• The Core-collapse rate from the Supernova Legacy Survey
• Measuring Ages and Elemental Abundances from Unresolved Stellar Populations: Fe, Mg, C, N, and Ca
• Dissecting the Red Sequence--I. Star Formation Histories of Quiescent Galaxies: The Color-Magnitude vs. the Color-Sigma Relation
• High-Resolution Spectroscopic Study of Extremely Metal-Poor Star Candidates from the SkyMapper Survey
• Abundance scaling in stars, nebulae and galaxies
• The End of Nucleosynthesis: Production of Lead and Thorium in the Early Galaxy
• Supernovae in the Subaru Deep Field: the rate and delay-time distribution of type Ia supernovae out to redshift 2
• Overabundance of alpha-elements in exoplanet host stars
• Discovery of 90 Type Ia supernovae among 700,000 Sloan spectra: the Type-Ia supernova rate versus galaxy mass and star-formation rate at redshift ~0.1
• Chemical element ratios of SDSS early-type galaxies
• Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg] and [K/Mg] in the Milky Way
• Modelling Element Abundances in Semi-analytic Models of Galaxy Formation
• The distant Type Ia supernova rate
• Anisotropic Diffusion in Mesh-Free Numerical Magnetohydrodynamics
• Chemical Abundances of the Milky Way Thick Disk and Stellar Halo I.: Implications of [alpha/Fe] for Star Formation Histories in Their Progenitors
• Supernova rates from the SUDARE VST-Omegacam search. I
• The Extended Hubble Space Telescope Supernova Survey: The Rate of Core Collapse Supernovae to z~1
• The chemical evolution of Barium and Europium in the Milky Way
• The Galactic Nova Rate Revisited
• The Extended HST Supernova Survey: The Rate of SNe Ia at z>1.4 Remains Low
• Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey
• Abundance ratios in hierarchical galaxy formation
• The Core Collapse Supernova Rate from the SDSS-II Supernova Survey
• Evolution in the Volumetric Type Ia Supernova Rate from the Supernova Legacy Survey
• Death rate of massive stars at redshift ~0.3
• Type Ia supernova rate at a redshift of ~ 0.1
• A unified explanation for the supernova rate-galaxy mass dependency based on supernovae discovered in Sloan galaxy spectra
• A Correction to the Standard Galactic Reddening Map: Passive Galaxies as Standard Crayons
• The Rate of Supernovae at Redshift 0.1-1.0 - the Stockholm VIMOS Supernova Survey IV
• The Metallicity Dependence of the Minimum Mass for Core-Collapse Supernovae
• The chemical enrichment of the ICM from hydrodynamical simulations
• Zirconium, Barium, Lanthanum and Europium Abundances in Open Clusters
• Interpreting Short Gamma Ray Burst Progenitor Kicks and Time Delays Using the Host Galaxy-Dark Matter Halo Connection
• Compact Stellar Binary Assembly in the First Nuclear Star Clusters and r-Process Synthesis in the Early Universe
• The Distribution of Coalescing Compact Binaries in the Local Universe: Prospects for Gravitational-Wave Observations
• Europium abundances in F and G disk dwarfs
• A Stringent Limit on the Mass Production Rate of $r$-Process Elements in the Milky Way
• Following The Cosmic Evolution Of Pristine Gas I: Implications For Milky Way Halo Stars
• Estimating the Galactic Mass Profile in the Presence of Incomplete Data
• The Hubble Space Telescope Cluster Supernova Survey: VI. The Volumetric Type Ia Supernova Rate
• Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
• The Rate of Type Ia Supernovae at z~0.2 from SDSS-I Overlapping Fields
• AGN feedback and the origin of the $\alpha$ enhancement in early type galaxies - insights from the GAEA model
• Transport and mixing of r-process elements in neutron star binary merger blast waves
• Revised Supernova Rates from the IfA Deep Survey
• Halo Retention and Evolution of Coalescing Compact Binaries in Cosmological Simulations of Structure Formation: Implications for Short Gamma-Ray Bursts
• A dynamics-free lower bound on the mass of our galaxy
• Enrichment of lead (Pb) in the Galactic halo
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey
• Self-similarity in the chemical evolution of galaxies and the delay time distribution of SNe Ia
• On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium
• Implications of GRB 130603B and its macronova for r-process nucleosynthesis

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• Is there enough star formation in simulated protoclusters?
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• Star formation characteristics of CNN-identified post-mergers in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)
• Decoupling the rotation of stars and gas -- I: the relationship with morphology and halo spin
• Tidally induced warps of spiral galaxies in IllustrisTNG
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• Probabilistic Mass Mapping with Neural Score Estimation
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Active galactic nucleus jet feedback in hydrostatic halos
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• Reconstructing the Assembly of Massive Galaxies. I: The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at $z\approx 2$
• Statistical modelling of the cosmological dispersion measure
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
• Priors on Lagrangian bias parameters from galaxy formation modelling
• The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• Box/peanut-shaped bulges in action space
• Neutron star mergers as the astrophysical site of the r-process in the Milky Way and its satellite galaxies
• Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754
• Galaxy formation in the brane world I: overview and first results
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
• Massive Black Hole Binaries from the TNG50-3 Simulation: I. Coalescence and LISA Detection Rates
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• Formation of massive disk galaxies in the IllustrisTNG simulation
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Finding universal relations in subhalo properties with artificial intelligence
• 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
• North Ecliptic Pole merging galaxy catalogue
• The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• Deep Learning-Based Super-Resolution and De-Noising for XMM-Newton Images
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• Quenching Timescales in the IllustrisTNG Simulation
• The First Quiescent Galaxies in TNG300
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• 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
• Simulating the effect of photoheating feedback during reionization
• The Fornax3D project: discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427
• 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
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Evolution of the Stellar Mass-Metallicity Relation. II. Constraints on Galactic Outflows from the Mg Abundances of Quiescent Galaxies
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• A deep learning view of the census of galaxy clusters in IllustrisTNG
• The connection between the escape of ionizing radiation and galaxy properties at z~3 in the Keck Lyman Continuum Spectroscopic Survey
• The impact of galactic feedback on the shapes of dark-matter haloes
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• R-process enrichment in ultrafaint dwarf galaxies
• The scatter in the galaxy-halo connection: a machine learning analysis
• Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063
• 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
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• UV to submillimetre luminosity functions of TNG50 galaxies
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• Constraining Collapsar r-Process Models through Stellar Abundances
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• The Physical Origin of Galactic Conformity: From Theory to Observation
• Identifying Galaxy Mergers in Simulated CEERS NIRCam Images using Random Forests
• Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances
• The cosmological dependence of halo and galaxy assembly bias
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• 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
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• How cosmological merger histories shape the diversity of stellar haloes
• Elemental Abundances in M31: Gradients in the Giant Stellar Stream
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• 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
• Turbulent mixing of r-process elements in the Milky Way
• 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
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• Radiogenic Heating and its Influence on Rocky Planet Dynamos and Habitability
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Bar-like galaxies in IllustrisTNG
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• Highly r-process enhanced stars in ultra-faint dwarf galaxies
• 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
• On Neutron Star Mergers as the Source of r-process Enhanced Metal Poor Stars in the Milky Way
• Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• The impact of natal kicks on galactic r-process enrichment by neutron star mergers
• No Tension: JWST Galaxies at $z>10$ Consistent with Cosmological Simulations
• Towards an Understanding of the Massive Red Spiral Galaxy Formation
• Milky Way globular clusters on cosmological timescales. I. Evolution of the orbital parameters in time-varying potentials
• Variations of Observed Lyman-α Spectra Shapes due to the Intergalactic Absorption
• Modeling HI at the field level
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• 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
• INSPIRE: INvestigating Stellar Population In RElics II. First Data Release (DR1)
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Towards robust determination of non-parametric morphologies in marginal astronomical data: resolving uncertainties with cosmological hydrodynamical simulations
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• SHAM through the lens of a hydrodynamical simulation
• Strongly lensed cluster substructures are not in tension with $\Lambda$CDM
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• 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
• 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 $z\sim 2$
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• Conditional HI mass functions and the HI-to-halo mass relation in the local Universe
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• 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
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• 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
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• 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
• Weak-Lensing Detection of Intracluster Filaments in the Coma Cluster
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
• 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
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• Baryonic effects on CMB lensing and neutrino mass constraints
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• The cosmic web in Lyman-alpha emission
• Continuous wavelet analysis of matter clustering using the Gaussian-derived wavelet
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Neutron-capture elements in dwarf galaxies I: Chemical clocks & the short timescale of the r-process
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• Effects of Baryonic Feedback on the Cosmic Web
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• 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
• Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• The Gaia-ESO Survey: Oxygen abundance in the Galactic thin and thick disks
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• The Stars in M15 Were Born with the r-process
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• 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
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The IllustrisTNG Simulations: Public Data Release
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• KLLR: A scale-dependent, multivariate model class for regression analysis
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• The lopsided distribution of satellites of isolated central galaxies
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• 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 Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Modeling Redshift-Space Clustering with Abundance Matching
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• 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
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• The Dispersion Measure Contributions of the Cosmic Web
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• There and back again: understanding the critical properties of backsplash galaxies
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• 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$z\gtrsim 1$
• The evolutionary pathways of disk galaxies with different sizes
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Rosella: A mock catalogue from the P-Millennium simulation
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• The THESAN project: Lyman-alpha emitter luminosity function calibration
• Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field
• 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
• Teaching neural networks to generate Fast Sunyaev Zel'dovich Maps
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Realistic galaxy images and improved robustness in machine learning tasks from generative modelling
• BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
• Understanding the early stages of galaxy formation using very metal-poor stars from the Hamburg/ESO survey
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
• Lopsided galactic disks in IllustrisTNG
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• The mass-metallicity and fundamental metallicity relations in non-AGN and AGN-host galaxies
• The role of AGN on the structure, kinematics and evolution of ETGs in the Horizon simulations
• Unveiling the origins of galactic bars: insights from barred and unbarred galaxies
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• The Gaia-ESO survey: placing constraints on the origin of r-process elements
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• 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
• Merging galaxy clusters in IllustrisTNG
• 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
• The formation pathways of compact elliptical galaxies
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• s-process Enirchment of Ultrafaint Dwarf Galaxies
• 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
• Evaluating hydrodynamical simulations with green valley galaxies
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• Planting a Lyman alpha forest on AbacusSummit
• Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim 4$ gas-rich halo
• Mock HUBS observations of hot gas with IllustrisTNG
• 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
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• Evolution of central galaxy alignments in simulations
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• Toward a Physical Understanding of Galaxy-Halo Alignment
• 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
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• 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
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• Disk flaring with TNG50: diversity across Milky Way and M31 analogs
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Evolution of Starburst Galaxies in the Illustris Simulation
• An intergalactic medium temperature from a giant radio galaxy
• Formation of a barred galaxy in a major merger: The role of AGN feedback
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Intrinsic alignments of bulges and discs
• Lopsided Satellite Distributions around Isolated Host Galaxies in a LCDM Universe
• MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Galaxy stellar and total mass estimation using machine learning
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Differential rotation of the halo traced by the K-giant stars
• The CO universe: Modelling CO emission and H${}_2$ abundance in cosmological galaxy formation simulations
• Debiased Galaxy Cluster Pressure Profiles from X-ray Observations and Simulations
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• 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
• Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation
• Mass Dependence of Galaxy-Halo Alignment in LOWZ and CMASS
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• The cooler past of the intracluster medium in TNG-Cluster
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Anisotropic Satellite Galaxy Quenching: A Unique Signature of Energetic Feedback by Supermassive Black Holes?
• Imprint of baryons and massive neutrinos on velocity statistics
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• The continuous wavelet derived by smoothing function and its application in cosmology
• 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 ${\sigma }_{\mathrm{e}}$
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Milky Way globular clusters on cosmological timescales. II. Interaction with the Galactic centre
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• 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
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Formation of super-thin galaxies in Illustris-TNG
• MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• The effect of selection -- a tale of cluster mass measurement bias induced by correlation and projection
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Intrinsic shapes of Brightest Cluster Galaxies
• Formation and fate of low metallicity stars in IllustrisTNG50
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• Europium enrichment and hierarchical formation of the Galactic halo
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• Constraints on the frequency and mass content of r-process events derived from turbulent mixing in galactic disks
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• MusE GAs FLOw and Wind (MEGAFLOW) XIII. Cool gas traced by MgII around isolated galaxies
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• 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
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• Probabilistic model for dynamic galaxy decomposition
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Off-centre supermassive black holes in bright central galaxies
• Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• The Alcock Paczynski test with 21cm intensity field
• Mass-morphology relation of TNG50 galaxies
• MOSEL and IllustrisTNG: Massive Extended Galaxies at z=2 Quench Later Than Normal-size Galaxies
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• 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 mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• 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
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• The four cosmic tidal web elements from the $\beta$-skeleton
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• Where binary neutron stars merge: predictions from IllustrisTNG
• What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• 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
• Cosmology from one galaxy in a void?
• Enrichment of the Galactic disc with neutron-capture elements: Gd, Dy, and Th
• Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• The origin and properties of red spirals: Insights from cosmological simulations
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• Resolved star formation in TNG100 central and satellite galaxies
• Chemodynamic evolution of Sun-like stars in nearby moving groups
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• Galaxy populations in protoclusters at cosmic noon
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
• Metallicity beats sSFR: The connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
• 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
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• The diverse physical origins of stars in the dynamically hot bulge: CALIFA vs. IllustrisTNG
• The contribution of magnetized galactic outflows to extragalactic Faraday rotation
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
• Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• 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
• The formation of compact massive relic galaxies in MOND
• Studying galaxy cluster morphological metrics with Mock-X
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Preprocessing in small groups: Three simulated galaxies interacting prior to cluster infall
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Measuring Galaxy Asymmetries in 3D
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Realistic consecutive galaxy mergers form eccentric PTA sources
• Determining the time before or after a galaxy merger event
• Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• The effects of the orbital configurations of mergers on reshaping galaxy structures
• 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
• Exploring the physical origins of halo assembly bias from early times
• A new long gamma-ray burst formation pathway at solar metallicity
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• 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
• 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
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
• 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 power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
• The galaxy bias profile of cosmic voids
• The spatial distribution deviation and the power suppression of baryons from dark matter
• Clash of Titans: a MUSE dynamical study of the extreme cluster merger SPT-CL J0307-6225
• Polynomial expansion of the star formation history in galaxies
• Stellar Migration and Chemical Enrichment in the Milky Way Disc: A Hybrid Model
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Living with Neighbors. IV. Dissecting the Spin$-$Orbit Alignment of Dark Matter Halos: Interacting Neighbors and the Local Large-scale Structure
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
• The neutron-capture and alpha-elements abundance ratios scatter in old stellar populations. Cosmological simulations of the stellar halo
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• 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
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• 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
• On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• Constraint on magnetized galactic outflows from LOFAR rotation measure data
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• Robust machine learning model of inferring the ex-situ stellar fraction of galaxies from photometric data
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• Turbulence revealed by wavelet transform: power spectrum and intermittency for the velocity field of the cosmic baryonic fluid
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• 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
• The VANDELS Survey: Star formation and quenching in two over-densities at 3 < z < 4
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Spin alignment around TNG300-1 voids
• 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
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
• Negligible Effects of Baryons on the Angular Momentum Scaling Relations of Galactic Dark Matter Halos
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• Reorientation Rates of Structural and Kinematic Axes in Simulated Massive Galaxies and the Origins of Prolate Rotation
• 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
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Turbulence, Thermal Pressure, and Their Dynamical Effects on Cosmic Baryonic Fluid
• Challenges in Cosmic Magnification Reconstruction by Magnification Response
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• The evolution of the barred galaxy population in the TNG50 simulation
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type galaxies
• IFUM Integrated Field Spectroscopy of Ten M104 Satellite Galaxy Candidates
• Physically motivated modeling of LyC escape fraction during reionization
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• Densified pupil spectrograph as high-precision radial velocimetry: From direct measurement of the Universe's expansion history to characterization of nearby habitable planet candidates
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Effects of large-scale magnetic fields on the observed composition of ultra high-energy cosmic rays
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Gaussian Lagrangian Galaxy Bias
• Inferring halo masses with Graph Neural Networks
• Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• 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
• Estimating infall times of galaxies around clusters: how accurately can it be done with observational data?
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Major merger fraction along the massive galaxy quenching channel at 0.2$<z<$0.7
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• Tidally induced bar-like galaxies in simulated clusters
• The oldest tidally induced bar-like galaxy in the IllustrisTNG cluster
• MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z$\sim$2
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• 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
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• zELDA II: reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• ZFIRE -- The Gas Inflow Inequality for Satellite Galaxies in Cluster and Field Halos at z = 2
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• You Are What You Eat: The Circumgalactic Medium Around BreakBRD Galaxies has Low Mass and Angular Momentum
• Tracing black hole and galaxy growth across environments since cosmic noon
• The major merger-active galactic nucleus connection up to the cosmic noon
• 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
• Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ~ 0.8 with BOSS and DESI
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• The multi-component fitting to the star formation histories in the TNG simulation
• Galaxy-halo internal alignments across cosmic time
• Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• The Formation of Dwarf Galaxy Disks
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• The impact of cosmic filaments on the abundance of satellite galaxies
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• The merger-driven evolution of massive early-type galaxies
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• A statistical method for the identification of stars enriched in neutron-capture elements from medium-resolution spectra
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• On the signature of black holes on the quenched stellar mass function
• Distribution of Europium in The Milky Way Disk; Its Connection to Planetary Habitability and The Source of The R-Process
• The Milky Way and M31 Orbital History: Did the Local Group evolve in isolation?
• Disc instability and bar formation: view from the IllustrisTNG simulations
• The mass and redshift dependence of halo star clustering
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• The assembly history of NGC 1365 through chemical archaeology
• The Tremaine-Weinberg method at high redshifts
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
• The large-scale distribution of ionized metals in IllustrisTNG
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• DeepVoid: A Deep Learning Void Detector
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Stellar Abundances at the Center of Early Type Galaxies with Fine Structure
• Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
• Stealing galaxies from galaxy clusters
• Mimicking the halo-galaxy connection using machine learning
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• The dynamical lineage of ultra-diffuse galaxies from TNG50-1
• Identification of Compact Groups of Galaxies in IllustrisTNG300
• A Simulation Driven Deep Learning Approach for Separating Mergers and Star Forming Galaxies: The Formation Histories of Clumpy Galaxies in all the CANDELS Fields
• The History of Galaxy Mergers in IllustrisTNG
• Scaling Relations in the Phase-Space Structure of Dark Matter Haloes
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
• Spatially non-parametric recovery of intrinsic kinematic maps in pre- to post-merger galaxies
• Mesoscopic Energy Ranking Constraints in the IllustrisTNG Simulations
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• Quasar clustering at redshift 6
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
• Determining the Dark Matter distribution in galaxies with Deep Learning
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• Cavendish experiment with fast radio bursts on cosmological scales
• Dark Matter profiles of "in silico" galaxies: deep learning inference
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• 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
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
• 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
• Inferring the mass of the circumgalactic medium using X-ray resonant scattering
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• 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
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Measuring Scaling Relationships: Fitting Technique Matters
• The Distribution of Satellite Galaxies in the TNG100 Simulation