First results from the IllustrisTNG simulations: matter and galaxy clustering

Abstract

Hydrodynamical simulations of galaxy formation have now reached sufficient volume to make precision predictions for clustering on cosmologically relevant scales. Here we use our new IllustrisTNG simulations to study the non-linear correlation functions and power spectra of baryons, dark matter, galaxies and haloes over an exceptionally large range of scales. We find that baryonic effects increase the clustering of dark matter on small scales and damp the total matter power spectrum on scales up to k ~ 10 h/Mpc by 20%. The non-linear two-point correlation function of the stellar mass is close to a power-law over a wide range of scales and approximately invariant in time from very high redshift to the present. The two-point correlation function of the simulated galaxies agrees well with SDSS at its mean redshift z ~ 0.1, both as a function of stellar mass and when split according to galaxy colour, apart from a mild excess in the clustering of red galaxies in the stellar mass range 10^9-10^10 Msun/h^2. Given this agreement, the TNG simulations can make valuable theoretical predictions for the clustering bias of different galaxy samples. We find that the clustering length of the galaxy auto-correlation function depends strongly on stellar mass and redshift. Its power-law slope gamma is nearly invariant with stellar mass, but declines from gamma ~ 1.8 at redshift z=0 to gamma ~ 1.6 at redshift z ~ 1, beyond which the slope steepens again. We detect significant scale-dependencies in the bias of different observational tracers of large-scale structure, extending well into the range of the baryonic acoustic oscillations and causing nominal (yet fortunately correctable) shifts of the acoustic peaks of around ~5%.

accepted by MNRAS, 21 figures, 24 pages, updated to match published version. For IllustrisTNG visualizations see http://www.tng-project.org

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• Effects of baryons on weak lensing peak statistics
• Active galactic nucleus jet feedback in hydrostatic halos
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Priors on Lagrangian bias parameters from galaxy formation modelling
• Reconstructing the Assembly of Massive Galaxies. I: The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at $z\approx 2$
• Probing Dark Matter Self-interaction with Ultra-faint Dwarf Galaxies
• Statistical modelling of the cosmological dispersion measure
• Box/peanut-shaped bulges in action space
• The boundary of cosmic filaments
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• Galaxy formation in the brane world I: overview and first results
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
• Beyond UVJ: Color Selection of Galaxies in the JWST Era
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• Massive Black Hole Binaries from the TNG50-3 Simulation: I. Coalescence and LISA Detection Rates
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Formation of massive disk galaxies in the IllustrisTNG simulation
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• 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
• Finding universal relations in subhalo properties with artificial intelligence
• The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Deep Learning-Based Super-Resolution and De-Noising for XMM-Newton Images
• 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
• From large-scale environment to CGM angular momentum to star forming activities -- I: star-forming galaxies
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• North Ecliptic Pole merging galaxy catalogue
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• Quenching Timescales in the IllustrisTNG Simulation
• 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
• Exploring a new definition of the green valley and its implications
• The First Quiescent Galaxies in TNG300
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• 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
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
• Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Reaching for the Edge I: Probing the Outskirts of Massive Galaxies with HSC, DECaLS, SDSS, and Dragonfly
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Simulating the effect of photoheating feedback during reionization
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• The impact of galactic feedback on the shapes of dark-matter haloes
• The connection between the escape of ionizing radiation and galaxy properties at z~3 in the Keck Lyman Continuum Spectroscopic Survey
• UV to submillimetre luminosity functions of TNG50 galaxies
• The scatter in the galaxy-halo connection: a machine learning analysis
• A deep learning view of the census of galaxy clusters in IllustrisTNG
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• An 8.0\% Determination of the Baryon Fraction in the Intergalactic Medium from Localized Fast Radio Bursts
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems
• Cosmic Evolution of Barred Galaxies up to z ~ 0.84
• The cosmological dependence of halo and galaxy assembly bias
• The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
• J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
• Stellar halos from The Dragonfly Edge-on Galaxies Survey
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• Gas Accretion Can Drive Turbulence in Galaxies
• The Physical Origin of Galactic Conformity: From Theory to Observation
• On the Co-Orbitation of Satellite Galaxies Along the Great Plane of Andromeda: NGC 147, NGC 185, and Expectations from Cosmological Simulations
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• The impact of Lyman-$\alpha$ radiative transfer on large-scale clustering in the Illustris simulation
• Identifying Galaxy Mergers in Simulated CEERS NIRCam Images using Random Forests
• An Intensity Mapping Constraint on the CO-Galaxy Cross Power Spectrum at Redshift ~ 3
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• How cosmological merger histories shape the diversity of stellar haloes
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Power Spectrum of Intrinsic Alignments of Galaxies in IllustrisTNG
• A Graphical Interpretation of Circumgalactic Precipitation
• 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
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Cosmic evolution of radio-AGN feedback: confronting models with data
• Bar-like galaxies in IllustrisTNG
• Towards an improved model of self-interacting dark matter haloes
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• The MillenniumTNG Project: The large-scale clustering of galaxies
• 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
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Cosmological Constraints from the eBOSS Lyman-$\alpha$ Forest using the PRIYA Simulations
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• The origin of the relation between metallicity and size in star-forming galaxies
• AGN in post-mergers from the Ultraviolet Near Infrared Optical Northern Survey
• Decoupling the rotation of stars and gas -- II: the link between black hole activity and MaNGA kinematics in TNG
• Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
• Towards an Understanding of the Massive Red Spiral Galaxy Formation
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• The Halo Void (Dust) Model of Large Scale Structure
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Filament rotation in the California L1482 cloud
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• Milky Way globular clusters on cosmological timescales. I. Evolution of the orbital parameters in time-varying potentials
• Direct measurement of the distribution of dark matter with strongly lensed gravitational waves
• The halo light cone catalogues of \Abacus{AbacusSummit}
• Modeling HI at the field level
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Statistical correlation between the distribution of Ly$\alpha$ emitters and IGM HI at $z\sim 2.2$ mapped by Subaru/Hyper Suprime-Cam
• Total mass density slopes of early-type galaxies using Jeans dynamical modelling at redshifts $0.29<z<0.55$
• Variations of Observed Lyman-α Spectra Shapes due to the Intergalactic Absorption
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• SHAM through the lens of a hydrodynamical simulation
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• INSPIRE: INvestigating Stellar Population In RElics II. First Data Release (DR1)
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• 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
• Towards robust determination of non-parametric morphologies in marginal astronomical data: resolving uncertainties with cosmological hydrodynamical simulations
• LoCuSS: The splashback radius of massive galaxy clusters and its dependence on cluster merger history
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• The cosmic build-up of dust and metals. Accurate abundances from GRB-selected star-forming galaxies at $1.7<z<6.3$
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• SDSS-IV MaNGA : spatial resolved properties of kinematically misaligned galaxies
• The halo mass function of late-type galaxies from HI kinematics
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• The FLAMINGO project: Baryon effects on the matter power spectrum
• 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
• Kinematics of the diffuse intragroup and intracluster light in groups and clusters of galaxies in the Local Universe within 100 Mpc distance
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• 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
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Strongly lensed cluster substructures are not in tension with $\Lambda$CDM
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$). Mass budget, satellites spin alignment and gas infall in a massive $z\sim 3$ quasar host halo
• An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
• Baryonic effects on CMB lensing and neutrino mass constraints
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Dynamics of Intermediate-Mass Black Holes Wandering in the Milky Way Galaxy Using the Illustris TNG50 Simulation
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• Weak-Lensing Detection of Intracluster Filaments in the Coma Cluster
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• The HectoMAP Cluster Survey: Spectroscopically Identified Clusters and their Brightest Cluster Galaxies (BCGs)
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• The large-scale environment from cosmological simulations II: The redshift evolution and distributions of baryons
• The cosmic web in Lyman-alpha emission
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• Continuous wavelet analysis of matter clustering using the Gaussian-derived wavelet
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Effects of Baryonic Feedback on the Cosmic Web
• Probing primordial non-Gaussianity with Fast Radio Bursts
• Local Group timing argument and virial theorem mass estimators from cosmological simulations
• Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• 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
• A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• Ram pressure stripping of HI-rich galaxies infalling into massive clusters
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• The lopsided distribution of satellites of isolated central galaxies
• Dark matter substructures affect dark matter-electron scattering in xenon-based direct detection experiments
• Estimating redshift distributions using Hierarchical Logistic Gaussian processes
• A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• Lopsided galactic bars
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The IllustrisTNG Simulations: Public Data Release
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• KLLR: A scale-dependent, multivariate model class for regression analysis
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Modeling Redshift-Space Clustering with Abundance Matching
• WALLABY Pre-Pilot and Pilot Survey: the Tully Fisher Relation in Eridanus, Hydra, Norma and NGC4636 fields
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• High mass and halo resolution from fast low resolution simulations
• There and back again: understanding the critical properties of backsplash galaxies
• The Dispersion Measure Contributions of the Cosmic Web
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• DS+: a method for the identification of cluster substructures
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• 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
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• The evolutionary pathways of disk galaxies with different sizes
• Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
• BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
• Teaching neural networks to generate Fast Sunyaev Zel'dovich Maps
• When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath$z\gtrsim 1$
• Realistic galaxy images and improved robustness in machine learning tasks from generative modelling
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Testing the consistency of three-point halo clustering in Fourier and configuration space
• Minimising the impact of scale-dependent galaxy bias on the joint cosmological analysis of large scale structures
• Spatial and orbital planes of the Milky Way satellites: unusual but consistent with $\Lambda$CDM
• Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• 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
• Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• The role of AGN on the structure, kinematics and evolution of ETGs in the Horizon simulations
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• Unveiling the origins of galactic bars: insights from barred and unbarred galaxies
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• Understanding the early stages of galaxy formation using very metal-poor stars from the Hamburg/ESO survey
• Lopsided galactic disks in IllustrisTNG
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• The satellite galaxy plane of NGC 4490 in light of ΛCDM - Sparsity of similarly extreme analogs and a possible role of satellite pairs
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Evaluating hydrodynamical simulations with green valley galaxies
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Big Three Dragons: Molecular Gas in a Bright Lyman-Break Galaxy at $z=7.15$
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• The outermost edges of the Milky Way halo from galaxy kinematics
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• Constraining the scatter in the galaxy-halo connection at Milky Way masses
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• The formation pathways of compact elliptical galaxies
• The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
• Merging galaxy clusters in IllustrisTNG
• Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
• Local and global gas metallicity versus stellar age relation in MaNGA galaxies
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• A simple spectroscopic technique to identify rejuvenating 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
• The imprint of galaxy mergers on satellite planes in a cosmological context
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Mock HUBS observations of hot gas with IllustrisTNG
• What has quenched the massive spiral galaxies?
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• The Structural Evolution of Isolated Galaxies at Low Redshift in the IllustrisTNG Simulation
• Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim 4$ gas-rich halo
• Evolution of central galaxy alignments in simulations
• Baryonic feedback measurement from KV450 cosmic shear analysis
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• A Study of Gas Entropy Profiles of 47 Galaxy Clusters and Groups Out to the Virial Radius
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• The ALPINE-ALMA [CII] Survey: Dust emission effective radius up to 3 kpc in the Early Universe
• The Velocity Dispersion Function for Quiescent Galaxies in Nine Strong-Lensing Clusters
• Evolution of Starburst Galaxies in the Illustris Simulation
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• Formation of a barred galaxy in a major merger: The role of AGN feedback
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• An intergalactic medium temperature from a giant radio galaxy
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Galaxy cluster mass accretion rates from IllustrisTNG
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Toward a Physical Understanding of Galaxy-Halo Alignment
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• A too-many dwarf galaxy satellites problem in the M83 group
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• Disk flaring with TNG50: diversity across Milky Way and M31 analogs
• Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Differential rotation of the halo traced by the K-giant stars
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• 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
• 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
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• The cooler past of the intracluster medium in TNG-Cluster
• 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
• An IllustrisTNG View of the Caustic Technique for Galaxy Cluster Mass Estimation
• Mass Dependence of Galaxy-Halo Alignment in LOWZ and CMASS
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical 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
• Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation
• Intrinsic alignments of bulges and discs
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Imprint of baryons and massive neutrinos on velocity statistics
• Debiased Galaxy Cluster Pressure Profiles from X-ray Observations and Simulations
• Asymptotic expansions for the Large Scale Structure
• Impact of uncertainties in the halo velocity profile on direct detection of sub-GeV dark matter
• Gravity- and temperature-driven phase transitions in a model for collapsed axionic condensates
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Observing the stellar halo of Andromeda in cosmological simulations: the Auriga2PAndAS pipeline
• Formation of super-thin galaxies in Illustris-TNG
• 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 ${\sigma }_{\mathrm{e}}$
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Accuracy of power spectra in dissipationless cosmological simulations
• SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1$-$1148 at $z\sim 0.5$
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation
• Probing Saraswati's heart: evaluating the dynamical state of the massive galaxy cluster A2631 through a comprehensive weak-lensing and dynamical analysis
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• 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
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Milky Way globular clusters on cosmological timescales. II. Interaction with the Galactic centre
• The continuous wavelet derived by smoothing function and its application in cosmology
• Milky Way globular clusters on cosmological timescales. III. Interaction rates
• Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• A Distinct Radial Acceleration Relation across Brightest Cluster Galaxies and Galaxy Clusters
• Probing Feedback in Galaxy Formation with Millimeter-wave Observations
• The effect of selection -- a tale of cluster mass measurement bias induced by correlation and projection
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Galaxy flows within 8,000 km/s from Numerical Action methods
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• MAGAZ3NE: Massive, Extremely Dusty Galaxies at $z\sim 2$ Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at $3<z<4$
• Off-centre supermassive black holes in bright central galaxies
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Scalable stellar evolution forecasting: Deep learning emulation vs. hierarchical nearest neighbor interpolation
• An off-centred bulge or a satellite? Hydrodynamical $N$-body simulations of the disc galaxy NGC 5474
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• 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
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Accretion onto supermassive and intermediate mass black holes in cosmological simulations
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• QSO MUSEUM II: Search for extended Ly$\alpha$ emission around eight $z\sim 3$ quasar pairs
• Formation and fate of low metallicity stars in IllustrisTNG50
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Constraining Mixed Dark Matter models with high redshift Lyman-alpha forest data
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Probabilistic model for dynamic galaxy decomposition
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• Intrinsic shapes of Brightest Cluster Galaxies
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• The Alcock Paczynski test with 21cm intensity field
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Resolved star formation in TNG100 central and satellite galaxies
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• Color dependence of clustering of massive galaxies at 0.5$\le z\le$2.5: similar spatial distributions between green valley galaxies and AGNs
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Kinetic Field Theory for Cosmic Structure Formation
• MOSEL and IllustrisTNG: Massive Extended Galaxies at z=2 Quench Later Than Normal-size Galaxies
• Mass-morphology relation of TNG50 galaxies
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• MIGHTEE-HI: Discovery of an HI-rich galaxy group at z = 0.044 with MeerKAT
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• The origin of star-forming rings in S0 galaxies
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• Understanding the Fundamental Plane and the Tully Fisher Relation
• 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
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
• Entropy-Conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• The origin and properties of red spirals: Insights from cosmological simulations
• Galaxy populations in haloes in high-density environments
• 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
• Where binary neutron stars merge: predictions from IllustrisTNG
• Baryonic Effects on Lagrangian Clustering and Angular Momentum Reconstruction
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• 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
• 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
• Turbulence-induced deviation between baryonic field and dark matter field in the spatial distribution of the Universe
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Beyond Mass: Detecting Secondary Halo Properties with Galaxy-Galaxy Lensing
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• Multi-wavelength consensus of large-scale linear bias
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• The diverse physical origins of stars in the dynamically hot bulge: CALIFA vs. IllustrisTNG
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• Mass accretion rates of the HectoMAP clusters of galaxies
• Spin speed correlations and the evolution of galaxy-halo systems
• Studying galaxy cluster morphological metrics with Mock-X
• Fingerprints of modified gravity on galaxies in voids
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• The contribution of magnetized galactic outflows to extragalactic Faraday rotation
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• The significant effects of stellar mass estimation on galaxy pair fractions
• Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
• Galaxy populations in protoclusters at cosmic noon
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• Host Galaxy Demographics Of Individually Detectable Supermassive Black-hole Binaries with Pulsar Timing Arrays
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• A new long gamma-ray burst formation pathway at solar metallicity
• A serendipitous discovery of HI-rich galaxy groups with MeerKAT
• An interesting case of the formation and evolution of a barred galaxy in the cosmological context
• The effects of the orbital configurations of mergers on reshaping galaxy structures
• Determining the time before or after a galaxy merger event
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Are early-type galaxies quenched by present-day environment? A study of dwarfs in the Fornax Cluster
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• The Effect of Impact Parameter on Tidal Disruption Events
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• Stage IV baryonic feedback correction for non-Gaussianity inference
• Measuring Galaxy Asymmetries in 3D
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Realistic consecutive galaxy mergers form eccentric PTA sources
• Preprocessing in small groups: Three simulated galaxies interacting prior to cluster infall
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Prospects for disentangling dark matter with weak lensing
• Exploring the physical origins of halo assembly bias from early times
• On the asymptotic behaviour of cosmic density-fluctuation power spectra
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Gravitational Turbulence: the Small-Scale Limit of the Cold-Dark-Matter Power Spectrum
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• FIRST J1419+3940 as the First Observed Radio Flare from a Neutron Star Merger
• The global energetics of radio AGN kinetic feedback in the local universe
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• 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
• Living with Neighbors. IV. Dissecting the Spin$-$Orbit Alignment of Dark Matter Halos: Interacting Neighbors and the Local Large-scale Structure
• Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses
• The scaling relations of galaxies back in time: the road toward virialization
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• N-body simulations of structure formation in thermal inflation cosmologies
• Recent Observations of the Rotation of Distant Galaxies and the Implication for Dark Matter
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Polynomial expansion of the star formation history in galaxies
• A Sagittarius-like simulated dwarf spheroidal galaxy from TNG50
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• 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
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
• What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• The galaxy bias profile of cosmic voids
• Red riding on hood: Exploring how galaxy colour depends on environment
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• Fast Radio Bursts
• Untangling Stellar Components of Galaxies: Evaluation of Dynamical Decomposition Methods in Simulated Galaxies with GalaxyChop
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• Mock Observations: Three Different Types of Galaxy Alignment in TNG100 Simulations
• Robust machine learning model of inferring the ex-situ stellar fraction of galaxies from photometric data
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
• Turbulence revealed by wavelet transform: power spectrum and intermittency for the velocity field of the cosmic baryonic fluid
• Cosmic filament spin -- I: a comparative study in observation
• Constraint on magnetized galactic outflows from LOFAR rotation measure data
• The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Andromeda's asymmetric satellite system as a challenge to cold dark matter cosmology
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint
• PoPE: A population-based approach to model spatial structure of astronomical systems
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Is Abell 2261 a fossil galaxy cluster in a transitional dynamical state?
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• 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
• Evolution of Star Cluster Within Galaxy using Self-consistent Hybrid Hydro/N-body Simulation
• On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• Spin alignment around TNG300-1 voids
• Reoriented Memory of Galaxy Spins for the Early Universe
• Spherical accretion of collisional gas in modified gravity I: self-similar solutions and a new cosmological hydrodynamical code
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• A new framework for understanding the evolution of early-type galaxies
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• 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
• The S-PLUS Fornax Project (S+FP): Mapping H$\alpha$+[NII] emission in 77 Fornax galaxy members reaching $\sim$4 Rvir
• Resummed Kinetic Field Theory: a model of coupled baryonic and dark matter
• Detection of pure warm-hot intergalactic medium emission from a $7.2$ Mpc long filament in the Shapley supercluster using X-ray spectroscopy
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• 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
• Searching for photon-ALPs mixing effects in AGN gamma-ray energy spectra
• A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models
• Simulation-guided galaxy evolution inference: A case study with strong lensing galaxies
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Generative modelling for mass-mapping with fast uncertainty quantification
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type 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
• How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?
• The evolution of the barred galaxy population in the TNG50 simulation
• Physically motivated modeling of LyC escape fraction during reionization
• Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
• Time Delay Anomalies of Fuzzy Gravitational Lenses
• Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering
• MEGS: Morphological Evaluation of Galactic Structure
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• 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
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Exploring selection biases in FRB dispersion-galaxy cross-correlations with magnetohydrodynamical simulations
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• Traces of the evolution of cosmic void galaxies: An Integral Field Spectroscopy based analysis
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• High-redshift AGN population in radiation-hydrodynamics simulations
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• IFUM Integrated Field Spectroscopy of Ten M104 Satellite Galaxy Candidates
• Turbulence, Thermal Pressure, and Their Dynamical Effects on Cosmic Baryonic Fluid
• Challenges in Cosmic Magnification Reconstruction by Magnification Response
• Caustic and hydrostatic mass bias: Implications for modified gravity
• Properties of subhalos in the interacting dark matter scenario
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• Effects of large-scale magnetic fields on the observed composition of ultra high-energy cosmic rays
• Negligible Effects of Baryons on the Angular Momentum Scaling Relations of Galactic Dark Matter Halos
• Reorientation Rates of Structural and Kinematic Axes in Simulated Massive Galaxies and the Origins of Prolate Rotation
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• The intervelocity of galaxy pairs in $\Lambda$CDM -- The observed velocity peak at ~130 km/s is not unique to MOND
• Gaussian Lagrangian Galaxy Bias
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• MCMC generation of cosmological fields far beyond Gaussianity
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Testing an entropy estimator related to the dynamical state of galaxy clusters
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Estimating infall times of galaxies around clusters: how accurately can it be done with observational data?
• Inferring halo masses with Graph Neural Networks
• A MeerKAT study of a neutral hydrogen rich grouping of galaxies with megaparsec-scale filamentary-like structure
• Predicting far-infrared maps of galaxies via machine learning techniques
• Assessing the connection between galactic conformity and assembly-type bias
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• 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
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Major merger fraction along the massive galaxy quenching channel at 0.2$<z<$0.7
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• On the effects of parameters on galaxy properties in CAMELS and the predictability of ${\Omega }_{\mathrm{m}}$
• The THESAN project: environmental drivers of Local Group reionization
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Mapping luminous and dark matter in the Universe
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• A New View of Observed Galaxies through 3D Modelling and Visualisation
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• zELDA II: reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• The oldest tidally induced bar-like galaxy in the IllustrisTNG cluster
• You Are What You Eat: The Circumgalactic Medium Around BreakBRD Galaxies has Low Mass and Angular Momentum
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
• Exploring the halo-galaxy connection with probabilistic approaches
• Tidally induced bar-like galaxies in simulated clusters
• ZFIRE -- The Gas Inflow Inequality for Satellite Galaxies in Cluster and Field Halos at z = 2
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• On the tomographic cluster clustering as a cosmological probe
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Tracing black hole and galaxy growth across environments since cosmic noon
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• On the signature of black holes on the quenched stellar mass function
• The impact of cosmic filaments on the abundance of satellite galaxies
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• The clustering of C IV and Si IV at the end of reionisation: A perspective from the E-XQR-30 survey
• The invariance of group occupation across the cosmic web
• STRAWBERRY: Finding haloes in the gravitational potential
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• The multi-component fitting to the star formation histories in the TNG simulation
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• The Formation of Dwarf Galaxy Disks
• The Milky Way and M31 Orbital History: Did the Local Group evolve in isolation?
• Tracing satellite planes in the Sculptor group: II. Discovery of five faint dwarf galaxies in the DESI Legacy Survey
• Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• The merger-driven evolution of massive early-type galaxies
• Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera
• Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ~ 0.8 with BOSS and DESI
• The major merger-active galactic nucleus connection up to the cosmic noon
• Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Galaxy-halo internal alignments across cosmic time
• Multiscale exploration of SMACS J0723.3--7327's intracluster light and past dynamical history
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• The large-scale distribution of ionized metals in IllustrisTNG
• The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
• Kinetic field theory: generic effects of alternative gravity theories on non-linear cosmic density-fluctuations
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• The assembly history of NGC 1365 through chemical archaeology
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Non-ideal self-gravity and cosmology: the importance of correlations in the dynamics of the large-scale structures of the Universe
• Testing the role of AGN on the star formation and metal enrichment of "twin galaxies"
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• KRIOS: A new basis-expansion $N$-body code for collisional stellar dynamics
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Dipole Distortions in the Intergalactic Medium
• Reduced Gas Accretion onto Galaxies due to Effects of External Giant Radio Lobes
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• The Tremaine-Weinberg method at high redshifts
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• 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
• Cosmological evolution of gas and supermassive black holes in idealized isolated halos
• The mass and redshift dependence of halo star clustering
• A momentum conserving $N$-body scheme with individual timesteps
• Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Symmetries of the Large Scale Structures of the Universe as a Phenomenology of a Fractal Turbulence: The Role of the Plasma Component
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Cavendish experiment with fast radio bursts on cosmological scales
• Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
• Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• Phase-space perturbation theory for cosmic large-scale structure
• 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
• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
• 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
• Inferring the mass of the circumgalactic medium using X-ray resonant scattering
• Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• Identification of Compact Groups of Galaxies in IllustrisTNG300
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• The History of Galaxy Mergers in IllustrisTNG
• Spatially non-parametric recovery of intrinsic kinematic maps in pre- to post-merger galaxies
• Mesoscopic Energy Ranking Constraints in the IllustrisTNG Simulations
• The dynamical lineage of ultra-diffuse galaxies from TNG50-1
• Stealing galaxies from galaxy clusters
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Relativistic Angular Redshift Fluctuations embedded in Large Scale Varying Gravitational Potentials
• DeepVoid: A Deep Learning Void Detector
• Mimicking the halo-galaxy connection using machine learning
• Measuring Scaling Relationships: Fitting Technique Matters
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Scaling Relations in the Phase-Space Structure of Dark Matter Haloes
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• 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
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• 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
• Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
• A Simulation Driven Deep Learning Approach for Separating Mergers and Star Forming Galaxies: The Formation Histories of Clumpy Galaxies in all the CANDELS Fields
• Baryon-photon interactions in Resummed Kinetic Field Theory
• On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
• Quasar clustering at redshift 6
• Determining the Dark Matter distribution in galaxies with Deep Learning
• Overdensity of SubMillimiter Galaxies in the GJ526 Field mapped with the NIKA2 Camera
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• A general framework for unbiased tests of gravity using galaxy clusters
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
• Estimating Transient Rates from Cosmological Simulations and BPASS
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Intrinsic alignments of galaxies in multiple projections
• Searching for Dark Structures: A Comparison of Weak-lensing Convergence Maps and Lensing-weighted Galaxy Density Maps
• 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
• Dark Matter profiles of "in silico" galaxies: deep learning inference