Dancing in the dark: galactic properties trace spin swings along the cosmic web

Abstract

A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments above redshift 1.2. The analysis of more than 150 000 galaxies per time step in the redshift range 1.2<z<1.8 with morphological diversity shows that the spin of low-mass blue galaxies is preferentially aligned with their neighbouring filaments, while high-mass red galaxies tend to have a perpendicular spin. The reorientation of the spin of massive galaxies is provided by galaxy mergers, which are significant in their mass build-up. We find that the stellar mass transition from alignment to misalignment happens around 3.10^10 M_sun. Galaxies form in the vorticity-rich neighbourhood of filaments, and migrate towards the nodes of the cosmic web as they convert their orbital angular momentum into spin. The signature of this process can be traced to the properties of galaxies, as measured relative to the cosmic web. We argue that a strong source of feedback such as active galactic nuclei is mandatory to quench in situ star formation in massive galaxies and promote various morphologies. It allows mergers to play their key role by reducing post-merger gas inflows and, therefore, keeping spins misaligned with cosmic filaments.

18 pages, 19 figures, accepted for publication in MNRAS, movies and pictures of the simulation can be found at this address http://horizon-AGN.projet-horizon.fr

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• Statistics of Galactic-Scale Quasar Pairs at Cosmic Noon
• Probing the cold magnetized Universe with SPICA-POL (B-BOP)
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• A Candidate Kiloparsec-scale Quasar Pair at $z=5.66$
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Radio galaxies in galaxy groups: kinematics, scaling relations and AGN feedback
• Galaxy and Mass Assembly (GAMA): Extended Intra-Group Light in a group at $z=0.2$ from deep Hyper-Suprime Cam images
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• Properties of Galaxies in Cosmic Filaments around the Virgo Cluster
• Pairing of Massive Black Holes in Merger Galaxies Driven by Dynamical Friction
• Projected Axis Ratios of Galaxy Clusters in the Horizon-AGN Simulation: Impact of Baryon Physics and Comparison with Observations
• The evolution of galaxy intrinsic alignments in the MassiveBlack II universe
• Intergalactic filaments spin
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• Hector - a new massively multiplexed IFS instrument for the Anglo-Australian Telescope
• The impact of baryonic physics and massive neutrinos on weak lensing peak statistics
• Cosmological evolution of the Nitrogen abundance
• A hidden population of massive black holes in simulated dwarf galaxies
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• The impact of AGN feedback on galaxy intrinsic alignments in the Horizon simulations
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• MIGHTEE-HI: The relation between the HI gas in galaxies and the cosmic web
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• I- A hydrodynamical CLONE of the Virgo cluster of galaxies to confirm observationally-driven formation scenarios
• Alignment between satellite and central galaxies in the SDSS DR7: dependence on large-scale environment
• Ancient Very Metal-Poor Stars Associated With the Galactic Disk in the H3 Survey
• Impact of Baryonic Physics on Intrinsic Alignments
• Spherical Cows in Dark Matter Indirect Detection
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• Intermittent AGN episodes drive outflows with a large spread of observable loading factors
• 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
• Baryonic effects on CMB lensing and neutrino mass constraints
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• Galaxy properties in the cosmic web of EAGLE simulation
• Multimessenger study of merging massive black holes in the OBELISK simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations
• Star formation in galaxies hosting AGN: A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey
• The complex case of MACSJ0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Black hole formation and growth with non-Gaussian primordial density perturbations
• Star-Gas Misalignment in Galaxies: II. Origins Found from the Horizon-AGN Simulation
• Wobbling galaxy spin axes in dense environments
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Assembly of the Intracluster Light in the Horizon-AGN Simulation
• AGN-driven quenching of satellite galaxies
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Hydrodynamical structure formation in Milgromian cosmology
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• The Effect of Massive Neutrinos on the Halo Spin Flip Phenomenon
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Star-gas misalignment in galaxies: I. The properties of galaxies from the Horizon-AGN simulation and comparisons to SAMI
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Strategies for optimal sky subtraction in the low surface brightness regime
• Difficulties in Mid-Infrared selection of AGN in dwarf galaxies
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• The properties of wind and jet from a super-Eddington accretion flow around a supermassive black hole
• Dust and Power: Unravelling the merger - active galactic nucleus connection in the second half of cosmic history
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• The IllustrisTNG Simulations: Public Data Release
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Non-isotropic feedback from accreting spinning black holes
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Bulge formation inside quiescent lopsided stellar disks: connecting accretion, star formation and morphological transformation in a z ~ 3 galaxy group
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• The Hector Survey: integral field spectroscopy of 100,000 galaxies
• Local Group star formation in warm and self-interacting dark matter cosmologies
• On the slow quenching of M* galaxies: heavily-obscured AGNs clarify the picture
• Revisiting the Galaxy Shape and Spin Alignments with the Large-Scale Tidal Field: An Effective Practical Model
• The Halo Spin Transition as a Probe of Dark Energy
• Spatially offset black holes in the Horizon-AGN simulation and comparison to observations
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• UV Background Fluctuations and Three-Point Correlations in the Large Scale Clustering of the Lyman-alpha Forest
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• The Obsidian model: Three regimes of black hole feedback
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Relaxed blue ellipticals: accretion-driven stellar growth is a key evolutionary channel for low mass elliptical galaxies
• Cosmological Probes of Structure Growth and Tests of Gravity
• The impact of black hole seeding in cosmological simulations
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Alignments of dark matter halos with large-scale tidal fields: mass and redshift dependence
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Kinematic unrest of low mass galaxy groups
• Measuring alignments between galaxies and the cosmic web at $z\sim 2-3$ using IGM tomography
• Exploring Active Galactic Nuclei and Little Red Dots with the Obelisk simulation
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Evidence for non-merger co-evolution of galaxies and their supermassive black holes
• Tracking Halo Orbits and Their Mass Evolution around Large-scale Filaments
• The role of AGN on the structure, kinematics and evolution of ETGs in the Horizon simulations
• Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• Using Real and Simulated Measurements of the Thermal Sunyaev-Zel'dovich Effect to Constrain Models of AGN Feedback
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Simplified galaxy formation with mesh-less hydrodynamics
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• Formation of compact galaxies in the Extreme-Horizon simulation
• Testing galaxy formation models with galaxy stellar mass functions
• Massive spheroids can form in single minor mergers
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Predicting the Observability of Population III Stars with ELT-HARMONI via the Helium $1640\mathring{\mathrm{A}}$ emission line
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Galaxy Structural Analysis with the Curvature of the Brightness Profile
• Correlated orientations of the axes of large quasar groups on Gpc scales
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy
• Black hole mergers as tracers of spinning massive black hole and galaxy populations in the OBELISK simulation
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• COSMOS-Web: A history of galaxy migrations over the stellar mass-star formation rate plane
• Spatially resolved observations of outflows in the radio loud AGN of UGC 8782
• Measuring the surface mass density ellipticity of redMaPPer galaxy clusters using weak-lensing
• The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
• A ~6 Mpc overdensity at z = 2.7 detected along a pair of quasar sight lines: filament or protocluster?
• Supermassive Black Holes from self-gravitating Bose-Einstein Condensates comprised of Ultra-light Bosonic Dark Matter
• The origin of star-gas misalignments in simulated galaxies
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• Black hole fueling in galaxy mergers: A high-resolution analysis
• The SRG/eROSITA All-Sky Survey : Subaru/HSC-SSP weak-lensing mass measurements for the eRASS1 Galaxy Clusters
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• An Observed Transition of Galaxy Spins on the Void Surfaces
• When galaxies align: intrinsic alignments of the progenitors of elliptical galaxies in the Horizon-AGN simulation
• Intrinsic alignments of bulges and discs
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Evolution of superclusters and supercluster cocoons in various cosmologies
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Molecular gas excitation and outflow properties of obscured quasars at z$\sim$0.1
• LyMAS reloaded: improving the predictions of the large-scale Lyman-α forest statistics from dark matter density and velocity fields
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Merger Effects on the Spin and Shape Alignments of Galaxy Stellar, Cold and Hot Gas, and Dark Matter Components
• An environment-dependent halo mass function as a driver for the early quenching of $z\ge 1.5$ cluster galaxies
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• Can the splashback radius be an observable boundary of galaxy clusters?
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Colour-magnitude diagram in simulations of galaxy formation
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• History of the gas fuelling star formation in eagle galaxies
• Relation between halo spin and cosmic web filaments at z=3
• Cosmological evolution of orientations of cluster-sized dark matter haloes and their central galaxies in the Horizon-AGN simulation
• Close Major Merger Pairs at $z=0$: Bulge-to-Total Ratio and Star Formation Enhancement
• QSO MUSEUM II: Search for extended Ly$\alpha$ emission around eight $z\sim 3$ quasar pairs
• Intracluster light is a biased tracer of the dark matter distribution in clusters
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• NOEMA Observations of CO Emission in Arp 142 and Arp 238
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• Testing self-interacting dark matter with galaxy warps
• A field-level emulator for modeling baryonic effects across hydrodynamic simulations
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• Wandering and escaping: recoiling massive black holes in cosmological simulations
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• On the detectability of massive black hole merger eventsby LISA
• Ecology of dark matter haloes -II. Effects of interactions on the alignment of halo pairs
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• Discovery of the kinematic alignment of early-type galaxies in the Virgo cluster
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Modeling Lyman-α Forest Cross-Correlations with LyMAS
• Real galaxy mergers from galaxy pair catalogs
• On the alignment of haloes, filaments and magnetic fields in the simulated cosmic web
• Mitigating baryonic effects with a theoretical error covariance
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• On the projected mass distribution around galaxy clusters : a Lagrangian theory of harmonic power spectra
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• The impact of the cosmological constant on past and future star formation
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• The impact of filaments on dwarf galaxy properties in the Auriga simulations
• A Deep Learning Approach for Characterizing Major Galaxy Mergers
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Linear Tidal Vestige found in the WM Sheet
• Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
• Determining the time before or after a galaxy merger event
• Astrophysics with the Laser Interferometer Space Antenna
• Statistical properties of filaments in the cosmic web
• A comprehensive study on the relation between the metal enrichment of ionised and atomic gas in star-forming galaxies
• Vortical Motions of Baryonic Gas in the Cosmic Web: Growth History and Scaling Relation
• A rising tide: Intrinsic alignments since the turn of the millennium
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• Infall Profiles for Supercluster-Scale Filaments
• Large-scale asymmetry in galaxy spin directions -- analysis of galaxies with spectra in DES, SDSS, and DESI Legacy Survey
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• 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
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• Calibrating galaxy formation effects in galactic tests of fundamental physics
• Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• 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
• Searching for dark matter subhalos in the Fermi-LAT catalog with Bayesian neural networks
• Red riding on hood: Exploring how galaxy colour depends on environment
• Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with [CII]
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• Intrinsic correlations of galaxy sizes in a hydrodynamical cosmological simulation
• On the Viability of Determining Galaxy Properties from Observations I: Star Formation Rates and Kinematics
• Reoriented Memory of Galaxy Spins for the Early Universe
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Modelling LAEs in the Epoch of Reionization with OBELISK
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• JWST reveals extended stellar disks for ALMA-bright dusty star-forming galaxies in the Spiderweb protocluster
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• Born to be Starless: Revisiting the Missing Satellite Problem
• A jet-driven bipolar outflow in NGC 1125
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• Lagrangian Volume Deformations around Simulated Galaxies
• SAGAN-VI: When Jets Meet Filaments -- Environmental Imprints on the Growth of Giant Radio Galaxies
• Growth and Feedback from the First Black Holes
• How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?
• The galaxy-environment connection revealed by constrained simulations
• The FLAMINGO simulations data release
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster
• Photometric and Kinematic Misalignments and Their Evolution Among Fast and Slow Rotators in the Illustris Simulation
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• A 15 Mpc rotating galaxy filament at redshift z = 0.032
• Mapping luminous and dark matter in the Universe
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• The impact of cosmic filaments on the abundance of satellite galaxies
• Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5
• Extended Hernquist-Springel formalism for cosmic star formation
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• Constraining Galaxy-Halo Connection Using Machine Learning
• Alignment of spiral and elliptical galaxies from Siena Galaxy Atlas with filaments
• Dipole Distortions in the Intergalactic Medium
• A Comprehensive Multiwavelength Study of the OH Megamaser galaxy IRAS 09320+6134
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• Caught in the web: galaxy mergers along cosmic filaments
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• Morphology of dark matter haloes beyond triaxiality
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
• The major merger-active galactic nucleus connection up to the cosmic noon
• The NewHorizon Simulation -- To Bar Or Not To Bar
• Understanding mechanical feedback from HERGs and LERGs
• Simulated X-ray Emission in Galaxy Clusters with Feedback from Active Galactic Nuclei
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Spin Alignment in Analogues of The Local Sheet
• Intrinsic alignments of galaxies in multiple projections
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Evaluating star formation rates at z = 5
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• Boosting (In)direct Detection of Dark Matter
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Massive black holes and their galaxies
• Ionized Gas Outflows and Shock-Heated Emission in the Highly Inclined Active Galaxy CGCG 012-070
• Cosmic Web-Halo Connection Between Twin Universes