How Filaments are Woven into the Cosmic Web

Abstract

Observations indicate galaxies are distributed in a filament-dominated web-like structure. Numerical experiments at high and low redshift of viable structure formation theories also show filament-dominance. We present a simple quantitative explanation of why this is so, showing that the final-state web is actually present in embryonic form in the overdensity pattern of the initial fluctuations, with nonlinear dynamics just sharpening the image. The web is largely defined by the position and primordial tidal fields of rare events in the medium, with the strongest filaments between nearby clusters whose tidal tensors are nearly aligned. Applications of the cosmic web theory to observations include probing cluster-cluster bridges by weak gravitational lensing, X-rays, and the Sunyaev-Zeldovich effect and probing high redshift galaxy-galaxy bridges by low column density Lyman alpha absorption lines.

9 pages, gzipped uuencoded postscript file, 4 figures in separate files. The text + figures are also available from anonymous ftp site: ftp://ftp.cita.utoronto.ca/ftp/cita/bond/bkp_nature

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• Fisher Forecasts for Primordial non-Gaussianity from Persistent Homology
• Properties of brightest group galaxies in cosmic web filaments
• Cluster Winds Blow along Supercluster Axes
• Probing large scale filaments with HI and ${}^3$HeII
• Encoding large scale cosmological structure with Generative Adversarial Networks
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• The universal multiplicity function: counting halos and voids
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• An estimate of the electron density in filaments of galaxies at z~0.1
• The Caltech Faint Galaxy Redshift Survey XII: Clustering of Galaxies
• The Massively Accreting Cluster A2029
• COWS: A filament finder for Hessian cosmic web identifiers
• The Gravitational Instability of Adiabatic Filaments
• The complex case of MACSJ0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations
• Bayesian cosmic density field inference from redshift space dark matter maps
• Could multiple voids explain the Cosmic Microwave Background Cold Spot anomaly?
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations
• The peculiar velocities of satellites of external disk galaxies
• The Variation of Galaxy Morphological Type with the Shear of Environment
• Gravitational Instability in Collisionless Cosmological Pancakes
• The eROSITA view of the Abell 3391/95 field: Cluster Outskirts and Filaments
• Partitioning the universe into gravitational basins using the cosmic velocity field
• The cosmic web in Lyman-alpha emission
• The impact of filamentary accretion of subhaloes on the shape and orientation of haloes
• Comparing cosmic web classifiers using information theory
• Effects of Baryonic Feedback on the Cosmic Web
• The Effect of Massive Neutrinos on the Halo Spin Flip Phenomenon
• Patchy blazar heating: diversifying the thermal history of the intergalactic medium
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Swarm Intelligence-based Extraction and Manifold Crawling Along the Large-Scale Structure
• Galaxy alignment as a probe of large-scale filaments
• Multiple-streaming and the Probability Distribution of Density in Redshift Space
• Turning Around along the Cosmic Web
• Infalling Faint [OII] Emitters in Abell 851. II. Environment, Kinematics, and Star Formation History
• A gravitational lensing detection of filamentary structures connecting luminous red galaxies
• The spectroscopically confirmed huge cosmic structure at z=0.55
• The Size Distribution of Void Filaments in a LCDM Cosmology
• Zipf's law for cosmic structures: how large are the greatest structures in the universe?
• The cosmic web connection to the dark matter halo distribution through gravity
• Configuration entropy of the Cosmic Web: Can voids mimic the dark energy?
• A Census of the Extended Neutral Hydrogen Around 18 MHONGOOSE Galaxies
• DeFiNe: an optimisation-based method for robust disentangling of filamentous networks
• Large scale structure of the Universe
• MeTACAST: Target- and Context-aware Spatial Selection in VR
• Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
• The clustering of critical points in the evolving cosmic web
• Spatial Distribution of Globular Clusters in the Galaxy
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• 1-DREAM: 1D Recovery, Extraction and Analysis of Manifolds in noisy environments
• Network Analysis of Cosmic Structures : Network Centrality and Topological Environment
• Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS
• On the initial shear field of the cosmic web
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Star-forming Dwarf Galaxies in Filamentary Structures around the Virgo Cluster: Probing Chemical Pre-processing in Filament Environments
• Redshifts and Velocity Dispersions of Galaxy Clusters in the Horologium-Reticulum Supercluster
• The Void Galaxy Survey
• Evolution of skewness and kurtosis of cosmic density fields
• Large-scale magnetic field in the Monoceros OB-1 East molecular cloud
• Cosmology with Persistent Homology: a Fisher Forecast
• Connections between galaxy properties and halo formation time in the cosmic web
• The orientation of galaxy pairs with filamentary structures: dependence on morphology
• Entrainment of Hot Gas into Cold Streams: The Origin of Excessive Star-formation Rates at Cosmic Noon
• Statistical properties of the linear tidal shear
• Measuring alignments between galaxies and the cosmic web at $z\sim 2-3$ using IGM tomography
• Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
• Alignments of dark matter halos with large-scale tidal fields: mass and redshift dependence
• The Stellar Kinematics of Void Dwarf Galaxies Using KCWI
• Tracing the gas at redshift 1.7-3.5 with the Lyman-alpha forest: the FLO approach
• The VIMOS VLT Deep Survey: Testing the gravitational instability paradigm at z ~ 1
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Faint Blue Galaxies and Merging: the Evolution of the Luminosity Function
• Massive Cooling Flow Clusters Inhabit Crowded Environments
• Topology and geometry of the dark matter web: a multistream view
• Persistent topology of the reionization bubble network. II: Evolution & Classification
• Pulling out Threads from the Cosmic Tapestry: Defining Filaments of Galaxies
• Galaxy interactions in filaments and sheets: effects of the large-scale structures versus the local density
• Dynamics of Abell 3266 - I. An Optical View of a Complex Merging Cluster
• The evolution of high-density cores of the BOSS Great Wall superclusters
• Intergalactic baryon-rich regions at high redshift
• The influence of the void environment on the ratio of dark matter halo mass to stellar mass in SDSS MaNGA galaxies
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Star Formation and Gas Phase History of the Cosmic Web
• Excursion set peaks in energy as a model for haloes
• The large-scale structure around the Fornax-Eridanus Complex
• Alignments of the Galaxies in and around the Virgo Cluster with the Local Velocity Shear
• The structure of the merging RCS 231953+00 Supercluster at z ~ 0.9
• Galaxy Luminosity Function of Dynamically Young Abell 119 Cluster: Probing the Cluster Assembly
• Search and analysis of giant radio galaxies with associated nuclei (SAGAN) IV. Interplay with the Supercluster environment
• The origin of 'Great Walls'
• Spin conservation of cosmic filaments
• Shell-like structures in our cosmic neighbourhood
• Characterizing the Circumgalactic Medium of Quasars at z $\sim$ 2.2 through H$\alpha$ and Ly$\alpha$ Emission
• Detection of Molecular Gas in Void Galaxies : Implications for Star Formation in Isolated Environments
• Dynamical Ejections of Stars due to an Accelerating Gas Filament
• A ~6 Mpc overdensity at z = 2.7 detected along a pair of quasar sight lines: filament or protocluster?
• The relationship between gas and galaxies at z<1 using the Q0107 quasar triplet
• PhotoWeb redshift: boosting photometric redshift accuracy with large spectroscopic surveys
• Peaks and dips in Gaussian random fields: a new algorithm for the shear eigenvalues, and the excursion set theory
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• Analytical halo models of cosmic tidal fields
• The Fabric of the Universe: Exploring the cosmic web in 3D prints and woven textiles
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• COS Observations of the Cosmic Web: A Search for the Cooler Components of a Hot, X-ray Identified Filament
• MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
• The COSMOS-Web deep galaxy group catalog up to $z=3.7$
• Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
• Determining the large-scale environmental dependence of gas-phase metallicity in dwarf galaxies
• A New Dynamical Mass Measurement for the Virgo Cluster using the Radial Velocity Profile of the Filament Galaxies
• The Anisotropic Two-Point Correlation Functions of the Nonlinear Traceless Tidal Field in the Principal-Axis Frame
• The density distribution of accreting cosmic filaments as shaped by Kelvin-Helmholtz instability
• Baryon Acoustic Oscillations in the Lyman Alpha Forest
• How dark are filaments in the cosmic web?
• Hydrodynamical simulations of galaxy properties: Environmental effects
• Machine-learning cosmology from void properties
• When galaxies align: intrinsic alignments of the progenitors of elliptical galaxies in the Horizon-AGN simulation
• Anisotropic satellite accretion onto the Local Group with HESTIA
• ASW${}^2$DF: Census of the obscured star formation in a galaxy cluster in formation at $z=2.2$
• The mass-size relation of galaxy clusters
• The Bridge Effect of Void Filaments
• Hickson-like compact groups inhabiting different environments
• Discovery of a >13 Mpc long X-ray filament between two galaxy clusters beyond three times their virial radii
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Network analysis of the COSMOS galaxy field
• A robust determination of halo environment in the cosmic field
• ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• The biasing phenomenon
• The causal effect of environment on halo mass and concentration
• Detection of the velocity shear effect on the spatial distributions of the galactic satellites in isolated systems
• Morphologies of galaxies within voids
• The three-dimensional geometry and merger history of the massive galaxy cluster MACS J0358.8-2955
• The large-scale environment of thermonuclear and core-collapse supernovae
• Influence of the Void Environment on Chemical Abundances in Dwarf Galaxies and Implications for Connecting Star Formation and Halo Mass
• Clusters of galaxies and the cosmic web with SKA
• Cosmic Filaments from Cosmic Strings
• Spitzer observations of Abell 1763 - II: Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton data
• Thermal and Chemical Evolution of Collapsing Filaments
• Statistical properties of filaments in weak gravitational lensing
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Probing modified gravity in cosmic filaments
• Ridges in the Dark Energy Survey for cosmic trough identification
• On the Environmental Dependence of Galaxy Properties Established by the Initial Cosmological Conditions
• Large-scale environmental dependence of the abundance ratio of nitrogen to oxygen in blue, star-forming galaxies fainter than L*
• On the origin of red spirals: Does assembly bias play a role?
• Active Galactic Nuclei Abundance in Cosmic Voids
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• A New Perspective on the Large-Scale Tidal Effect on the Galaxy Luminosity and Morphology
• MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
• Anisotropic Halo Model
• Non-perturbative halo clustering from cosmological density peaks
• Discovery of a Large-scale Wall in the Direction of Abell 22
• Combining Strong Lensing and Dynamics in Galaxy Clusters: integrating MAMPOSSt within LENSTOOL I. Application on SL2S J02140-0535
• The Anisotropy in the Galaxy Velocity Field Originated from the Gravitational Pancaking Effect
• Non-Halo Structures and their Effects on Gravitational Lensing
• Cosmological Filaments in the light of Excursion Set of Saddle Points
• Lagrangian Methods Of Cosmic Web Classification
• The distribution of galaxies gravitational field stemming from their tidal interaction
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• Reconstructing the Triaxial Shapes of Dark Matter Halos from the Anisotropic Spatial Distributions of their Substructures in the Concordance Cosmology
• Ecology of dark matter haloes -II. Effects of interactions on the alignment of halo pairs
• The four cosmic tidal web elements from the $\beta$-skeleton
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
• Stability of Rotating Self-Gravitating Filaments:Stability of Rotating Self-Gravitating Filaments: Effects of Magnetic Field
• The shape distribution of superclusters in SDSS DR 12
• The cosmic spiderweb: equivalence of cosmic, architectural, and origami tessellations
• SUZAKU Observation of a New Merging Group of Galaxies at a Filamentary Junction
• MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISM
• On the alignment of haloes, filaments and magnetic fields in the simulated cosmic web
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• A theoretical view of the T-web statistical description of the cosmic web
• The M101 galaxy group as a node in the nearby cosmic filament
• Do minor interactions trigger star formation in galaxy pairs?
• Segmenting the Universe into dynamically coherent basins
• Modeling the Intergalactic Medium during the Epoch of Reionization
• The correlations between galaxy properties in different environments of the cosmic web
• SCONCE: A cosmic web finder for spherical and conic geometries
• On the projected mass distribution around galaxy clusters : a Lagrangian theory of harmonic power spectra
• Dark Sector Coupling Bends the Superclusters
• Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
• Clusters in the Disperse cosmic web
• The abundance and environment of dark matter haloes
• 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
• The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations
• Cosmic Web & Caustic Skeleton: non-linear Constrained Realizations -- 2D case studies
• Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission
• Statistical properties of filaments in the cosmic web
• Modeling the Alignment Profile of Satellite Galaxies in Clusters
• The maximum extent of the filaments and sheets in the cosmic web: an analysis of the SDSS DR17
• The large-separation expansion of peak clustering in Gaussian random fields
• Local Supercluster Dynamics: External Tidal Impact of the PSCz sample traced by Optimized Numerical Least Action Method
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• Constraining the Neutrino Mass with the Drifting Coefficient of the Field Cluster Mass Function
• Early evolution of spin direction in dark matter halos and the effect of the surrounding large-scale tidal field
• Measuring cosmic filament spin with the kinetic Sunyaev-Zel'dovich effect
• The PAU Survey: Close galaxy pairs identification and analysis
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• CO-CAVITY project: Molecular gas and star formation in void galaxies
• Alpha Shape Topology of the Cosmic Web
• A Comparison of Void-Finding Algorithms using Crossing Numbers
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Constrained simulations and excursion sets: understanding the risks and benefits of `genetically modified' haloes
• Bayesian Cosmic Web Reconstruction: BARCODE for Clusters
• An observational detection of the bridge effect of void filaments
• Black holes inside cosmic voids
• Probing cosmology via the clustering of critical points
• Prospects for detecting cosmic filaments in Lyman-alpha emission across redshifts $z=2-5$
• Statistical characteristics of simulated walls
• Voids in the Cosmic Web as a probe of dark energy
• Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses
• Structure formation and quasi-spherical collapse from initial curvature perturbations with numerical relativity simulations
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• The Rotational Profiles of Cluster Galaxies
• Understanding the cosmic web
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• A Simple Gravitational Lens Model For Cosmic Voids
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• Red riding on hood: Exploring how galaxy colour depends on environment
• Abell 2626 and friends: large and small scale structure
• Dark matter
• Pair Lines of Sight Observations of Multiphase Gas Bearing O VI in a Galaxy Environment
• Lyman Alpha Line Spectra of the First Galaxies: Dependence on Observed Direction to the Underlying CDM Filament
• A Scaling Relation of the Evolving Tidal Fields in a LCDM Cosmology
• Unveiling galaxy pair alignment in cosmic filaments: A 3D exploration using EAGLE simulation
• Kinematics of the Local Group gas and galaxies in the Hestia simulations
• A Primeval Magellanic Stream and Others
• Witnessing a Transformation to Blue-cored Dwarf Early-type Galaxies in Filaments and the Cluster Outskirts: Gas-phase Abundances and Internal Kinematics Perspectives
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• Extended Void Merging Tree Algorithm for Self-Similar Models
• Tracing gaseous filaments connected to galaxy clusters: the case study of Abell 2744
• A New Multi-Scale Structure Finding Algorithm to Identify Cosmological Structure
• Galaxy Superclusters and Their Complexes in the Cosmic Web
• Detection of pure warm-hot intergalactic medium emission from a $7.2$ Mpc long filament in the Shapley supercluster using X-ray spectroscopy
• The eventful life journey of galaxy clusters. I. Impact of DM halo and ICM properties on their full assembly histories
• Relation between the local width and linear halo mass density of cosmic filaments
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• An ultra-high-resolution map of (dark) matter
• Morpho-Photometric Classification of KiDS DR5 Sources Based on Neural Networks: A Comprehensive Star-Quasar-Galaxy Catalog
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• Probing large-scale structures with the two-point function and the power spectrum: insights into cosmic clustering evolution
• Quantifying the Active Galactic Nuclei Fraction in Cosmic Voids via Mid-Infrared Variability
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Spin alignment around TNG300-1 voids
• An Optimized Ly$\alpha$ Forest Inversion Tool Based on a Quantitative Comparison of Existing Reconstruction Methods
• A spherical hydrodynamical model of cosmic voids in ΛCDM and beyond
• Dark matter haloes: a multistream view
• The KALEIDOSCOPE survey : A new strong and weak gravitational lensing view of the massive galaxy cluster MACS J1423.8+2404
• Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• Alignment between Satellite and Central Galaxies in the EAGLE Simulation: Dependence on the Large-Scale Environments
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Cosmic filament spin -- I: a comparative study in observation
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• A Global Census of Metals in the Universe
• An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclusters
• A Simulated Annealing algorithm to quantify patterns in astronomical data
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• Directional Invariants of Doubly Periodic Tangles
• GrAviPaSt's Lens to the Past: Unveiling the Evolution of Filamentary Structures
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• SAGAN-VI: When Jets Meet Filaments -- Environmental Imprints on the Growth of Giant Radio Galaxies
• Mean maps for cosmic web structures in cosmological initial conditions
• Dependence of the dynamical properties of light-cone simulation dark matter halos on their environment
• Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations
• Statistical exploration of halo anisotropic clustering and intrinsic alignments with the mass-Peak Patch algorithm
• The influence of superstructures on bright galaxy environments: clustering properties
• An X-ray/optical study of the geometry and dynamics of MACS J0140.0-0555, a massive post-collision cluster merger
• Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
• Interstellar Filaments and the Statistics of Galactic HI
• Exploring the Cosmic Web in the Sloan Digital Sky Survey Data Release Seven using the Local Dimension
• Statistical Properties of Supercluster-Like Filaments from Cosmological Simulations
• How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?
• The energy shear of protohaloes
• Photometric redshift galaxies as tracers of the filamentary network
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: strategy, observations and validation
• Lagrangian Volume Deformations around Simulated Galaxies
• Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
• A universal and physically motivated threshold for Hessian-based cosmic web identification: V-Web case
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• Traces of Anisotropic Quasi-Regular Structure in the SDSS Data
• Statistical Decoupling of Lagrangian Fluid Parcel in Newtonian Cosmology
• ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09
• VEGA: Voids idEntification using Genetic Algorithm
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• Galaxy Spin Alignment with Tidal Fields in the SDSS-IV MaNGA Survey
• Chemodynamic evidence of pristine gas accretion in the void galaxy VGS 12
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• Self-sustaining star formation fronts in filaments during cosmic dawn
• Spatial correlations of extended cosmological structures
• Luminosity Bias (II): The Cosmic Web of the First Stars
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
• Bending the web: exploring the impact of modified gravity on the density field and halo properties within the cosmic web
• Cosmology with Topological Deep Learning
• A 15 Mpc rotating galaxy filament at redshift z = 0.032
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament
• Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe
• Tensor anisotropy as a tracer of cosmic voids
• Impact of filaments on galaxy cluster properties in The Three Hundred simulation
• Merging Rates of the First Objects and the Formation of First Mini-Filaments in Models with Massive Neutrinos
• MOSS I: Double radio relics in the Saraswati supercluster
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• Evolution of the Pancaking Effect in a LCDM Cosmology
• Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• A positive correlation between broad HI Ly$\alpha$ absorptions and local overdensities of galaxies
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• Line versus Flux Statistics -- Considerations for the Low Redshift Lyman-alpha Forest
• Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50
• The invariance of group occupation across the cosmic web
• Alignment of spiral and elliptical galaxies from Siena Galaxy Atlas with filaments
• The impact of cosmic filaments on the abundance of satellite galaxies
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Excursion Sets with a "Perfect" Collapse Model
• Tracing the environmental history of observed galaxies via extended fast action minimization method
• Virgo Filaments VI: H$\alpha$ clumps in the filaments around the Virgo galaxy cluster
• Galaxy clustering in the VVV Near-IR Galaxy Catalogue
• Alignment of the central galaxies with the environment
• Unveiling the faint ultraviolet Universe
• Investigating the origin of the Milky Way streams. A revised look at their orbital pole distribution in light of precession effects
• Estimating major merger rates and spin parameters ab initio via the clustering of critical events
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• The BUFFALO HST Survey
• Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation
• The cosmic web in CosmoGrid void regions
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• Differentiable Fuzzy Cosmic-Web for Field Level Inference
• The intergalactic medium in the cosmic web
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• A novel Cosmic Filament catalogue from SDSS data
• DeepVoid: A Deep Learning Void Detector
• Overdensity of SubMillimiter Galaxies in the GJ526 Field mapped with the NIKA2 Camera
• The NuSTAR, XMM-Newton, and Suzaku view of A3395 at the intercluster filament interface
• Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim 1.74$ MaDCoWS2 galaxy cluster candidate
• Void spin distribution as a powerful probe of ${\sigma }_8$
• The influence of the Cosmic Web on the properties of dwarf galaxies in the Fornax-Eridanus Supercluster
• Cosmological simulation of a radio synchrotron bridge between pre-merging galaxy clusters
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• Initial Investigations of the Outskirts of XLSSC 122
• The cosmic environment overtakes the local density in shaping galaxy star formation
• Interstellar filament detection and characterization: methods and implications for studies of magnetized interstellar medium