Baryons in the Warm-Hot Intergalactic Medium

Abstract

Approximately 30-40% of all baryons in the present day universe reside in a warm-hot intergalactic medium (WHIM), with temperatures between 10^5<T<10^7 K. This is a generic prediction from six hydrodynamic simulations of currently favored structure formation models having a wide variety of numerical methods, input physics, volumes, and spatial resolutions. Most of these warm-hot baryons reside in diffuse large-scale structures with a median overdensity around 10-30, not in virialized objects such as galaxy groups or galactic halos. The evolution of the WHIM is primarily driven by shock heating from gravitational perturbations breaking on mildly nonlinear, non-equilibrium structures such as filaments. Supernova feedback energy and radiative cooling play lesser roles in its evolution. WHIM gas is consistent with observations of the 0.25 keV X-ray background without being significantly heated by non-gravitational processes because the emitting gas is very diffuse. Our results confirm and extend previous work by Cen & Ostriker and Dave' et al.

9 pages, emulateapj, submitted to ApJ

References in corpus (8)

• Resolving the extragalactic hard X-ray background
• A Model of Supernovae Feedback in Galaxy Formation
• Intervening O VI Quasar Absorption Systems at Low Redshift: A Significant Baryon Reservoir
• The baryon content of the Universe
• Gas Rich Dwarf Spheroidals
• O VI and Multicomponent H I Absorption Associated with a Galaxy Group in the Direction of PG0953+415: Physical Conditions and Baryonic Content
• Hydrodynamic Simulation of the Cosmological X-ray Background
• Is There Still Room for Warm/Hot Gas? Simulating the X-ray Background Spectrum

Cited by in corpus (582)

• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• Cosmology and Fundamental Physics with the Euclid Satellite
• Cosmological SPH simulations: The entropy equation
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• The history of star formation in a LCDM universe
• The Baryon Census in a Multiphase Intergalactic Medium: 30% of the Baryons May Still Be Missing
• Highly-Ionized High-Velocity Gas in the Vicinity of the Galaxy
• The Progenitors of Dwarf Spheroidal Galaxies
• Diffuse Radio Emission from Galaxy Clusters
• Cosmological Shock Waves and Their Role in the Large Scale Structure of the Universe
• Galaxy Evolution in Cosmological Simulations with Outflows II: Metallicities and Gas Fractions
• Science with ASKAP - the Australian Square Kilometre Array Pathfinder
• Where Are the Baryons? II: Feedback Effects
• Smoothed Particle Hydrodynamics in Astrophysics
• Effects of Baryons and Dissipation on the Matter Power Spectrum
• Fundamental Physics with the Square Kilometre Array
• The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere
• A Revised Parallel-Sequence Morphological Classification of Galaxies: Structure and Formation of S0 and Spheroidal Galaxies
• Time-Dependent Ionization in Radiatively Cooling Gas
• Absolute measurement of the unresolved cosmic X-ray background in the 0.5-8 keV band with Chandra
• The Physics of the Intergalactic Medium
• Galaxy Evolution in Cosmological Simulations With Outflows I: Stellar Masses and Star Formation Rates
• The Evolution of the Intergalactic Medium
• The Search for the Missing Baryons at Low Redshift
• The Cosmic Baryon and Metal Cycles
• Probing the IGM/Galaxy Connection V: On the Origin of Lya and OVI Absorption at z<0.2
• Observations of the MIssing Baryons in the warm-hot intergalactic medium
• Ubiquitous giant Ly $\alpha$ nebulae around the brightest quasars at $z\sim 3.5$ revealed with MUSE
• Quasar Feedback: the Missing Link in Structure Formation
• The Birmingham-CfA cluster scaling project - III: entropy and similarity in galaxy systems
• The Global 21 Centimeter Background from High Redshifts
• Cosmic Dispersion Measure from Gamma-Ray Burst Afterglows: Probing the Reionization History and the Burst Environment
• A High-Resolution Survey of Low-Redshift QSO Absorption Lines: Statistics and Physical Conditions of O VI Absorbers
• Constrained Simulations of the Real Universe: II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region
• Revisiting the Cosmic Cooling Crisis
• Detecting shock waves in cosmological smoothed particle hydrodynamics simulations
• Probing the Cosmic Reionization History and Local Environment of Gamma-Ray Bursts through Radio Dispersion
• The Low-z Intergalactic Medium. III. HI and Metal Absorbers at z<0.4
• An analytical model for the history of cosmic star formation
• Chandra Discovery of a Tree in the X-ray Forest towards PKS 2155-304: the Local Filament?
• The Distribution of Metallicity in the IGM at z~2.5: OVI and CIV Absorption in the Spectra of 7 QSOs
• The evolution of the mass-metallicity relation in IllustrisTNG
• Inter-cluster filaments in a $\Lambda$CDM Universe
• Do Hot Haloes Around Galaxies Contain the Missing Baryons?
• Simulations of the Microwave Sky
• CANDELS: The Contribution of the Observed Galaxy Population to Cosmic Reionization
• Baryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids
• Warm-hot baryons comprise 5-10 per cent of filaments in the cosmic web
• Moving mesh cosmology: numerical techniques and global statistics
• The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
• Diffuse Radio Emission in/around the Coma Cluster: Beyond Simple Accretion
• Detection of hot gas in the filament connecting the clusters of galaxies Abell 222 and Abell 223
• Physical Implications of the X-ray Properties of Galaxy Groups and Clusters
• Simulating cosmic rays in clusters of galaxies - II. A unified scheme for radio halos and relics with predictions of the gamma-ray emission
• The Local Ly-alpha Forest IV: STIS G140M Spectra and Results on the Distribution and Baryon Content of HI Absorbers
• A Census of Oxygen in Star-Forming Galaxies: An Empirical Model Linking Metallicities, Star Formation Rates and Outflows
• Gamma-Rays from Intergalactic Shocks
• Probing the missing baryons with the Sunyaev-Zel'dovich effect from filaments
• A Limit from the X-ray Background on the Contribution of Quasars to Reionization
• A uniform metal distribution in the intergalactic medium of the Perseus cluster of galaxies
• An OVI Baryon Census of the Low-z Warm-Hot Intergalactic Medium
• The Bimodal Galaxy Stellar Mass Function in the COSMOS Survey to z~1: A Steep Faint End and a New Galaxy Dichotomy
• The WSRT wide-field HI survey: II. Local Group features
• Observations of Chemically Enriched QSO Absorbers near z ~ 2.3 Galaxies: Galaxy-Formation Feedback Signatures in the IGM
• Effect of Hot Baryons on the Weak-Lensing Shear Power Spectrum
• Galaxy Clustering and Galaxy Bias in a Lambda-CDM Universe
• Chandra Detection of the First X-ray Forest along the Line of Sight To Mkn 421
• Chandra Detection of OVIII Ly-alpha Absorption from an Overdense Region in the Intergalactic Medium
• The effect of non--gravitational gas heating in groups and clusters of galaxies
• Physical Properties, Baryon Content, and Evolution of the LyαForest: New Insights from High Resolution Observations at z < 0.4
• A filament of dark matter between two clusters of galaxies
• The intergalactic medium over the last 10 billion years I: Lyman alpha absorption and physical conditions
• Lyman-alpha Emission from Structure Formation
• The Nature and Origin of Low-Redshift O VI Absorbers
• On the Physical Origin of OVI Absorption-Line Systems
• The Commensal Real-time ASKAP Fast Transients (CRAFT) survey
• The intergalactic medium over the last 10 billion years II: Metal-line absorption and physical conditions
• The Galaxy Environment of O VI Absorption Systems
• AGN Feedback Causes Downsizing
• The Nature of the Warm/Hot Intergalactic Medium I. Numerical Methods, Convergence, and OVI Absorption
• The Relationship Between Intergalactic HI/OVI and Nearby (z<0.017) Galaxies
• Massive Coronae of Galaxies
• The Properties of Low Redshift Intergalactic O VI Absorbers Determined from High S/N Observations of 14 QSOs with the Cosmic Origins Spectrograph
• Simulating the gamma-ray emission from galaxy clusters: a universal cosmic ray spectrum and spatial distribution
• Hydrogen and Metal Line Absorption Around Low-Redshift Galaxies in Cosmological Hydrodynamic Simulations
• Probing the IGM-Galaxy Connection at z < 0.5 I: A Galaxy Survey in QSO Fields and a Galaxy-Absorber Cross-Correlation Study
• Simulating the physical properties of dark matter and gas inside the cosmic web
• Tracing the Warm-Hot Intergalactic Medium at Low Redshift: X-ray Forest Observations Towards H1821+643
• Physical Properties and Baryonic Content of Low-Redshift Intergalactic Ly-alpha and O VI Absorption Systems: The PG1116+215 Sight Line
• The XMM Cluster Outskirts Project (X-COP)
• The Fluctuating Intergalactic Radiation Field at Redshifts z = 2.3-2.9 from He II and H I Absorption towards HE 2347-4342
• AEGIS: The Morphologies of Green Galaxies at 0.4<z<1.2
• Cosmic Web of Galaxies in the COSMOS Field: Public Catalog and Different Quenching for Centrals and Satellites
• The Ionization and Metallicity of the Intervening O VI Absorber at z = 0.1212 in the Spectrum of H1821+643
• The Collision Between The Milky Way And Andromeda
• XMM-Newton discovery of an X-ray filament in Coma
• The dynamical state of brightest cluster galaxies and the formation of clusters
• Confirmation of X-Ray Absorption by WHIM in the Sculptor Wall
• X-Ray Absorption By WHIM in the Sculptor Wall
• Detection of Ne VIII in the Low-Redshift Warm-Hot IGM
• Reconstructing the Cosmic Velocity and Tidal Fields with Galaxy Groups Selected from the Sloan Digital Sky Survey
• The O VII X-ray forest toward Markarian 421: Consistency between XMM-Newton and Chandra
• The Enrichment History of Baryons in the Universe
• Hot Atmospheres, Cold Gas, AGN Feedback and the Evolution of Early Type Galaxies: a Topical Perspective
• Where Are the Baryons? III: Non-Equilibrium Effects and Observables
• Characterizing the Warm-Hot IGM at High Redshift: A High Resolution Survey for O VI at z = 2.5
• The missing metals problem. III How many metals are expelled from galaxies?
• A Survey of O VI, C III, and H I in Highly Ionized High-Velocity Clouds
• Intensity Mapping of Lyman-alpha Emission During the Epoch of Reionization
• Trident: a universal tool for generating synthetic absorption spectra from astrophysical simulations
• A New Prescription for Protogalactic Feedback and Outflows: Where Have All the Baryons Gone?
• X-Ray Scaling Relations of Galaxy Groups in a Hydrodynamic Cosmological Simulation
• Hot gas halos around disk galaxies: Confronting cosmological simulations with observations
• Revealing the Warm-Hot Intergalactic Medium with OVI Absorption
• Warm-Hot Gas in and around the Milky Way: Detection and Implications of OVII Absorption toward LMC X-3
• Chemical evolution in Sersic 159-03 observed with XMM-Newton
• The route to massive black hole formation via merger-driven direct collapse: a review
• Hydrodynamic Simulation of the Cosmological X-ray Background
• Imprint of Intergalactic Shocks on the Radio Sky
• Gas Condensation in the Galactic Halo
• Characterizing the Pressure Smoothing Scale of the Intergalactic Medium
• Signatures of Galactic Superwinds: Inhomogeneous Metal Enrichment of the Lyman Alpha Forest
• Chandra Detection of Local OVII He-alpha Absorption Along the Sight Line Toward 3C 273
• Reconstructing the cosmic density field with the distribution of dark matter halos
• Detection of warm and diffuse baryons in large scale structure from the cross-correlation of gravitational lensing and the thermal Sunyaev-Zeldovich effect
• Shock-Heated Gas in the Large Scale Structure of the Universe
• Star Formation Feedback and Metal Enrichment History Of The Intergalactic Medium
• Discovery of Magnetic Fields Along Stacked Cosmic Filaments as Revealed by Radio and X-Ray Emission
• Resolving the unresolved cosmic X-ray background in the Chandra Deep Fields
• Large-scale mass distribution in the Illustris simulation
• On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• Probing the Local Group Medium Toward Mkn 421 with Chandra and FUSE
• Preheating by Previrialization and its Impact on Galaxy Formation
• Testing Sunyaev-Zel'dovich measurements of the hot gas content of dark matter haloes using synthetic skies
• Hot Halos around High Redshift Protogalaxies: Observations of O VI and N V Absorption in Damped Lyman Alpha systems
• The Epoch of Helium Reionization
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• QSO Absorption Systems Detected in Ne VIII: High-Metallicity Clouds with a Large Effective Cross Section
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• Are we missing baryons in Galaxy Clusters?
• X-ray absorption evolution in Gamma-Ray Bursts: intergalactic medium or evolutionary signature of their host galaxies?
• Effects of the Intergalactic Plasma on Supernova Dimming via Photon-Axion Oscillations
• Probing the IGM/Galaxy Connection Toward PKS0405-123 I: UV Spectroscopy and Metal-Line Systems
• Large-Scale Structure Shocks at Low and High Redshifts
• Entropy Injection as a Global Feedback Mechanism
• Discovery of a Primitive Damped Lyman alpha Absorber Near an X-ray Bright Galaxy Group in the Virgo Cluster
• Formation of Cool Cores in Galaxy Clusters via Hierarchical Mergers
• Cosmological shock waves
• Mass assembly of galaxies: Smooth accretion versus mergers
• The Low-z Intergalactic Medium. II. LyB, OVI, and CIII Forest
• An EAGLE view of the missing baryons
• Forecasts for the detection of the magnetised cosmic web from cosmological simulations
• X-ray observations of the galaxy cluster Abell 2029 to the virial radius
• X-ray Absorption by the Low-redshift Intergalactic Medium: A Numerical Study of the Lambda CDM model
• Discrete clouds of neutral gas between the galaxies M31 and M33
• The Dynamic Radio Sky
• Broad HI Absorbers as Metallicity-Independent Tracers of the Warm-Hot Intergalactic Medium
• On the Structure of Hot Gas in Halos: Implications for the Lx-Tx Relation & Missing Baryons
• On the relationship between a giant radio galaxy MSH 05-22 and the ambient large-scale galaxy structure
• The warm-hot intergalactic medium at z~2.2: Metal enrichment and ionization source
• A STIS Survey for OVI Absorption Systems at 0.12 < z < 0.5 II.: Physical Conditions of the Ionised Gas
• The intergalactic magnetic field probed by a giant radio galaxy
• The phase-diagram of cosmological baryons
• The low-redshift intergalactic medium as seen in archival legacy Hubble/STIS and FUSE data
• The Heavy Element Enrichment of Lyman alpha Clouds in the Virgo Supercluster
• Probing the Intergalactic Medium with the OVI Forest
• Low Frequency Radio Constraints on the Synchrotron Cosmic Web
• The impact of feedback on the low redshift Intergalactic Medium
• Properties of the cosmological filament between two clusters: A possible detection of a large-scale accretion shock by $Suzaku$
• Tracing baryons in the warm-hot intergalactic medium with broad Ly alpha absorption
• The baryonic mass function of galaxies
• Detectability of the Warm/Hot Intergalactic Medium Through Emission Lines of OVII and OVIII
• Where are the missing cosmic metals ?
• Characterizing the Low-Redshift Intergalactic Medium towards PKS1302-102
• The Hot Intergalactic Medium - Galaxy Connection: Two Strong Absorbers in the Sightline Toward PG 1211+143
• The Simulated HI Sky at low redshift
• O VII and O VIII absorption by hot gas in the vicinity of the Galaxy
• A STIS Survey for OVI Absorption Systems at 0.12 < z < 0.5 I.: The Statistical Properties of Ionized Gas
• Absorption signatures of warm-hot gas at low redshift: OVI
• The ThreeHundred: the structure and properties of cosmic filaments in the outskirts of galaxy clusters
• Limiting Magnetic Fields in the Cosmic Web with Diffuse Radio Emission
• The Multiphase Intergalactic Medium towards PKS 2155-304
• A Near-Solar Metallicity, Nitrogen-Deficient Lyman Limit Absorber Associated with two S0 Galaxies
• Intergalactic Lyman continuum photon budget in the past 5 billion years
• Can the soft X-ray opacity towards high redshift sources probe the missing baryons?
• Lyman Break Galaxies and the Lyman-alpha Forest
• Disentangling the Cosmic Web Towards FRB 190608
• Virgo Cluster and field dwarf ellipticals in 3D: I. On the variety of stellar kinematic and line-strength properties
• Nonequilibrium ionization states and cooling rates of the photoionized enriched gas
• FUV and X-ray absorption in the Warm-Hot Intergalactic Medium
• The soft X-ray emission in a large sample of galaxy clusters with ROSAT PSPC
• An Introductory Review on Cosmic Reionization
• Absorption signatures of warm-hot gas at low redshift: Broad HI Lyman-Alpha Absorbers
• Soft X-ray excess emission in clusters of galaxies observed with XMM-Newton
• Cosmological Information from Quasar-Galaxy Correlations induced by Weak Lensing
• Exploring the magnetized cosmic web through low frequency radio emission
• The Accretion of Gas onto Galaxies as Traced by their Satellites
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Equilibration processes in the Warm-Hot Intergalactic Medium
• Simulating galaxy clusters -- I. Thermal and chemical properties of the intra-cluster medium
• A New Method to Directly Measure the Jeans Scale of the Intergalactic Medium Using Close Quasar Pairs
• Detection of the Missing Baryons toward the Sightline of H1821+643
• The Non-isothermality and Extent of Galactic Diffuse Hot Gas Toward Mrk~421
• The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
• Warm-hot intergalactic baryons revealed
• Dimming of Supernovae by Photon-Pseudoscalar Conversion and the Intergalactic Plasma
• O VI Absorbers Tracing Hot Gas Associated with a Pair of Galaxies at z = 0.167
• Probing the IGM/Galaxy Connection Toward PKS0405-123 III: The Galaxy Survey and Correlations with OVI Absorbers
• MRC B0319-454: Probing the large-scale structure with a giant radio galaxy
• Observations of a nearby filament of galaxy clusters with the Sardinia Radio Telescope
• The Impact of ICM Substructure on Ram Pressure Stripping
• The Low Redshift Circumgalactic Medium in Simba
• Improving the Accuracy of Cosmic Magnification Statistics
• First measurement of the bulk flow of nearby galaxies using the cosmic microwave background
• Probing the IGM-Galaxy Connection Toward PKS0405-123 II : A Cross-Correlation Study of Lya Absorbers and Galaxies at z<0.5
• Cosmic Origins Spectrograph Detection of Ne VIII Tracing Warm - Hot Gas Towards PKS 0405-123
• The kinetic SZ tomography with spectroscopic redshift surveys
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• Metal-line emission from the warm-hot intergalactic medium: I. Soft X-rays
• Studying the WHIM Content of the Galaxy Large-Scale Structures along the Line of Sight to H 2356-309
• Measuring Omega_0 with higher-order Quasar-Galaxy Correlations induced by Weak Lensing
• Towards the statistical detection of the warm-hot intergalactic medium in inter-cluster filaments of the cosmic web
• Inhomogeneous Helium Reionization and the Equation of State of the Intergalactic Medium
• High Metallicity, Photoionised Gas in Intergalactic Large-Scale Filaments
• Warm-hot Gas in X-ray Bright Galaxy Clusters and the H I-deficient Circumgalactic Medium in Dense Environments
• Cosmological baryon transfer in the SIMBA simulations
• Was the Cosmic Web of Protogalactic Material Permeated by Lobes of Radio Galaxies During the Quasar Era?
• Evolution of cosmic filaments and of their galaxy population from MHD cosmological simulations
• Chandra and XMM-Newton Observations of the Abell 3391/Abell 3395 Intercluster Filament
• Population III Generated Cosmic Rays and the Production of Li6
• Probing the IGM/Galaxy Connection IV: The LCO/WFCCD Galaxy Survey of 20 Fields Surrounding UV Bright Quasars
• Angular Broadening of Intraday Variable AGN. II. Interstellar and Intergalactic Scattering
• Warm Gas in the Virgo Cluster: I. Distribution of Lya Absorbers
• A massive warm baryonic halo in the Coma cluster
• Simulations of thermally broadened HI Lya absorption arising in the warm-hot intergalactic medium
• Chemical abundances in the polar disk of NGC4650A: implications for cold accretion scenario
• Properties of the diffuse X-ray background in a high-resolution hydrodynamical simulation
• Confirming the Detection of an Intergalactic X-ray Absorber Toward PKS 2155-304
• A survey of the thermal and non-thermal properties of cosmic filaments
• Detecting shocked intergalactic gas with X-ray and radio observations
• Missing baryons traced by the galaxy luminosity density in the large-scale WHIM filaments
• Properties of Cosmological Filaments extracted from Eulerian Simulations
• Bent-Double Radio Sources as Probes of Intergalactic Gas
• Metal-Absorption Column Densities in Fast Radiative Shocks
• Probing the Large-Scale Structure Around the Most Distant Galaxy Clusters from the Massive Cluster Survey
• Detection of highly ionized O and Ne absorption lines in the X-ray spectrum of 4U1820-303 in the globular cluster, NGC 6624
• Non-equilibrium Ionization State of Warm-Hot Intergalactic Medium
• Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster
• X-ray Constraints on the AGN Properties in Spitzer-IRS identified z~2 Ultraluminous Infrared Galaxies
• Hot Baryons and the Distribution of Metals in the Intergalactic Medium
• Multicomponent and Variable Velocity Galactic Outflow in Cosmological Hydrodynamic Simulations
• Chandra and Far Ultraviolet Spectroscopic Explorer Observations of z~0 Warm-Hot Gas Toward PKS 2155-304
• Warm-Hot Intergalactic Medium Associated with the Coma Cluster
• Finding the Missing Baryons with Fast Radio Bursts and Sunyaev-Zeldovich Maps
• Metal-Enriched Plasma in Protogalactic Halos: A Survey of N V Absorption in High-z Damped & Sub-Damped Lyman-alpha Systems
• Jet Feedback and the Photon Underproduction Crisis in Simba
• The Role of Cold Flows and Reservoirs in Galaxy Formation With Strong Feedback
• Gas distribution from clusters to filaments in IllustrisTNG
• Cross correlation of Lyman-alpha absorbers with gas-rich galaxies
• Giant Radio Galaxies: I. Intergalactic Barometers
• Numerical simulations of the Warm-Hot Intergalactic Medium
• A possible Chandra and Hubble Space Telescope detection of extragalactic WHIM towards PG 1116+215
• Intergalactic Gas in Groups of Galaxies: Implications for Dwarf Spheroidal Formation and The Missing Baryons Problem
• High-Velocity Clouds and the Local Intergalactic Medium
• Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster
• Detection of Ne VIII in an Intervening Multi-Phase Absorption System Towards 3C 263
• Detection of missing baryons in galaxy groups with kinetic Sunyaev-Zel'dovich effect
• Effects of metal enrichment and metal cooling in galaxy growth and cosmic star formation history
• Cosmic Origins Spectrograph and FUSE Observations of T ~ 10^5 K Gas In A Nearby Galaxy Filament
• PKS B1545-321: Bow shocks of a relativistic jet?
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• Metal-line emission from the warm-hot intergalactic medium: II. Ultraviolet
• The Probability Distribution of the Lya transmitted flux from a sample of SDSS quasars
• A high resolution study of intergalactic O VI absorbers at z~2.3
• The Low-Redshift Lyman Alpha Forest toward PKS 0405-123
• The Lyman-alpha emission of high-z damped Lyman-alpha systems
• The Temperature Structure of the Warm-Hot Intergalactic Medium
• The LOFAR view of intergalactic magnetic fields with giant radio galaxies
• Soft X-ray and extreme ultraviolet excess emission from clusters of galaxies
• Detecting the warm-hot intergalactic medium through X-ray absorption lines
• Relativistic AGN jets I. The delicate interplay between jet structure, cocoon morphology and jet-head propagation
• Chandra X-ray observations of Abell 1835 to the virial radius
• The eROSITA view of the Abell 3391/95 field: a case study from the Magneticum cosmological simulation
• The baryonic mass-velocity relation; clues to feedback processes during structure formation and the cosmic baryon inventory
• Thermodynamic evolution of cosmological baryonic gas: I. Influence of non-equipartition processes
• The intergalactic medium temperature and Compton y parameter
• Chandra Detection of Local Warm-Hot Gas Toward Markarian 279
• Ultraviolet Line Emission from Metals in the Low-Redshift Intergalactic Medium
• Constraints on hot metals in the Vicinity of the Galaxy
• An optical view of the filament region of Abell 85
• A VSA search for the extended Sunyaev-Zel'dovich Effect in the Corona Borealis Supercluster
• Simulation of Soft X-ray Emission Lines from the Missing Baryons
• Probing Warm-Hot Intergalactic Medium Associated with the Virgo Cluster using an Oxygen Absorption Line
• The effect of feedback on the emission properties of the Warm-Hot Intergalactic Medium
• Stellar kinematics for the central spheroid in the Polar Disk Galaxy NGC4650A
• Detection of diffuse radio emission at large distance from the center of the galaxy cluster A2255
• Warm-Hot Intergalactic Medium in the Sculptor Supercluster
• Evolution of mass and velocity filed in comic web: comparison between baryonic and dark matter
• The Sources of Extreme Ultraviolet and Soft X-ray Backgrounds
• The Epoch of Reionization in the R_h=ct Universe
• HST/COS detection of a Ne VIII absorber towards PG 1407+265: An unambiguous tracer of collisionally ionized hot gas?
• The polytropic approximation and X-ray scaling relations: constraints on gas and dark matter profiles for galaxy groups and clusters
• Locating the Warm-Hot Intergalactic Medium in the Simulated Local Universe
• New constraints on the magnetic field in filaments of the cosmic web
• A Possible Origin of Magnetic Fields in Galaxies and Clusters: Strong Magnetic fields at z~10?
• GALEX UV properties of the polar ring galaxy MCG-05-07-001 and the shell galaxies NGC 1210 and NGC 5329
• Sensitive 21cm Observations of Neutral Hydrogen in the Local Group near M31
• Simulations of bent-double radio sources in galaxy groups
• X-ray absorption towards high-redshift sources: probing the intergalactic medium with blazars
• Composition of Low Redshift Halo Gas
• HI in Group Interactions: HCG 44
• A Chandra HETG Observation of the Quasar H 1821+643 and Its Surrounding Cluster
• A warm hot intergalactic medium towards 3C 120?
• Future Evolution of the Intergalactic Medium in a Universe Dominated by a Cosmological Constant
• Missing baryons and the soft X-ray background
• Highly-Ionized Oxygen Absorbers in the Intergalactic Medium
• Decoding the giant extragalactic radio sources
• A Pair of O VI and Broad Ly-alpha Absorbers Probing Warm Gas in a Galaxy Group Environment at z ~ 0.4
• XMM-{\em Newton} and FUSE Tentative Evidence for a WHIM filament along the Line of Sight to PKS~0558-504
• Star Formation in Dwarf Galaxies of the Nearby Centaurus A Group
• Properties of clumps and filaments around galaxy clusters
• X-ray emission from warm-hot intergalactic medium: the role of resonantly scattered cosmic X-ray background
• Observable Signatures of the low-z Circum-Galactic and Inter-Galactic Medium : UV Line Emission in Simulations
• Simulating the Soft X-ray excess in clusters of galaxies
• Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
• Search for X-Ray Emission Associated with the Shapley Supercluster with Suzaku
• Tracing the Warm Hot Intergalactic Medium in the local Universe
• Chandra Observations of Two High-Redshift Quasars
• Searching for Intergalactic Shocks with the SKA
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• Testing Models of the Individual and Cosmological Evolutions of Powerful Radio Galaxies
• Photoionized OVI absorbers toward the bright QSO HE 0515-4414
• The Surprisingly Constant Strength of O VI Absorbers over Cosmic Time
• High-resolution O VI absorption line observations at 1.2 < z < 1.7 in the bright QSO HE 0515-4414
• Turbulence driven by structure formation in the circum-galactic medium
• Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
• XMM-Newton View of the z>0 Warm-Hot Intergalactic Medium Toward Markarian 421
• A view of PKS 2155-304 with XMM-Newton Reflection Grating Spectrometers
• Dual-Frequency Observations of 140 Compact, Flat-Spectrum Active Galactic Nuclei for Scintillation-Induced Variability
• Heating of the Hot Intergalactic Medium by Powerful Radio Galaxies and Associated High Energy Gamma-Ray Emission
• Reconstructing emission from pre-reionization sources with cosmic infrared background fluctuation measurements by the JWST
• The eROSITA view of the Abell 3391/95 field: The Northern Clump. The largest infalling structure in the longest known gas filament observed with eROSITA, XMM-Newton, and Chandra
• Testing Models of Radio Galaxy Evolution and the Cosmological Impact of FR II Radio Galaxies
• Multiphase Plasma in Sub-Damped Lyman Alpha Systems: A Hidden Metal Reservoir
• On the Heterogeneity of Metal-Line and Ly-Alpha Absorption in Galaxy "Halos" at z~0.7
• Implications of an updated ultraviolet background for the ionization mechanisms of intervening Ne VIII absorbers
• Baryons: What, When and Where?
• Temperature and Entropy Fields of Baryonic Gas in the Universe
• Studying Inter-Cluster Galaxy Filaments Through Stacking GMBCG Galaxy Cluster Pairs
• Studying the Warm-Hot Intergalactic Medium in Emission
• The first bent double lobe radio source in a known cluster filament: Constraints on the intra-filament medium
• Kinematic Sunyaev-Zeldovich Cosmic Microwave Background Temperature Anisotropies Generated by Gas in Cosmic Structures
• Joint modeling of the probability distribution and power spectrum of the Lya forest: comparison with observations at z=3
• X-raying the Intergalactic OVI Absorbers
• The hydrodynamic stability of gaseous cosmic filaments
• The effects of an ionizing background on the HI column density distribution in the local Universe
• Turbulence in the Inter-galactic Medium: Solenoidal and Dilatational Motions, and the Impact of Numerical Viscosity
• Chemical and Photometric Evolution of the Local Group Galaxy NGC 6822 in a Cosmological Context
• The Contribution of the Intergalactic Medium to Cosmic Microwave Background Anisotropies
• The Red Halo Phenomenon
• Synchrotron Emission on the Largest Scales: Radio Detection of the Cosmic-Web
• Future instrumentation for the study of the Warm-Hot Intergalactic Medium
• Discovery of a pre-merger shock in an intercluster filament in Abell 98
• Distributions of the Baryon Fraction on Large Scales in the Universe
• Absorption signatures of warm-hot gas at low redshift: NeVIII
• Detection of Two Intervening Ne VIII Absorbers Probing Warm Gas at z~0.6
• Numerical Simulations Unravel the Cosmic Web
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• A Study of Quasar Proximity in O VI Absorbers at z=2-3
• The Effect of Galactic Feedback on Gas Accretion and Wind Recycling
• The hot circumgalactic medium of the Milky-Way: new insights from XMM-Newton observations
• Galaxy properties in the cosmic web of EAGLE simulation
• Spectral shape of the UV ionizing background and OVI absorbers at z ~ 1.5 towards HS0747+4259
• X-Ray Absorption by the Warm-Hot Intergalactic Medium in the Hercules Supercluster
• A survey of HI gas toward the Andromeda Galaxy
• The large-scale environment from cosmological simulations II: The redshift evolution and distributions of baryons
• The eROSITA view of the Abell 3391/95 field: Cluster Outskirts and Filaments
• To be or not to be: hot WHIM absorption in the blazar PKS 2155-304 sight line?
• Filaments and sheets of the warm-hot intergalactic medium
• The X-ray background from groups and clusters of galaxies
• Thermal and non-thermal nature of the soft excess emission from Sersic 159-03 observed with XMM-Newton
• Cosmic evolution of metal densities: the enrichment of the Inter-Galactic Medium
• Soft X-ray Transmission Spectroscopy of Warm/Hot Intergalactic Medium with XEUS
• Extracting the late-time kinetic Sunyaev-Zel'dovich effect
• Relativistic AGN jets II. Jet properties and mixing effects for episodic jet activity
• The Galactic Environment of the NeVIII Absorber toward HE0226-4110
• Predicted Sizes of Pressure-Supported HI Clouds in the Outskirts of the Virgo Cluster
• A detailed study of the bridge of excess X-ray emission between the galaxy clusters Abell 2029 and Abell 2033
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot
• Soft and hard X-ray excess emission in Abell 3112 observed with Chandra
• Effect of the Metallicity on the X-ray Emission from the Warm-Hot Intergalactic Medium
• Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
• The Cross-correlation of KSZ Effect and 21 cm Intensity Mapping with Tidal Reconstruction
• The Santa Fe Light Cone Simulation Project: II. The Prospects for Direct Detection of the WHIM with SZE Surveys
• The diffuse soft excess emission in the Coma cluster from the ROSAT All-Sky Survey
• The Herschel Filament: a signature of the environmental drivers of galaxy evolution during the assembly of massive clusters at z=0.9
• X-Ray Searches for Emission from the WHIM in the Galactic Halo and the Intergalactic Medium
• Search for Oxygen Emission from Warm-Hot Intergalactic Medium around A2218 with Suzaku
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• Detecting X-ray filaments in the low redshift Universe with XEUS and Constellation-X
• Search for WHIM around A2744 using Suzaku
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• Cosmic Filaments in Superclusters
• An Observational Test for the Anthropic Origin of the Cosmological Constant
• Probing WHIM around Galaxy Clusters with Fast Radio Bursts and the Sunyaev-Zel'dovich effect
• The COS-legacy survey of C IV absorbers: properties and origins of the intervening systems
• The Kinematic Sunyaev-Zel'dovich Effect with ACT, DES, and BOSS: a Novel Hybrid Estimator
• Study of the Intracluster and Intergalactic Medium in the Sculptor Supercluster with Suzaku
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• The phase-diagram of the IGM and the entropy floor of groups and clusters: are clusters born warm?
• Can radiative cooling and nongravitational heating explain simultaneously the global X-ray properties of clusters and the unresolved cosmic X-ray background ?
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Discovery of a large-scale galaxy filament near a candidate intergalactic X-ray absorption system
• High Resolution Spectroscopy of X-ray Quasars: Searching for the X-ray Absorption from the Warm-Hot Intergalactic Medium
• Searching for the Intra-Group Medium in Loose Groups of Galaxies
• The Low-Redshift Lyman Alpha Forest toward 3C 273
• Cosmic gas highways in C-EAGLE simulations
• SGRS J0515-8100: a Fat-Double giant radio galaxy
• Influence of baryonic physics in galaxy simulations: a semi-analytic treatment of the molecular component
• Agnostic Stacking of Intergalactic Doublet Absorption: Measuring the NeVIII Population
• The WSRT Virgo HI filament survey I; Total Power Data
• A Unified Fitting of HI and HeII LyαTransmitted Flux of QSO HE2347 with LCDM Hydrodynamic Simulations
• Prospects of detecting soft X-ray emission from typical WHIM filaments around massive clusters and the Coma cluster soft excess
• Analytical Models for the Energetics of Cosmic Accretion Shocks, their Cosmological Evolution, and the Effect of Environment
• A detailed view of filaments and sheets in the warm-hot intergalactic medium. I. Pancake formation
• ELUCID VII: Using Constrained Hydro Simulations to Explore the Gas Component of the Cosmic Web
• A VLT/MUSE galaxy survey towards QSO Q1410: looking for a WHIM traced by BLAs in inter-cluster filaments
• Star Formation and Gas Phase History of the Cosmic Web
• Intergalactic baryon-rich regions at high redshift
• FIGARO Simulation: FIlaments & GAlactic RadiO Simulation
• Searching for HI imprints in cosmic web filaments with 21-cm intensity mapping
• Cross-Correlation of Diffuse Synchrotron and Large-Scale Structures
• Revisiting the formation History of the minor-axis dust lane galaxy NGC1947
• Constraining the baryon fraction in the Warm Hot Intergalactic Medium at low redshifts with PLANCK data
• Warm-hot intergalactic medium contribution to baryonic matter
• Hydrogen-like nitrogen radio line from hot interstellar and warm-hot intergalactic gas
• Scintillation as a Probe of the Intergalactic Medium
• Revisiting the He II to H I ratio in the Intergalactic Medium
• The diffuse X-ray background
• Detection of WHIM in the Planck data using Stack First approach
• Scatter broadening of compact radio sources by the ionized intergalactic medium: Prospects for detection with Space VLBI and the SKA
• A search for inter-cluster filaments with LOFAR and eROSITA
• The HeII Lyman alpha forest and the thermal state of the IGM
• COS Observations of the Cosmic Web: A Search for the Cooler Components of a Hot, X-ray Identified Filament
• An X-ray WHIM metal absorber from a Mpc-scale empty region of space
• Detection capabilities of the Athena X-IFU for the warm-hot intergalactic medium using gamma-ray burst X-ray afterglows
• Evolution of CIV Absorbers. II. Where does CIV live?
• Balancing the Baryon Budget: The fraction of the IGM due to Galaxy Mergers
• Tilted outer and inner structures in edge-on galaxies?
• Soft X-ray emission from warm gas in IllustrisTNG circum-cluster environments
• The contribution of the kinematic Sunyaev-Zel'dovich Effect from the Warm Hot Intergalactic Medium to the Five-Year WMAP Data
• Exploring the thermal energy contents of the intergalactic medium with the Sunyaev-Zel'dovich effect
• Observing the Sunyaev-Zel'dovich Effect Closer to Home
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• Correlations between O VI Absorbers and Galaxies at Low Redshift
• Simulating the LOcal Web (SLOW) -- III: Synchrotron emission from the local cosmic web
• The spatial distribution of galaxies within the CMB cold spot in the Corona Borealis supercluster
• Detection of a Multiphase Intragroup Medium: Results from the COS-IGrM Survey
• The relation between Lyman-alpha absorbers and gas--rich galaxies in the local universe
• Measuring Feedback Using the Intergalactic Medium State and Evolution Inferred from the Soft X-ray Background
• Carbon ionization states and the cosmic far-UV background with HeII absorption
• A galaxy overdensity at z=0.401 associated with an X-ray emitting structure of Warm-Hot Intergalactic Medium
• An HST/COS Observation of Broad Ly$\alpha$ Emission and Associated Absorption Lines of the BL Lacertae Object H 2356-309
• Tracing the 10${}^7$K Warm-Hot Intergalactic Medium with UV absorption lines
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters
• Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• ROSAT observations of the soft X-ray background and of the cluster soft excess emission in the Hercules supercluster
• The Relationship Between Baryons and Dark Matter in Extended Galaxy Halos
• Lyman Alpha Flux Power Spectrum and Its Covariance
• Constraining the thermal history of the Warm-Hot Intergalactic Medium
• Building galaxies, stars, planets and the ingredients for life between the stars. A scientific proposal for a European Ultraviolet-Visible Observatory (EUVO)
• Cross-correlation between the soft X-ray background and SZ Sky
• Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift
• The baryon density at z=0.9-1.9 - Tracing the warm-hot intergalactic medium with broad Lyman alpha absorption
• The Molecular Hydrogen Explorer H2EX
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• Estimating Power Spectrum of Sunyaev-Zeldovich Effect from the Cross-Correlation between WMAP and 2MASS
• Studying the ICM in clusters of galaxies via surface brightness fluctuations of the cosmic X-ray background
• CMB Anisotropy Due to Filamentary Gas: Power Spectrum and Cosmological Parameter Bias
• A Soft X-ray Component in the Abell 754 Cluster
• Stacking the Synchrotron Cosmic Web with FIGARO
• The contribution of the Warm-Hot Intergalactic Medium to the CMB anisotropies via the Sunyaev-Zeldovich effect
• Constraints on the Sunyaev-Zel'dovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
• Diffuse neutral hydrogen in the HI Parkes All Sky Survey
• A search for Warm-Hot Intergalactic Medium features in the X-ray spectra of Mkn 421 with the XMM-Newton RGS
• Bringing Simulation and Observation Together to Better Understand the Intergalactic Medium
• A new limit on intergalactic magnetic fields on sub-kpc scales from fast radio bursts
• On the projected mass distribution around galaxy clusters : a Lagrangian theory of harmonic power spectra
• Galaxy clusters as probes for cosmology and dark matter
• A search for the missing baryons with X--ray absorption lines towards the blazar 1ES 1553+113
• Technique for detecting warm-hot intergalactic gas in quasar UV spectra
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• A WHIM origin for the soft excess emission in the Coma cluster
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• Autocorrelation function of the soft X-ray background produced by warm-hot gas in dark halos
• Measuring cosmic filament spin with the kinetic Sunyaev-Zel'dovich effect
• Constituents of the soft X-ray background
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Lensing and the Warm Hot Intergalactic Medium
• High-resolution absorption spectroscopy of the circumgalactic medium of the Milky Way
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• Understanding Galaxy Formation and Evolution
• The Glow of Axion Quark Nugget Dark Matter: (II) Galaxy Clusters
• Resilience of Sloshing Cold Fronts against Subsequent Minor Mergers
• Discovery of X-shaped Morphology of the Giant Radio Galaxy GRG 0503-286
• A study of the galaxy redshift distribution toward the cosmic microwave background cold spot in the Corona Borealis supercluster
• A new way of detecting intergalactic baryons
• Searching for the Synchrotron Cosmic Web Again: A replication attempt
• Are the red halos of galaxies made of low-mass stars? Constraints from subdwarf star counts in the Milky Way halo
• Statistical and dynamical decoupling of the IGM from Dark Matter
• Structure and Evolution of Dwarf Galaxies
• X-ray spectroscopy of Abell S1101 with Chandra, XMM-Newton and ROSAT: band-pass dependence of he temperature profile and soft excess emission
• The End of the Rainbow: What Can We Say About the Extragalactic Sub-Megahertz Radio Sky?
• The signature of the Warm Hot Intergalactic Medium in WMAP and the forthcoming PLANCK data
• The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Cluster outskirts and their connection to the cosmic web
• Relation between the local width and linear halo mass density of cosmic filaments
• Robust detection of hot intragroup medium in optically selected, poor galaxy groups by eROSITA
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Galaxy cluster photons alter the ionisation state of the nearby warm-hot intergalactic medium
• Constraining the ionized gas evolution with CMB-spectroscopic survey cross-correlation
• Joint inference on the redshift distribution of fast radio burst and on the intergalactic baryon content
• Measurement of the dispersion of radiation from a steady cosmological source
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• From Nearby Low Luminosity AGN to High Redshift Radio Galaxies: Science Interests with SKA
• High-redshift AGN population in radiation-hydrodynamics simulations
• Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements
• Tentative detection of warm intervening gas towards PKS 0548-322 with XMM-Newton
• The Evolution of the Baryon Distribution in the Universe from Cosmological Simulations
• The temperature of IGM at high redshifts: shock heating and high mach problem
• Soft X-ray excess of clusters: a thermal filament model, and the strong lensing of background galaxy groups
• Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations
• A high-redshift quasar absorber without CIV - a galactic outflow caught in the act?
• Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
• X-ray Halos around Massive Galaxies: Data and Theory
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• High-resolution observations of two OVI absorbers at z=2 towards PKS 1448-232
• HI Imaging the Low Red-shift Cosmic Web
• Convolutional Deep Denoising Autoencoders for Radio Astronomical Images
• The WSRT virgo filament survey
• Lyman Alpha Absorber Correlations and the Bias of the Lyman Alpha Forest
• Characterization of the warm--hot intergalactic medium near the Coma cluster through high--resolution spectroscopy of X Comae
• Looking for the Signals of the Missing Baryons in the Extragalactic Background Light
• Multiple Absorption-Line Spectroscopy of the Intergalactic Medium. I. Model
• A New Census of the Universe's Entropy
• A search for sub-second radio variability predicted to arise toward 3C 84 from intergalactic dispersion
• Correlation between the Mean Matter Density and the Width of the Saturated Lyman Alpha Absorption
• Partially Cooled Shocks: Detectable Precursors in the Warm/Hot Intergalactic Medium
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• A positive correlation between broad HI Ly$\alpha$ absorptions and local overdensities of galaxies
• A Search for X-Ray Reionization Signatures from Cross-Correlation of Wmap and ROSAT Rass Data
• FUSE Observations of Galactic and Intrinsic Absorption in the Spectrum of the Seyfert 1 Galaxy 2MASX J21362313-6224008
• Searching for the Missing Baryons in the Warm-Hot Intergalactic Medium
• The large-scale distribution of ionized metals in IllustrisTNG
• The Scaling Relation between Galaxy Luminosity and WHIM Density from EAGLE Simulations with application to SDSS data
• The intergalactic medium in the cosmic web
• The eventful life journey of galaxy clusters. II. Impact of mass accretion on the thermodynamical structure of the ICM
• Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena
• Cosmological simulation of a radio synchrotron bridge between pre-merging galaxy clusters
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• X-ray emission in IllustrisTNG circum-cluster environments. II -- Possible origins of the soft X-ray excess emission
• WHIM emission and the cluster soft excess: a model comparison
• The thermodynamic structure and large-scale structure filament in MACS J0717.5+3745
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• Sample Variance in Cosmological Observations with a Narrow Field-of-View
• Chandra Detection of X-ray Absorption from Local Warm/Hot Gas
• X-ray Observations of the Warm-Hot Intergalactic Medium
• Chandra and FUSE view of the WHIM: the Local Group and beyond
• Does light from steady sources bear any observable imprint of the dispersive intergalactic medium?
• Profiles of cosmic filaments since z=4.0 in cosmological hydrodynamical simulation