The Cosmic Energy Inventory

Abstract

We present an inventory of the cosmic mean densities of energy associated with all the known states of matter and radiation at the present epoch. The observational and theoretical bases for the inventory have become rich enough to allow estimates with observational support for the densities of energy in some 40 forms. The result is a global portrait of the effects of the physical processes of cosmic evolution.

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Cited by in corpus (391)

• The Simons Observatory: Science goals and forecasts
• Cosmological Constraints from the SDSS Luminous Red Galaxies
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• Cool Gas in High Redshift Galaxies
• Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions
• Dusty Star-Forming Galaxies at High Redshift
• Damped Lyman alpha Systems
• A census of baryons in the Universe from localized fast radio bursts
• Cold gas accretion in galaxies
• Updated Nearby Galaxy Catalog
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• The Baryon Census in a Multiphase Intergalactic Medium: 30% of the Baryons May Still Be Missing
• The Evolution of Compact Binary Star Systems
• The Cosmic Origins Spectrograph
• CMB-S4 Science Case, Reference Design, and Project Plan
• A single fast radio burst localized to a massive galaxy at cosmological distance
• Damped Lyman Alpha Systems at z<1.65: The Expanded SDSS HST Sample
• The Evolution of the Intergalactic Medium
• A Budget and Accounting of Metals at z~0: Results from the COS-Halos Survey
• The Search for the Missing Baryons at Low Redshift
• The Cosmic Baryon and Metal Cycles
• New Relationships between Galaxy Properties and Host Halo Mass, and the Role of Feedbacks in Galaxy Formation
• Locating the "missing" baryons with extragalactic dispersion measure estimates
• Galaxies in LCDM with Halo Abundance Matching: luminosity-velocity relation, baryonic mass-velocity relation, velocity function and clustering
• The Arecibo Legacy Fast ALFA Survey: X. The HI Mass Function and Omega_HI From the 40% ALFALFA Survey
• Gravity and Large-Scale Non-local Bias
• Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II - Data Release 7
• A Fast Radio Burst Host Galaxy
• Herschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years
• The MORGANA model for the rise of galaxies and active nuclei
• A Larger Estimate of the Entropy of the Universe
• Star formation sustained by gas accretion
• Do Hot Haloes Around Galaxies Contain the Missing Baryons?
• Simulations of Cosmic Chemical Enrichment
• The Space Motion of Leo I: The Mass of the Milky Way's Dark Matter Halo
• Galaxy groups and clouds in the Local (z~0.01) universe
• Reconciling the local galaxy population with damped Ly-alpha cross sections and metal abundances
• The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
• Measuring the galaxy-mass and galaxy-dust correlations through magnification and reddening
• The evolution of AGN across cosmic time: what is downsizing?
• The Evolution of Galaxy Number Density at z < 8 and its Implications
• Herschel-ATLAS Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies
• A census of metals and baryons in stars in the local Universe
• Production and evolution of Li, Be and B isotopes in the Galaxy
• The ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass Density
• A Census of Oxygen in Star-Forming Galaxies: An Empirical Model Linking Metallicities, Star Formation Rates and Outflows
• The Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos
• Probing the missing baryons with the Sunyaev-Zel'dovich effect from filaments
• Building galaxies by accretion and in-situ star formation
• New Colour-Mass to Light Relations: the role of the Asymptotic Giant Branch phase and of interstellar dust
• Using the X-ray Morphologies of Young Supernova Remnants to Constrain Explosion Type, Ejecta Distribution, and Chemical Mixing
• Simulating the dust content of galaxies: successes and failures
• Massive Warm/Hot Galaxy Coronae as Probed by UV/X-ray Oxygen Absorption and Emission: I - Basic Model
• Comparison of Cluster Lensing Profiles with Lambda CDM Predictions
• Tracing the cosmological assembly of stars and supermassive black holes in galaxies
• Discovery of an Enormous Ly$\alpha$ nebula in a massive galaxy overdensity at $z=2.3$
• How do central and satellite galaxies quench? -- Insights from spatially resolved spectroscopy in the MaNGA survey
• A Search for Warm/Hot Gas Filaments Between Pairs of SDSS Luminous Red Galaxies
• The Hubble flow around the Local Group
• Evidence for the kinematic Sunyaev-Zeľdovich effect with ACTPol and velocity reconstruction from BOSS
• Are galactic star formation and quenching governed by local, global or environmental phenomena?
• Outskirts of Galaxy Clusters
• The Cosmic Web: Geometric Analysis
• The intergalactic medium over the last 10 billion years I: Lyman alpha absorption and physical conditions
• On the Evolutionary History of Stars and their Fossil Mass and Light
• The Atacama Cosmology Telescope: Modeling the Gas Thermodynamics in BOSS CMASS galaxies from Kinematic and Thermal Sunyaev-Zel'dovich Measurements
• The Nature and Origin of Low-Redshift O VI Absorbers
• The intergalactic medium over the last 10 billion years II: Metal-line absorption and physical conditions
• The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
• Dark Matter investigation by DAMA at Gran Sasso
• 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
• Supernovae in the Subaru Deep Field: the rate and delay-time distribution of type Ia supernovae out to redshift 2
• Very high redshift quasars and the rapid emergence of super-massive black holes
• IGM Emission Observations with the Cosmic Web Imager: I. The Circum-QSO Medium of QSO 1549+19, and Evidence for a Filamentary Gas Inflow
• Massive Coronae of Galaxies
• The History of Cosmological Star Formation: Three Independent Approaches and a Critical Test Using the Extragalactic Background Light
• Galactic fountains and the rotation of disc-galaxy coronae
• The Evolution of Compact Binary Star Systems
• X-ray Group and cluster mass profiles in MOND: Unexplained mass on the group scale
• The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift
• The star formation history of early-type galaxies as a function of mass and environment
• Star formation properties in the Local Volume galaxies via $H\alpha$ and FUV fluxes
• Cosmological simulation with dust formation and destruction
• Primordial nucleosynthesis
• The missing metals problem. III How many metals are expelled from galaxies?
• The Galactic Halo Contribution to the Dispersion Measure of Extragalactic Fast Radio Bursts
• Short Gamma-Ray Bursts and Binary Mergers in Spiral and Elliptical Galaxies: Redshift Distribution and Hosts
• Gas Accretion via Condensation and Fountains
• Taking the Universe's Temperature with Spectral Distortions of the Cosmic Microwave Background
• The History and Morphology of Helium Reionization
• Characterizing the Pressure Smoothing Scale of the Intergalactic Medium
• Cosmic dust in MgII absorbers
• The mode of gas accretion onto star-forming galaxies
• Dust in the Circumgalactic Medium of Low-Redshift Galaxies
• Large-scale mass distribution in the Illustris simulation
• An Investigation of Sloan Digital Sky Survey Imaging Data and Multi-Band Scaling Relations of Spiral Galaxies (with Dynamical Information)
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Observational Upper Bound on the Cosmic Abundances of Negative-mass Compact Objects and Ellis Wormholes from the Sloan Digital Sky Survey Quasar Lens Search
• Constraints on the missing baryons from the kinetic Sunyaev-Zeldovich effect in Planck data
• A new measurement of the Hubble constant using Fast Radio Bursts
• The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data
• The Role of Sub-damped Lyman-alpha Absorbers in the Cosmic Evolution of Metals
• Energetics of High-Energy Cosmic Radiations
• Are the distributions of Fast Radio Burst properties consistent with a cosmological population?
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
• A Measurement of the Galaxy Group-Thermal Sunyaev-Zel'dovich Effect Cross-Correlation Function
• The Millennium Galaxy Catalogue: The local supermassive black hole mass function in early- and late-type galaxies
• Discrete clouds of neutral gas between the galaxies M31 and M33
• A STIS Survey for OVI Absorption Systems at 0.12 < z < 0.5 II.: Physical Conditions of the Ionised Gas
• The stellar contribution to the extra-galactic background light and absorption of high-energy gamma-rays
• The impact of feedback on the low redshift Intergalactic Medium
• IGM Emission Observations with the Cosmic Web Imager: II. Discovery of Extended, Kinematically-Linked Emission around SSA22 Lyman-alpha Blob 2
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• Dynamical Interactions and the Black Hole Merger Rate of the Universe
• Constraints on frequency-dependent violations of Shapiro delay from GW150914
• Antimatter and antistars in the universe and in the Galaxy
• The baryonic mass function of galaxies
• Probing Dark Matter Substructure with Pulsar Timing
• Characterizing the Low-Redshift Intergalactic Medium towards PKS1302-102
• The baryonic Tully-Fisher relation and galactic outflows
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• The meV mass frontier of axion physics
• Observability of Dark Matter Substructure with Pulsar Timing Correlations
• The dust content of QSO hosts at high redshift
• Cosmology-independent estimate of the fraction of baryon mass in the IGM from fast radio burst observations
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• Seeding Black Holes in Cosmological Simulations
• Can the soft X-ray opacity towards high redshift sources probe the missing baryons?
• Hierarchical Growth and Cosmic Star Formation: Enrichment, Outflows and Supernova Rates
• Cosmological model with non-minimally coupled fermionic field
• Metal-rich Damped/sub-Damped Lyman-alpha Quasar Absorbers at z<1
• Cosmology-insensitive estimate of IGM baryon mass fraction from five localized fast radio bursts
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• H-ATLAS: The cosmic abundance of dust from the far-infrared background power spectrum
• Nonequilibrium ionization states and cooling rates of the photoionized enriched gas
• uvby-βphotometry of high-velocity and metal-poor stars XI. Ages of halo and old disk stars
• Measuring the circum- and inter-galactic baryon contents with fast radio bursts
• Orbital masses of nearby luminous galaxies
• The Degree of Fine-Tuning in our Universe -- and Others
• A New Empirical Constraint on the Prevalence of Technological Species in the Universe
• Probing the diffuse baryon distribution with the lensing-tSZ cross-correlation
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• The metallicity distribution of the halo and the satellites of the Milky way in the hierarchical merging paradigm
• A Comparison of Absorption and Emission Line Abundances in the Nearby Damped Lyman-alpha Galaxy SBS 1543+593
• Chemical enrichment of Damped Lyman Alpha systems as a direct constraint on Population III star formation
• A Multiphase Absorber Containing O VI and Broad H I Directly Tracing 10^6 K Plasma at Low-Redshift Toward HE 0153-4520
• Studying the WHIM Content of the Galaxy Large-Scale Structures along the Line of Sight to H 2356-309
• Finding the missing baryons in the intergalactic medium with localized fast radio bursts
• Metal-line emission from the warm-hot intergalactic medium: I. Soft X-rays
• The kinetic SZ tomography with spectroscopic redshift surveys
• Cosmic Origins Spectrograph Detection of Ne VIII Tracing Warm - Hot Gas Towards PKS 0405-123
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Marriage à-la-MOND: Baryonic dark matter in galaxy clusters and the cooling flow puzzle
• Tools for Dissecting Supernova Remnants Observed with Chandra: Methods and Application to the Galactic Remnant W49B
• Monolithic or hierarchical star formation? A new statistical analysis
• Studying the WHIM with Gamma Ray Bursts
• Primordial Globular Clusters, X-Ray Binaries & Cosmological Reionisation
• Conditions For Successful Helium Detonations In Astrophysical Environments
• Bent-Double Radio Sources as Probes of Intergalactic Gas
• The missing metals problem: II. How many metals are in z ~ 2.2 galaxies?
• The local Tully-Fisher relation for dwarf galaxies
• Effective photon mass and (dark) photon conversion in the inhomogeneous Universe
• Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• Axion decay and anisotropy of near-IR extragalactic background light
• The Future of Fast Radio Burst Science
• The Effect of Hot Gas in WMAP's First Year Data
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Effects of Inhomogeneities on Cosmic Expansion
• A List of Groups of Dwarf Galaxies in the Local Supercluster
• More galaxies in the Local Volume imaged in H-alpha
• Numerical simulations of the Warm-Hot Intergalactic Medium
• Missing Dark Matter in the Local Universe
• Intergalactic Gas in Groups of Galaxies: Implications for Dwarf Spheroidal Formation and The Missing Baryons Problem
• An Introduction to Galactic Chemical Evolution
• Detection of Ne VIII in an Intervening Multi-Phase Absorption System Towards 3C 263
• Cosmic Origins Spectrograph and FUSE Observations of T ~ 10^5 K Gas In A Nearby Galaxy Filament
• Supernova progenitors and iron density evolution from SN rate evolution measurements
• 1I/2017 'Oumuamua-like Interstellar Asteroids as Possible Messengers from the Dead Stars
• Numerical Simulations of Hot Halo Gas in Galaxy Mergers
• Constraining Magnetic Fields in the Circumgalactic Medium
• Perspectives of High Energy Neutrino Astronomy
• Catalog of Nearby Isolated Galaxies in the Volume z<0.01
• Statistical modelling of the cosmological dispersion measure
• The Cosmological Evolution of the Average Mass Per Baryon
• The dust mass function from z~0 to z~2
• Detecting the warm-hot intergalactic medium through X-ray absorption lines
• Gas contents of galaxy groups from thermal Sunyaev-Zel'dovich effects
• Measurement of the thermal Sunyaev-Zel'dovich effect around cosmic voids
• Constraining non-minimally coupled tachyon fields by Noether symmetry
• The cosmic dust rate across the Universe
• Kinematics, ages and metallicities for F and G type stars in the solar neighbourhood
• The star formation history of damped Lyman alpha absorbers
• First stars and the extragalactic background light: How recent gamma-ray observations constrain the early universe
• Probing Diffuse Gas with Fast Radio Bursts
• Stellar and dark matter density in the Local Universe
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• The local supermassive black hole mass density: corrections for dependencies on the Hubble constant
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• The Atacama Cosmology Telescope: Probing the Baryon Content of SDSS DR15 Galaxies with the Thermal and Kinematic Sunyaev-Zel'dovich Effects
• Stellar prospects for FRB gravitational lensing
• H$\alpha$ intensity map of the repeating fast radio burst FRB 121102 host galaxy from Subaru/Kyoto 3DII AO-assisted optical integral-field spectroscopy
• Simulations of galactic disks including a dark baryonic component
• Stellar Black Holes and the Origin of Cosmic Acceleration
• Dwarf Galaxies in the Local Volume
• The energetics, evolution, and stellar depletion of Li6 in the early Galaxy
• Ultra-diffuse cluster galaxies as key to the MOND cluster conundrum
• Evolution of active galactic nuclei
• An 8.0\% Determination of the Baryon Fraction in the Intergalactic Medium from Localized Fast Radio Bursts
• The QCD phase transition behind a PBH origin of LIGO/Virgo events?
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• Large Scale Structure in Absorption: Gas within and around Galaxy Voids
• HST/COS detection of a Ne VIII absorber towards PG 1407+265: An unambiguous tracer of collisionally ionized hot gas?
• X-ray emission from cosmic web filaments in SRG/eROSITA data
• Detected fluctuations in SDSS LRG magnitudes: Bulk flow signature or systematic?
• Intense look at Virgo Southern Extension
• Simulations of bent-double radio sources in galaxy groups
• Constraining the Evolution of the Baryon Fraction in the IGM with FRB and H(z) data
• Model for a Universe described by a non-minimally coupled scalar field and interacting dark matter
• Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
• Rest-frame UV line emission from the intergalactic medium at 2<z<5
• The thermal Sunyaev-Zel'dovich Signature of Baryons in the Local Universe
• Observable Signatures of the low-z Circum-Galactic and Inter-Galactic Medium : UV Line Emission in Simulations
• The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations
• How the diffuse Universe cools
• Dark energy interacting with neutrinos and dark matter: a phenomenological theory
• Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
• A Conditional Luminosity Function Model of the Cosmic Far-Infrared Background Anisotropy Power Spectrum
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• The phantom dark matter halos of the Local Volume in the context of modified Newtonian dynamics
• Dual-Frequency Observations of 140 Compact, Flat-Spectrum Active Galactic Nuclei for Scintillation-Induced Variability
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• On the evolution of the Fe abundance and of the Type Ia SN rate in clusters of galaxies
• The Black Hole Mass Function Across Cosmic Times I. Stellar Black Holes and Light Seed Distribution
• Fast motions of galaxies in the Coma I cloud: a case of Dark Attractor?
• Kinematic Sunyaev-Zeldovich Cosmic Microwave Background Temperature Anisotropies Generated by Gas in Cosmic Structures
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• Studying the Warm-Hot Intergalactic Medium in Emission
• The Contribution of the Intergalactic Medium to Cosmic Microwave Background Anisotropies
• Chemical and Photometric Evolution of the Local Group Galaxy NGC 6822 in a Cosmological Context
• Probing large scale filaments with HI and ${}^3$HeII
• Future instrumentation for the study of the Warm-Hot Intergalactic Medium
• Discovery of a pre-merger shock in an intercluster filament in Abell 98
• The metallicity distribution of HI systems in the EAGLE cosmological simulation
• Methodological Reflections on the MOND/Dark Matter Debate
• Gravitational-Wave Constraints on the Progenitors of Fast Radio Bursts
• The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
• On the peculiar momentum of baryons after Reionization
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• Fermion field as inflaton, dark energy and dark matter
• Loss of star forming gas in SDSS galaxies
• Chemical constraints on the contribution of Population III stars to cosmic reionization
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Comparing Dark Energy Survey and HST-CLASH observations of the galaxy cluster RXC J2248.7-4431: implications for stellar mass versus dark matter
• The imprint of the cosmic supermassive black hole growth history on the 21 cm background radiation
• Matter Distribution around Galaxies
• Soft X-ray Transmission Spectroscopy of Warm/Hot Intergalactic Medium with XEUS
• Extracting the late-time kinetic Sunyaev-Zel'dovich effect
• Discussion on the energy content of the galactic dark matter Bose-Einstein condensate halo in the Thomas-Fermi approximation
• X-Ray Searches for Emission from the WHIM in the Galactic Halo and the Intergalactic Medium
• Understanding Giant Radio Galaxy J1420-0545: Large-Scale Morphology, Environment, and Energetics
• The Cross-correlation of KSZ Effect and 21 cm Intensity Mapping with Tidal Reconstruction
• The Cosmological Unimportance of Low Surface Brightness Galaxies
• The galaxy HI-(sub)halo connection and the HI spatial clustering of local galaxies
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Backlighting extended gas halos around luminous red galaxies: kinematic Sunyaev-Zel'dovich effect from DESI Y1 x ACT
• Are rotation curves in NGC 6946 and the Milky Way magnetically supported?
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• Cosmic explosions, life in the Universe and the Cosmological Constant
• Fast radio bursts' recipes for the distributions of dispersion measures, flux densities, and fluences
• Constraints on differential Shapiro delay between neutrinos and photons from IceCube-170922A
• 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
• Influence of baryonic physics in galaxy simulations: a semi-analytic treatment of the molecular component
• Implementation of a Fourier Matched Filter in CMB Analyses. Application to ISW Studies
• Direct Search for Dark Matter - Striking the Balance - and the Future
• Agnostic Stacking of Intergalactic Doublet Absorption: Measuring the NeVIII Population
• Geometry and growth contributions to cosmic shear observables
• Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM
• A Decade-Baseline Study of the Plasma States of Ejecta Knots in Cassiopeia A
• The Cosmic Evolution of Fast Radio Bursts Inferred from the CHIME/FRB Baseband Catalog 1
• Searching for HI imprints in cosmic web filaments with 21-cm intensity mapping
• Cross-Correlation of Near and Far-Infrared Background Anisotropies as Traced by Spitzer and Herschel
• Star Formation and Gas Phase History of the Cosmic Web
• Probing the baryon mass fraction in IGM and its redshift evolution with fast radio bursts using Bayesian inference method
• Observations of the High Redshift Universe
• HI Clouds in the M81 Filament as Dark Matter Minihalos--A Phase-Space Mismatch
• Photometric classification of HSC transients using machine learning
• The cosmic transparency measured with Type Ia supernovae: implications for intergalactic dust
• Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data
• Hydrogen-like nitrogen radio line from hot interstellar and warm-hot intergalactic gas
• Constraining the baryon fraction in the Warm Hot Intergalactic Medium at low redshifts with PLANCK data
• H_2D^+: a light on baryonic dark matter?
• The Origin of Neutral Hydrogen Clouds in Nearby Galaxy Groups: Exploring the Range Of Galaxy Interactions
• Scatter broadening of compact radio sources by the ionized intergalactic medium: Prospects for detection with Space VLBI and the SKA
• An X-ray WHIM metal absorber from a Mpc-scale empty region of space
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Generalizing the Cosmic Energy Equation
• Reconstruction of Baryon Fraction in Intergalactic Medium through Dispersion Measurements of Fast Radio Bursts
• On Iron Enrichment, Star Formation, and Type Ia Supernovae in Galaxy Clusters
• Exploring the thermal energy contents of the intergalactic medium with the Sunyaev-Zel'dovich effect
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• Balancing the Baryon Budget: The fraction of the IGM due to Galaxy Mergers
• Halting eternal acceleration with an effective negative cosmological constant
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• The circumgalactic medium in Lyman-alpha: a new constraint on galactic outflow models
• Chemical evolution models: GRB host identification and cosmic dust predictions
• Dark Sector from Interacting Canonical and Non-Canonical Scalar Fields
• Detection of Metal-Rich, Cool-Warm Gas in the Outskirts of Galaxy Clusters
• High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
• Star Formation in Nearby Isolated Galaxies
• The B-L Phase Transition: Implications for Cosmology and Neutrinos
• Missing baryons, bulk flows and the E-mode polarization of the Cosmic Microwave Background
• The nature of Damped Lyman-α and MgII absorbers explored with their dust contents
• Detecting neutral hydrogen at z > 3 in large spectroscopic surveys of quasars
• Searching for decaying axion-like dark matter from clusters of galaxies
• Generalized Layzer-Irvine equation: the role of dark energy perturbations in cosmic structure formation
• A galaxy overdensity at z=0.401 associated with an X-ray emitting structure of Warm-Hot Intergalactic Medium
• Cosmological Covariance of Fast Radio Burst Dispersions
• Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
• Maximal X-ray feedback in the pre-reionization universe
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• Removal and mixing of the coronal gas from satellites in galaxy groups: cooling the intragoup gas
• Life Products of Stars
• FRB Line-of-sight Ionization Measurement From Lightcone AAOmega Mapping Survey: the First Data Release
• The extragalactic background light from the measurements of the attenuation of high-energy gamma-ray spectrum
• Low Density Structures in the Local Universe. I. Diffuse Agglomerates of Galaxies
• A possible dearth of hot gas in galaxy groups at intermediate redshift
• The Molecular Hydrogen Explorer H2EX
• Astrophysics in 2005
• Bringing Simulation and Observation Together to Better Understand the Intergalactic Medium
• Concentrating the Dark Matter in Galaxy Clusters through Tidal Stripping of Baryonically-Compressed Galactic Halos
• Nearby groups of galaxies in the Hercules-Bootes constellations
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• Self-forced evolutions of an implicit rotating source: A natural framework to model comparable and intermediate mass-ratio systems from inspiral through ringdown
• Star Formation in Nearby Dwarf Galaxies
• Constraints on the Sunyaev-Zel'dovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
• That is not dead which can eternal lie: the aestivation hypothesis for resolving Fermi's paradox
• The contribution of the Warm-Hot Intergalactic Medium to the CMB anisotropies via the Sunyaev-Zeldovich effect
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Ultra-Flat Galaxies Selected from RFGC Catalog. III. Star Formation Rate
• "Firewall" Phenomenology with Astrophysical Neutrinos
• Vortical Motions of Baryonic Gas in the Cosmic Web: Growth History and Scaling Relation
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
• Understanding Galaxy Formation and Evolution
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• A Bayesian chemical evolution model of the DustPedia Galaxy M74
• Velocities hasten to tell us about the Universe
• A high-resolution view of the filament of gas between Abell 399 and Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2
• Cosmological Time, Entropy and Infinity
• Weak lensing corrections to tSZ-lensing cross correlation
• Are the red halos of galaxies made of low-mass stars? Constraints from subdwarf star counts in the Milky Way halo
• Constraints on running vacuum models with the baryon-to-photon ratio
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• The End of the Rainbow: What Can We Say About the Extragalactic Sub-Megahertz Radio Sky?
• The Effect of Gravitational Lensing on Fast Transient Event Rates
• Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
• Layzer-Irvine equation: new perspectives and the role of interacting dark energy
• The signature of the Warm Hot Intergalactic Medium in WMAP and the forthcoming PLANCK data
• A Global Census of Metals in the Universe
• Constraining the ionized gas evolution with CMB-spectroscopic survey cross-correlation
• Variation of the baryon-to-photon ratio due to decay of dark matter particles
• Can Massive Gravity Explain the Mass Discrepancy - Acceleration Relation of Disk Galaxies?
• The Hydrogen Mixing Portal, Its Origins, and Its Cosmological Effects
• Star formation rates in nearby Markarian galaxies
• Dust Evolution in Simulated Multiphase Galactic Outflows
• Star formation in thin disks of spiral galaxies seen face-on
• A numerical fit of analytical to simulated density profiles in dark matter haloes
• Constrain intergalactic medium from the SZ effect map
• The expanding universe: an introduction
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• Cosmic Radioactivity and Galactic Chemical Evolution
• The Edges of Our Universe
• Red Halos of Galaxies - Reservoirs of Baryonic Dark Matter?
• Physics of star formation history and the luminosity function of galaxies therefrom
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• Constraining the Size of the Circumgalactic Medium Using the Transverse Autocorrelation Function of C IV Absorbers in Paired Quasar Spectra
• Cavendish experiment with fast radio bursts on cosmological scales
• Applied Nanofabrication for X-ray Grating Spectroscopy
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Bound or blown: the fate of hot gas in galaxy groups
• Early Cosmic Chemical Evolution: Relating the Origin of a Diffuse Intergalactic Medium and the First Long-Lived Stars
• On the capability of high redshift kSZ measurement with galaxy surveys
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• H2 MAGIE: H2 as a Major Agent to Galaxy Interaction and Evolution