Radiative transfer in a clumpy universe: IV. New synthesis models of the cosmic UV/X-ray background
arXiv:1105.2039 · doi:10.1088/0004-637X/746/2/125
Abstract
We present improved synthesis models of the evolving spectrum of the UV/X-ray diffuse background, updating and extending our previous results. Five new main components are added to our radiative transfer code CUBA: (1) the sawtooth modulation of the background intensity from resonant line absorption in the Lyman series of cosmic hydrogen and helium; (2) the X-ray emission from obscured and unobscured quasars; (3) a piecewise parameterization of the distribution in redshift and column density of intergalactic absorbers that fits recent measurements of the mean free path of 1 ryd photons; (4) an accurate treatment of the photoionization structure of absorbers; and (5) the UV emission from star-forming galaxies at all redshifts. We provide tables of the predicted HI and HeII photoionization and photoheating rates for use, e.g., in cosmological hydrodynamics simulations of the Lya forest, and a new metallicity-dependent calibration to the UV luminosity density-star formation rate density relation. A "minimal cosmic reionization model" is also presented in which the galaxy UV emissivity traces recent determinations of the cosmic history of star formation, the luminosity-weighted escape fraction of hydrogen-ionizing radiation increases rapidly with lookback time, the clumping factor of the high-redshift intergalactic medium evolves following the results of recent hydrodynamic simulations, and Population III stars and miniquasars make a negligible contribution to the metagalactic flux. The model provides a good fit to the hydrogen-ionization rates inferred from flux decrement and proximity effect measurements, predicts that cosmological HII (HeIII) regions overlap at redshift 6.7 (2.8), and yields an optical depth to Thomson scattering that is in agreement with WMAP results. (Abridged)
28 pages, 17 figures, accepted for publication in The Astrophysical Journal
Cited by in corpus (917)
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- The Reionization of Carbon
- Metal Mixing and Ejection in Dwarf Galaxies is Dependent on Nucleosynthetic Source
- Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field
- Hot phase generation by supernovae: resolution, chemistry and thermal conduction
- Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies
- Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies
- Constraining Reionization with the Lyman- Forest Power Spectrum: the Outlook after Planck
- Figuring Out Gas & Galaxies in Enzo (FOGGIE). II. Emission from the z=3 Circumgalactic Medium
- HST/COS Observations of Ionized Gas Accretion at the Disk-halo Interface of M33
- Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
- The Dispersion of Fast Radio Bursts from a Structured Intergalactic Medium at Redshifts z < 1.5
- Warm-hot Gas in X-ray Bright Galaxy Clusters and the H I-deficient Circumgalactic Medium in Dense Environments
- The Impact of Different Physical Processes on the Statistics of Lyman-limit and Damped Lyman-alpha Absorbers
- Imprints of temperature fluctuations on the Lyman- forest: a view from radiation-hydrodynamic simulations of reionization
- A new Measurement of the Intergalactic Temperature at
- Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
- Cold Dark Matter Substructures in Early-Type Galaxy Halos
- Detection of hot, metal-enriched outflowing gas around 2.3 star-forming galaxies in the Keck Baryonic Structure Survey
- The COS Absorption Survey of Baryon Harbors: Unveiling the Physical Conditions of Circumgalactic Gas through Multiphase Bayesian Ionization Modeling
- Large scale simulations of H and He reionization and heating driven by stars and more energetic sources
- Probing the end of reionization with the near-zones of z > 6 QSOs
- SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
- Winds of change: reionization by starburst galaxies
- The Power Spectrum of the Lyman- Forest at z < 0.5
- HST/COS Spectra of Three QSOs That Probe The Circumgalactic Medium of a Single Spiral Galaxy: Evidence for Gas Recycling and Outflow
- Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption
- The Evolution of the HeII-Ionizing Background at Redshifts 2.3<z<3.8 Inferred from a Statistical Sample of 24 HST/COS HeII Ly Absorption Spectra
- Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
- Sample variance and Lyman-alpha forest transmission statistics
- Enrichment of Zinc in galactic chemodynamical evolution models
- Satellite dwarf galaxies: Stripped but not quenched
- RAMSES-RTZ: Non-Equilibrium Metal Chemistry and Cooling Coupled to On-The-Fly Radiation Hydrodynamics
- The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
- The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
- Quenched Cold Accretion of a Large Scale Metal-Poor Filament due to Virial Shocking in the Halo of a Massive z=0.7 Galaxy
- Young and turbulent: the early life of massive galaxy progenitors
- An HST/COS survey of molecular hydrogen in DLAs & sub-DLAs at z < 1: Molecular fraction and excitation temperature
- Observations of a Magellanic Corona
- The Unchanging Circumgalactic Medium Over the Past 11 Billion Years
- The Mass and Absorption Columns of Galactic Gaseous Halos
- General framework for cosmological dark matter bounds using -body simulations
- Effective photon mass and (dark) photon conversion in the inhomogeneous Universe
- Starbursts in low-mass haloes at Cosmic Dawn. I. The critical halo mass for star formation
- Magnetization of the intergalactic medium in the IllustrisTNG simulations: the importance of extended, outflow-driven bubbles
- A chemical model for the interstellar medium in galaxies
- X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
- Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background
- Constraints on QSO emissivity using H I and He II Lyman alpha forest
- Exploring the Thermal State of the Low-Density Intergalactic Medium at z=3 with an Ultra-High Signal-to-Noise QSO Spectrum
- Helium Reionization Simulations. II. Signatures of Quasar Activity on the IGM
- The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
- Chasing Lyman alpha-emitting galaxies at z = 8.8
- The AGORA High-resolution Galaxy Simulations Comparison Project. III: Cosmological zoom-in simulation of a Milky Way-mass halo
- Stacking the Cosmic Web in Fluorescent Lyman alpha Emission with MUSE
- The Relationship Between Galaxy ISM and Circumgalactic Gas Metallicities
- Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
- Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
- The Incidence of Low-Metallicity Lyman-Limit Systems at z~3.5: Implications for the Cold-Flow Hypothesis of Baryonic Accretion
- The Pan-STARRS1 Quasar Survey: III. The Quasar Luminosity Function
- Ultra-Compact High Velocity Clouds as Minihalos and Dwarf Galaxies
- Dual Effects of Ram Pressure on Star Formation in Multi-phase Disk Galaxies with Strong Stellar Feedback
- Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
- Galaxy formation with radiative and chemical feedback
- Galactic angular momentum in cosmological zoom-in simulations. I. Disk and bulge components and the galaxy--halo connection
- Jet Feedback and the Photon Underproduction Crisis in Simba
- Estimating the effective lifetime of the quasar population from the composite proximity zone profile
- NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
- The CGM and IGM at z5: metal budget and physical connection
- NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
- Observational constraints on key-parameters of cosmic reionisation history
- A novel approach to correcting -based mass-metallicity relations
- Empirically Constrained Predictions for Metal-Line Emission from the Circumgalactic Medium
- Inferring the Thermal History of the Intergalactic Medium from the Properties of the Hydrogen and Helium Lyman-alpha Forest
- He II Proximity Effect and the Lifetime of Quasars
- Origin of Cosmic Chemical Abundances
- The CGM Survey: Circumgalactic O VI from dwarf to massive star-forming galaxies
- Galaxies Probing Galaxies in PRIMUS - II. The Coherence Scale of the Cool Circumgalactic Medium
- Inhomogeneous HeII reionization in Hydrodynamic Simulations
- The 21-cm Line as a Probe of Reionization
- X-ray Twinkles and Pop III Stars
- The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
- Lyα emission from galaxies in the Epoch of Reionization
- NIHAO-XXIII: Dark Matter density shaped by Black Hole feedback
- COS-Weak: Probing the CGM using analogs of weak Mg II absorbers at z < 0.3
- Large 21 cm signals from AGN-dominated reionization
- The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase
- The evolution of the Si IV content in the Universe from the epoch of reionization to cosmic noon
- RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
- Rapid Black Hole Growth at the Dawn of the Universe: A Super-Eddington Quasar at z=6.6
- The Effects of Ram-pressure Stripping and Supernova Winds on the Tidal Stirring of Disky Dwarfs: Enhanced Transformation into Dwarf Spheroidals
- Observations of metals in the intergalactic medium and comparison to the EAGLE simulations
- Cosmic Ray Driven Outflows from the Large Magellanic Cloud: Contributions to the LMC Filament
- Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies
- HST/COS Observations of Thirteen New He II Quasars
- Direct collapse to supermassive black hole seeds: the critical conditions for suppression of cooling
- Modeling the Lyman-alpha Forest in Collisionless Simulations
- Mapping metals at high redshift with far-infrared lines
- AGN-driven helium reionization and the incidence of extended HeIII regions at redshift z>3
- Time-Dependent Cooling in Photoionized Plasma
- Circumgalactic Pressure Profiles Indicate Precipitation-Limited Atmospheres for
- Not So Heavy Metals: Black Hole Feedback Enriches The Circumgalactic Medium
- Efficiency of metal mixing in dwarf galaxies
- The effect of non-equilibrium metal cooling on the interstellar medium
- The Effect Of AGN Heating On The Low-Redshift Lyα Forest
- Self-shielding of hydrogen in the IGM during the epoch of reionization
- In search of cool flow accretion onto galaxies where does the disk gas end?
- AGNs as main contributors to the UV ionizing emissivity at high redshifts: predictions from a Lambda-CDM model with linked AGN/galaxy evolution
- Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts 2.3-4.1
- How Ram Pressure Drives Radial Gas Motions in the Surviving Disk
- The circumgalactic medium of high redshift galaxies
- A Short Introduction to Reionization Physics
- High redshift AGNs and HI reionisation: limits from the unresolved X-ray background
- Figuring Out Gas & Galaxies in Enzo (FOGGIE). III. The Mocky Way: Investigating Biases in Observing the Milky Way's Circumgalactic Medium
- The global structure of magnetic fields and gas in simulated Milky Way-analogue galaxies
- The Relation Between Galaxy ISM and Circumgalactic OVI Gas Kinematics Derived from Observations and CDM Simulations
- Emission from the circumgalactic medium: from cosmological zoom-in simulations to multiwavelength observables
- Molecular Hydrogen Absorption from the Halo of a z ~ 0.4 Galaxy
- Osaka Feedback Model II: Modeling Supernova Feedback Based on High-Resolution Simulations
- Simulating the effect of photoheating feedback during reionization
- Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
- The Infrared Medium-deep Survey. VIII. Quasar Luminosity Function at
- What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations
- A self-consistent semi-analytic model for Population III star formation in minihalos
- The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
- The Star Formation Rate Efficiency of Neutral Atomic-dominated Hydrogen Gas in the Outskirts of Star Forming Galaxies from z~1 to z~3
- The baryonic Tully-Fisher relation in the Simba simulation
- CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass and radius
- The MUSE Extremely Deep Field: a first panoramic view of an Mg II emitting intragroup medium
- Anomaly in the Opacity of the Post-Reionization Intergalactic Medium in the Ly and Ly Forest
- The Lyman continuum escape fraction and the Mean Free Path of hydrogen ionizing photons for bright z~4 QSOs from SDSS DR14
- The Cosmic Ultraviolet Baryon Survey (CUBS) IV: The Complex Multiphase Circumgalactic Medium as Revealed by Partial Lyman Limit Systems
- Evolution of active galactic nuclei
- Barred galaxies in cosmological zoom-in simulations: the importance of feedback
- How much metals did the first stars provide to the ultra-faint dwarfs?
- Cloud-by-cloud, multiphase, Bayesian modeling: Application to four weak, low ionization absorbers
- HST-COS Observations of AGNs. III. Spectral Constraints in the Lyman Continuum from Composite COS/G140L Data
- HST/COS detection of a Ne VIII absorber towards PG 1407+265: An unambiguous tracer of collisionally ionized hot gas?
- KODIAQ-Z: Metals and Baryons in the Cool Intergalactic and Circumgalactic Gas at 2.2<z<3.6
- Simulating the H2 content of high-redshift galaxies
- Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
- Urchin: A Reverse Ray Tracer for Astrophysical Applications
- The Sources of Extreme Ultraviolet and Soft X-ray Backgrounds
- Origin of highly -process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
- Small-scale structure and the Lyman- forest baryon acoustic oscillation feature
- A high space density of L* Active Galactic Nuclei at z~4 in the COSMOS field
- Bar resilience to flybys in a cosmological framework
- An HST/COS legacy survey of intervening SiIII absorption in the extended gaseous halos of low-redshift galaxies
- Evolution of CIV Absorbers I. The Cosmic Incidence
- A self-consistent 3D model of fluctuations in the helium-ionizing background
- X-ray emission from warm-hot intergalactic medium: the role of resonantly scattered cosmic X-ray background
- Composition of Low Redshift Halo Gas
- The Effect of Fluctuations on the Helium-Ionizing Background
- A Pair of O VI and Broad Ly-alpha Absorbers Probing Warm Gas in a Galaxy Group Environment at z ~ 0.4
- First study of reionization in the Planck 2015 normalized closed CDM inflation model
- Models of the Cosmological 21 cm Signal from the Epoch of Reionization Calibrated with Lyman-alpha and CMB Data
- Modeling the HeII Transverse Proximity Effect: Constraints on Quasar Lifetime and Obscuration
- Distribution of Faint Atomic Gas in Hickson Compact Groups
- Revealing the Ionization Properties of the Magellanic Stream using Optical Emission
- Viscosity, pressure, and support of the gas in simulations of merging cool-core clusters
- On the detectability of visible-wavelength line emission from the local circumgalactic and intergalactic medium
- The Faint Host Galaxies of C IV Absorbers at z > 5
- The ACCELERATION programme: I. Cosmology with the redshift drift
- Boosting galactic outflows with enhanced resolution
- NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
- Possible Population III Remnants at Redshift 3.5
- Black-hole mass estimates for a homogeneous sample of bright flat-spectrum radio quasars
- The effect of inhomogeneous reionisation on the Lyman- forest power spectrum at redshift : implications for thermal parameter recovery
- The scattering of FRBs by the intergalactic medium: variations, strength and dependence on dispersion measures
- Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
- Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
- HIFlow: Generating Diverse HI Maps and Inferring Cosmology while Marginalizing over Astrophysics using Normalizing Flows
- Probing Feedback via IGM tomography and Ly forest with Subaru PFS, TMT/ELT, and JWST
- Properties of Molecular Gas in Galaxies in Early and Mid Stage of Interaction: II. Molecular Gas Fraction
- EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
- Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
- Discovery of intergalactic bridges connecting two faint quasars
- The Luminosity Function of bright QSOs at z~4 and implications for the cosmic ionizing background
- Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
- The CGM at Cosmic Noon with KCWI: Outflows from a Star-forming Galaxy at z=2.071
- Simba: The average properties of the circumgalactic medium of quasars are determined primarily by stellar feedback
- Highly r-process enhanced stars in ultra-faint dwarf galaxies
- Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT
- Exploring the origins of a new, apparently metal-free gas cloud at z = 4.4
- A universal average spectral energy distribution for quasars from optical to extreme ultraviolet
- Implications of an updated ultraviolet background for the ionization mechanisms of intervening Ne VIII absorbers
- High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5
- Evidence of First Stars-enriched Gas in High-redshift Absorbers
- New Evidence for Extended HeII Reionization at z>3.5 from HeII Lyman Alpha and Beta Transmission Spikes
- Empirically-motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations
- On the origin of low escape fractions of ionizing radiation from massive star-forming galaxies at high redshift
- Mapping quasar light echoes in 3D with Lyα forest tomography
- Effect of non-equilibrium ionization on derived physical conditions of the high- intergalactic medium
- The Dawn of Disk Formation in a Milky Way-sized Galaxy Halo: Thin Stellar Disks at
- Atomic and molecular gas from the epoch of reionization down to redshift 2
- The spectral and environment properties of quasar pairs
- Modelling the cosmological Lyman-Werner background radiation field in the Early Universe
- Texas Spectroscopic Search for Ly Emission at the End of Reionization II. The Deepest Near-Infrared Spectroscopic Observation at
- A first estimate of the Milky Way dark matter halo spin
- The effect of stellar and AGN feedback on the low redshift Lyman- forest in the Sherwood simulation suite
- A Fundamental Test for Galaxy Formation Models: Matching the Lyman- Absorption Profiles of Galactic Halos over Three Decades in Distance
- Constraints on Dark Matter-Baryon Scattering from the Temperature Evolution of the Intergalactic Medium
- Constraining the Tail-End of Reionization Using Lyman- Transmission Spikes
- The Impact of Cosmic Rays on the Kinematics of the Circumgalactic Medium
- The co-evolution of molecular hydrogen and the grain size distribution in an isolated galaxy
- The Lyman-alpha forest in f(R) modified gravity
- OVI Traces Photoionized Streams With Collisionally Ionized Boundaries in Cosmological Simulations of Massive Galaxies
- Compressing the cosmological information in one-dimensional correlations of the Lyman- forest
- The Thermal Proximity Effect: A New Probe of He II Reionization History and the Quasar Lifetime
- On the inconsistency between cosmic stellar mass density and star formation rate up to
- Evolution of Neutral Oxygen During the Epoch of Reionization and its Use in Estimating the Neutral Hydrogen Fraction
- Alone on a wide wide sea. The origin of SECCO 1, an isolated star-forming gas cloud in the Virgo cluster
- On the contribution of active galactic nuclei to reionization (Research Note)
- Gauging Metallicity of Diffuse Gas Under An Uncertain Ionizing Radiation Field
- Dating individual quasars with the HeII proximity effect
- A high molecular fraction in a sub-damped absorber at z=0.56
- Observing the circumgalactic medium of simulated galaxies through synthetic absorption spectra
- Hot and Turbulent Gas in Clusters
- Enrichment of Strontium in Dwarf Galaxies
- Evolution of Cold Streams and Emergence of the Hubble Sequence
- Origins of carbon-enhanced metal-poor stars
- Probing large scale filaments with HI and HeII
- Absorption signatures of warm-hot gas at low redshift: NeVIII
- Cosmic Galaxy-IGM HI Relation at Probed in the COSMOS/UltraVISTA deg Field
- Hydrodynamic simulations of an isolated star-forming gas cloud in the Virgo cluster
- Detection of Two Intervening Ne VIII Absorbers Probing Warm Gas at z~0.6
- Dwarf Spheroidal Satellite Formation in a Reionized Local Group
- An Ultraviolet Survey of Low-Redshift Partial Lyman-Limit Systems with the HST Cosmic Origins Spectrograph
- The complementary roles of feedback and mergers in building the gaseous halo and the X-ray corona of Milky Way-sized galaxies
- Constraining the Contribution of Galaxies and Active Galactic Nuclei to Cosmic Reionization
- SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
- Enhanced star formation in quasar companions
- Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
- Self-ionizing galactic winds
- IslandFAST: A Semi-numerical Tool for Simulating the Late Epoch of Reionization
- Effects of Photoionization and Photoheating on Lyman-alpha Forest Properties from Cholla Cosmological Simulations
- He II optical depth and UV escape fraction of galaxies
- Efficient long-range AGN feedback affects the low redshift Lyman- forest
- Shaping the structure of a GMC with radiation and winds
- A high baryon fraction in massive haloes at z~3
- The redshift evolution of the baryonic Tully-Fisher relation in Simba
- Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
- AGN-driven quenching of satellite galaxies
- Chemical constraints on the contribution of Population III stars to cosmic reionization
- Gas around galaxy haloes - II: hydrogen absorption signatures from the environments of galaxies at redshifts 2 < z < 3
- The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z
- A tale of seven narrow spikes and a long trough: constraining the timing of the percolation of HII bubbles at the tail-end of reionization with ULAS J1120+0641
- The Infrared Medium-deep Survey. VI. Discovery of Faint Quasars at with a Medium-band-based Approach
- A new model framework for circumgalactic Ly radiative transfer constrained by galaxy-Ly forest clustering
- Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
- Atomic Chemistry in Turbulent Astrophysical Media II: Effect of the Redshift Zero Metagalactic Background
- Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
- Connecting cosmological accretion to strong Lyman-alpha absorbers
- The AGORA High-resolution Galaxy Simulations Comparison Project. V: Satellite Galaxy Populations In A Cosmological Zoom-in Simulation of A Milky Way-mass Halo
- The influence of metagalactic ultra-violet background fluctuations on the high-redshift Ly forest
- Discovery and origins of giant optical nebulae surrounding quasar PKS 0454-22
- Predominantly Low Metallicities Measured in a Stratified Sample of Lyman Limit Systems at z=3.7
- Distribution and kinematics of 26Al in the Galactic disc
- The HI mass function as a probe of photoionisation feedback on low mass galaxy formation
- Efficient adiabatic hydrodynamical simulations of the high-redshift intergalactic medium
- The low redshift Lyman- Forest as a constraint for models of AGN feedback
- Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
- Aligned metal absorbers and the ultraviolet background at the end of reionization
- Simulated metal and HI absorption lines at the conclusion of Reionization
- The Elephant in the Bathtub: when the physics of star formation regulate the baryon cycle of galaxies
- H2 chemistry in galaxy simulations: an improved supernova feedback model
- HI-to-H Transitions in Dust-Free Interstellar Gas
- The isotropic interplanetary dust cloud and near-infrared extragalactic background light observed with COBE/DIRBE
- A neural network emulator for the Lyman- 1D flux power spectrum
- The Anatomy of a Turbulent Radiative Mixing Layer: Insights from an Analytic Model with Turbulent Conduction and Viscosity
- The baryon cycle of Seven Dwarfs with superbubble feedback
- Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
- A Moving Mesh Hydrodynamic Solver for ChaNGa
- Imprints of the first billion years: Lyman limit systems at
- Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function
- Local photoionization feedback effects on galaxies
- The evolution of the low-density HI intergalactic medium from z=3.6 to 0: Data, transmitted flux and HI column density
- Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?
- Sub-damped Lyman alpha systems in the XQ-100 survey II -- Chemical evolution at 2.4<z<4.3
- Dust diffusion in SPH simulations of an isolated galaxy
- Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
- Using Artificial Neural Networks to extract the 21-cm Global Signal from the EDGES data
- UV Background Fluctuations and Three-Point Correlations in the Large Scale Clustering of the Lyman-alpha Forest
- One-Two Quench: A Double Minor Merger Scenario
- NIHAO XXVI: Nature versus nurture, the Star Formation Main Sequence and the origin of its scatter
- A bottom-up search for Lyman-continuum leakage in the Hubble Ultra Deep Field
- Impact of Population III homogeneous stellar evolution on early cosmic reionisation
- It's a Breeze: The Circumgalactic Medium of a Dwarf Galaxy is Easy to Strip
- First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
- Non-equilibrium ionisation and radiative transport in an evolving supernova remnant
- Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
- The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
- Ionization bias and the ghost proximity effect near quasars in the shadow of proximate absorption systems
- Mapping Lyman-alpha forest three-dimensional large scale structure in real and redshift space
- Gas clump formation via thermal instability in high-redshift dwarf galaxy mergers
- Multiwavelength Campaign on Mrk 509 X. Lower limit on the distance of the absorber from HST COS and STIS spectroscopy
- Probing the Dependence of the Intergalactic Medium on Large Scale Environment Using the Low Redshift Lyman Alpha Forest
- The COS-legacy survey of C IV absorbers: properties and origins of the intervening systems
- Multiwavelength campaign on Mrk 509 IX. The Galactic foreground
- Probing Reionization and Early Cosmic Enrichment with the MgII Forest
- A Long Stream of Metal-Poor Cool Gas around a Massive Starburst Galaxy at z = 2.67
- Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
- Calibration of a star formation and feedback model for cosmological simulations with Enzo
- Hunting for Metals Using XQ-100 Legacy Survey Composite Spectra
- {\it HST}/COS Observations of the Warm Ionized Gaseous Halo of NGC 891
- Revised estimates of CMB -mode polarization induced by patchy reionization
- Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
- The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
- Measuring alignments between galaxies and the cosmic web at using IGM tomography
- Radiative Turbulent Mixing Layers and the Survival of Magellanic Debris
- The Flatness and Sudden Evolution of the Intergalactic Ionizing Background
- Stellar cluster formation in a Milky Way-sized galaxy at z>4 -- I. The proto-globular cluster population and the imposter amongst us
- Lyman-tomography of cosmic infrared background fluctuations with Euclid: probing emissions and baryonic acoustic oscillations at z>10
- Neural networks: solving the chemistry of the interstellar medium
- The Mass and Absorption Columns of Galactic Gaseous Halos II -- The High Ionization State Ions
- How Robust are the Inferred Density and Metallicity of the Circumgalactic Medium?
- Measurements of effective optical depth in the Ly forest from the BOSS DR12 Quasar sample
- Probing the environment of high-z quasars using the proximity effect in projected quasar pairs
- Simplified galaxy formation with mesh-less hydrodynamics
- The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
- The Manhattan Suite: Accelerated galaxy evolution in the early Universe
- Fast, high-fidelity Lyman forests with convolutional neural networks
- Testable predictions of outside-in age gradients in dwarf galaxies of all types
- How Metals Are Transported In And Out Of A Galactic Disk: Dependence On The Hydrodynamic Schemes In Numerical Simulations
- ELUCID VII: Using Constrained Hydro Simulations to Explore the Gas Component of the Cosmic Web
- Implications of the Lyman- forest for the 21-cm power spectrum from the epoch of reionization
- The impact of temperature fluctuations on the large-scale clustering of the Ly forest
- The ESO UVES Advanced Data Products Quasar Sample - IV. On the deficiency of Argon in DLA systems
- HyPhy: Deep Generative Conditional Posterior Mapping of Hydrodynamical Physics
- Detecting the neutral IGM in filaments with the SKA
- Discovery of a cool, metal-rich gas reservoir in the outskirts of z ~ 0.5 clusters
- Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
- Multicomponent H2 in DLA at zabs = 2.05: physical conditions through observations and numerical models
- Role of ionizing background on the statistics of metal absorbers in hydrodynamical simulations
- The impact and response of minihalos and the inter-halo medium on cosmic reionization
- Simulating intergalactic quasar scintillation
- Helium Reionization Simulations. III. The Helium Lyman- Forest
- Novel bounds on decaying axionlike particle dark matter from the cosmic background
- The effects of binary stars on galaxies and metal-enriched gas during reionization
- Prospects for Observing the low-density Cosmic Web in Lyman-alpha Emission
- Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
- SCORCH. III. Analytical Models of Reionization with Varying Clumping Factors
- The THESAN-ZOOM project: Population III star formation continues until the end of reionization
- Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
- Simulating Hydrodynamics in Cosmology with CRK-HACC
- Testing Galaxy Formation Simulations with Damped Lyman- Abundance and Metallicity Evolution
- Non-equilibrium temperature evolution of ionization fronts during the Epoch of Reionization
- Clumping factors of HII, HeII and HeIII
- Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
- Modeling Photoionized Turbulent Material in the Circumgalactic Medium
- On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
- The distribution and properties of DLAs at z 2 in the EAGLE simulations
- Constraining IGM enrichment and metallicity with the C IV forest correlation function
- Constraining the temperature-density relation of the intergalactic medium with the Lyman- and forests
- Modeling Photoionized Turbulent Material in the Circumgalactic Medium II: Effect of Turbulence within a Stratified Medium
- Probing reionization using quasar near-zones at redshift z ~ 6
- Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
- High-Redshift Galaxy Surveys and the Reionization of the Universe
- The Physical Nature of Circumgalactic Medium Absorbers in Simba
- Metallicity profiles of Ultra Diffuse Galaxies in NIHAO simulations
- Probing delayed-end reionization histories with the 21cm-LAE cross-power spectrum
- Cold parsec-scale gas in a zabs~0.1 sub-DLA with disparate H2 and 21-cm absorption
- Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
- Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
- Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
- The high-redshift tail of stellar reionization in LCDM is beyond the reach of the low- CMB
- Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
- Column Density Profiles of Cold Clouds Driven by Galactic Outflows
- Lyman continuum leaker candidates among highly ionised, low-redshift dwarf galaxies selected from HeII
- Theoretical study of an LAE-CIV absorption pair at z = 5.7
- Constraining UV Continuum Slopes of Active Galactic Nuclei With CLOUDY Models of Broad Line Region EUV Emission Lines
- A new probe of magnetic fields in the pre-reionization epoch: II. Detectability
- Eddington accreting Black Holes in the Epoch of Reionization
- Star Formation Variability as a Probe for the Baryon Cycle within Galaxies
- The 21-cm bispectrum from neutral hydrogen islands at z < 6
- Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman- Forest Tomography at
- Estimating black hole masses: Accretion disk fitting versus reverberation mapping and single epoch
- Evolution of CIV Absorbers. II. Where does CIV live?
- Hunting Primordial Black Hole Dark Matter in Lyman- Forest
- The high-velocity clouds above the disk of the outer Milky Way: misty precipitating gas in a region roiled by stellar streams
- Non-parametric Reconstruction of Photon Escape Fraction from Reionization
- Gas Accretion via Lyman Limit Systems
- The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
- The circumgalactic medium in Lyman-alpha: a new constraint on galactic outflow models
- Gas Cooling in Hydrodynamic Simulations with An Exact Time Integration Scheme
- Detection of Low Metallicity Warm Plasma in a Galaxy Overdensity Environment at z ~ 0.2
- Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
- Star Formation and Chemical Enrichment in Protoclusters
- z ~ 2.5 - 3 Ionizers in the GOODS-N Field
- Probing the assembly of dwarf galaxies through cosmic time with damped Lyman- absorption spectroscopy
- On the Cosmic Evolution of Fe/Mg in QSO Absorption Line Systems
- Absorption Line Search Through Three Local Group Dwarf Galaxy Halos
- Metal Lines Associated with the Lyman-alpha Forest from eBOSS Data
- The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
- An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies
- Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters
- Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
- Circumgalactic Medium on the Largest Scales: Detecting X-ray Absorption Lines with Large-Area Microcalorimeters
- Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
- Forecasting constraints on the mean free path of ionizing photons at from the Lyman- forest flux auto-correlation function
- Probing helium reionization with kinetic Sunyaev Zel'dovich tomography
- Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
- Probing the physical properties of the intergalactic medium using gamma-ray bursts
- Discovery of extremely low-metallicity circumgalactic gas at toward Q0454-220
- Positive feedback at the disc-halo interface
- An HST/COS Observation of Broad Ly Emission and Associated Absorption Lines of the BL Lacertae Object H 2356-309
- ASymba: HI global profile asymmetries in the Simba simulation
- Evidence of bimodal physical properties of intervening, optically-thin CIII absorbers at z ~ 2.5
- UV & Ly halos of Ly emitters across environments at z=2.84
- The duration of reionization constrains the ionizing sources
- Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
- Particle initialization effects on Lyman- forest statistics in cosmological SPH simulations
- Probing patchy reionisation with JWST: IGM opacity constraints from the Lyman- forest of galaxies in legacy extragalactic fields
- Interpreting Observations of Absorption Lines in the Circumgalactic Medium with a Turbulent Medium
- The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
- Resolving the Internal Structure of Circum-Galactic Medium using Gravitationally Lensed Quasars
- Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
- C IV and He II Line Emission of Lyman Alpha Blobs: Powered by Shock Heated Gas
- A population of high-velocity absorption-line systems residing in the Local Group
- HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
- A new ionisation network and radiation transport module in PLUTO
- Measuring the thermal and ionization state of the low- IGM using likelihood free inference
- The Alcock Paczynski test with 21cm intensity field
- A Sub-Damped Ly Absorber with Unusual Abundances: Evidence of Gas Recycling in a Low-Redshift Galaxy Group
- A comparison of formation models at high redshift
- Probing Large-scale UV Background Inhomogeneity Associated with Quasars using Metal Absorption
- NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
- Seeking Self-Regulating Simulations of Idealized Milky Way-Like Galaxies
- Distinguishing Between Photoionized and Collisionally Ionized Gas in the Circumgalactic Medium
- The Circumgalactic H Spectrograph (CHS) I. Design, Engineering, and Early Commissioning
- Stability and Ly emission of Cold Stream in the Circumgalactic Medium: impact of magnetic fields and thermal conduction
- Observational signatures of the dust size evolution in isolated galaxy simulations
- Impact of star formation models on the growth of simulated galaxies at high redshifts
- Aeos: Transport of Metals from Minihalos following Population III Stellar Feedback
- A panoramic view of the circumgalactic medium in the photoionized precipitation model
- Candidate z ~ 2.5 Lyman Continuum Sources in the GOODS Fields
- Modelling H and its effects on star formation using a joint implementation of GADGET-3 and KROME
- Fluorescent rings in star-free dark matter haloes
- Haloes at the ragged edge: The importance of the splashback radius
- Bursty star formation feedback and cooling outflows
- Probing Large Scale Ionizing Background Fluctuation with Lyman Forest and Galaxy Cross-correlation at z=2.4
- MCMC determination of the cosmic UV background at from H fluorescence
- The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
- A comprehensive study on the relation between the metal enrichment of ionised and atomic gas in star-forming galaxies
- Photometric IGM Tomography: Efficiently Mapping Quasar Light Echoes with Deep Narrow Band Imaging
- Far-UV Emission Properties of FR1 Radio Galaxies
- Modeling Photoionized Turbulent Material in the Circumgalactic Medium III: Effects of Co-rotation and Magnetic Fields
- Cosmic reionization of hydrogen and helium: contribution from both mini-quasars and stars
- The Lyman-alpha and Continuum Origins Survey II: the connection between the escape of ionizing radiation and Lyman-alpha halos in star-forming galaxies
- NIHAO XXVII: Crossing the green valley
- Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
- A MARVEL-ous study of how well galaxy shapes reflect Dark Matter halo shapes in Cold Dark Matter Simulations
- A Detection of Gas Associated with the M 31 Stellar Stream
- UV background fluctuations traced by metal ions at
- The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium
- The Lyman-limit photon mean free path at the end of late reionisation in the Sherwood-Relics simulations
- Blue galaxies: modelling nebular He II emission in high redshift galaxies
- CEMPlifying reionization
- Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
- HeII Ly Transmission Spikes and Absorption Troughs in Eight High-resolution Spectra Probing the End of HeII Reionization
- Does radiative feedback make faint z>6 galaxies look small?
- Physical conditions in two high-redshift H-bearing GRB-DLAs, 120815A and 121024A
- Cosmological probes of helium reionization
- Modelling the escape of Lyman Continuum photons from galaxies in the Epoch of Reionization
- Prospects for detecting cosmic filaments in Lyman-alpha emission across redshifts
- The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
- The Composite Spectral Energy Distribution of Quasars is Surprisingly Universal Since Cosmic Noon
- Fluctuations of the intergalactic ionization field at redshift z ~ 2
- Galaxy formation from a timescale perspective
- The optical luminosity function of LOFAR radio-selected quasars at in the NDWFS-Boötes field
- A survey of extremely metal-poor gas at cosmic noon: evidence of elevated [O/Fe]
- Modeling Warm Absorption in HST/COS Spectrum of Mrk 290 with XSTAR
- Upper Limits on the Mass of Cool Gas in the Circumgalactic Medium of Dwarf Galaxies
- The Physical Nature of the Most Metal-Poor Damped Lyman Alpha Systems
- A comparison of numerical methods for computing the reionization of intergalacitc hydrogen and helium by a central radiating source
- Galaxy cluster photons alter the ionisation state of the nearby warm-hot intergalactic medium
- Measurement of redshift-space two- and three-point correlation of Ly absorbers at : Implications on evolution of the physical properties of IGM
- Development of Hydrogen and Helium Proximity Zones around Quasars
- Effect of Separate Initial Conditions on the Lyman- Forest in Simulations
- Upcoming searches for decaying dark matter with ULTRASAT ultraviolet maps
- Multi-phase gas properties of extremely strong intervening DLAs towards quasars
- Cold-mode and hot-mode accretion in galaxy formation: an entropy approach
- Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
- The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
- Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters
- Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs
- An extremely metal-poor Lyman emitter candidate at revealed through absorption spectroscopy
- Using Lyman Alpha Absorption to Measure the Intensity and Variability of Ultraviolet Background Light
- Lognormal semi-numerical simulations of the Lyman- forest: comparison with full hydrodynamic simulations
- The Epoch of Reionization in Warm Dark Matter Scenarios
- Environments around quasars at 3 revealed by wide-field imaging with Subaru HSC and CFHT
- Constraining the physical properties of gas in high-z galaxies with far-infrared and submillimetre line ratios
- 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
- Misty, patchy, and turbulent: constraining the cool circumgalactic medium with mCC
- The Three Hundred: relation
- Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
- Forecasts for Broadband Intensity Mapping of the Ultraviolet-Optical Background with CASTOR and SPHEREx
- A Global Census of Metals in the Universe
- Clues to the nature of dark matter from first galaxies
- Fading in the Flow: Suppression of cold gas growth in expanding galactic outflows
- Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies
- Differentiating Warm Dark Matter Models through 21cm Line Intensity Mapping: A Convolutional Neural Network Approach
- Cospatial 21 cm and metal-line absorbers in the epoch of reionization -- I : Incidence and observability
- Physical conditions in highz optically thin C III absorbers: Origin of cloud sizes and associated correlations
- The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier
- On the Size and Mass of Photo-ionized Clouds in Extended Spiral Galaxy Halos
- Machine-guided Exploration and Calibration of Astrophysical Simulations
- Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
- Impact of the external radiation field on the structure and evolution of supernova remnants
- Constraining the ratio of median pixel optical depth profile around z ~ 4 quasars using the longitudinal proximity effect
- IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L Galaxies
- Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution
- The impact of cosmic ray feedback during the epoch of reionisation
- Constraining blazar heating with the 2<z<3 Lyman- forest
- Intermediate Mass Ratio Inspirals in Milky Way Galaxies
- Merging Black Holes in Dwarf Galaxies: Calculating Binary Black Hole Coalescence Timescales from Simulations for LISA Detection
- Constraining the Temperature-Density Relation of the Inter-Galactic Medium from Analytically Modeling Lyman-alpha Forest Absorbers
- The disk-torus system in active galactic nuclei: possible evidence of highly spinning black holes
- Quantitatively rating galaxy simulations against real observations with anomaly detection
- HI asymmetries in spatially resolved SIMBA galaxies
- A high-redshift quasar absorber without CIV - a galactic outflow caught in the act?
- Cosmic wallflowers: the circumgalactic origins of isolated ultra-compact star clusters at
- Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars
- Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
- The Cosmic Evolution of CIV Absorbers at : Insights from Systems in DESI Quasars
- Wind of Change: Faraday Rotation in a Simulated Large Magellanic Cloud
- ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization
- Measuring photo-ionization rate and mean free path of HeII ionizing photons at : Evidence for late and rapid HeII reionization Part-II
- Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
- Updated Models for the Creation of a Low-z QSO Absorber by a Dwarf Galaxy Wind
- Physical conditions and redshift evolution of optically thin C III absorbers: Low-z sample
- ForestFlow: predicting the Lyman- forest clustering from linear to nonlinear scales
- Intergalactic-Absorption Confounding Circumgalactic Observations
- The imprint of magnetic fields on absorption spectra from circumgalactic wind-cloud systems
- Constraining ultraviolet emission with the upcoming ULTRASAT satellite
- An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
- Slow Cooling in Low Metallicity Clouds: An Origin of Globular Cluster Bimodality?
- Exploratory Study of Transverse Proximity Effect around BAL Quasars
- Discovery of three new near-pristine absorption clouds at -4.4
- Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
- The Lyman-alpha Forest as a tool for disentangling non-Gaussianities
- The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
- The haloes that reionized the Universe
- Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
- Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman Forest
- What goes around comes around: the fate of stars in stripped tails of gas
- A Hierarchical Shock Model of Ultra-High-Energy Cosmic Rays
- Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
- Constraining cosmic ray transport models using circumgalactic medium properties and observables
- Black-hole mass estimation through accretion disk spectral fitting for high-redshift blazars
- The effect of helium reionization on the Lyman-alpha forest hydrogen flux statistics
- Kinematic analysis of an Ultra-Strong MgII absorber at z~1.13 linking to Circumgalactic Gas Structures
- Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
- A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
- The thermal history of the intergalactic medium at
- Origin of Weak MgII and Higher Ionization Absorption Lines in an Outflow from an Intermediate-Redshift Dwarf Satellite Galaxy
- The Role of Mass and Environment on Satellite distributions around Milky Way analogs in the Romulus25 simulation
- Impact of astrophysical effects on the dark matter mass constraint with 21cm intensity mapping
- Prospects for constraining quasar ages with fiber spectrographs: quasar-induced Ly emission from the intergalactic medium
- Rabacus: A Python Package for Analytic Cosmological Radiative Transfer Calculations
- Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
- Population III Star Formation in an X-ray background: I. Critical Halo Mass of Formation and Total Mass in Stars
- Imladris: a detailed and flexible model for galaxy simulations with individual stars
- Lyman Continuum escaping from in-situ formed stars in a tidal bridge at z = 3
- CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
- Turbulence in the intragroup and circumgalactic medium
- Constraints on cosmic rays in the Milky Way circumgalactic medium from OVIII observations
- Modelling intergalactic low ionisation metal absorption line systems near the epoch of reionization
- Validating the CROCODILE model within the AGORA galaxy simulation framework
- Measurements of quasar proximity zones with the Ly forest of DESI Y1 quasars
- Can UVB variations reconcile simulated quasar absorption lines at high redshift?
- Search for Dark Matter Annihilation and Decay with H Line Emission
- Detecting the signature of helium reionization through 3HeII 3.46cm line-intensity mapping
- The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra
- A quantitative assessment of completeness correction methods and public release of a versatile simulation code
- Simulating High-Velocity Clouds in the Observational Plane: An Initial Study with the Smith Cloud
- The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies