Early star-forming galaxies and the reionization of the Universe
arXiv:1011.0727 · doi:10.1038/nature09527
Abstract
Star forming galaxies represent a valuable tracer of cosmic history. Recent observational progress with Hubble Space Telescope has led to the discovery and study of the earliest-known galaxies corresponding to a period when the Universe was only ~800 million years old. Intense ultraviolet radiation from these early galaxies probably induced a major event in cosmic history: the reionization of intergalactic hydrogen. New techniques are being developed to understand the properties of these most distant galaxies and determine their influence on the evolution of the universe.
Review article appearing in Nature. This posting reflects a submitted version of the review formatted by the authors, in accordance with Nature publication policies. For the official, published version of the review, please see http://www.nature.com/nature/archive/index.html
References in corpus (25)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The James Webb Space Telescope
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Observational constraints on Cosmic Reionization
- UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History
- The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN
- Efficient Simulations of Early Structure Formation and Reionization
- The End of the Reionization Epoch Probed by Ly-alpha Emitters at z=6.5 in the Subaru Deep Field
- The observed ionization rate of the intergalactic medium and the ionizing emissivity at z >5: Evidence for a photon starved and extended epoch of reionization
- The morphology of HII regions during reionization
- The Direct Detection of Lyman-Continuum Emission from Star-forming Galaxies at z~3
- A galaxy at a redshift z = 6.96
- Studying Reionization with Ly-alpha Emitters
- Keeping the Universe ionised: Photo-heating and the clumping factor of the high-redshift intergalactic medium
- Inside-out or Outside-in: The topology of reionization in the photon-starved regime suggested by Lyman-alpha forest data
- A radiative transfer scheme for cosmological reionization based on a local Eddington tensor
- Imprint of Inhomogeneous Hydrogen Reionization on the Temperature Distribution of the Intergalactic Medium
- Spectroscopic confirmation of a galaxy at redshift z=8.6
- The Stellar Mass Density at z~6 from Spitzer Imaging of i-drop Galaxies
- A Hubble & Spitzer Space Telescope Survey for Gravitationally-Lensed Galaxies: Further Evidence for a Significant Population of Low Luminosity Galaxies beyond Redshift Seven
- Fast Large-Scale Reionization Simulations
- Lyman Alpha Emitters at z=7 in the Subaru/XMM-Newton Deep Survey Field: Photometric Candidates and Luminosity Function
- Connecting Reionization to the Local Universe
- A New Moment Method for Continuum Radiative Transfer in Cosmological Reionization
- Detecting the Most Distant (z>7) Objects with ALMA
Cited by in corpus (245)
- Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and Hubble Space Telescope
- A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
- New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign
- The Abundance of Star-Forming Galaxies in the Redshift Range 8.5 to 12: New Results from the 2012 Hubble Ultra Deep Field Campaign
- The First Galaxies
- UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z>=4 star-forming galaxies
- Keck Spectroscopy of 3<z<7 Faint Lyman Break Galaxies: The Importance of Nebular Emission in Understanding the Specific Star Formation Rate and Stellar Mass Density
- A new multi-field determination of the galaxy luminosity function at z=7-9 incorporating the 2012 Hubble Ultra Deep Field imaging
- The Birth of a Galaxy - III. Propelling reionisation with the faintest galaxies
- CLASH: Three Strongly Lensed Images of a Candidate z ~ 11 Galaxy
- Cosmic Reionization after Planck: Could Quasars Do It All?
- Formation of the First Stars
- The Evolution of the Intergalactic Medium
- Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries
- A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs old
- Concordance models of reionization: implications for faint galaxies and escape fraction evolution
- The mass evolution of the first galaxies: stellar mass functions and star formation rates at in the CANDELS GOODS-South field
- Keck Spectroscopy of Faint 3<z<8 Lyman Break Galaxies:- Evidence for a Declining Fraction of Emission Line Sources In the Redshift Range 6<z<8
- The GLASS James Webb Space Telescope Early Release Science Program. I. Survey Design and Release Plans
- Lower-Luminosity Galaxies could reionize the Universe: Very Steep Faint-End Slopes to the UV Luminosity Functions at z>=5-8 from the HUDF09 WFC3/IR Observations
- The UV Luminosity Function of star-forming galaxies via dropout selection at redshifts z ~ 7 and 8 from the 2012 Ultra Deep Field campaign
- Spectroscopic confirmation of two luminous galaxies at
- Planck intermediate results. XLVII. Planck constraints on reionization history
- Data Analysis for Precision 21 cm Cosmology
- Connecting the Gamma Ray Burst Rate and the Cosmic Star Formation History: Implications for Reionization and Galaxy Evolution
- Galaxy Formation and Reionization: Key Unknowns and Expected Breakthroughs by the James Webb Space Telescope
- Ultraviolet Emission Lines in Young Low Mass Galaxies at z~2: Physical Properties and Implications for Studies at z>7
- Galaxy Properties and UV Escape Fractions During Epoch of Reionization: Results from the Renaissance Simulations
- Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.9
- CANDELS: The Contribution of the Observed Galaxy Population to Cosmic Reionization
- Bright [CII] and dust emission in three z>6.6 quasar host galaxies observed by ALMA
- Spectroscopic detections of CIII]1909 at z~6-7: A new probe of early star forming galaxies and cosmic reionisation
- Hubble imaging of the ionizing radiation from a star-forming galaxy at z=3.2 with fesc>50%
- A robust sample of galaxies at redshifts 6.0<z<8.7: stellar populations, star-formation rates and stellar masses
- The spectral evolution of the first galaxies. II. Spectral signatures of Lyman continuum leakage from galaxies in the reionization epoch
- The Lyman Continuum Escape Survey: Ionizing Radiation from [O III]-Strong Sources at a Redshift of 3.1
- The UV continua and inferred stellar populations of galaxies at z ~ 7 - 9 revealed by the Hubble Ultra Deep Field 2012 campaign
- Rapid Decline of Lyman-alpha Emission Toward the Reionization Era
- Hubble Frontier Fields First Complete Cluster Data: Faint Galaxies at for UV Luminosity Functions and Cosmic Reionization
- Extragalactic Background Light from Hierarchical Galaxy Formation: Gamma-ray Attenuation up to the Epoch of Cosmic Reionization and the First Stars
- Accelerated Evolution of Ly Luminosity Function at Revealed by the Subaru Ultra-Deep Survey for Ly Emitters at
- The stellar mass function of star-forming galaxies and the mass-dependent SFR function since z=2.23 from HiZELS
- New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density
- On Lyman-limit Systems and the Evolution of the Intergalactic Ionizing Background
- New Constraints on the Faint-end of the UV Luminosity Function at z~7-8 using the Gravitational Lensing of the Hubble Frontier Fields Cluster A2744
- No evidence for a significant AGN contribution to cosmic hydrogen reionization
- A critical analysis of the UV-continuum slopes of high-redshift galaxies; no evidence (yet) for extreme stellar populations at z > 6
- The Brightest Of Reionizing Galaxies Survey: Design and Preliminary Results
- On The Detection Of Ionizing Radiation Arising From Star-Forming Galaxies At Redshift z ~ 3-4 : Looking For Analogs Of "Stellar Reionizers"
- Observational Searches for Galaxies at z > 6
- Improving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations
- The Bright End of the UV Luminosity Function at z~8: New Constraints from CANDELS Data in GOODS-South
- Keck Spectroscopy of Faint 3 < z < 7 Lyman Break Galaxies: III. The Mean Ultraviolet Spectrum at z=4
- Narrowband imaging of Escaping Lyman-Continuum Emission in the SSA22 Field
- The Connection Between Reddening, Gas Covering Fraction, and the Escape of Ionizing Radiation at High Redshift
- Probing the thermal state of the intergalactic medium at with the transmission spikes in high-resolution Ly forest spectra
- Evidence for a Hard Ionizing Spectrum from a z=6.11 Stellar Population
- Evolution of the Quasar Luminosity Function Over 3 < z < 5 in the COSMOS Survey Field
- Supernovae in the Subaru Deep Field: the rate and delay-time distribution of type Ia supernovae out to redshift 2
- Gamma-ray Burst Cosmology
- First Spectroscopic Evidence for High Ionization State and Low Oxygen Abundance in Lya Emitters
- The ultraviolet continuum slopes () of galaxies at from JWST and ground-based near-infrared imaging
- The Brightest Galaxies over the COSMOS UltraVISTA Field
- Searching for Extremely Blue UV Continuum Slopes at in JWST/NIRCam Imaging: Implications for Stellar Metallicity and Ionizing Photon Escape in Early Galaxies
- The galaxy UV luminosity function at z ~ 2 - 4; new results on faint-end slope and the evolution of luminosity density
- The Lyman-alpha luminosity function at z=5.7-6.6 and the steep drop of the faint end: implications for reionization
- Radiative Feedback from high mass X-ray binaries on the formation of the first galaxies and early reionization
- The impact of primordial supersonic flows on early structure formation, reionization and the lowest-mass dwarf galaxies
- Expanded Search for z~10 Galaxies from HUDF09, ERS, and CANDELS Data: Evidence for Accelerated Evolution at z>8?
- Metals in the IGM approaching the re-ionization epoch: results from X-shooter at the VLT
- On the Use of Ly-alpha Emitters as Probes of Reionization
- The CASSOWARY spectroscopy survey: A new sample of gravitationally lensed galaxies in SDSS
- ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] line and dust emission in 6<z<8 galaxies
- The impact of stars stripped in binaries on the integrated spectra of stellar populations
- The IACOB project. V. Spectroscopic parameters of the O-type stars in the modern grid of standards for spectral classification
- On the relative Contribution of high-redshift Galaxies and Active Galactic Nuclei to Reionization
- Models of the Thermal Evolution of the Intergalactic Medium After Reionization
- The First Billion Years project - IV: Proto-galaxies reionising the Universe
- Inferences on the distribution of Ly-alpha emission of z~7 and z~8 galaxies
- First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
- The First Galaxies: Assembly of Disks and Prospects for Direct Detection
- Recovery from population III supernova explosions and the onset of second generation star formation
- The bright-end galaxy candidates at z ~ 9 from 79 independent HST fields
- Discovery of bright z ~ 7 galaxies in the UltraVISTA survey
- A VLT/FORS2 view at : Lyman- emitter fraction and galaxy physical properties at the edge of the epoch of cosmic reionization
- Escape of ionizing radiation from high redshift dwarf galaxies: role of AGN feedback
- The First Galaxies: Assembly under Radiative Feedback from the First Stars
- The properties of He II 1640 emitters at z ~ 2.5-5 from the VANDELS survey
- The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly Visibility During the Epoch of Reionization
- The deepest X-ray view of high-redshift galaxies: constraints on low-rate black-hole accretion
- Model-independent constraints on the hydrogen-ionizing emissivity at z>6
- Ly-Lyman Continuum connection in 3.5 < z < 4.3 star-forming galaxies from the VUDS survey
- The THESAN project: ionizing escape fractions of reionization-era galaxies
- Physical Properties of Spectroscopically-Confirmed Galaxies at z >= 6. I. Basic Characteristics of the Rest-Frame UV Continuum and Lyman-alpha emission
- Constraining the UV emissivity of AGN throughout cosmic time via X-ray surveys
- Formation of the first stars and black holes
- Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
- Intensity mapping of molecular gas during cosmic reionization
- Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
- An Ultraluminous Lyman Alpha Emitter with a Blue Wing at z=6.6
- Filamentary Infall of Cold Gas and Escape of Lyman Alpha and Hydrogen Ionizing Radiation from an Interacting High-Redshift Galaxy
- Simulating the assembly of galaxies at redshifts z = 6 - 12
- An MCMC approach to extracting the global 21-cm signal during the cosmic dawn from sky-averaged radio observations
- Probing Intergalactic Neutral Hydrogen by the Lyman Alpha Red Damping Wing of Gamma-Ray Burst 130606A Afterglow Spectrum at z = 5.913
- The high-redshift star formation rate derived from GRBs: possible origin and cosmic reionization
- The Effect of Galactic Properties on the Escape Fraction of Ionizing Photons
- Direct Numerical Simulation of Reionization II: Recombinations, Clumping Factors, and the Photon Budget for Reionization
- UV Spectral-Slopes at in the Hubble Frontier Fields: Lack of Evidence for Unusual or Pop III Stellar Populations
- The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
- Complex Lyman Alpha Profiles in Redshift 6.6 Ultraluminous Lyman Alpha Emitters
- An Empirical Study of the Relationship between Lyα and UV selected Galaxies: Do Theorists and Observers `Select' the Same Objects?
- Winds of low-metallicity OB-type stars: HST-COS spectroscopy in IC1613
- On the Evolution of the Cosmic Ionizing Background
- Intergalactic Lyman continuum photon budget in the past 5 billion years
- The production of ionizing photons in UV-faint z~3-7 galaxies
- Evidence for Low Extinction in Actively Star Forming Galaxies at z6.5
- The unbiased measurement of UV spectral slopes in low luminosity galaxies at z=7
- Constraints on the Lyman continuum escape fraction for faint star forming galaxies
- CLASH-VLT: spectroscopic confirmation of a z=6.11 quintuply lensed galaxy in the Frontier Fields Cluster RXC J2248.7-4431
- The Chandra Deep Fields: Lifting the Veil on Distant Active Galactic Nuclei and X-Ray Emitting Galaxies
- The ages, masses and star-formation rates of spectroscopically confirmed z~6 galaxies in CANDELS
- The Hydrodynamic Feedback of Cosmic Reionization on Small-Scale Structures and Its Impact on Photon Consumption during the Epoch of Reionization
- Modeling UV Radiation Feedback from Massive Stars: III. Escape of Radiation from Star-forming Giant Molecular Clouds
- The first galaxies: simulating their feedback-regulated assembly
- Definitive upper bound on the negligible contribution of quasars to cosmic reionization
- The Mass-Metallicity Relation of Dwarf Galaxies at Cosmic Noon from JWST Observations
- Probing the stellar initial mass function with high- supernovae
- The UV colours and dust attenuation of Lyman-break galaxies
- Spitzer UltRa Faint SUrvey Program (SURFS UP). II. IRAC-Detected Lyman-Break Galaxies at 6 < z < 10 Behind Strong-Lensing Clusters
- Spitzer UltRa Faint SUrvey Program (SURFS UP) I: An Overview
- Characterizing faint galaxies in the reionization epoch: LBT confirms two L<0.2L* sources at z=6.4 behind the CLASH/Frontier Fields cluster MACS0717.5+3745
- A faint optical flash in dust-obscured GRB 080603A - implications for GRB prompt emission mechanisms
- AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization
- Connecting Faint End Slopes of the Lyman- emitter and Lyman-break Galaxy Luminosity Functions
- Feedback from High-Mass X-Ray Binaries on the High Redshift Intergalactic Medium : Model Spectra
- The CubeSpec space mission. I. Asteroseismology of massive stars from time series optical spectroscopy: science requirements and target list prioritisation
- Physical Properties of Spectroscopically-Confirmed Galaxies at . III. Stellar Populations from SED Modeling with Secure Ly Emission and Redshifts
- Do Cosmic Rays Heat the Early Intergalactic Medium?
- Physical Properties of UDF12 Galaxies in Cosmological simulations
- Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
- Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
- Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
- Lyman-alpha transmission properties of the intergalactic medium in the CoDaII simulation
- Recombination clumping factor during cosmic reionization
- Predictions for the 21cm-galaxy cross-power spectrum observable with LOFAR and Subaru
- The First Stars: formation under X-ray feedback
- Accounting for Cosmic Variance in Studies of Gravitationally-Lensed High-Redshift Galaxies in the Hubble Frontier Field Clusters
- High redshift AGNs and HI reionisation: limits from the unresolved X-ray background
- Measuring the reionization optical depth without large-scale CMB polarization
- High Precision Analyses of Lyman alpha Damping Wing of Gamma-Ray Bursts in the Reionization Era: On the Controversial Results from GRB 130606A at z = 5.91
- First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions
- Constraining the nature of the most distant Gamma-Ray Burst host galaxies
- Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
- Simulating the UV Escape Fractions from Molecular Cloud Populations in Star-forming Dwarf and Spiral Galaxies
- Nebular line emission from z > 7 galaxies in cosmological simulations: rest-frame UV to Optical lines
- Spectroscopic Confirmation of a z=6.740 Galaxy behind the Bullet Cluster
- Gravitational Lensing - Einstein's Unfinished Symphony
- Evidence for inhomogeneous reionization in the local Universe from metal-poor globular cluster systems
- A new parameterization of the reionisation history
- SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
- X-ray properties of He II 1640 emitting galaxies in VANDELS
- Properties of the KISS Green Pea Galaxies
- The Faint Host Galaxies of C IV Absorbers at z > 5
- OB stars at the lowest Local Group metallicity: GTC-OSIRIS observations of Sextans A
- A 52 hours VLT/FORS2 spectrum of a bright z~7 HUDF galaxy: no Ly-alpha emission
- Early Results From GLASS-JWST. XVII: Building the First Galaxies -- Chapter 1. Star Formation Histories at 5<z < 7
- Statistical properties of mass, star formation, chemical content and rotational patterns in early z > 9 structures
- Observing patchy reionization with future CMB polarization experiments
- First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations
- Signature of the first galaxies in JWST deep field observations
- The Thermal Proximity Effect: A New Probe of He II Reionization History and the Quasar Lifetime
- The properties of the brightest Lyman alpha emitters at z~5.7
- Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
- Effects of Star Formation Stochasticity on the Ly-alpha & Lyman Continuum Emission from Dwarf Galaxies during Reionization
- Green Peas in X-rays
- Interactions between Ultra-High-Energy Particles and Protogalactic Environments
- Stars and Reionization: The Cross-Correlation of the 21cm Line and the Near Infrared Background
- Differences and similarities of stellar populations in LAEs and LBGs at 3.4 - 6.8
- High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth
- Keck-I MOSFIRE spectroscopy of the z~12 candidate galaxy UDFj-39546284
- Chemical constraints on the contribution of Population III stars to cosmic reionization
- The Dark Ages of the Universe and Hydrogen Reionization
- What Powers Lyman alpha Blobs?
- The HI mass function as a probe of photoionisation feedback on low mass galaxy formation
- The Contribution of Supernovae to Cosmic Reionization
- Dust attenuation of the nebular regions and optical emission lines of star-forming galaxies
- Heating and Ionization of the Primordial Intergalactic Medium by High Mass X-ray Binaries
- Space Debris -- Optical Measurements
- Probing the peak of the star formation rate density with the extragalactic background light
- Infrared-Faint Radio Sources are at high redshifts
- Joining bits and pieces of reionization history
- Distinctive 21 cm structures of the first stars, galaxies, and quasars
- Starburst galaxies
- Microquasars as heating sources of the intergalactic medium during reionisation of the Universe
- The First Stars: formation under cosmic ray feedback
- Machine-learning recovery of foreground wedge-removed 21-cm light cones for high- galaxy mapping
- Spectroscopy of CASSOWARY gravitationally-lensed galaxies in SDSS: characterisation of an extremely bright reionization-era analog at
- Mapping the core of the Tarantula Nebula with VLT-MUSE II. The spectroscopic Hertzsprung-Russell diagram of OB stars in NGC 2070
- SHARDS Frontier Fields: Physical properties of a low mass Lyman-alpha emitter at z=5.75
- A modern guide to quantitative spectroscopy of massive OB stars
- A bright lensed galaxy at with strong Ly emission
- Distinguishing the impact and signature of black holes from different origins in early cosmic history
- Evolution of the UV slope of galaxies at cosmic morning (z > 4): the properties of extremely blue galaxies
- The CCAT-Prime Submillimeter Observatory
- Low-redshift Lyman Continuum Survey: Radio continuum properties of low- Lyman continuum emitters
- The End of an Era - The Population III to Population II Transition and the Near Infrared Background
- RCS2 J232727.6-020437: An Efficient Cosmic Telescope at
- Extragalactic background light models and GeV-TeV observation of blazars
- Extending Semi-numeric Reionisation Models to the First Stars and Galaxies
- z ~ 2.5 - 3 Ionizers in the GOODS-N Field
- Long Gamma Ray Bursts Trace The Star Formation History
- A Novel Approach to Constrain the Escape Fraction and Dust Content at High Redshift Using the Cosmic Infrared Background Fractional Anisotropy
- Dark Twilight Joined with the Light of Dawn to Unveil the Reionization History
- Detectability of the -21cm cross-correlation: a tomographic probe of patchy reionization
- Investigating the Lyman photon escape in local starburst galaxies with the Cosmic Origins Spectrograph
- Strong [O III] λ5007 Compact Galaxies Identified from SDSS DR16 and Their Scaling Relations
- Candidate z ~ 2.5 Lyman Continuum Sources in the GOODS Fields
- Inferring the Distribution of the Ionising Photon Escape Fraction
- Cosmic reionization of hydrogen and helium: contribution from both mini-quasars and stars
- X-ray observations of Blueberry galaxies
- Laboratory Photoionization Fronts in Nitrogen Gas: A Numerical Feasibility and Parameter Study
- Observations of Ly Emitters at High Redshift
- Ultra-faint [CII] emission in a redshift = 2 gravitationally-lensed metal-poor dwarf galaxy
- The Composite Spectral Energy Distribution of Quasars is Surprisingly Universal Since Cosmic Noon
- JWST observations constrain the time evolution of fine structure constants and dark energy - electromagnetic coupling
- Atomic Modeling of Photoionization Fronts in Nitrogen Gas
- The near-infrared radiation background, gravitational wave background and star formation rate of Pop III and Pop II during cosmic reionization
- On the theory of mass loss in dwarf galaxies: I - basic equations and the case of wave/thermal driven winds
- Semi analytical description of formation of galaxies and clusters of galaxies
- Disentangling the X-ray variability in the Lyman continuum emitter Haro 11
- Evolving beyond z=0: insights about the future of stars and the intergalactic medium
- Effect of Separate Initial Conditions on the Lyman- Forest in Simulations
- Near-IR narrow-band imaging with CIRCE at the Gran Telescopio Canarias: Searching for Ly-emitters at
- Formation Mechanism of Laser-Driven Magnetized "Pillars of Creation"
- The star formation history inferred from long gamma-ray bursts with high pseudo-redshifts
- Towards a multi-input astrophotonic AWG spectrograph
- Star Formation for Predictive Primordial Galaxy Formation
- Radiative transfer of 21-cm line through ionised cavities in an expanding universe
- Modelling stellar populations at high redshift
- Cross-correlating the patchy screening and kinetic Sunyaev-Zel'dovich effects as a new probe of reionization
- Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
- Stellar black holes: cosmic history and feedback at the dawn of the universe
- Near-Field Cosmology with the Lowest-Mass Galaxies
- The BUFFALO HST Survey
- Resolving dust and Lyα emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS