A dusty, normal galaxy in the epoch of reionization

Abstract

Candidates for the modest galaxies that formed most of the stars in the early universe, at redshifts $z>7$, have been found in large numbers with extremely deep restframe-UV imaging. But it has proved difficult for existing spectrographs to characterise them in the UV. The detailed properties of these galaxies could be measured from dust and cool gas emission at far-infrared wavelengths if the galaxies have become sufficiently enriched in dust and metals. So far, however, the most distant UV-selected galaxy detected in dust emission is only at $z=3.25$, and recent results have cast doubt on whether dust and molecules can be found in typical galaxies at this early epoch. Here we report thermal dust emission from an archetypal early universe star-forming galaxy, A1689-zD1. We detect its stellar continuum in spectroscopy and determine its redshift to be $z=7.5\pm 0.2$ from a spectroscopic detection of the Lyα break. A1689-zD1 is representative of the star-forming population during reionisation, with a total star-formation rate of about 12M${}_{\odot }$ yr${}^{-1}$. The galaxy is highly evolved: it has a large stellar mass, and is heavily enriched in dust, with a dust-to-gas ratio close to that of the Milky Way. Dusty, evolved galaxies are thus present among the fainter star-forming population at $z>7$, in spite of the very short time since they first appeared.

arXiv commentNature in press. 14 pages, 10 figures, including methods section

References in corpus (44)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Star Formation in Galaxies Along the Hubble Sequence
• Star Formation in the Milky Way and Nearby Galaxies
• A Simple Model for the Absorption of Starlight by Dust in Galaxies
• A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
• The ages and metallicities of galaxies in the local universe
• Dust Absorption And The Ultraviolet Luminosity Density At z \approx 3 As Calibrated By Local Starburst Galaxies
• Cool Gas in High Redshift Galaxies
• Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
• A glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3
• A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
• On the effect of the Cosmic Microwave Background in high-redshift (sub-)millimeter observations
• A galaxy at a redshift z = 6.96
• Evidence for Ubiquitous, High-EW Nebular Emission in z~7 Galaxies: Towards a Clean Measurement of the Specific Star Formation Rate using a Sample of Bright, Magnified Galaxies
• A Redshift z = 6.56 Galaxy Behind the Cluster Abell 370
• Explaining the [CII]158um Deficit in Luminous Infrared Galaxies - First Results from a Herschel/PACS Study of the GOALS Sample
• A Rapidly Star-forming Galaxy 700 Million Years After the Big Bang at z=7.51
• Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly
• Ultraviolet Emission Lines in Young Low Mass Galaxies at z~2: Physical Properties and Implications for Studies at z>7
• New Constraints on the Star Formation Histories and Dust Attenuation of Galaxies in the Local Universe from GALEX
• An Intensely Star-Forming Galaxy at z~7 with Low Dust and Metal Content Revealed by Deep ALMA and HST Observations
• The changing Lya optical depth in the range 6<z<9 from MOSFIRE spectroscopy of Y-dropouts
• Rapid dust production in submillimeter galaxies at z>4?
• The First Systematic Survey for Lyman Alpha Emitters at z=7.3 with Red-sensitive Subaru/Suprime-Cam
• The Star Formation Rate Function for Redshift z~4-7 Galaxies: Evidence for a Uniform Build-Up of Star-Forming Galaxies During the First 3 Gyr of Cosmic Time
• Discovery of a Very Bright Strongly-Lensed Galaxy Candidate at z ~ 7.6
• Gravitationally Lensed Galaxies at 2<z<3.5: Direct Abundance Measurements of Lya Emitters
• Star formation in the early universe: beyond the tip of the iceberg
• ALMA Observation of 158 micron [CII] Line and Dust Continuum of a z=7 Normally Star-forming Galaxy in the Epoch of Reionization
• The Molecular Gas Content of z = 3 Lyman Break Galaxies; Evidence of a non Evolving Gas Fraction in Main Sequence Galaxies at z > 2
• The Low Mass End of the Fundamental Relation for Gravitationally Lensed Star Forming Galaxies at 1<z<6
• Physical Properties of Spectroscopically-Confirmed Galaxies at z >= 6. II. Morphology of the Rest-Frame UV Continuum and Lyman-alpha Emission
• New constraints on dust emission and UV attenuation of z=6.5-7.5 galaxies from millimeter observations
• UV to IR SEDs of UV selected galaxies in the ELAIS fields: evolution of dust attenuation and star formation activity from z=0.7 to z=0.2
• Physical Properties of Spectroscopically-Confirmed Galaxies at z >= 6. I. Basic Characteristics of the Rest-Frame UV Continuum and Lyman-alpha emission
• HerMES: The Rest-Frame UV Emission and A Lensing Model for the z=6.34 Luminous Dusty Starburst Galaxy HFLS3
• The metals-to-dust ratio to very low metallicities using GRB and QSO absorbers; extremely rapid dust formation
• Through the Looking Glass: Bright, Highly Magnified Galaxy Candidates at z~7 Behind Abell 1703
• Photometric Redshifts based on standard SED fitting procedures
• A deep search for molecular gas in two massive Lyman break galaxies at z=3 and 4: vanishing CO-emission due to low metallicity?
• ALMA Observations of the Host Galaxy of GRB090423 at z=8.23: Deep Limits on Obscured Star Formation 630 Million Years After the Big Bang
• Dust correction factors over $0<z<3$ in massive star-forming galaxies from stacking in \emph{Herschel}

Cited by in corpus (262)

• A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy
• The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang
• A deep ALMA image of the Hubble Ultra Deep Field
• Dust in the reionization era: ALMA observations of a $z$=8.38 Galaxy
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass
• The dust content of galaxies from z = 0 to z = 9
• Galaxy growth in a massive halo in the first billion years of cosmic history
• The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties
• "Big Three Dragons": a z = 7.15 Lyman BreakGalaxy Detected in [OIII] 88 $\mu$m, [CII] 158 $\mu$m, and Dust Continuum with ALMA
• The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift
• Detection of an oxygen emission line from a high redshift galaxy in the reionization epoch
• Galaxy Formation and Reionization: Key Unknowns and Expected Breakthroughs by the James Webb Space Telescope
• The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies
• Detection of the Far-infrared [O III] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era
• The brightest galaxies at Cosmic Dawn
• Cosmic Dawn (CoDa): the First Radiation-Hydrodynamics Simulation of Reionization and Galaxy Formation in the Local Universe
• Rotation in [CII]-emitting gas in two galaxies at a redshift of 6.8
• On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times
• Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe
• RELICS: Reionization Lensing Cluster Survey
• High-redshift star formation in the ALMA era
• The [CII] 158 micron line emission in high-redshift galaxies
• Large Population of ALMA Galaxies at z>6 with Very High [OIII]88um to [CII]158um Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?
• The Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years
• Tracing the reionization epoch with ALMA: [CII] emission in z~7 galaxies
• The ALPINE-ALMA [CII] Survey: Multi-Wavelength Ancillary Data and Basic Physical Measurements
• Dust Formation in Milky Way-like Galaxies
• Star formation and the interstellar medium in z>6 UV-luminous Lyman-break galaxies
• ALMA uncovers the [CII] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
• The dust mass in z > 6 normal star forming galaxies
• The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z=1.5-10 UV-selected Galaxies and the Implied High-Redshift Star Formation History
• The dust mass in Cassiopeia A from a spatially resolved Herschel analysis
• Simulating the dust content of galaxies: successes and failures
• The ALPINE-ALMA [CII] Survey: Size of Individual Star-Forming Galaxies at z=4-6 and their Extended Halo Structure
• On the dust temperatures of high redshift galaxies
• Reionization and high-redshift galaxies: the view from quasar absorption lines
• First Identification of 10-kpc Scale [CII] 158um Halos around Star-Forming Galaxies at z=5-7
• Observational Searches for Galaxies at z > 6
• Normal, Dust-Obscured Galaxies in the Epoch of Reionization
• Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field
• Dust attenuation, dust emission, and dust temperature in galaxies at z>=5: a view from the FIRE-2 simulations
• The REBELS ALMA Survey: cosmic dust temperature evolution out to z $\sim$ 7
• Dusty galaxies in the Epoch of Reionization: simulations
• The impact of chemistry on the structure of high-z galaxies
• SILVERRUSH. V. Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC
• [CII] emission in z ~ 6 strongly lensed, star-forming galaxies
• The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5
• The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8
• The ALMA REBELS Survey: the dust content of $z\sim 7$ Lyman Break Galaxies
• Copious Amounts of Dust and Gas in a z=7.5 Quasar Host Galaxy
• CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch
• Dust production 680-850 million years after the Big Bang
• Simulating galactic dust grain evolution on a moving mesh
• Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties
• The IRX-Beta Dust Attenuation Relation in Cosmological Galaxy Formation Simulations
• The Lyman-alpha luminosity function at z=5.7-6.6 and the steep drop of the faint end: implications for reionization
• A dusty star-forming galaxy at z=6 revealed by strong gravitational lensing
• The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg2 of 850-um imaging
• The assembly of dusty galaxies at $z\ge 4$: statistical properties
• The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7
• The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at $z\approx 7$
• ALMA reveals metals yet no dust within multiple components in CR7
• Inferred Hα Flux as a Star-Formation Rate Indicator at z ~ 4-5: Implications for Dust Properties, Burstiness, and the z = 4-8 Star-Formation-Rate Functions
• High angular resolution ALMA images of dust and molecules in the SN 1987A ejecta
• A survey of high-$z$ galaxies: SERRA simulations
• Carbonaceous dust grains seen in the first billion years of cosmic time
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• A merger in the dusty, $z=7.5$ galaxy A1689-zD1?
• Dissecting the IRX - $\beta$ dust attenuation relation: exploring the physical origin of observed variations in galaxies
• Modelling supernova line profile asymmetries to determine ejecta dust masses: SN 1987A from days 714 to 3604
• Dust grains from the heart of supernovae
• Dust Destruction by the Reverse Shock in the Cassiopeia A Supernova Remnant
• Dual constraints with ALMA: new [O III] 88 $\mu$m and dust-continuum observations reveal the ISM conditions of luminous LBGs at $z\sim 7$
• Obscured star-formation in bright z ~ 7 Lyman-break galaxies
• Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
• The properties of the first galaxies in the BLUETIDES simulation
• Dust survival rates in clumps passing through the Cas A reverse shock I: results for a range of clump densities
• Spectroscopic Constraints on UV Metal Line Emission at z~6-9: The Nature of Lyman-alpha Emitting Galaxies in the Reionization-Era
• The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts
• Accurate dust temperature determination in a $z=7.13$ galaxy
• The nature of an ultra-faint galaxy in the cosmic Dark Ages seen with JWST
• The Local Group as a time machine: studying the high-redshift Universe with nearby galaxies
• The First Billion Years project: constraining the dust attenuation law of star-forming galaxies at z $\simeq$ 5
• Dust scaling relations in a cosmological simulation
• Newly Discovered Bright z~9-10 Galaxies and Improved Constraints on Their Prevalence Using the Full CANDELS Area
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey
• Looking at cosmic near-infrared background radiation anisotropies
• Interpreting the Spitzer/IRAC Colours of 7<z<9 Galaxies: Distinguishing Between Line Emission and Starlight Using ALMA
• The Grism Lens-Amplified Survey from Space (GLASS). III. A census of Lyα Emission at $z\gtrsim$7 from HST Spectroscopy
• The spectral evolution of the first Galaxies. III. Simulated James Webb Space Telescope spectra of reionization-epoch galaxies with Lyman continuum leakage
• Bright [CII] 158$\mu$m emission in a quasar host galaxy at $z=6.54$
• Significant Dust-Obscured Star Formation in Luminous Lyman-break Galaxies at $z$$\sim$$7$$-$$8$
• Dust Properties of [CII] Detected z $\sim$ 5.5 Galaxies: New HST/WFC3 Near-IR Observations
• The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ~ 7 Lyman-break galaxies
• A Dust Twin of Cas A: Cool Dust and 21-micron Silicate Dust Feature in the Supernova Remnant G54.1+0.3
• On the nature and physical conditions of the luminous Lya emitter CR7 and its rest-frame UV components
• Where does galactic dust come from?
• The Grism Lens-Amplified Survey from Space (GLASS). XI. Detection of CIV in Multiple Images of $z=6.11$ Ly$\alpha$ Emitter Behind RXCJ2248.7-4431
• ALMA reveals extended cool gas and hot ionized outflows in a typical star-forming galaxy at $z=7.13$
• Interpreting the evolution of galaxy colours from $z=8$ to $z=5$
• The infrared-dark dust content of high redshift galaxies
• Early Results from GLASS-JWST. I: Confirmation of Lensed $z⩾7$ Lyman-Break Galaxies Behind the Abell 2744 Cluster With NIRISS
• Keck/MOSFIRE Spectroscopy of z=7-8 Galaxies: Ly$\alpha$ Emission from a Galaxy at z=7.66
• First results from Faint Infrared Grism Survey (FIGS): first simultaneous detection of Lyman-alpha emission and Lyman break from a galaxy at z=7.51
• JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe
• The Contribution of Host Galaxies to the Infrared Energy Output of $z\gtrsim 5.0$ QUASARS
• An empirical study of dust properties at the earliest epochs
• The properties of GRB 120923A at a spectroscopic redshift of z=7.8
• Origins Space Telescope Mission Concept Study Report
• The assembly of dusty galaxies at $z\ge 4$: the build-up of stellar mass and its scaling relations with hints from early JWST data
• The dust content of the most metal-poor star-forming galaxies
• Evaluating the QSO contribution to the 21-cm signal from the Cosmic Dawn
• The dust content of the Crab Nebula
• Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies
• Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10
• The VANDELS survey: Dust attenuation in star-forming galaxies at $\mathbf{z}=3-4$
• The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe
• Young and turbulent: the early life of massive galaxy progenitors
• Maximally dusty star-forming galaxies: Supernova dust production and recycling in Local Group and high-redshift galaxies
• Near-Infrared Spectroscopy of SN 2017eaw in 2017: Carbon Monoxide and Dust Formation in a Type II-P Supernova
• Origin of Cosmic Chemical Abundances
• The mass, location and heating of the dust in the Cassiopeia A supernova remnant
• Late formation of silicon carbide in type II supernovae
• The ALMA REBELS Survey: The First Infrared Luminosity Function Measurement at $\mathbf{z \sim 7}
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• The LOFAR Two-metre Sky Survey: the radio view of the cosmic star formation history
• Dust Obscured Star Forming Galaxies in the Early Universe
• The IRX-$\beta$ relation of high-redshift galaxies
• Physical Properties of Spectroscopically-Confirmed Galaxies at $z\ge 6$. III. Stellar Populations from SED Modeling with Secure Ly$\alpha$ Emission and Redshifts
• SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-$\mu$m-selected galaxies
• ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-Forming Galaxies across $z\simeq 0.5-6$
• Dust depletion of metals from local to distant galaxies I: Peculiar nucleosynthesis effects and grain growth in the ISM
• The Distance and the near-IR extinction of the Monoceros Supernova Remnant
• Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies
• The ALPINE-ALMA [CII] survey: dust attenuation curves at z=4.4-5.5
• The cosmic dust rate across the Universe
• A decade of ejecta dust formation in the Type IIn SN 2005ip
• Revisiting the dust destruction efficiency of supernovae
• The IRX-$\beta$ relation: Insights from simulations
• Radiative properties of the first galaxies: rapid transition between blue and red
• A strong He II $\lambda$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?
• Dust masses for a large sample of core-collapse supernovae from optical emission line asymmetries: dust formation on 30-year timescales
• An analytic model for OIII fine structure emission from high redshift galaxies
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• Properties of five z~0.3-0.4 confirmed LyC leakers: VLT/XShooter observations
• Early structure formation from primordial density fluctuations with a blue-tilted power spectrum
• The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6
• Dust reddening and extinction curves towards gamma-ray bursts at z > 4
• Nebular line emission from z > 7 galaxies in cosmological simulations: rest-frame UV to Optical lines
• SuperBoRG: Exploration of point sources at $z\sim 8$ in HST parallel fields
• Modelling dust processing and the evolution of grain sizes in the ISM using the method of moments
• ALMA Lensing Cluster Survey: a strongly lensed multiply imaged dusty system at $z\ge$6
• Supernova induced processing of interstellar dust: impact of ISM gas density and gas turbulence
• JADES: Balmer Decrement Measurements at redshifts 4 < z < 7
• X-shooting GRBs at high redshift: probing dust production history
• A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5<z<6.8: Program Overview and a Sample of the Brightest Lyman-alpha Emitters
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• Early Science with the Large Millimeter Telescope: Detection of dust emission in multiple images of a normal galaxy at $z>4$ lensed by a Frontier Fields cluster
• JINGLE V: Dust properties of nearby galaxies derived from hierarchical Bayesian SED fitting
• A census of optically dark massive galaxies in the early Universe from magnification by lensing galaxy clusters
• Radiative transfer of ionizing radiation through gas and dust: stellar source case
• The Supernova -- Supernova Remnant Connection
• A Pilot Survey for CIII] Emission in the Reionization Era: Gravitationally-Lensed z$\sim 7-8$ Galaxies in the Frontier Fields Cluster Abell 2744
• A solar metallicity galaxy at $z>$ 7? Possible detection of the [N II] 122 $\mu$m and [O III] 52 $\mu$m lines
• SuperBoRG: Search for The Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
• CO (7-6), [CI] 370 micron and [NII] 205 micron Line Emission of the QSO BRI 1335-0417 at Redshift 4.407
• Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts
• The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at $z=7.31$
• Dust destruction and survival in the Cassiopeia A reverse shock
• Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
• The dust mass in Cassiopeia A from infrared and optical line flux differences
• Geometry effects on dust attenuation curves with different grain sources at high redshift
• Dusty Gas Accretion onto Massive Black Holes and Infrared Diagnosis of the Eddington Ratio
• The Detection of Ionized Carbon Emission at z~8
• CLEAR: Boosted Ly$\alpha$ Transmission of the Intergalactic Medium in UV bright Galaxies
• Gravitational-wave constraints on the cosmic opacity at $z\sim 5$: forecast from space gravitational-wave antenna DECIGO
• Estimating sizes of faint, distant galaxies in the submillimetre regime
• A resolved map of the infrared excess in a Lyman Break Galaxy at z=3
• Dust masses of $z>5$ galaxies from SED fitting and ALMA upper limits
• Metal and dust evolution in ALMA REBELS galaxies: insights for future JWST observations
• Possible Systematic Rotation in the Mature Stellar Population of a $z=9.1$ Galaxy
• Compatibility of JWST results with exotic halos
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• G.A.S. II: Dust extinction in galaxies; Luminosity functions and InfraRed eXcess
• Measuring dust in core-collapse supernovae with a Bayesian approach to line profile modelling
• Search for Polycyclic Aromatic Hydrocarbons in the Outflows from Dust-Producing Wolf-Rayet Stars
• ALMA Reveals Potential Localized Dust Enrichment from Massive Star Clusters in II Zw 40
• Exploring the cosmic dawn and epoch of reionization with 21cm line
• Galactic dust evolution with rapid dust formation in the interstellar medium due to hypersonic turbulence
• Constraint on dust evolution processes in normal galaxies at $z>6$ detected by ALMA
• Universe opacity and CMB
• Constraining C iii] Emission in a Sample of Five Luminous z = 5.7 Galaxies
• Expected dust grain size distributions in galaxies detected by ALMA at $z>7$
• The cold interstellar medium of a normal sub-$L^{\star }$ galaxy at the end of reionization
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies
• Radiation-pressure-driven dust transport to galaxy halos at $z\sim 10$
• Probing the baryon cycle of galaxies with SPICA mid- and far-infrared observations
• Multiscale mass transport in z~6 galactic discs: fueling black holes
• Estimating Dust Temperature and Far-IR Luminosity of High-Redshift Galaxies using ALMA Single-Band Continuum Observations
• Exploring the relation between dust mass and galaxy properties using Dusty SAGE
• Systematic errors in dust mass determinations: Insights from laboratory opacity measurements
• The archival discovery of a strong Lyman-$\alpha$ and [CII] emitter at z = 7.677
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• On the grain-size distribution of turbulent dust growth
• Properties of dust in the detached shells around U Ant, DR Ser, and V644 Sco
• The failure of testing for cosmic opacity via the distance-duality relation
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Exploring the dusty star-formation in the early Universe using intensity mapping
• Cosmic Reionization On Computers. Ultraviolet Continuum Slopes and Dust Opacities in High Redshift Galaxies
• Hadronic Interactions of Energetic Charged Particles in Protogalactic Outflow Environments and Implications for the Early Evolution of Galaxies
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• Spectroscopic confirmation of a gravitationally lensed Lyman break galaxy at z${}_{[CII]}$ = 6.827 using NOEMA
• A Submillimeter Survey of Faint Galaxies Behind Ten Strong Lensing Clusters
• Dust growth by accretion of molecules in supersonic interstellar turbulence
• Kpc-scale properties of dust temperature in terms of dust mass and star formation activity
• Early Science with the Large Millimeter Telescope: Dust constraints in a z~9.6 galaxy
• ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed $z\sim 6$ galaxies
• Limits on Intergalactic Dust During Reionization
• Analytic models of dust temperature in high-redshift galaxies
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Missing dust signature in the cosmic microwave background
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud
• Galaxy Formation and Symbiotic Evolution with the Inter-Galactic Medium in the Age of ELT-ANDES
• Ultra-massive black hole feedback in compact galaxies
• Enhanced spectrum of primordial perturbations, galaxy formation and small scale structure
• Hoyle-Lyttleton accretion on to black hole accretion disks with super-Eddington luminosity for dusty gas
• A simple numerical experiment on the dust temperature bias for Lyman break galaxies at $z\gtrsim 5$
• CEERS: Forging the First Dust Grains in the Universe? A Population of Galaxies with spectroscopically-derived Extremely Low Dust Attenuation (GELDA) at 4.0<z<11.4
• Ionized Carbon in Galaxies: The [C II] 158 $\mu$m Line as a Total Molecular Gas Mass Tracer Revisited
• Observations of Ly$\alpha$ Emitters at High Redshift
• Dust emission from the bulk of galaxies at the Epoch of Reionization
• Accelerated growth of seed black holes by dust in the early universe
• Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies. I: Cross-Section
• Galaxies into the Dark Ages
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• A Multiply-Imaged z $\sim$ 6.3 Lyman Alpha Emitter candidate behind Abell 2261
• Redshift Horizon for Detecting the First Galaxies in Far-Infared Surveys
• Can planet formation resolve the dust budget crisis in high redshift galaxies?
• Inferring properties of dust in supernovae with neural networks
• Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy at z~3.3
• Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies -- II: Uncertainties
• AGN radiative feedback in the early growth of massive black holes
• Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium
• Considering light-matter interactions in the Friedmann equations
• The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields
• ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
• Quantifying the dust in SN 2012aw and iPTF14hls with ORBYTS
• Observing galaxy mergers at the epoch of reionization
• The Ion and Charged Aerosol Growth Enhancement (ION-CAGE) code: A numerical model for the growth of charged and neutral aerosols
• Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$
• Galaxy evolution and radiative properties in the early Universe: multi-wavelength analysis in cosmological simulations
• Early galaxy evolution: The complex interstellar medium distribution of the z~7 galaxy A1689-zD1
• Dusty Galaxies at the Highest Redshifts
• Tight correlation of star formation with [Ci] and CO lines across cosmic time
• Astro2020 Science White Paper: Exploration and characterization of the earliest epoch of galaxy formation: beyond the re-ionization era
• Exploring the Dawn of Galaxies
• The ALMA View of High-Redshift Galaxy Formation
• What is the amount of baryonic dark matter in galaxies?
• Structure Formation in the Early Universe
• The cosmic journey of dust grains -- from nucleation to planetary system