Evolution of the dust-to-metals ratio in high-redshift galaxies probed by GRB-DLAs

Abstract

Context. Several issues regarding the nature of dust at high redshift remain unresolved: its composition, its production and growth mechanisms, and its effect on background sources. Aims. We provide a more accurate relation between dust depletion levels and dust-to-metals ratio (DTM), and to use the DTM to investigate the origin and evolution of dust in the high-redshift Universe via Gamma-ray burst damped Lyman-alpha absorbers (GRB-DLAs). Methods. We use absorption-line measured metal column densities for a total of 19 GRB-DLAs, including five new GRB afterglow spectra from VLT/X-shooter. We use the latest linear models to calculate the dust depletion strength factor in each DLA. Using these values we calculate total dust and metal column densities to determine a DTM. We explore the evolution of DTM with metallicity, and compare it to previous trends in DTM measured with different methods. Results. We find significant dust depletion in 16 of our 19 GRB-DLAs, yet 18 of the 19 have a DTM significantly lower than the Milky Way. We find that DTM is positively correlated with metallicity, which supports a dominant ISM grain-growth mode of dust formation. We find a substantial discrepancy between the dust content measured from depletion and that derived from the total V-band extinction, $A_V$ , measured by fitting the afterglow SED. We advise against using a measurement from one method to estimate that from the other until the discrepancy can be resolved.

arXiv commentPublished in Astronomy & Astrophysics. 24 pages, 34 figures

References in corpus (81)

• Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
• The Swift X-ray Telescope
• Theory of Star Formation
• Interstellar Dust Grains
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• Optical and Long Wavelength Afterglow from Gamma-Ray Bursts
• What Powers Ultra-luminous IRAS Galaxies?
• A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium
• Molecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments
• Damped Lyman alpha Systems
• The Relation Between Optical Extinction and Hydrogen Column Density in the Galaxy
• The Evolution of the Elemental Abundances in the Gas and Dust Phases of the Galaxy
• A glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3
• PAHs as a tracer of star formation?
• GROND - a 7-channel imager
• The Galaxy Population Hosting Gamma-Ray Bursts
• The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows
• A Budget and Accounting of Metals at z~0: Results from the COS-Halos Survey
• Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
• The 2175 A dust feature in a Gamma Ray Burst afterglow at redshift 2.45
• The nature of "dark" gamma-ray bursts
• A Population of Massive, Luminous Galaxies Hosting Heavily Dust-Obscured Gamma-Ray Bursts: Implications for the Use of GRBs as Tracers of Cosmic Star Formation
• The metallicity of the long GRB hosts and the Fundamental Metallicity Relation of low-mass galaxies
• The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold
• Dust Formation in Milky Way-like Galaxies
• Dust Extinction in High-z Galaxies with GRB Afterglow Spectroscopy - The 2175Å Feature at z=2.45
• Heavy Element Abundances and Dust Depletions in the Host Galaxies of Three Gamma-Ray Bursts
• The First Detections of the Extragalactic Background Light at 3000, 5500, and 8000A (I): Results
• Reconciling the Metallicity Distributions of Gamma-ray Burst, Damped Lyman-alpha, and Lyman-break Galaxies at z=3
• Highly Ionized Gas Surrounding High Velocity Cloud Complex C
• The Swift Gamma-Ray Burst Host Galaxy Legacy Survey - I. Sample Selection and Redshift Distribution
• The origin and evolution of the odd-Z iron-peak elements Sc, V, Mn, and Co in the Milky Way stellar disk
• The equilibrium view on dust and metals in galaxies: Galactic outflows drive low dust-to-metal ratios in dwarf galaxies
• A log N(HI) = 22.6 DLA in a dark gamma-ray burst: the environment of GRB 050401
• Dust and Metal Column Densities in Gamma-Ray Burst Host Galaxies
• The Troublesome Broadband Evolution of GRB 061126: Does a Grey Burst Imply Grey Dust?
• Dust-to-metal ratios in damped Lyman-alpha absorbers: Fresh clues to the origins of dust and optical extinction towards gamma-ray bursts
• Dust extinction for an unbiased sample of GRB afterglows
• Super-solar Metal Abundances in Two Galaxies at z ~ 3.57 revealed by the GRB 090323 Afterglow Spectrum
• The Galactic dust-to-metals ratio and metallicity using gamma-ray bursts
• Galaxy counterparts of metal-rich damped Lyman-alpha absorbers - II. A solar-metallicity and dusty DLA at z_abs=2.58
• The Dust Extinction Curves of Gamma-Ray Burst Host Galaxies
• GRB hosts through cosmic time - VLT/X-Shooter emission-line spectroscopy of 96 GRB-selected galaxies at 0.1 < z < 3.6
• GRB 100219A with X-shooter - abundances in a galaxy at z = 4.7
• Physical conditions in high-redshift GRB-DLA absorbers observed with VLT/UVES: Implications for molecular hydrogen searches
• The missing metals problem. III How many metals are expelled from galaxies?
• Evolution of Dust-to-Metal Ratio in Galaxies
• The X-ray absorbing column densities of Swift Gamma-ray bursts
• Iron: A Key Element for Understanding the Origin and Evolution of Interstellar Dust
• Molecular Hydrogen in the Damped Lyman-alpha System towards GRB 120815A at z=2.36
• Cosmic dust in MgII absorbers
• Dust in the Circumgalactic Medium of Low-Redshift Galaxies
• Gamma-Ray Burst afterglows as probes of environment and blastwave physics I: absorption by host galaxy gas and dust
• The warm, the excited, and the molecular gas: GRB 121024A shining through its star-forming galaxy
• The metallicity and dust content of a redshift 5 gamma-ray burst host galaxy
• Dust-depletion sequences in damped Lyman-α absorbers: a unified picture from low-metallicity systems to the Galaxy
• C IV absorption in damped and sub-damped Lyman-alpha systems: correlations with metallicity and implications for galactic winds at z~2-3
• The Role of Dust in the Early Universe I : Protogalaxy Evolution
• IGM metal enrichment through dust sputtering
• The Optically Unbiased Gamma-Ray Burst Host (TOUGH) Survey. VII. The Host Galaxy Luminosity Function: Probing the Relationship Between GRBs and Star Formation to Redshift $\sim 6$
• The metals-to-dust ratio to very low metallicities using GRB and QSO absorbers; extremely rapid dust formation
• Unveiling the Secrets of Metallicity and Massive Star Formation Using DLAs along Gamma-ray Bursts
• The Interstellar Medium of GRB Host Galaxies I. Echelle Spectra of Swift GRB Afterglows
• The Magellan Uniform Survey of Damped Lyman alpha Systems I: Cosmic Metallicity Evolution
• A Homogeneous Sample of Sub-DLAs IV: Global Metallicity Evolution
• The nature of proximate damped Lyman alpha systems
• VLT/X-shooter spectroscopy of the GRB 120327A afterglow
• Gamma-Ray Bursts Trace UV Metrics of Star Formation over 3 < z < 5
• A very metal poor Damped Lyman-alpha system revealed through the most energetic GRB 090926A
• The missing gas problem in GRB host galaxies: evidence for a highly ionised component
• On the Perils of Curve-of-Growth Analysis: Systematic Abundance Underestimates for the Gas in Gamma-Ray Burst Host Galaxies
• Elemental depletions in the Magellanic Clouds and the evolution of depletions with metallicity
• The early build-up of dust in galaxies: A study of Damped Ly alpha Systems
• On the (in)variance of the dust-to-metals ratio in galaxies
• VLT/X-shooter spectroscopy of the GRB 090926A afterglow
• Mn abundances in the stars of the Galactic disc with metallicities -1.0 < [Fe/H] < 0.3
• Evidence for Dust Destruction from the Early-time Colour Change of GRB 120119A
• Modelling dust processing and the evolution of grain sizes in the ISM using the method of moments
• The extended High A(V) Quasar Survey: Searching for dusty absorbers toward mid-infrared selected quasars
• The host-galaxy response to the afterglow of GRB 100901A
• Dust, Gas, and Metallicities of Cosmologically Distant Lens Galaxies

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• De Re Metallica: The cosmic chemical evolution of galaxies
• A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• The Dust-to-Gas and Dust-to-Metals Ratio in Galaxies from z=0-6
• High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
• On the dust temperatures of high redshift galaxies
• Galaxy Simulation with Dust Formation and Destruction
• Dusty galaxies in the Epoch of Reionization: simulations
• Consensus report on 25 years of searches for damped Ly$\alpha$ galaxies in emission: Confirming their metallicity-luminosity relation at $z\gtrsim 2$
• The assembly of dusty galaxies at $z\ge 4$: statistical properties
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• Synthetic nebular emission from massive galaxies I: origin of the cosmic evolution of optical emission-line ratios
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• The cosmic evolution of dust-corrected metallicity in the neutral gas
• Dust-depletion sequences in damped Lyman-α absorbers: a unified picture from low-metallicity systems to the Galaxy
• Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE project
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• The THESAN project: predictions for multi-tracer line intensity mapping in the epoch of reionization
• The origin of dust in galaxies across cosmic time
• Large Metallicity Variations in the Galactic Interstellar Medium
• Exploring HeII$\lambda$1640 emission line properties at $z\sim 2-4$
• Where does galactic dust come from?
• L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
• Evidence for diffuse molecular gas and dust in the hearts of gamma-ray burst host galaxies
• The gas and stellar content of a metal-poor galaxy at $z=8.496$ as revealed by JWST and ALMA
• The First Maps of ${\kappa }_d$ -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• The IRX-$\beta$ relation of high-redshift galaxies
• Highly-ionized metals as probes of the circumburst gas in the natal regions of gamma-ray bursts
• Dust depletion of metals from local to distant galaxies I: Peculiar nucleosynthesis effects and grain growth in the ISM
• VLT/X-shooter GRBs: Individual extinction curves of star-forming regions
• Dust reddening and extinction curves towards gamma-ray bursts at z > 4
• MusE GAs FLOw and Wind (MEGAFLOW) V. The dust/metallicity-anisotropy of the Circum-Galactic Medium
• Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations
• Metals and dust in the neutral ISM: the Galaxy, Magellanic Clouds, and damped Lyman-α absorbers
• X-shooting GRBs at high redshift: probing dust production history
• Dust depletion of of metals from local to distant galaxies II: Cosmic dust-to-metal ratio and dust composition
• Near Infrared spectroscopic observations of high redshift C~{\sc i} absorbers
• The first Hubble diagram and cosmological constraints using superluminous supernova
• A solar metallicity galaxy at $z>$ 7? Possible detection of the [N II] 122 $\mu$m and [O III] 52 $\mu$m lines
• The cosmic build-up of dust and metals. Accurate abundances from GRB-selected star-forming galaxies at $1.7<z<6.3$
• Cold gas in the early Universe. Survey for neutral atomic-carbon in GRB host galaxies at 1 < z < 6 from optical afterglow spectroscopy
• Gas inflow and outflow in an interacting high-redshift galaxy: The remarkable host environment of GRB 080810 at $z=3.35$
• A quasar hiding behind two dusty absorbers. Quantifying the selection bias of metal-rich, damped Lyman-alpha absorption systems
• Late-time cosmic evolution of dust: solving the puzzle
• Multiwavelength observations of the extraordinary accretion event AT2021lwx
• Early galaxy growth: mergers or gravitational instability?
• The dust-to-gas mass ratio of luminous galaxies as a function of their metallicity at cosmic noon
• Dynamical effects of the radiative stellar feedback on the H I-to-H2 transition
• The dust attenuation law in $z\sim 6$ quasars
• MgII 2797, 2803 emission in a large sample of low-metallicity star-forming galaxies from SDSS DR14
• New constraints on the physical conditions in H${}_2$-bearing GRB-host damped Lyman-$\alpha$ absorbers
• The CGM-GRB Study. I. Uncovering The CircumGalactic Medium around GRB hosts at redshifts 2-6
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• On the dust properties of high redshift molecular clouds and the connection to the 2175 Å extinction bump
• Why Are Some Gamma-Ray Bursts Hosted by Oxygen-rich Galaxies?
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Modelling of long gamma-ray burst host galaxies at cosmic noon from damped Lyman-α absorption statistics
• The Hubble Diagram: Jump from Supernovae to Gamma-Ray Bursts
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• The Chocolate Chip Cookie Model: dust-to-metal ratio of HII regions
• Silicon and iron dust in gamma-ray burst host galaxy absorbers
• First joint absorption and T${}_e$-based metallicity measured in a GRB host galaxy at $z=4.28$ using JWST/NIRSpec
• Exploration of the high-redshift universe enabled by THESEUS
• Rapid Response Mode observations of GRB 160203A: Looking for fine-structure line variability at z=3.52
• First IFU observations of two GRB host galaxies at cosmic noon with JWST/NIRSpec
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Connecting the dusty dots: dust depletion and extinction of local interstellar clouds
• Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models