High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions

Abstract

The James Webb Space Telescop (JWST) promises to revolutionise our understanding of the early Universe, and contrasting its upcoming observations with predictions of the $\Lambda$CDM model requires detailed theoretical forecasts. Here, we exploit the large dynamic range of the IllustrisTNG simulation suite, TNG50, TNG100, and TNG300, to derive multi-band galaxy luminosity functions from $z=2$ to $z=10$. We put particular emphasis on the exploration of different dust attenuation models to determine galaxy luminosity functions for the rest-frame ultraviolet (UV), and apparent wide NIRCam bands. Our most detailed dust model is based on continuum Monte Carlo radiative transfer calculations employing observationally calibrated dust properties. This calibration results in constraints on the redshift evolution of the dust attenuation normalisation and dust-to-metal ratios yielding a stronger redshift evolution of the attenuation normalisation compared to most previous theoretical studies. Overall we find good agreement between the rest-frame UV luminosity functions and observational data for all redshifts, also beyond the regimes used for the dust-model calibrations. Furthermore, we also recover the observed high redshift ($z=4-6$) UV luminosity versus stellar mass relation, the H$\alpha$ versus star formation rate relation, and the H$\alpha$ luminosity function at $z=2$. The bright end ($M_{\mathrm{UV}}>-19.5$) cumulative galaxy number densities are consistent with observational data. For the F200W NIRCam band, we predict that JWST will detect $\sim 80$ ($\sim 200$) galaxies with a signal-to-noise ratio of $10$ ($\sim 5$) within the NIRCam field of view, $2.2\times 2.2{\mathrm{arcmin}}^2$, for a total exposure time of $10^5\mathrm{s}$ in the redshift range $z=8\pm 0.5$. These numbers drop to $\sim 10$ ($\sim 40$) for an exposure time of $10^4\mathrm{s}$.

36 pages, 24 figures, MNRAS submitted

References in corpus (179)

• Planck 2015 results. XIII. Cosmological parameters
• Galactic Stellar and Substellar Initial Mass Function
• On the variation of the Initial Mass Function
• Star Formation in Galaxies Along the Hubble Sequence
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• Modules for Experiments in Stellar Astrophysics (MESA)
• Starburst99: Synthesis Models for Galaxies with Active Star Formation
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
• Populating a cluster of galaxies - I. Results at z=0
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
• High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
• Simulating Galaxy Formation with the IllustrisTNG Model
• MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• First results from the IllustrisTNG simulations: matter and galaxy clustering
• A Simple Model for the Absorption of Starlight by Dust in Galaxies
• First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
• The hierarchical formation of the brightest cluster galaxies
• MILES: A Medium resolution INT Library of Empirical Spectra
• First results from the IllustrisTNG simulations: the galaxy color bimodality
• Infrared Emission from Interstellar Dust. II. The Diffuse Interstellar Medium
• Properties of galaxies reproduced by a hydrodynamic simulation
• First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
• The propagation of uncertainties in stellar population synthesis modeling III: model calibration, comparison, and evaluation
• Dust Absorption And The Ultraviolet Luminosity Density At z \approx 3 As Calibrated By Local Starburst Galaxies
• Simba: Cosmological Simulations with Black Hole Growth and Feedback
• First results from the IllustrisTNG simulations: radio haloes and magnetic fields
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• Substructures in hydrodynamical cluster simulations
• First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
• A model for cosmological simulations of galaxy formation physics
• First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time
• Calibrating Extinction-Free Star Formation Rate Diagnostics with 33GHz Free-Free Emission in NGC6946
• The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years
• Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
• Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range
• The Illustris simulation: the evolving population of black holes across cosmic time
• The Frontier Fields: Survey Design
• A Steep Faint-End Slope of the UV Luminosity Function at z~2-3: Implications for the Global Stellar Mass Density and Star Formation in Low Mass Halos
• Spectroscopic Confirmation of a Population of Normal Star-Forming Galaxies at Redshifts z>3
• The Illustris Simulation: Public Data Release
• 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
• The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang
• The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
• 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
• The 2013 Release of Cloudy
• A unified multi-wavelength model of galaxy formation
• Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4
• Nebular Continuum and Line Emission in Stellar Population Synthesis Models
• UV-Continuum Slopes of >4000 z~4-8 Galaxies from the HUDF/XDF, HUDF09, ERS, CANDELS-South, and CANDELS-North Fields
• A new multi-field determination of the galaxy luminosity function at z=7-9 incorporating the 2012 Hubble Ultra Deep Field imaging
• The Evolutionary History of Lyman Break Galaxies Between Redshift 4 and 6: Observing Successive Generations of Massive Galaxies in Formation
• A Physical Model for the Origin of Quasar Lifetimes
• The Dust Attenuation Law in Distant Galaxies: Evidence for Variation with Spectral Type
• The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr
• Directly Observing the Galaxies Likely Responsible for Reionization
• A large Hα survey at z=2.23, 1.47, 0.84 & 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS
• Improving the convergence properties of the moving-mesh code AREPO
• Dust Obscuration and Metallicity at High Redshift: New Inferences from UV, H-alpha, and 8 Micron Observations of z~2 Star-Forming Galaxies
• Discovery of z~8 Galaxies in the HUDF from ultra-deep WFC3/IR Observations
• The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift
• A physical model for cosmological simulations of galaxy formation: multi-epoch validation
• The Most Luminous z~9-10 Galaxy Candidates yet Found: The Luminosity Function, Cosmic Star-Formation Rate, and the First Mass Density Estimate at 500 Myr
• Efficient 3D NLTE dust radiative transfer with SKIRT
• CANDELS: The Evolution of Galaxy Rest-Frame Ultraviolet Colors from z = 8 to 4
• The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
• SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture
• The mass evolution of the first galaxies: stellar mass functions and star formation rates at $4<z<7$ in the CANDELS GOODS-South field
• Large Area Survey for z=7 Galaxies in SDF and GOODS-N: Implications for Galaxy Formation and Cosmic Reionization
• Full-Data Results of Hubble Frontier Fields: UV Luminosity Functions at $z\sim 6-10$ and a Consistent Picture of Cosmic Reionization
• 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
• Probing the Dawn of Galaxies at z~9-12: New Constraints from HUDF12/XDF and CANDELS Data
• The Galaxy UV Luminosity Function Before the Epoch of Reionization
• The SPHINX Cosmological Simulations of the First Billion Years: the Impact of Binary Stars on Reionization
• The high redshift galaxy population in hierarchical galaxy formation models
• Star formation history and dust attenuation in galaxies drawn from ultraviolet surveys
• Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: IV The Controlling Parameters of the Starburst SED
• A redshift-independent efficiency model: star formation and stellar masses in dark matter halos at z>4
• Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations
• The UV Luminosity Function of star-forming galaxies via dropout selection at redshifts z ~ 7 and 8 from the 2012 Ultra Deep Field campaign
• The dust content of galaxies from z = 0 to z = 9
• The z~6 Luminosity Function Fainter than -15 mag from the Hubble Frontier Fields: The Impact of Magnification Uncertainties
• z~7 Galaxies in the HUDF: First Epoch WFC3/IR Results
• Galaxy Properties from the Ultra-violet to the Far-Infrared: Lambda-CDM models confront observations
• Evolution of Galaxy Stellar Mass Functions, Mass Densities, and Mass to Light Ratios from z 7 to z 4
• The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: The z=9 LF and further evidence for a smooth decline in UV luminosity at z >= 8
• The Extreme Faint End of the UV Luminosity Function at $z\sim 6$ Through Gravitational Telescopes: a comprehensive assessment of strong lensing uncertainties
• GOODS-Herschel Measurements of the Dust Attenuation of Typical Star-Forming Galaxies at High Redshift: Observations of UV-Selected Galaxies at z~2
• The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies
• A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios
• Galaxy Properties and UV Escape Fractions During Epoch of Reionization: Results from the Renaissance Simulations
• The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?
• Optical colours and spectral indices of $z=0.1$ EAGLE galaxies with 3D dust radiative transfer code SKIRT
• The galaxy luminosity function at z ~ 6 and evidence for rapid evolution in the bright end from z ~ 7 to 5
• Precise Strong Lensing Mass Modeling of Four Hubble Frontier Fields Clusters and a Sample of Magnified High-Redshift Galaxies
• Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions
• A Census of Star-Forming Galaxies in the z~9-10 Universe based on HST+Spitzer Observations Over 19 CLASH clusters: Three Candidate z~9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at z~9
• The UV continua and inferred stellar populations of galaxies at z ~ 7 - 9 revealed by the Hubble Ultra Deep Field 2012 campaign
• A new model of galaxy formation: How sensitive are predicted galaxy luminosities to the choice of SPS model?
• The Constant Average Relationship between Dust-obscured Star Formation and Stellar Mass from $z=0$ to $z=2.5$
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• The 2012 Hubble Ultra Deep Field (UDF12): Observational Overview
• New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density
• Lyman Break Galaxies and the Star Formation Rate of the Universe at z~6
• 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
• Are Dusty Galaxies Blue? Insights on UV Attenuation from Dust-Selected Galaxies
• Dust Formation in Milky Way-like Galaxies
• The luminosity function, halo masses and stellar masses of luminous Lyman-break galaxies at redshifts 5<z<6
• Evolution of the galaxy stellar mass functions and UV luminosity functions at $z=6-9$ in the Hubble Frontier Fields
• Simulating the dust content of galaxies: successes and failures
• The UV galaxy luminosity function at z=3-5 from the CFHT Legacy Survey Deep fields
• Ultra-faint Ultraviolet Galaxies at z~2 Behind the Lensing Cluster Abell 1689: the Luminosity Function, Dust Extinction and Star Formation Rate Density
• Observational Searches for Galaxies at z > 6
• The UV Properties of Star Forming Galaxies I: HST WFC3 Observations of Very-high Redshift Galaxies
• Breaking the Curve with CANDELS: A Bayesian Approach to Reveal the Non-Universality of the Dust-Attenuation Law at High Redshift
• 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
• Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field
• Galaxy Simulation with Dust Formation and Destruction
• The Evolution of the UV Luminosity Function from z ~ 0.75 to z ~ 2.5 using HST ERS WFC3/UVIS Observations
• Dust attenuation, dust emission, and dust temperature in galaxies at z>=5: a view from the FIRE-2 simulations
• Dusty galaxies in the Epoch of Reionization: simulations
• A physical model for the 0 < z < 8 redshift evolution of the galaxy UV luminosity and stellar mass functions
• Far-infrared and dust properties of present-day galaxies in the EAGLE simulations
• The Luminosity Function at z~8 from 97 Y-band dropouts: Inferences About Reionization
• Simulating galactic dust grain evolution on a moving mesh
• GMASS ultradeep spectroscopy of galaxies at z ~ 2. IV. The variety of dust populations
• Dust-to-metal ratios in damped Lyman-alpha absorbers: Fresh clues to the origins of dust and optical extinction towards gamma-ray bursts
• The galaxy UV luminosity function at z ~ 2 - 4; new results on faint-end slope and the evolution of luminosity density
• The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
• Detection of PAH and Far-Infrared Emission from the Cosmic Eye: Probing the Dust and Star Formation of Lyman Break Galaxies
• Evolution of Dust-to-Metal Ratio in Galaxies
• Star Formation at z~6: i-dropouts in the ACS GTO fields
• Evolution of the dust-to-metals ratio in high-redshift galaxies probed by GRB-DLAs
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• The First Billion Years project - IV: Proto-galaxies reionising the Universe
• GOODS-HERSCHEL: evidence for a UV extinction bump in galaxies at z > 1
• Dust Attenuation in High Redshift Galaxies -- 'Diamonds in the Sky'
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• The properties of the first galaxies in the BLUETIDES simulation
• Dust-depletion sequences in damped Lyman-α absorbers: a unified picture from low-metallicity systems to the Galaxy
• UV-dropout Galaxies in the GOODS-South Field from WFC3 Early Release Science Observations
• Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes
• Steep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 and the Implications for Reionisation
• The First Billion Years project: constraining the dust attenuation law of star-forming galaxies at z $\simeq$ 5
• Lens Models Under the Microscope: Comparison of Hubble Frontier Field Cluster Magnification Maps
• Evidence for a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field
• Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
• The metals-to-dust ratio to very low metallicities using GRB and QSO absorbers; extremely rapid dust formation
• Interpreting the observed UV continuum slopes of high-redshift galaxies
• Simulating the assembly of galaxies at redshifts z = 6 - 12
• Probing $\sim L_{\ast }$ Lyman-break Galaxies at $z\approx 7$ in GOODS-South with WFC3 on HST
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• Hierarchical octree and k-d tree grids for 3D radiative transfer simulations
• Evaluating and Improving Semi-analytic modelling of Dust in Galaxies based on Radiative Transfer Calculations
• Using 3D Voronoi grids in radiative transfer simulations
• Stellar and nebular diagnostics in the UV for star-forming galaxies
• The unbiased measurement of UV spectral slopes in low luminosity galaxies at z=7
• Dust in and around galaxies: dust in cluster environments and its impact on gas cooling
• A Dual Narrowband Survey for Hα Emitters at z=2.2: Demonstration of the Technique and Constraints on the Hα Luminosity Function
• A direct calibration of the IRX-β relation in Lyman-break Galaxies at z=3-5
• Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at $\mathbf{z}=0.4-4.7$
• UVUDF: UV Luminosity Functions at the cosmic high-noon
• High Redshift Galaxy Populations and their Descendants
• The Far-Infrared, UV and Molecular Gas Relation in Galaxies up to z=2.5
• Discovery of Lyman Break Galaxies at z~7 from the ZFOURGE Survey
• First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations
• The Photometric Properties of Galaxies in the Early Universe
• Physical Properties of UDF12 Galaxies in Cosmological simulations
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• Heavy dust obscuration of z=7 galaxies in a cosmological hydrodynamic simulation
• Dust properties of Lyman break galaxies in cosmological simulations
• Cosmic evolution of dust in galaxies: Methods and preliminary results
• Dust, Gas, and Metallicities of Cosmologically Distant Lens Galaxies

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