High-redshift quasars host galaxies: is there a stellar mass crisis?

Abstract

We investigate the evolutionary properties of a sample of quasars at 5<z<6.4 using the semi-analytical hierarchical model GAMETE/QSOdust. We find that the observed properties of these quasars are well reproduced by a common formation scenario in which stars form according to a standard IMF, via quiescent star formation and efficient merger-driven bursts, while the central BH grows via gas accretion and BH-BH mergers. Eventually, a strong AGN driven wind starts to clear up the ISM of dust and gas, damping the star formation and un-obscuring the line of sight toward the QSO. In this scenario, all the QSOs hosts have final stellar masses in the range $(4-6)\times 10^{11}{M}_{sun}$, a factor 3-30 larger than the upper limits allowed by the observations. We discuss alternative scenarios to alleviate this apparent tension: the most likely explanation resides in the large uncertainties that still affect dynamical mass measurements in these high-z galaxies. In addition, during the transition between the starburst-dominated and the active QSO phase, we predict that about 40% of the progenitor galaxies can be classified as Sub Millimeter Galaxies, although their number rapidly decreases with redshift.

arXiv comment14 pages, 9 figures, accepted for publication in MNRAS

References in corpus (134)

• The Global Schmidt Law in Star Forming Galaxies
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• Energy input from quasars regulates the growth and activity of black holes and their host galaxies
• Modeling feedback from stars and black holes in galaxy mergers
• The CO-to-H2 Conversion Factor
• A Unified, Merger-Driven Model for the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes and Galaxy Spheroids
• A luminous quasar at a redshift of z = 7.085
• Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• A Redshift Survey of the Submillimeter Galaxy Population
• Cool Gas in High Redshift Galaxies
• The Assembly and Merging History of Supermassive Black Holes in Hierarchical Models of Galaxy Formation
• A Survey of z>5.8 Quasars in the Sloan Digital Sky Survey I: Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z~6
• The Molecular Interstellar Medium in Ultraluminous Infrared Galaxies
• A unified model for AGN feedback in cosmological simulations of structure formation
• Molecular Gas at High Redshift
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
• Formation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos
• Formation of the First Supermassive Black Holes
• A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey II: Discovery of Three Additional Quasars at z>6
• Submillimeter Galaxies at z~2: Evidence for Major Mergers & Constraints on Lifetimes, IMF and CO-H2 Conversion Factor
• Merger rates in hierarchical models of galaxy formation. II: Comparison with N-body simulations
• Quasar feedback revealed by giant molecular outflows
• A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
• Direct cosmological simulations of the growth of black holes and galaxies
• Self-Regulated Star Formation in Galaxies via Momentum Input from Massive Stars
• The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point
• Evidence of strong quasar feedback in the early Universe
• Dust Formation and Survival in Supernova Ejecta
• Star Formation and Gas Kinematics of Quasar Host Galaxies at z~6: New insights from ALMA
• A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey III: Discovery of Five Additional Quasars
• Herschel Detects a Massive Dust Reservoir in Supernova 1987A
• On the cosmic evolution of the scaling relations between black holes and their host galaxies: Broad Line AGN in the zCOSMOS survey
• Dust emission from the most distant quasars
• 350 Micron Dust Emission from High Redshift Quasars
• Evolution of interstellar dust and stardust in the solar neighbourhood
• Formation of the first nuclear clusters and massive black holes at high redshift
• Resolved Molecular Gas in a Quasar Host Galaxy at Redshift z=6.42
• Formation of z ~ 6 quasars from hierarchical galaxy mergers
• Selection Bias in Observing the Cosmological Evolution of the Mbh-sigma and Mbh-L Relationships
• A Herschel view of the far-infrared properties of submillimetre galaxies
• Evolution of Dust in Primordial Supernova Remnants: Can Dust Grains Formed in the Ejecta Survive and be Injected into the Early Interstellar Medium?
• Cold flows and the first quasars
• A 3x10^9 solar mass black hole in the quasar SDSS J1148+5251 at z=6.41
• Observational Signatures of the First Quasars
• Four quasars above redshift 6 discovered by the Canada-France High-z Quasar Survey
• Molecular Gas in Redshift 6 Quasar Host Galaxies
• The Evolution of Dust in the Early Universe with Applications to the Galaxy SDSS J1148+5251
• Can Supermassive Black Holes Form in Metal-Enriched High-Redshift Protogalaxies ?
• Dust Formation In Early Galaxies
• Gemini Near-infrared Spectroscopy of Luminous z~6 Quasars: Chemical Abundances, Black Hole Masses, and MgII Absorption
• Stellar sources of dust in the high redshift Universe
• Evidence for non-evolving FeII/MgII ratios in rapidly accreting z~6 QSOs
• What Does a Submillimeter Galaxy Selection Actually Select? The Dependence of Submillimeter Flux Density on Star Formation Rate and Dust Mass
• Interferometric Observations of Powerful CO Emission from the three Submillimeter Galaxies at z=2.30, 2.51 and 3.35
• Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
• Quasars at z=6: the survival of the fittest
• The Spitzer/IRAC view of black hole - bulge scaling relations
• The Blast Wave Model for AGN Feedback: Effects on AGN Obscuration
• A Cool Dust Factory in the Crab Nebula: A Herschel Study of the Filaments
• The stellar masses and specific star-formation rates of submillimetre galaxies
• The origin of dust in high redshift QSOs: the case of SDSS J1148+5251
• The physics and the structure of the quasar-driven outflow in Mrk 231
• GOODS-Herschel~: Gas-to-dust mass ratios and CO-to-H_2 conversion factors in normal and starbursting galaxies at high-z
• Testing the Evolutionary Link Between Submillimetre Galaxies and Quasars: CO Observations of QSOs at z~2
• Growing the first bright quasars in cosmological simulations of structure formation
• Thermal Emission from Warm Dust in the Most Distant Quasars
• Iron Emission in the z=6.4 Quasar SDSS J114816.64+525150.3
• Energetics of the molecular gas in the H_2 luminous radio galaxy 3C 326: Evidence for negative AGN feedback
• The Origin of Dust in the Early Universe: Probing the Star Formation History of Galaxies by their Dust Content
• Three Modes of Metal-Enriched Star Formation in the Early Universe
• Probing the Coevolution of Supermassive Black Holes and Quasar Host Galaxies
• The metallicity of the most distant quasars
• What determines the grain size distribution in galaxies?
• The extinction law at high redshift and its implications
• Millimeter imaging of submillimeter galaxies in the COSMOS field: Redshift distribution
• Recipes for stellar jets: results of combined optical/infrared diagnostics
• How to distinguish starbursts and quiescently star-forming galaxies: The `bimodal' submillimetre galaxy population as a case study
• Smoking Quasars: a New Source for Cosmic Dust
• Deep 1.1 mm-wavelength imaging of the GOODS-South field by AzTEC/ASTE -- II. Redshift distribution and nature of the submillimetre galaxy population
• The dust budget crisis in high-redshift submillimetre galaxies
• Formation and Evolution of Dust in Type IIb Supernova with Application to the Cassiopeia A Supernova Remnant
• High-redshift formation and evolution of central massive objects II: The census of BH seeds
• High-resolution CO and radio imaging of z~2 ULIRGs: extended CO structures, and implications for the universal star formation law
• The dust production rate of AGB stars in the Magellanic Clouds
• The First Massive Black Hole Seeds and Their Hosts
• Quasars as probes of the submillimetre cosmos at z>5: I. Preliminary SCUBA photometry
• Effects of dust grains on early galaxy evolution
• Dust grain growth in the interstellar medium of 5<z<6.5 quasars
• The mass function of high redshift seed black holes
• Self-Regulated Black Hole Growth via Momentum Deposition in Galaxy Merger Simulations
• Imaging the Molecular Gas in a z=3.9 Quasar Host Galaxy at 0.3" Resolution: A Central, Sub-Kiloparsec Scale Star Formation Reservoir in APM 08279+5255
• The dust content of high-z submillimeter galaxies revealed by Herschel
• Life and times of dwarf spheroidal galaxies
• The dynamics of the ionized and molecular ISM in powerful obscured quasars at z>=3.5
• Glimpsing through the high redshift neutral hydrogen fog
• Submillimetre Observations of z>6 Quasars
• Variations on a theme - the evolution of hydrocarbon solids: III. Size-dependent properties - the optEC(s)(a) model
• Black Holes in the Early Universe
• Evaluating Semi-Analytic Halo Merging Histories
• ALMA reveals a chemically evolved submillimeter galaxy at z=4.76
• Dust input from AGB stars in the Large Magellanic Cloud
• Metals, dust and the cosmic microwave background: fragmentation of high-redshift star-forming clouds
• Chemical Evolution of High-Redshift Radio Galaxies
• Far-infrared properties of submillimeter and optically faint radio galaxies
• Molecular gas in QSO host galaxies at z>5
• The chemical evolution of elliptical galaxies with stellar and QSO dust production
• Assessing the redshift evolution of massive black holes and their hosts
• The metals-to-dust ratio to very low metallicities using GRB and QSO absorbers; extremely rapid dust formation
• Formation of Molecular Clouds and Global Conditions for Star Formation
• Modeling the Dust Properties of z ~ 6 Quasars with ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree
• Molecular Gas in Lensed z>2 Quasar Host Galaxies and the Star Formation Law for Galaxies with Luminous Active Galactic Nuclei
• Formation of a Quasar Host Galaxy through a Wet Merger 1.4 Billion Years after the Big Bang
• The Stellar Mass Spectrum in Warm and Dusty Gas: Deviations from Salpeter in the Galactic Centre and in Circum-Nuclear Starburst Regions
• The dust content of QSO hosts at high redshift
• Complete infrared spectral energy distributions of mm detected quasars at z>5
• High redshift formation and evolution of central massive objects I: model description
• Star Formation at Very Low Metallicity. V. The Greater Importance of Initial Conditions Compared to Metallicity Thresholds
• The Building Up of the Black Hole Mass - Stellar Mass Relation
• The transverse proximity effect in spectral hardness on the line of sight towards HE 2347-4342
• Implications of Quasar Black Hole Masses at High Redshifts
• Genesis and evolution of dust in galaxies in the early Universe II. Rapid dust evolution in quasars at z > 6
• Dust in the early Universe: Evidence for non-stellar dust production or observational errors?
• The Formation of Galaxies Hosting z~6 Quasars
• The Relative Role of Galaxy Mergers and Cosmic Flows in Feeding Black Holes
• Intermediate- and High-Velocity Ionized Gas toward zeta Orionis
• HerMES: Lyman Break Galaxies individually detected at 0.7 < z < 2.0 in GOODS-N with Herschel/SPIRE
• Quasar feedback in the early Universe: the case of SDSS J1148+5251
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• On inferring extinction laws in z~6 quasars as signatures of supernova dust
• The Origins and Physical Properties of the Complex of Local Interstellar Clouds
• Photometry and spectroscopy of the new sdBV CS 1246
• Prospects for AGN studies with ALMA
• Is GRB 050904 at z=6.3 absorbed by dust?

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• Bright [CII] and dust emission in three z>6.6 quasar host galaxies observed by ALMA
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• The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7
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• Decoding the stellar fossils of the dusty Milky Way progenitors
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• The gentle monster PDS 456: the kpc scale molecular outflow and its implications for QSO feedback
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• A dusty compact object bridging galaxies and quasars at cosmic dawn
• The dust-to-stellar mass ratio as a valuable tool to probe the evolution of local and distant star forming galaxies
• 400 pc Imaging of a Massive Quasar Host Galaxy at a Redshift of 6.6
• The WISSH quasars Project: II. Giant star nurseries in hyper-luminous quasars
• On the formation of the first quasars
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at $z\gtrsim 6$ studied with ALMA
• High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
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• Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
• Where does galactic dust come from?
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• 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
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• The origin of the Far-infrared continuum of z ~ 6 quasars: a radiative transfer model for SDSS J1148+5251
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• Chasing the observational signatures of seed black holes at z > 7: candidate statistics
• Physical properties of the first quasars
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• Unveiling early black hole growth with multi-frequency gravitational wave observations
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• The hyperluminous Compton-thick $z\sim 2$ quasar nucleus of the hot DOG W1835+4355 observed by NuSTAR
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