Luminosity-dependent evolution of soft X-ray selected AGN: New Chandra and XMM-Newton surveys
arXiv:astro-ph/0506118 · doi:10.1051/0004-6361:20042134
Abstract
We present new results on the cosmological evolution of unabsorbed (type-1) active galactic nuclei (AGN) selected in the soft (0.5-2 keV) X-ray band. From a variety of ROSAT, XMM-Newton and Chandra surveys we selected a total of ~1000 AGN with an unprecedented spectroscopic and photometric optical/NIR identification completeness. For the first time we are able to derive reliable space densities for low-luminosity (Seyfert-type) X-ray sources at cosmological redshifts. The evolutionary behaviour of AGN shows a strong dependence on X-ray luminosity: while the space density of high-luminosity AGN reaches a peak around z~2, similar to that of optically selected QSO, the space density of low-luminosity AGNs peaks at redshifts below z=1. This confirms previous ROSAT findings of a luminosity-dependent density evolution. Using a rigorous treatment of the optical identification completeness we are able to show that the space density of AGN with X-ray luminosities L_x < 10^45 erg s^-1 declines significantly towards high redshifts.
arXiv comment21 pages, 13 figures, A&A (in press)
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- X-ray constraints on the fraction of obscured AGN at high accretion luminosities
- The Chandra COSMOS Legacy survey: the z>3 sample
- Type 2 AGN host galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching
- Modelling the luminosities and sizes of radio galaxies: radio luminosity function at z = 6
- Galaxy-scale Bars in Late-type Sloan Digital Sky Survey Galaxies Do Not Influence the Average Accretion Rates of Supermassive Black Holes
- XZ: Deriving redshifts from X-ray spectra of obscured AGN
- X-ray spectra of sources in the 13H XMM-Newton / Chandra deep field
- Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe
- Supermassive Black Holes and Their Environments
- Linking the X-ray and infrared properties of star-forming galaxies at z<1.5
- Constraints on the faint end of the quasar luminosity function at z~5 in the COSMOS field
- Herschel Far-Infrared Photometry of the Swift Burst Alert Telescope Active Galactic Nuclei Sample of the Local Universe. II. SPIRE Observations
- On the co-evolution of supermassive black holes and their host galaxies since z = 3
- The Contribution of z<6 Sources to the Spatial Coherence in the Unresolved Cosmic near-Infrared and X-ray Backgrounds
- X-ray selected AGN in groups at redshifts z~1
- SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-m-selected galaxies
- The Largest X-ray Selected Sample of z>3 AGNs: C-COSMOS & ChaMP
- Supermassive Black-Hole Growth Over Cosmic Time: Active Galaxy Demography, Physics, and Ecology from Chandra Surveys
- Herschel ATLAS: The cosmic star formation history of quasar host galaxies
- Broad Band X-Ray Spectra of Two Low-luminosity Active Galactic Nuclei NGC 1566 and NGC 4941
- Obscured GOODS AGN and Their Host Galaxies at z < 1.25: The Slow Black Hole Growth Phase
- Eddington ratios of faint AGN at intermediate redshift: Evidence for a population of half-starved black holes
- AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
- Angular Anisotropies in the Cosmic Gamma-ray Background as a Probe of its Origin
- Determining the core radio luminosity function of radio AGNs via copula
- Linking the fate of massive black hole binaries to the active galactic nuclei luminosity function
- Cosmic downsizing of powerful radio galaxies to low radio luminosities
- Radio-AGN Feedback: When the Little Ones were Monsters
- Physics of Coevolution of Galaxies and Supermassive Black Holes
- Anti-hierarchical evolution of the Active Galactic Nucleus space density in a hierarchical universe
- The Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields
- Are dry mergers of Ellipticals the way to reconcile model predictions with the downsizing?
- J-PLUS: Unveiling the brightest-end of the Lyα luminosity function at 2.0<z<3.3 over 1000 deg^2
- Metals in the circumgalactic medium are out of ionization equilibrium due to fluctuating active galactic nuclei
- Angular correlation functions of X-ray point-like sources in the full exposure XMM-LSS field
- Supermassive black holes, star formation and downsizing of elliptical galaxies
- High-precision multi-band measurements of the angular clustering of X-ray sources
- AGN evolution from galaxy evolution viewpoint - II
- Radio continuum properties of luminous infrared galaxies. Identifying the presence of an AGN in the radio
- Accretion Properties of A Sample of Hard X-ray (<60keV) Selected Seyfert 1 Galaxies
- Testing the starburst/AGN connection with SWIRE X-ray/70 micron sources
- The average 0.5-200 keV spectrum of local active galactic nuclei and a new determination of the 2-10 keV luminosity function at z \approx 0
- Luminosity Dependent X-ray AGN Clustering ?
- On the origin of ultra high energy cosmic rays: Subluminal and superluminal relativistic shocks
- The RASS--6dFGS catalogue: a sample of X-ray selected AGN from the 6dF Galaxy Survey
- Constraints on Extragalactic Point Source Flux from Diffuse Neutrino Limits
- Evolution of active galactic nuclei
- The X-ray luminosity function of AGN at z~3
- HST/NICMOS Imaging of Bright High-Redshift 24μm-selected Galaxies: Merging Properties
- The Subaru-XMM-Newton Deep Survey (SXDS) VIII.: Multi-wavelength Identification, Optical/NIR Spectroscopic Properties, and Photometric Redshifts of X-ray Sources
- A Plethora of AGN Among Lyman Alpha Galaxies at Low Redshift
- On the Evolution of the Cores of Radio Sources and Their Extended Radio Emission
- The First Decade of Science with Chandra and XMM-Newton
- The Deep Chandra Survey of the Groth Strip - II. optical identification of the X-ray sources
- Ultraviolet Emission-Line Correlations in Hubble/COS Spectra of Active Galactic Nuclei: Single-Epoch Black Hole Masses
- Lower AGN Abundance in Galaxy Clusters at z < 0.5
- The ATLAS 5.5 GHz Survey of the Extended Chandra Deep Field South: The Second Data Release
- Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data
- XMM-Newton observations of the Galactic globular clusters NGC 2808 and NGC 4372
- The connection between star formation and supermassive Black Hole activity in the local Universe
- The OPTX Project III: X-ray versus Optical Spectral Type for AGNs
- Infrared-Faint Radio Sources: A Cosmological View - AGN Number Counts, the Cosmic X-Ray Background and SMBH Formation
- Disk Assembly and the M_BH-sigma Relation of Supermassive Black Holes
- Combined Chandra, XMM-Newton and Hubble Space Telescope observations of the Galactic globular cluster NGC 2808
- Comoving Space Density and Obscured Fraction of High-Redshift Active Galactic Nuclei in the Subaru/{\it XMM-Newton} Deep Survey
- Evolution of [OIII]5007 emission-line profiles in narrow emission-line galaxies
- Acceleration and propagation of ultra high energy cosmic rays
- Obscured and powerful AGN and starburst activities at z~3.5
- Demographics of z ~ 6 Quasars in the Black Hole Mass-Luminosity Plane
- Why are AGN found in High Mass Galaxies?
- Constraining the Emissivity of Ultrahigh Energy Cosmic Rays in the Distant Universe with the Diffuse Gamma-ray Emission
- The 2-10 keV unabsorbed luminosity function of AGN from the XMM-Newton LSS, CDFS and COSMOS surveys
- Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
- Curious case of the maximum rigidity distribution of cosmic-ray accelerators
- The Type II AGN-host galaxy connection: insights from the VVDS and VIPERS surveys
- Placing High-Redshift Quasars in Perspective: a Catalog of Spectroscopic Properties from the Gemini Near Infrared Spectrograph -- Distant Quasar Survey
- On ultra high energy cosmic rays and their resultant gamma rays
- AGN and QSOs in the eROSITA All-Sky Survey -- Part II: The large-scale structure
- Probing the Cosmic X-ray and MeV Gamma-ray Background Radiation through the Anisotropy
- The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
- The WISSH quasars project XI. The mean Spectral Energy Distribution and Bolometric Corrections of the most luminous quasars
- A mixture evolution scenario of the AGN radio luminosity function. II. Do low- and high-power radio-loud AGNs evolve differently?
- Constraints on the Local Sources of Ultra High-Energy Cosmic Rays
- Prospects for Very High Energy Blazar Survey by the Next Generation Cherenkov Telescopes
- A Uniform History for Galaxy Evolution
- The Cosmic History of Black Hole Growth from Deep Multiwavelength Surveys
- Infrared luminosity functions and dust mass functions in the EAGLE simulation
- Spectral Properties and the Effect on Redshift Cut-off of Compact AGNs from the AT20G Survey
- AGN X-ray luminosity function and absorption function in the Early Universe ()
- The neutrino background from non-jetted active galactic nuclei
- Modeling the spectrum and composition of ultrahigh-energy cosmic rays with two populations of extragalactic sources
- Self-consistent model of extragalactic neutrino flux from evolving blazar population
- Faint COSMOS AGN at z~3.3 - I. Black Hole Properties and Constraints on Early Black Hole Growth
- Higher prevalence of X-ray selected AGN in intermediate age galaxies up to z~1
- Radio observations of the CDF-South: a possible link between radio emission and star formation in X-ray selected AGN
- Is the dependence of spectral index on luminosity real in optically selected AGN samples?
- Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alerts
- The preferentially magnified active nucleus in IRAS F10214+4724 - II. Spatially resolved cold molecular gas
- Systematically smaller single-epoch quasar black hole masses using a radius-luminosity relationship corrected for spectral bias
- The X-Ray Point-Source Population of NGC 1365: The Puzzle of Two Highly-Variable Ultraluminous X-ray Sources
- A dwarf nova in the globular cluster M13
- SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-m-selected sub-millimeter galaxies
- The XXL Survey: XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters
- Measuring the jet power of flat spectrum radio quasars
- A thin diffuse component of the Galactic Ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries
- Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution
- Astrophysical interpretation of the anisotropies in the unresolved gamma-ray background
- Mildly obscured active galaxies and the cosmic X-ray background
- Origin of the light cosmic ray component below the ankle
- Large-scale variations of the cosmic X-ray background and the X-ray emissivity of the local Universe
- AGN Activity and Black Hole Masses in Low Surface Brightness Galaxies
- Gamma-ray and Neutrino Signals from Accretion Disk Coronae of Active Galactic Nuclei
- X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z=6.56
- Relativistic accretion disk reflection in AGN X-ray spectra at z=0.5--4: a study of four \textit{Chandra} deep fields
- An XMM-Newton view of the merging activity in the Centaurus cluster
- The XXL Survey XIX. A realistic population of simulated X-ray AGN: Comparison of models with observations
- Prospects for future very high-energy gamma-ray sky survey: impact of secondary gamma rays
- Cosmological Tests with the FSRQ Gamma-ray Luminosity Function
- BAT AGN Spectroscopic Survey -- XIII. The nature of the most luminous obscured AGN in the low-redshift universe
- Heavily Obscured AGN detection: a Radio vs X-ray challenge
- Mid-Infrared Selected Quasars I: Virial Black Hole Mass and Eddington Ratios
- Faint, Evolving Radio AGN in SDSS Luminous Red Galaxies
- A Joint Model Of X-ray And Infrared Backgrounds. II. Compton-Thick AGN Abundance
- The spatial clustering of ROSAT all-sky survey Active Galactic Nuclei: V. The evolution of broad-line AGN clustering properties in the last 6 Gyr
- Modeling active galactic nuclei: ongoing problems for the faint-end of the luminosity function
- The SWIFT AGN and Cluster Survey I: Number Counts of AGN and Galaxy Clusters
- On the radio properties of the highest redshift quasars
- Can AGN and galaxy clusters explain the surface brightness fluctuations of the cosmic X-ray background?
- Lyman Alpha Constraints on Very Low Luminosity AGN
- The environment and redshift dependence of accretion onto dark matter halos and subhalos
- The contribution from blazar cascade emission to the extragalactic gamma-ray background: What a role does the extragalactic magnetic field play?
- The Evolution of AGN Activity in Brightest Cluster Galaxies
- Searching for the most distant blazars with the Fermi Gamma-ray Space Telescope
- XMM-Newton observation of a sample of four close dSph galaxies
- Selected Topics in Cosmic Ray Physics
- The growth of supermassive black holes fed by accretion disks
- A flexible method for estimating luminosity functions via Kernel Density Estimation
- Revisiting the Completeness and the Luminosity Function in High-Redshift Low-Luminosity Quasar Surveys
- Neural-network selection of high-redshift radio quasars, and the luminosity function at z~4
- A catalogue of faint local radio AGN and the properties of their host galaxies
- An XMM-Newton search for X-ray sources in the Fornax dwarf galaxy
- Astrophysics in 2006
- Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared
- Galaxy kinematics in the XMMU J2235-2557 cluster field at z~1.4
- Linking X-ray AGN with dark matter halos: a model compatible with AGN luminosity function and large-scale clustering properties
- The Star Formation and Nuclear Accretion Histories of Normal Galaxies in the AGES Survey
- The XMM-Newton Wide Angle Survey (XWAS)
- Propagation of ultra high energy cosmic rays
- Environment from cross-correlations: connecting hot gas and the quenching of galaxies
- Characterization of AGN and their hosts in the Extended Groth Strip: a multiwavelength analysis
- Role of Feedback in AGN-HOST Coevolution: A Study from Partially Obscured Active Galactic Nuclei
- Insights Into AGN and Host Galaxy Co-evolution From Hard X-ray Emission
- Understanding AGN-host connection in partially obscured active galactic nuclei. Part III: Properties of ROSAT-selected SDSS AGNs
- Bimodal AGNs in Bimodal Galaxies
- Rolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds
- Clustering, Cosmology and a New Era of Black Hole Demographics -- II. The Conditional Luminosity Functions of Type 2 and Type 1 Active Galactic Nuclei
- The soft X-ray Cluster-AGN spatial cross-correlation function in the ROSAT-NEP survey
- On the Evolution of High-Redshift Active Galactic Nuclei
- Unveiling Gargantua: A new search strategy for the most massive central cluster black holes
- e-MERLIN observations at 5 GHz of the GOODS-N region: pinpointing AGN cores in high redshift galaxies
- Hard X-ray properties of radio-selected blazars
- eROSITA Final Equatorial-Depth Survey (eFEDS): eFEDS X-ray view of WERGS Radio Galaxies selected by the Subaru/HSC and VLA/FIRST survey
- Sub-Eddington super-massive black hole activity in Fornax early type galaxies
- Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations
- The AGN fraction in high-redshift protocluster candidates selected by Planck and Herschel
- Fundamental properties of Fanaroff-Riley II radio galaxies investigated via Monte Carlo simulations
- Studying the ICM in clusters of galaxies via surface brightness fluctuations of the cosmic X-ray background
- SDSS AGNs with X-ray Emission from ROSAT PSPC Pointed Observations
- Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
- SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 m and Data Release for the COSMOS Field
- Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
- When did round disk galaxies form?
- A NuSTAR and XMM-Newton Study of the Two Most Actively Star-forming Green Pea Galaxies (SDSS J0749+3337 and SDSS J0822+2241)
- The X-ray Zurich Environmental Study (X-ZENS). I. Chandra and XMM-Newton observations of AGNs in galaxies in nearby groups
- An Optically Faint Quasar Survey at z~5 in the CFHTLS Wide Field: Estimates of the Black Hole Masses and Eddington Ratios
- Host Galaxies of Hard X-ray Selected Type-2 Active Galactic Nuclei at Intermediate Redshifts
- Ultra High Energy Neutrinos: Absorption, Thermal Effects and Signatures
- Chandra Observations of Six QSOs at z 3
- The miniJPAS & J-NEP surveys: Identification and characterization of the Ly Emitter population and the Ly Luminosity Function
- Detecting quasars at very high redshift with next generation X-ray telescopes
- The Co-Evolution of Galaxies and Black Holes: Current Status and Future Prospects
- The optical luminosity function of LOFAR radio-selected quasars at in the NDWFS-Boötes field
- Measuring the Cosmic X-ray Background accurately
- The parallel lives of supermassive black holes and their host galaxies
- Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ~ 1.4
- The PAU Survey: The quasar UV and Ly luminosity functions at
- X-Ray Redshifts of Obscured Chandra Source Catalog AGN
- The Luminosity function of Narrow-Line Seyfert galaxies based on SDSS data
- Effects of large-scale magnetic fields on the observed composition of ultra high-energy cosmic rays
- Obscuration by Gas and Dust in Luminous Quasars
- Newly born extragalactic millisecond pulsars as efficient emitters of PeV neutrinos
- Supermassive black holes with higher Eddington ratios preferentially form in gas-rich galaxies
- The redshift distribution of the X-ray background
- Active Galactic Nuclei and their demography through cosmic time
- X-ray Sources in the SSA22 Chandra Field
- Systematic search for lensed X-ray sources in the CLASH fields
- Constraining the baryon loading factor of AGN jets: implication from the gamma-ray emission of the Coma cluster
- Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
- Fraction of the X-ray selected AGNs with optical emission lines in galaxy groups
- The X-ray-Infrared/Submillimetre Connection and the Legacy Era of Cosmology
- X-ray luminosity functions of different morphological and X-ray type AGN populations
- Diffuse flux of PeV neutrinos from centrifugally accelerated protons in active galactic nuclei
- X-Ray bright optically faint active galactic nuclei in the Subaru Hyper Suprime-Cam wide survey
- Obscured and unobscured X-ray AGNs I: Host galaxy properties
- Modeling the High-z Universe: Probing Galaxy Formation
- The Swift Serendipitous Survey in deep XRT GRB fields (SwiftFT) I. The X-ray catalog and number counts
- A New Method to Determine X-ray Luminosity Functions of AGN and their Evolution with Redshift
- BASS XXX: Distribution Functions of DR2 Eddington-ratios, Black Hole Masses, and X-ray Luminosities
- The Cosmogony of Super-Massive Black Holes
- Ultra high-energy cosmic rays from beyond the Greisen-Zatsepin-Kuz'min horizon
- Ultra-luminous high-redshift quasars from SkyMapper -- II. New quasars and the bright end of the luminosity function
- High-Energy Neutrino Production in Clusters of Galaxies
- The Gamma-ray Luminosity Function of Flat-Spectrum Radio Quasars
- SRG/eROSITA-SDSS view on the relation between X-ray and UV emission for quasars
- The Sensitivity of PUEO to Cosmogenic Neutrinos and Exotic Physics Scenarios
- The Drivers of the Decline in Supermassive Black Hole Growth at