High-redshift AGN in the Chandra Deep Fields : The obscured fraction and space density of the sub-L * population
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- Type
- article
- Published
- 2017-09-22
- Cited by
- 103
- References
- 133
- Access
- Open access
- OpenAlex
- https://openalex.org/W2760203217
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:56563085
Keywords
Physics, Astrophysics, Redshift, Galaxy, Luminosity
References
- THE SLOAN DIGITAL SKY SURVEY/XMM-NEWTON QUASAR SURVEY: CORRELATION BETWEEN X-RAY SPECTRAL SLOPE AND EDDINGTON RATIO
- Beyond Chandra: the x-ray Surveyor
- Astronomical Data Analysis Software and Systems V
- COSMIC REIONIZATION AFTER PLANCK: COULD QUASARS DO IT ALL?
- THE RELATION BETWEEN STAR FORMATION RATE AND STELLAR MASS FOR GALAXIES AT 3.5 ⩽ z ⩽ 6.5 IN CANDELS
- The largest X-ray-selected sample of z>3 AGNs: C-COSMOS and ChaMP
- The formation and growth of the earliest supermassive black holes
- The Illustris simulation: the evolving population of black holes across cosmic time
- THREE-YEAR SWIFT–BAT SURVEY OF ACTIVE GALACTIC NUCLEI: RECONCILING THEORY AND OBSERVATIONS?
- THE POPULATION OF HIGH-REDSHIFT ACTIVE GALACTIC NUCLEI IN THE CHANDRA-COSMOS SURVEY
- Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in the XMM-COSMOS survey
- The high-redshift (z > 3) active galactic nucleus population in the 4-Ms Chandra Deep Field-South
- Frequentism and Bayesianism: A Python-driven Primer
- The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z ~ 5
- The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS
- An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30
- THE STAR FORMATION RATE FUNCTION FOR REDSHIFT z ∼ 4–7 GALAXIES: EVIDENCE FOR A UNIFORM BUILDUP OF STAR-FORMING GALAXIES DURING THE FIRST 3 Gyr OF COSMIC TIME
- OBSCURATION-DEPENDENT EVOLUTION OF ACTIVE GALACTIC NUCLEI
- A luminous quasar at a redshift of z = 7.085
- The X-Ray Spectral Properties and Variability of Luminous High-Redshift Active Galactic Nuclei
Cited by
- Linking black hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution
- Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification
- BlueTides simulation: establishing black hole−galaxy relations at high redshift
- The 500 ks Chandra observation of the z = 6.31 QSO SDSS J1030 + 0524
- New synthesis models of consistent extragalactic background light over cosmic time
- “Super-deblended” Dust Emission in Galaxies. II. Far-IR to (Sub)millimeter Photometry and High-redshift Galaxy Candidates in the Full COSMOS Field
- The role of AGN jets in the reionization epoch
- Variability-selected Low-luminosity Active Galactic Nuclei Candidates in the 7 Ms Chandra Deep Field-South
- Abundant serendipitous emission line sources with JWST/NIRSpec
- Black hole obscuration and duty-cycles mediated by AGN feedback in high-redshift galaxies
- The space density ofz > 4 blazars
- X-ray emission of z > 2.5 active galactic nuclei can be obscured by their host galaxies
- The Advanced X-ray Imaging Satellite
- The advanced telescope for high energy astrophysics
- Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. I. X-Ray Spectral and Long-term Variability Analyses
- The hierarchical assembly of galaxies and black holes in the first billion years: predictions for the era of gravitational wave astronomy
- Evidence for Low Radiative Efficiency or Highly Obscured Growth of z > 7 Quasars
- Tracing black hole and galaxy co-evolution in the Romulus simulations
- Space Densities and Emissivities of Active Galactic Nuclei at z > 4
- The Galaxy’s Gas Content Regulated by the Dark Matter Halo Mass Results in a Superlinear MBH–M⋆ Relation
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