about
The close environments of accreting massive black holes are shaped by radiative feedback.An over-massive black hole in a typical star-forming galaxy, 2 billion years after the Big BangA view of the narrow-line region in the infrared: active galactic nuclei with resolved fine-structure lines in the Spitzer archiveBAT AGN Spectroscopic Survey – XII. The relation between coronal properties of active galactic nuclei and the Eddington ratioBAT AGN Spectroscopic Survey. VIII. Type 1 AGN with Massive Absorbing ColumnsDetermining the radio active galactic nuclei contribution to the radio–far-infrared correlation using the black hole Fundamental Plane relationThe Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNsA population of luminous accreting black holes with hidden mergersA model for AGN variability on multiple time-scalesThe fraction of AGNs in major merger galaxies and its luminosity dependenceBAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN CatalogBAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN DemographicsInferring Compton-thick AGN candidates at z > 2 with Chandra using the >8 keV rest-frame spectral curvatureThe Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-Ray SurveyBAT AGN Spectroscopic Survey (BASS) – VI. The ΓX–L/LEdd relationAGNs and Their Host Galaxies in the Local Universe: Two Mass-independent Eddington Ratio Distribution Functions Characterize Black Hole GrowthBAT AGN Spectroscopic Survey - IV: Near-Infrared Coronal Lines, Hidden Broad Lines, and Correlation with Hard X-ray EmissionBAT AGN Spectroscopic Survey – III. An observed link between AGN Eddington ratio and narrow-emission-line ratiosThe Chandra COSMOS-Legacy survey: the z>3 sampleA new population of Compton-thick AGNs identified using the spectral curvature above 10 kevThe Chandra COSMOS legacy survey: optical/IR identificationsBAT AGN spectroscopic survey–II. X-ray emission and high-ionization optical emission linesThe search for active black holes in nearby low-mass galaxies using optical and mid-IR dataThe systematic search for z ≳ 5 active galactic nuclei in the Chandra Deep Field SouthCompton thick AGN in the XMM-COSMOS surveyCompton-thick accretion in the local universeThe Chandra COSMOS Legacy survey: clustering of X-ray-selected AGNs at 2.9 {\leq} z {\leq} 5.5 using photometric redshift probability distribution functionsThe mean star-forming properties of QSO host galaxiesActive galactic nucleus X-ray variability in the XMM-COSMOS surveyFaint COSMOS AGNs at z~3.3. I. Black hole properties and constraints on early black hole growthThe 105-Month Swift-BAT All-sky Hard X-Ray SurveyType 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven QuenchingTesting the completeness of the SDSS colour selection for ultramassive, slowly spinning black holesA new catalog of type 1 AGNs and its implications on the AGN unified modelSDSS1133: an unusually persistent transient in a nearby dwarf galaxyAGN Evolution from the Galaxy Evolution Viewpoint. IICan we improve C iv-based single-epoch black hole mass estimations?The effect of nuclear gas distribution on the mass determination of supermassive black holesThe Virial Factor and Biases in Single Epoch Black Hole Mass DeterminationsFast-Growing SMBHs in Fast-Growing Galaxies, at High Redshifts: The Role of Major Mergers As Revealed by ALMA
P50
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P50
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B. Trakhtenbrot
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Benny Trakhtenbrot
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Benny Trakhtenbrot
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P214
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