Lista de obras - Benny Trakhtenbrot - Dominio Público Uruguay

A New Look at Quasar Accretion Disks

A model for AGN variability on multiple time-scales

A new catalog of type 1 AGNs and its implications on the AGN unified model ⬇️

article

A new class of flares from accreting supermassive black holes

artículo científico publicado en 2019

A new population of Compton-thick AGNs identified using the spectral curvature above 10 kev ⬇️

artículo científico publicado en 2016

A population of luminous accreting black holes with hidden mergers

artículo científico publicado en 2018

A view of the narrow-line region in the infrared: active galactic nuclei with resolved fine-structure lines in the Spitzer archive ⬇️

scientific article published in the Astrophysical Journal

AGN Evolution from the Galaxy Evolution Viewpoint. II

artículo científico publicado en 2018

AGN evolution from a galaxy evolution viewpoint ⬇️

scientific article published in the Astrophysical Journal

AGNs and Their Host Galaxies in the Local Universe: Two Mass-independent Eddington Ratio Distribution Functions Characterize Black Hole Growth

artículo científico publicado en 2017

ALMA Observations Show Major Mergers Among the Host Galaxies of Fast-growing, High-redshift, Supermassive Black Holes ⬇️

artículo científico publicado en 2017

ALMA Observations of Quasar Host Galaxies at <i>z</i> ≃ 4.8

artículo científico publicado en 2020

Active galactic nuclei at z ∼ 1.5 – I. Spectral energy distribution and accretion discs ⬇️

artículo científico publicado en 2014

Active galactic nuclei atz ∼ 1.5 – III. Accretion discs and black hole spin ⬇️

scholarly article by D. M. Capellupo et al published 21 April 2016 in Monthly Notices of the Royal Astronomical Society

Active galactic nuclei atz∼ 1.5 – II. Black hole mass estimation by means of broad emission lines ⬇️

scholarly article by J. E. Mejía-Restrepo et al published 28 March 2016 in Monthly Notices of the Royal Astronomical Society

Active galactic nucleus X-ray variability in the XMM-COSMOS survey ⬇️

artículo científico publicado en 2014

An FMOS Survey of Moderate-luminosity, Broad-line AGNs in COSMOS, SXDS, and E-CDF-S

artículo científico publicado en 2018

An over-massive black hole in a typical star-forming galaxy, 2 billion years after the Big Bang

artículo científico publicado en 2015

Author Correction: A population of luminous accreting black holes with hidden mergers

scientific article published on 01 April 2019

BASS XXXI: Outflow scaling relations in low redshift X-ray AGN host galaxies with MUSE

artículo científico publicado en 2022

BASS. XXIII. A New Mid-infrared Diagnostic for Absorption in Active Galactic Nuclei

artículo científico publicado en 2022

BASS. XXVIII. Near-infrared Data Release 2: High-ionization and Broad Lines in Active Galactic Nuclei*

artículo científico publicado en 2022

BASS. XXX. Distribution Functions of DR2 Eddington Ratios, Black Hole Masses, and X-Ray Luminosities

artículo científico publicado en 2022

BAT AGN Spectroscopic Survey (BASS) – VI. The ΓX–L/LEdd relation

artículo científico publicado en 2017

BAT AGN Spectroscopic Survey - IV: Near-Infrared Coronal Lines, Hidden Broad Lines, and Correlation with Hard X-ray Emission ⬇️

artículo científico publicado en 2017

BAT AGN Spectroscopic Survey – III. An observed link between AGN Eddington ratio and narrow-emission-line ratios ⬇️

artículo científico publicado en 2016

BAT AGN Spectroscopic Survey – XII. The relation between coronal properties of active galactic nuclei and the Eddington ratio

artículo científico publicado en 2018

BAT AGN Spectroscopic Survey – XIII. The nature of the most luminous obscured AGN in the low-redshift universe

scholarly article

BAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN Demographics

artículo científico publicado en 2017

BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog

article by Claudio Ricci et al published 5 December 2017 in The Astrophysical Journal Supplement Series

BAT AGN Spectroscopic Survey. VIII. Type 1 AGN with Massive Absorbing Columns

artículo científico publicado en 2018

BAT AGN Spectroscopic Survey. XI. The Covering Factor of Dust and Gas in Swift/BAT Active Galactic Nuclei

scientific article published in the Astrophysical Journal

BAT AGN spectroscopic survey - XV: the high frequency radio cores of ultra-hard X-ray selected AGN

artículo científico publicado en 2020

BAT AGN spectroscopic survey–II. X-ray emission and high-ionization optical emission lines ⬇️

article

Black Hole Mass and Growth Rate at High Redshift ⬇️

scientific article published in the Astrophysical Journal

Black hole growth to z = 2 - I. Improved virial methods for measuring MBH and L/LEdd

scholarly article by Benny Trakhtenbrot & H. Netzer published 21 December 2012 in Monthly Notices of the Royal Astronomical Society

Black hole mass and growth rate at z =~ 4.8: a short episode of fast growth followed by short duty cycle activity ⬇️

scientific article published in the Astrophysical Journal

Bolometric luminosity black hole growth time and slim accretion discs in active galactic nuclei

scholarly article by Hagai Netzer & Benny Trakhtenbrot published 14 December 2013 in Monthly Notices of the Royal Astronomical Society

Can we improve C iv-based single-epoch black hole mass estimations?

scholarly article by J E Mejía-Restrepo et al published 1 May 2018 in Monthly Notices of the Royal Astronomical Society

Compton thick AGN in the XMM-COSMOS survey ⬇️

artículo científico publicado en 2015

Compton-thick accretion in the local universe ⬇️

scholarly article

Cosmic Evolution of Mass Accretion Rate and Metallicity in Active Galactic Nuclei ⬇️

artículo científico publicado en 2007

Detection of rest-frame optical lines from X-shooter spectroscopy of weak emission line quasars ⬇️

artículo científico publicado en 2015

Detection of stellar light from quasar host galaxies at redshifts above 6

scientific article published on 28 June 2023

Determining the radio active galactic nuclei contribution to the radio–far-infrared correlation using the black hole Fundamental Plane relation ⬇️

scholarly article by O. Ivy Wong et al published 26 April 2016 in Monthly Notices of the Royal Astronomical Society

Discovery and follow-up of the unusual nuclear transient OGLE17aaj

artículo científico publicado en 2019

ERRATUM: “SCIENCE WITH A WIDE-FIELD UV TRANSIENT EXPLORER” (2014, AJ, 147, 79)

artículo científico publicado en 2014

Enhanced star formation in narrow-line Seyfert 1 active galactic nuclei revealed bySpitzer

scholarly article

Extreme star formation in the host galaxies of the fastest growing supermassive black holes at z = 4.8 ⬇️

scholarly article by Rivay Mor et al published 30 March 2012 in Letters of the Astrophysical Journal

Faint COSMOS AGNs at z~3.3. I. Black hole properties and constraints on early black hole growth ⬇️

artículo científico publicado en 2016

Fast-Growing SMBHs in Fast-Growing Galaxies, at High Redshifts: The Role of Major Mergers As Revealed by ALMA

scholarly article in Frontiers in Astronomy and Space Sciences, vol. 4, November 2017

Hot-dust clouds with pure-graphite composition around type-I active galactic nuclei ⬇️

article

Inferring Compton-thick AGN candidates at z > 2 with Chandra using the >8 keV rest-frame spectral curvature

scholarly article

On the Accretion Rates and Radiative Efficiencies of the Highest-redshift Quasars ⬇️

artículo científico publicado en 2017

Optical variability of AGNs in the PTF/iPTF survey ⬇️

artículo científico publicado en 2017

Pan-STARRS1 variability of XMM-COSMOS AGN ⬇️

artículo científico publicado en 2016

Probing the Evolution of Black Hole Mass Through Cosmic Time

scholarly article by Benny Trakhtenbrot et al published August 2009 in Proceedings of the International Astronomical Union

SDSS1133: an unusually persistent transient in a nearby dwarf galaxy ⬇️

scholarly article

Science with a wide-field UV transient explorer

artículo científico publicado en 2014

Star formation and black hole growth at z =~ 4.8 ⬇️

artículo científico publicado en 2014

Star formation black hole growth and dusty tori in the most luminous AGNs at z=2-3.5 ⬇️

artículo científico publicado en 2016

Testing the completeness of the SDSS colour selection for ultramassive, slowly spinning black holes ⬇️

scholarly article by Caroline Bertemes et al published 2 September 2016 in Monthly Notices of the Royal Astronomical Society

The 105-Month Swift-BAT All-sky Hard X-Ray Survey

artículo científico publicado en 2018

The Chandra COSMOS Legacy survey: clustering of X-ray-selected AGNs at 2.9 {\leq} z {\leq} 5.5 using photometric redshift probability distribution functions ⬇️

artículo científico publicado en 2016

The Chandra COSMOS legacy survey: optical/IR identifications ⬇️

scientific article published in the Astrophysical Journal

The Chandra COSMOS-Legacy survey: the z>3 sample ⬇️

artículo científico publicado en 2016

The Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-Ray Survey

artículo científico publicado en 2017

The Sloan Digital Sky Survey Reverberation Mapping Project: Investigation of Continuum Lag Dependence on Broad-line Contamination and Quasar Properties

artículo científico publicado en 2024

The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs

artículo científico publicado en 2018

The Virial Factor and Biases in Single Epoch Black Hole Mass Determinations

article

The close environments of accreting massive black holes are shaped by radiative feedback

artículo científico publicado en 2017

The complete infrared view of active galactic nuclei from the 70 month Swift/BAT catalog ⬇️

artículo científico publicado en 2017

The correlation of narrow line emission and X-ray luminosity in active galactic nuclei

artículo científico publicado en 2006

The detection rate of early UV emission from supernovae: a dedicated Galex/PTF survey and calibrated theoretical estimates ⬇️

artículo científico publicado en 2016

The effect of nuclear gas distribution on the mass determination of supermassive black holes

The evolution of M*/MBH between z= 2 and z= 0

The fraction of AGNs in major merger galaxies and its luminosity dependence

artículo científico publicado en 2018

The mean star-forming properties of QSO host galaxies

artículo científico publicado en 2013

The most massive active black holes at z ~ 1.5-3.5 have high spins and radiative efficiencies ⬇️

scholarly article by Benny Trakhtenbrot published 13 June 2014 in Letters of the Astrophysical Journal

The search for active black holes in nearby low-mass galaxies using optical and mid-IR data ⬇️

scholarly article by Lia F. Sartori et al published 20 October 2015 in Monthly Notices of the Royal Astronomical Society

The systematic search for z ≳ 5 active galactic nuclei in the Chandra Deep Field South ⬇️

artículo científico publicado en 2015

Tracing the rise of supermassive black holes

artículo científico publicado en 2024

Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching

artículo científico publicado en 2017

Weak line quasars at high redshift: extremely high accretion rates or anemic broad-line regions? ⬇️

[O iii]λ5007 AND X-RAY PROPERTIES OF A COMPLETE SAMPLE OF HARD X-RAY SELECTED AGNs IN THE LOCAL UNIVERSE ⬇️

artículo científico publicado en 2015

Lista de obras de Benny Trakhtenbrot

A New Look at Quasar Accretion Disks

A model for AGN variability on multiple time-scales

A new catalog of type 1 AGNs and its implications on the AGN unified model ⬇️

A new class of flares from accreting supermassive black holes

A new population of Compton-thick AGNs identified using the spectral curvature above 10 kev ⬇️

A population of luminous accreting black holes with hidden mergers

A view of the narrow-line region in the infrared: active galactic nuclei with resolved fine-structure lines in the Spitzer archive ⬇️

AGN Evolution from the Galaxy Evolution Viewpoint. II

AGN evolution from a galaxy evolution viewpoint ⬇️

AGNs and Their Host Galaxies in the Local Universe: Two Mass-independent Eddington Ratio Distribution Functions Characterize Black Hole Growth

ALMA Observations Show Major Mergers Among the Host Galaxies of Fast-growing, High-redshift, Supermassive Black Holes ⬇️

ALMA Observations of Quasar Host Galaxies at <i>z</i> ≃ 4.8

Active galactic nuclei at z ∼ 1.5 – I. Spectral energy distribution and accretion discs ⬇️

Active galactic nuclei atz ∼ 1.5 – III. Accretion discs and black hole spin ⬇️

Active galactic nuclei atz∼ 1.5 – II. Black hole mass estimation by means of broad emission lines ⬇️

Active galactic nucleus X-ray variability in the XMM-COSMOS survey ⬇️

An FMOS Survey of Moderate-luminosity, Broad-line AGNs in COSMOS, SXDS, and E-CDF-S

An over-massive black hole in a typical star-forming galaxy, 2 billion years after the Big Bang

Author Correction: A population of luminous accreting black holes with hidden mergers

BASS XXXI: Outflow scaling relations in low redshift X-ray AGN host galaxies with MUSE

BASS. XXIII. A New Mid-infrared Diagnostic for Absorption in Active Galactic Nuclei

BASS. XXVIII. Near-infrared Data Release 2: High-ionization and Broad Lines in Active Galactic Nuclei*

BASS. XXX. Distribution Functions of DR2 Eddington Ratios, Black Hole Masses, and X-Ray Luminosities

BAT AGN Spectroscopic Survey (BASS) – VI. The ΓX–L/LEdd relation

BAT AGN Spectroscopic Survey - IV: Near-Infrared Coronal Lines, Hidden Broad Lines, and Correlation with Hard X-ray Emission ⬇️

BAT AGN Spectroscopic Survey – III. An observed link between AGN Eddington ratio and narrow-emission-line ratios ⬇️

BAT AGN Spectroscopic Survey – XII. The relation between coronal properties of active galactic nuclei and the Eddington ratio

BAT AGN Spectroscopic Survey – XIII. The nature of the most luminous obscured AGN in the low-redshift universe

BAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN Demographics

BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog

BAT AGN Spectroscopic Survey. VIII. Type 1 AGN with Massive Absorbing Columns

BAT AGN Spectroscopic Survey. XI. The Covering Factor of Dust and Gas in Swift/BAT Active Galactic Nuclei

BAT AGN spectroscopic survey - XV: the high frequency radio cores of ultra-hard X-ray selected AGN

BAT AGN spectroscopic survey–II. X-ray emission and high-ionization optical emission lines ⬇️

Black Hole Mass and Growth Rate at High Redshift ⬇️

Black hole growth to z = 2 - I. Improved virial methods for measuring MBH and L/LEdd

Black hole mass and growth rate at z =~ 4.8: a short episode of fast growth followed by short duty cycle activity ⬇️

Bolometric luminosity black hole growth time and slim accretion discs in active galactic nuclei

Can we improve C iv-based single-epoch black hole mass estimations?

Compton thick AGN in the XMM-COSMOS survey ⬇️

Compton-thick accretion in the local universe ⬇️

Cosmic Evolution of Mass Accretion Rate and Metallicity in Active Galactic Nuclei ⬇️

Detection of rest-frame optical lines from X-shooter spectroscopy of weak emission line quasars ⬇️

Detection of stellar light from quasar host galaxies at redshifts above 6

Determining the radio active galactic nuclei contribution to the radio–far-infrared correlation using the black hole Fundamental Plane relation ⬇️

Discovery and follow-up of the unusual nuclear transient OGLE17aaj

ERRATUM: “SCIENCE WITH A WIDE-FIELD UV TRANSIENT EXPLORER” (2014, AJ, 147, 79)

Enhanced star formation in narrow-line Seyfert 1 active galactic nuclei revealed bySpitzer

Extreme star formation in the host galaxies of the fastest growing supermassive black holes at z = 4.8 ⬇️

Faint COSMOS AGNs at z~3.3. I. Black hole properties and constraints on early black hole growth ⬇️

Fast-Growing SMBHs in Fast-Growing Galaxies, at High Redshifts: The Role of Major Mergers As Revealed by ALMA

Hot-dust clouds with pure-graphite composition around type-I active galactic nuclei ⬇️

Inferring Compton-thick AGN candidates at z > 2 with Chandra using the >8 keV rest-frame spectral curvature

On the Accretion Rates and Radiative Efficiencies of the Highest-redshift Quasars ⬇️

Optical variability of AGNs in the PTF/iPTF survey ⬇️

Pan-STARRS1 variability of XMM-COSMOS AGN ⬇️

Probing the Evolution of Black Hole Mass Through Cosmic Time

SDSS1133: an unusually persistent transient in a nearby dwarf galaxy ⬇️

Science with a wide-field UV transient explorer

Star formation and black hole growth at z =~ 4.8 ⬇️

Star formation black hole growth and dusty tori in the most luminous AGNs at z=2-3.5 ⬇️

Testing the completeness of the SDSS colour selection for ultramassive, slowly spinning black holes ⬇️

The 105-Month Swift-BAT All-sky Hard X-Ray Survey

The Chandra COSMOS Legacy survey: clustering of X-ray-selected AGNs at 2.9 {\leq} z {\leq} 5.5 using photometric redshift probability distribution functions ⬇️

The Chandra COSMOS legacy survey: optical/IR identifications ⬇️

The Chandra COSMOS-Legacy survey: the z>3 sample ⬇️

The Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-Ray Survey

The Sloan Digital Sky Survey Reverberation Mapping Project: Investigation of Continuum Lag Dependence on Broad-line Contamination and Quasar Properties

The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs

The Virial Factor and Biases in Single Epoch Black Hole Mass Determinations

The close environments of accreting massive black holes are shaped by radiative feedback

The complete infrared view of active galactic nuclei from the 70 month Swift/BAT catalog ⬇️

The correlation of narrow line emission and X-ray luminosity in active galactic nuclei

The detection rate of early UV emission from supernovae: a dedicated Galex/PTF survey and calibrated theoretical estimates ⬇️

The effect of nuclear gas distribution on the mass determination of supermassive black holes

The evolution of M*/MBH between z= 2 and z= 0

The fraction of AGNs in major merger galaxies and its luminosity dependence

The mean star-forming properties of QSO host galaxies

The most massive active black holes at z ~ 1.5-3.5 have high spins and radiative efficiencies ⬇️