Lista de obras - Elisabeta Lusso - Dominio Público Uruguay

A runaway black hole in COSMOS: gravitational wave or slingshot recoil? ⬇️

artículo científico publicado en 2010

A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys

artículo científico publicado en 2013

AGNfitter: A BAYESIAN MCMC APPROACH TO FITTING SPECTRAL ENERGY DISTRIBUTIONS OF AGNs ⬇️

artículo científico publicado en 2016

Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies

scholarly article by Angela Bongiorno et al published 21 December 2012 in Monthly Notices of the Royal Astronomical Society

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

artículo científico publicado en 2014

Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS

artículo científico publicado en 2011

Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey

artículo científico publicado en 2012

Compton thick AGN in the XMM-COSMOS survey ⬇️

artículo científico publicado en 2015

Cosmological test with the QSO Hubble diagram ⬇️

ERRATUM: “THE OBSCURED FRACTION OF ACTIVE GALACTIC NUCLEI IN THE XMM-COSMOS SURVEY: A SPECTRAL ENERGY DISTRIBUTION PERSPECTIVE” (2013, ApJ, 777, 86)

scientific article published in the Astrophysical Journal

Erratum: “X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range” (2018, ApJ, 859, 65)

artículo científico publicado en 2018

Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP

artículo científico publicado en 2024

Evidence for feedback in action from the molecular gas content in thez~ 1.6 outflowing QSO XID2028 ⬇️

artículo científico publicado en 2015

Fe K emission from active galaxies in the COSMOS field

artículo científico publicado en 2012

Fitting Spectral Energy Distributions of AGN A Markov Chain Monte Carlo Approach

Fundamental differences in the radio properties of red and blue quasars: evolution strongly favoured over orientation

artículo científico publicado en 2019

GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection

artículo científico publicado en 2012

Galaxy-wide outflows inz~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy ⬇️

scientific article published in Astronomy and Astrophysics

Hot-dust-poor type 1 active galactic nuclei in the COSMOS survey ⬇️

scholarly article

Is there any evidence that ionized outflows quench star formation in type 1 quasars atz< 1? ⬇️

article

On the cosmic evolution of the scaling relations between black holes and their host galaxies: broad-line active galactic nuclei in the zCOSMOS survey ⬇️

artículo científico publicado en 2009

Spectral energy distributions of type 1 active galactic nuclei in the COSMOS survey. I. The XMM-COSMOS sample ⬇️

scientific article published in the Astrophysical Journal

The Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sources

The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS

artículo científico publicado en 2010

The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei ⬇️

artículo científico publicado en 2010

The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey

artículo científico publicado en 2011

The bulk of the black hole growth since z ~ 1 occurs in a secular universe: no Major Merger-AGN connection ⬇️

artículo científico publicado en 2010

The first ultraviolet quasar-stacked spectrum at z ≃ 2.4 from WFC3 ⬇️

artículo científico publicado en 2015

The incidence of obscuration in active galactic nuclei

artículo científico publicado en 2013

The mean star-forming properties of QSO host galaxies

artículo científico publicado en 2013

The nature of massive black hole binary candidates – I. Spectral properties and evolution

scholarly article by Roberto Decarli et al published 4 June 2013 in Monthly Notices of the Royal Astronomical Society

The nature of massive black hole binary candidates – II. Spectral energy distribution atlas ⬇️

scholarly article by Elisabeta Lusso et al published 24 April 2014 in Monthly Notices of the Royal Astronomical Society

The obscured fraction of active galactic nuclei in the XMM-COSMOS survey: a spectral energy distribution perspective ⬇️

artículo científico publicado en 2013

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

artículo científico publicado en 2017

X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects ⬇️

artículo científico publicado en 2014

Lista de obras de Elisabeta Lusso

A runaway black hole in COSMOS: gravitational wave or slingshot recoil? ⬇️

A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys

AGNfitter: A BAYESIAN MCMC APPROACH TO FITTING SPECTRAL ENERGY DISTRIBUTIONS OF AGNs ⬇️

Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies

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

Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS

Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey

Compton thick AGN in the XMM-COSMOS survey ⬇️

Cosmological test with the QSO Hubble diagram ⬇️

ERRATUM: “THE OBSCURED FRACTION OF ACTIVE GALACTIC NUCLEI IN THE XMM-COSMOS SURVEY: A SPECTRAL ENERGY DISTRIBUTION PERSPECTIVE” (2013, ApJ, 777, 86)

Erratum: “X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the <i>Chandra</i> Archive in the 0.2 < <i>z</i> < 0.3 and 0.55 < <i>z</i> < 0.75 Redshift Range” (2018, ApJ, 859, 65)

Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP

Evidence for feedback in action from the molecular gas content in thez~ 1.6 outflowing QSO XID2028 ⬇️

Fe K emission from active galaxies in the COSMOS field

Fitting Spectral Energy Distributions of AGN A Markov Chain Monte Carlo Approach

Fundamental differences in the radio properties of red and blue quasars: evolution strongly favoured over orientation

GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection

Galaxy-wide outflows inz~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy ⬇️

Hot-dust-poor type 1 active galactic nuclei in the COSMOS survey ⬇️

Is there any evidence that ionized outflows quench star formation in type 1 quasars atz< 1? ⬇️

On the cosmic evolution of the scaling relations between black holes and their host galaxies: broad-line active galactic nuclei in the zCOSMOS survey ⬇️

Spectral energy distributions of type 1 active galactic nuclei in the COSMOS survey. I. The XMM-COSMOS sample ⬇️

The Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sources

The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS

The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei ⬇️

The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey

The bulk of the black hole growth since z ~ 1 occurs in a secular universe: no Major Merger-AGN connection ⬇️

The first ultraviolet quasar-stacked spectrum at z ≃ 2.4 from WFC3 ⬇️

The incidence of obscuration in active galactic nuclei

The mean star-forming properties of QSO host galaxies

The nature of massive black hole binary candidates – I. Spectral properties and evolution

The nature of massive black hole binary candidates – II. Spectral energy distribution atlas ⬇️

The obscured fraction of active galactic nuclei in the XMM-COSMOS survey: a spectral energy distribution perspective ⬇️

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

X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects ⬇️

Lista de obras de Elisabeta Lusso

A runaway black hole in COSMOS: gravitational wave or slingshot recoil? ⬇️

A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys

AGNfitter: A BAYESIAN MCMC APPROACH TO FITTING SPECTRAL ENERGY DISTRIBUTIONS OF AGNs ⬇️

Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies

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

Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS

Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey

Compton thick AGN in the XMM-COSMOS survey ⬇️

Cosmological test with the QSO Hubble diagram ⬇️

ERRATUM: “THE OBSCURED FRACTION OF ACTIVE GALACTIC NUCLEI IN THE XMM-COSMOS SURVEY: A SPECTRAL ENERGY DISTRIBUTION PERSPECTIVE” (2013, ApJ, 777, 86)

Erratum: “X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the <i>Chandra</i> Archive in the 0.2 &lt; <i>z</i> &lt; 0.3 and 0.55 &lt; <i>z</i> &lt; 0.75 Redshift Range” (2018, ApJ, 859, 65)

Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP

Evidence for feedback in action from the molecular gas content in thez~ 1.6 outflowing QSO XID2028 ⬇️

Fe K emission from active galaxies in the COSMOS field

Fitting Spectral Energy Distributions of AGN A Markov Chain Monte Carlo Approach

Fundamental differences in the radio properties of red and blue quasars: evolution strongly favoured over orientation

GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection

Galaxy-wide outflows inz~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy ⬇️

Hot-dust-poor type 1 active galactic nuclei in the COSMOS survey ⬇️

Is there any evidence that ionized outflows quench star formation in type 1 quasars atz< 1? ⬇️

On the cosmic evolution of the scaling relations between black holes and their host galaxies: broad-line active galactic nuclei in the zCOSMOS survey ⬇️

Spectral energy distributions of type 1 active galactic nuclei in the COSMOS survey. I. The XMM-COSMOS sample ⬇️

The Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sources

The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS

The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei ⬇️

The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey

The bulk of the black hole growth since z ~ 1 occurs in a secular universe: no Major Merger-AGN connection ⬇️

The first ultraviolet quasar-stacked spectrum at z ≃ 2.4 from WFC3 ⬇️

The incidence of obscuration in active galactic nuclei

The mean star-forming properties of QSO host galaxies

The nature of massive black hole binary candidates – I. Spectral properties and evolution

The nature of massive black hole binary candidates – II. Spectral energy distribution atlas ⬇️

The obscured fraction of active galactic nuclei in the XMM-COSMOS survey: a spectral energy distribution perspective ⬇️

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

X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects ⬇️

Erratum: “X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the <i>Chandra</i> Archive in the 0.2 < <i>z</i> < 0.3 and 0.55 < <i>z</i> < 0.75 Redshift Range” (2018, ApJ, 859, 65)