Lista de obras - Roberto Gilli - Dominio Público Uruguay

A Classic Type 2 QSO ⬇️

artículo científico publicado en 2002

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

artículo científico publicado en 2011

ChandraDeep Field South: The 1 Ms Catalog

scholarly article

Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy atz= 1.7: star formation promoted by large-scale AGN feedback?

artículo científico publicado en 2019

EXTraS discovery of an X-ray superflare from an L dwarf

artículo científico publicado en 2020

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

Magnifying the Early Episodes of Star Formation: Super Star Clusters at Cosmological Distances

scientific article published in the Astrophysical Journal

Massive star cluster formation under the microscope at z = 6

scholarly article

Probing black hole accretion in quasar pairs at high redshift

scholarly article by C Vignali et al published 15 March 2018 in Monthly Notices of the Royal Astronomical Society

RADIO LOUD AGNs ARE MERGERS ⬇️

scientific article published in the Astrophysical Journal

Rolling down from the 30 keV peak: Modelling the Hard X-Ray and γ-Ray Backgrounds

Rolling down from the 30 keV peak: Modelling the hard X-ray and γ-ray backgrounds

Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies’ interstellar medium

scientific article published in 2022

The 2–10 keV unabsorbed luminosity function of AGN from the LSS, CDFS, and COSMOS surveys ⬇️

artículo científico publicado en 2016

The Chandra COSMOS survey. I. Overview and point source catalog

article

The Chandra-COSMOS survey – IV. X-ray spectra of the bright sample

artículo científico publicado en 2013

The Extended Chandra Deep Field-South survey: optical spectroscopy of faint X-ray sources with the VLT and Keck

scholarly article

The Iron Line Background ⬇️

artículo científico publicado en 2005

The X‐Ray–derived Cosmological Star Formation History and the Galaxy X‐Ray Luminosity Functions in the Chandra Deep Fields North and South ⬇️

artículo científico publicado en 2004

The cosmic reality check

scientific article published on 01 March 2002

The evolution of obscured accretion

The most obscured AGN in the COSMOS field

scientific article published in Astronomy and Astrophysics

The spatial distribution of X-ray selected AGN in theChandradeep fields: a theoretical perspective

artículo científico publicado en 2009

TheXMM‐NewtonWide‐Field Survey in the COSMOS Field. V. Angular Clustering of the X‐Ray Point Sources

scholarly article

Ultraluminous X-ray sources out to z ~ 0.3 in the COSMOS field

scientific article published in Astronomy and Astrophysics

Understanding the X-ray background after the deep surveys

artículo científico publicado en 2003

Unresolved z ∼ 8 Point Sources and Their Impact on the Bright End of the Galaxy Luminosity Function

artículo científico publicado en 2022

X-Ray Spectral Analyses of AGNs from the 7Ms Chandra Deep Field-South Survey: The Distribution, Variability, and Evolutions of AGN Obscuration

article

X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field

artículo científico publicado en 2018

XEUS: the physics of the hot evolving universe

artículo científico publicado en 2008

Lista de obras de Roberto Gilli

A Classic Type 2 QSO ⬇️

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

ChandraDeep Field South: The 1 Ms Catalog

Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at<i>z</i>= 1.7: star formation promoted by large-scale AGN feedback?

EXTraS discovery of an X-ray superflare from an L dwarf

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)

Magnifying the Early Episodes of Star Formation: Super Star Clusters at Cosmological Distances

Massive star cluster formation under the microscope at z = 6

Probing black hole accretion in quasar pairs at high redshift

RADIO LOUD AGNs ARE MERGERS ⬇️

Rolling down from the 30 keV peak: Modelling the Hard X-Ray and γ-Ray Backgrounds

Rolling down from the 30 keV peak: Modelling the hard X-ray and γ-ray backgrounds

Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies’ interstellar medium

The 2–10 keV unabsorbed luminosity function of AGN from the LSS, CDFS, and COSMOS surveys ⬇️

The Chandra COSMOS survey. I. Overview and point source catalog

The Chandra-COSMOS survey – IV. X-ray spectra of the bright sample

The Extended Chandra Deep Field-South survey: optical spectroscopy of faint X-ray sources with the VLT and Keck

The Iron Line Background ⬇️

The X‐Ray–derived Cosmological Star Formation History and the Galaxy X‐Ray Luminosity Functions in the Chandra Deep Fields North and South ⬇️

The cosmic reality check

The evolution of obscured accretion

The most obscured AGN in the COSMOS field

The spatial distribution of X-ray selected AGN in theChandradeep fields: a theoretical perspective

TheXMM‐NewtonWide‐Field Survey in the COSMOS Field. V. Angular Clustering of the X‐Ray Point Sources

Ultraluminous X-ray sources out to z ~ 0.3 in the COSMOS field

Understanding the X-ray background after the deep surveys

Unresolved z ∼ 8 Point Sources and Their Impact on the Bright End of the Galaxy Luminosity Function

X-Ray Spectral Analyses of AGNs from the 7Ms Chandra Deep Field-South Survey: The Distribution, Variability, and Evolutions of AGN Obscuration

X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field

XEUS: the physics of the hot evolving universe

Lista de obras de Roberto Gilli

A Classic Type 2 QSO ⬇️

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

ChandraDeep Field South: The 1 Ms Catalog

Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at<i>z</i>= 1.7: star formation promoted by large-scale AGN feedback?

EXTraS discovery of an X-ray superflare from an L dwarf

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)

Magnifying the Early Episodes of Star Formation: Super Star Clusters at Cosmological Distances

Massive star cluster formation under the microscope at z = 6

Probing black hole accretion in quasar pairs at high redshift

RADIO LOUD AGNs ARE MERGERS ⬇️

Rolling down from the 30 keV peak: Modelling the Hard X-Ray and γ-Ray Backgrounds

Rolling down from the 30 keV peak: Modelling the hard X-ray and γ-ray backgrounds

Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies’ interstellar medium

The 2–10 keV unabsorbed luminosity function of AGN from the LSS, CDFS, and COSMOS surveys ⬇️

The Chandra COSMOS survey. I. Overview and point source catalog

The Chandra-COSMOS survey – IV. X-ray spectra of the bright sample

The Extended Chandra Deep Field-South survey: optical spectroscopy of faint X-ray sources with the VLT and Keck

The Iron Line Background ⬇️

The X‐Ray–derived Cosmological Star Formation History and the Galaxy X‐Ray Luminosity Functions in the Chandra Deep Fields North and South ⬇️

The cosmic reality check

The evolution of obscured accretion

The most obscured AGN in the COSMOS field

The spatial distribution of X-ray selected AGN in theChandradeep fields: a theoretical perspective

TheXMM‐NewtonWide‐Field Survey in the COSMOS Field. V. Angular Clustering of the X‐Ray Point Sources

Ultraluminous X-ray sources out to z ~ 0.3 in the COSMOS field

Understanding the X-ray background after the deep surveys

Unresolved z ∼ 8 Point Sources and Their Impact on the Bright End of the Galaxy Luminosity Function

X-Ray Spectral Analyses of AGNs from the 7Ms Chandra Deep Field-South Survey: The Distribution, Variability, and Evolutions of AGN Obscuration

X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field

XEUS: the physics of the hot evolving universe

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)