Lista de obras - Ivan Delvecchio - Dominio Público Uruguay

(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies ⬇️

artículo científico publicado en 2016

(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. IV. Physical properties derived from spectral energy distributions ⬇️

artículo científico publicado en 2016

A fast ionised wind in a star-forming quasar system atz~ 1.5 resolved through adaptive optics assisted near-infrared data ⬇️

artículo científico publicado en 2016

ALMA view of a massive spheroid progenitor: a compact rotating core of molecular gas in an AGN host at z = 2.226

scholarly article

Active galactic nuclei in dusty starbursts at z = 2: feedback still to kick in ⬇️

artículo científico publicado en 2019

Active galactic nuclei vs. host galaxy properties in the COSMOS field

artículo científico publicado en 2017

An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution

artículo científico publicado en 2017

An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling

artículo científico publicado en 2017

An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array

artículo científico publicado en 2017

An Eddington ratio-driven origin for the LX − M* relation in quiescent and star-forming active galaxies

artículo científico publicado en 2022

Compton thick AGN in the XMM-COSMOS survey ⬇️

artículo científico publicado en 2015

Constraints on submicrojansky radio number counts based on evolving VLA-COSMOS luminosity functions

artículo científico publicado en 2018

Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies at z ∼ 0.7

scholarly article

Erratum: The Herschel PEP/HerMES Luminosity Function – I. Probing the Evolution of PACS selected Galaxies to z ≃ 4

scholarly article published in Monthly Notices of the Royal Astronomical Society

Herschel far-IR counterparts of SDSS galaxies: analysis of commonly used star formation rate estimates ⬇️

article

Linear radio size evolution of μJy populations

scientific article published in Astronomy and Astrophysics

Mapping the average AGN accretion rate in the SFR–M* plane for Herschel★-selected galaxies at 0 < z ≤ 2.5 ⬇️

artículo científico publicado en 2015

Merger induced clump formation in distant infrared luminous starburst galaxies

artículo científico publicado en 2019

On the Kennicutt-Schmidt scaling law of submillimetre galaxies

artículo científico publicado en 2017

Optical and mid-infrared line emission in nearby Seyfert galaxies

artículo científico publicado en 2023

Probing black hole accretion tracks, scaling relations, and radiative efficiencies from stacked X-ray active galactic nuclei

artículo científico publicado en 2019

Radio Selection of the Most Distant Galaxy Clusters ⬇️

scholarly article

Relationship between star formation rate and black hole accretion at z = 2: the different contributions in quiescent, normal, and starburst galaxies ⬇️

scholarly article by Rodighiero G. et al published 10 February 2015 in Letters of the Astrophysical Journal

SINFONI spectra of heavily obscured AGNs in COSMOS: Evidence of outflows in a MIR/O target atz~ 2.5 ⬇️

scientific article published in Astronomy and Astrophysics

SMBH accretion properties of radio-selected AGN out to z ∼ 4

artículo científico publicado en 2018

Star formation inHerschel's Monsters versus semi-analytic models

artículo científico publicado en 2015

The AGN content in luminous infrared galaxies at z∼ 2 from a global SED analysis including Herschel data

artículo científico publicado en 2012

The COSMOS2015 galaxy stellar mass function. Thirteen billion years of stellar mass assembly in ten snapshots

artículo científico publicado en 2017

The Evolving Interstellar Medium of Star-forming Galaxies, as Traced by Stardust*

artículo científico publicado en 2021

The Herschel PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4

artículo científico publicado en 2013

The Typical Massive Quiescent Galaxy at z ∼ 3 is a Post-starburst

artículo científico publicado en 2020

The VIMOS Ultra-Deep Survey: Emerging from the dark, a massive proto-cluster at z ~ 4.57

scholarly article

The VLA-COSMOS 3 GHz Large Project: AGN and host-galaxy properties out to z ≲ 6

artículo científico publicado en 2017

The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of highly star-forming galaxies

scholarly article

The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release

artículo científico publicado en 2017

The VLA-COSMOS 3 GHz Large Project: Cosmic evolution of radio AGN and implications for radio-mode feedback since z~ 5

artículo científico publicado en 2017

The VLA-COSMOS 3 GHz Large Project: Cosmic star formation history since z ~ 5

artículo científico publicado en 2017

The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population

artículo científico publicado en 2017

The VLA-COSMOS 3 GHz Large Project: Star formation properties and radio luminosity functions of AGN with moderate-to-high radiative luminosities out to z~ 6

scholarly article

The VLA-COSMOS 3 GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to z ≲ 6

artículo científico publicado en 2017

The XXL Survey

The XXL Survey. XXI. The environment and clustering of X-ray AGN in the XXL-South field

artículo científico publicado en 2018

The XXL Survey. XXXI. Classification and host galaxy properties of 2.1 GHz ATCA XXL-S radio sources

artículo científico publicado en 2018

The XXL survey: First results and future

The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field

artículo científico publicado en 2018

The effect of active galactic nuclei on the cold interstellar medium in distant star-forming galaxies

scientific article published in 2021

The faint radio sky: VLBA observations of the COSMOS field

artículo científico publicado en 2017

The infrared-radio correlation of star-forming galaxies is stronglyM⋆-dependent but nearly redshift-invariant sincez∼ 4

scientific article published in 2021

The main sequence at z ~ 1.3 contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts? ⬇️

artículo científico publicado en 2019

The most obscured AGN in the COSMOS field

scientific article published in Astronomy and Astrophysics

Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel ⬇️

scholarly article by Ivan Delvecchio et al published 25 February 2014 in Monthly Notices of the Royal Astronomical Society

VLBA+GBT observations of the COSMOS field and radio source counts at 1.4 GHz

artículo científico publicado en 2018

“Super-deblended” Dust Emission in Galaxies. II. Far-IR to (Sub)millimeter Photometry and High-redshift Galaxy Candidates in the Full COSMOS Field

artículo científico publicado en 2018

Lista de obras de Ivan Delvecchio

(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies ⬇️

(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. IV. Physical properties derived from spectral energy distributions ⬇️

A fast ionised wind in a star-forming quasar system atz~ 1.5 resolved through adaptive optics assisted near-infrared data ⬇️

ALMA view of a massive spheroid progenitor: a compact rotating core of molecular gas in an AGN host at z = 2.226

Active galactic nuclei in dusty starbursts at z = 2: feedback still to kick in ⬇️

Active galactic nuclei vs. host galaxy properties in the COSMOS field

An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution

An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling

An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array

An Eddington ratio-driven origin for the LX − M* relation in quiescent and star-forming active galaxies

Compton thick AGN in the XMM-COSMOS survey ⬇️

Constraints on submicrojansky radio number counts based on evolving VLA-COSMOS luminosity functions

Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies at z ∼ 0.7

Erratum: The Herschel PEP/HerMES Luminosity Function – I. Probing the Evolution of PACS selected Galaxies to z ≃ 4

Herschel far-IR counterparts of SDSS galaxies: analysis of commonly used star formation rate estimates ⬇️

Linear radio size evolution of μJy populations

Mapping the average AGN accretion rate in the SFR–M* plane for Herschel★-selected galaxies at 0 < z ≤ 2.5 ⬇️

Merger induced clump formation in distant infrared luminous starburst galaxies

On the Kennicutt-Schmidt scaling law of submillimetre galaxies

Optical and mid-infrared line emission in nearby Seyfert galaxies

Probing black hole accretion tracks, scaling relations, and radiative efficiencies from stacked X-ray active galactic nuclei

Radio Selection of the Most Distant Galaxy Clusters ⬇️

Relationship between star formation rate and black hole accretion at z = 2: the different contributions in quiescent, normal, and starburst galaxies ⬇️

SINFONI spectra of heavily obscured AGNs in COSMOS: Evidence of outflows in a MIR/O target atz~ 2.5 ⬇️

SMBH accretion properties of radio-selected AGN out to z ∼ 4

Star formation inHerschel's Monsters versus semi-analytic models

The AGN content in luminous infrared galaxies at z∼ 2 from a global SED analysis including Herschel data

The COSMOS2015 galaxy stellar mass function. Thirteen billion years of stellar mass assembly in ten snapshots

The Evolving Interstellar Medium of Star-forming Galaxies, as Traced by Stardust*

The Herschel PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4

The Typical Massive Quiescent Galaxy at <i>z</i> ∼ 3 is a Post-starburst

The VIMOS Ultra-Deep Survey: Emerging from the dark, a massive proto-cluster at z ~ 4.57

The VLA-COSMOS 3 GHz Large Project: AGN and host-galaxy properties out to z ≲ 6

The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of highly star-forming galaxies

The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release

The VLA-COSMOS 3 GHz Large Project: Cosmic evolution of radio AGN and implications for radio-mode feedback since z~ 5

The VLA-COSMOS 3 GHz Large Project: Cosmic star formation history since z ~ 5

The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population

The VLA-COSMOS 3 GHz Large Project: Star formation properties and radio luminosity functions of AGN with moderate-to-high radiative luminosities out to z~ 6

The VLA-COSMOS 3 GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to z ≲ 6

The XXL Survey

The XXL Survey. XXI. The environment and clustering of X-ray AGN in the XXL-South field

The XXL Survey. XXXI. Classification and host galaxy properties of 2.1 GHz ATCA XXL-S radio sources

The XXL survey: First results and future

The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field

The effect of active galactic nuclei on the cold interstellar medium in distant star-forming galaxies

The faint radio sky: VLBA observations of the COSMOS field

The infrared-radio correlation of star-forming galaxies is strongly<i>M</i><sub>⋆</sub>-dependent but nearly redshift-invariant since<i>z</i>∼ 4

The main sequence at z ~ 1.3 contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts? ⬇️

The most obscured AGN in the COSMOS field

Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel ⬇️

VLBA+GBT observations of the COSMOS field and radio source counts at 1.4 GHz

“Super-deblended” Dust Emission in Galaxies. II. Far-IR to (Sub)millimeter Photometry and High-redshift Galaxy Candidates in the Full COSMOS Field