Lista de obras - Paul Torrey - Dominio Público Uruguay

A census of cool-core galaxy clusters in IllustrisTNG

scholarly article

A model for cosmological simulations of galaxy formation physics

article

A model for cosmological simulations of galaxy formation physics: multi-epoch validation

artículo científico publicado en 2014

An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations ⬇️

scholarly article

An integral field study of abundance gradients in nearby luminous infrared galaxies ⬇️

artículo científico publicado en 2012

Baryons in the Cosmic Web of IllustrisTNG – II. The connection among galaxies, haloes, their formation time, and their location in the Cosmic Web ⬇️

scholarly article

Can We Constrain Warm Dark Matter Masses with Individual Galaxies?

artículo científico publicado en 2024

Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations

Damped Lyman α absorbers as a probe of stellar feedback ⬇️

scholarly article

Deep learning predictions of galaxy merger stage and the importance of observational realism

artículo científico publicado en 2019

Early-type galaxy density profiles from IllustrisTNG – I. Galaxy correlations and the impact of baryons ⬇️

scholarly article

Early-type galaxy density profiles from IllustrisTNG – II. Evolutionary trend of the total density profile ⬇️

artículo científico publicado en 2019

Empirical constraints for the magnitude and composition of galactic winds

article

Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction

artículo científico publicado en 2019

Erratum: A model for cosmological simulations of galaxy formation physics

article

First results from the IllustrisTNG simulations: a tale of two elements – chemical evolution of magnesium and europium

scholarly article by Jill P Naiman et al published 8 March 2018 in Monthly Notices of the Royal Astronomical Society

First results from the IllustrisTNG simulations: matter and galaxy clustering

scholarly article

First results from the IllustrisTNG simulations: radio haloes and magnetic fields

artículo científico publicado en 2018

First results from the IllustrisTNG simulations: the galaxy colour bimodality

scholarly article

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

artículo científico publicado en 2017

First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time

scholarly article

Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion

scholarly article

Galaxy mergers moulding the circum-galactic medium – I. The impact of a major merger

artículo científico publicado en 2017

Galaxy mergers on a moving mesh: a comparison with smoothed particle hydrodynamics

scholarly article

Galaxy morphology and star formation in the Illustris Simulation atz = 0 ⬇️

artículo científico publicado en 2015

Galaxy pairs in the Sloan Digital Sky Survey - V. Tracing changes in star formation rate and metallicity out to separations of 80 kpc

article by Jillian M Scudder et al published 18 September 2012 in Monthly Notices of the Royal Astronomical Society

Galaxy pairs in the Sloan Digital Sky Survey - VI. The orbital extent of enhanced star formation in interacting galaxies

artículo científico publicado en 2013

Galaxy pairs in the Sloan Digital Sky Survey – X. Does gas content alter star formation rate enhancement in galaxy interactions? ⬇️

article by Jillian M Scudder et al published 10 April 2015 in Monthly Notices of the Royal Astronomical Society

Gas-phase metallicity gradients of TNG50 star-forming galaxies

artículo científico publicado en 2021

H α emission in local galaxies: star formation, time variability, and the diffuse ionized gas

artículo científico publicado en 2022

Halo mass and assembly history exposed in the faint outskirts: the stellar and dark matter haloes of Illustris galaxies ⬇️

artículo científico publicado en 2014

High-redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves

scientific article published in 2020

High-redshift JWST predictions from IllustrisTNG: dust modelling and galaxy luminosity functions

scientific article published in 2020

High-redshift predictions from IllustrisTNG – III. Infrared luminosity functions, obscured star formation, and dust temperature of high-redshift galaxies

artículo científico publicado en 2022

Hot gaseous Coronae around spiral galaxies: probing the illustris simulation ⬇️

artículo científico publicado en 2015

Hydrogen reionization in the Illustris universe ⬇️

artículo científico publicado en 2015

Interacting galaxies in the IllustrisTNG simulations – II: star formation in the post-merger stage

scientific article published in 2020

Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe ⬇️

artículo científico publicado en 2014

Introducing the Illustris project: the evolution of galaxy populations across cosmic time ⬇️

scholarly article

Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG

scholarly article by Mélanie Habouzit et al published 16 January 2019 in Monthly Notices of the Royal Astronomical Society

Low- and High-velocity O vi in Milky Way-like Galaxies: The Role of Stellar Feedback

artículo científico publicado en 2024

Mapping galaxy encounters in numerical simulations: the spatial extent of induced star formation ⬇️

scholarly article

Modelling galactic conformity with the colour–halo age relation in the Illustris simulation ⬇️

artículo científico publicado en 2015

Moving-mesh cosmology: properties of gas discs

scholarly article by Paul Torrey et al published 20 November 2012 in Monthly Notices of the Royal Astronomical Society

On the assembly of dwarf galaxies in clusters and their efficient formation of globular clusters ⬇️

artículo científico publicado en 2015

On the cosmic evolution of Fe/Mg in QSO absorption line systems ⬇️

scholarly article

Properties of galaxies reproduced by a hydrodynamic simulation

artículo científico publicado en 2014

Similar star formation rate and metallicity variability time-scales drive the fundamental metallicity relation

Simulating galactic dust grain evolution on a moving mesh

scholarly article

Supermassive black holes and their feedback effects in the IllustrisTNG simulation

scholarly article by Rainer Weinberger et al published 29 June 2018 in Monthly Notices of the Royal Astronomical Society

Synthetic galaxy images and spectra from the Illustris simulation ⬇️

artículo científico publicado en 2015

The Illustris simulation: the evolving population of black holes across cosmic time ⬇️

scholarly article by Debora Sijacki et al published 6 July 2015 in Monthly Notices of the Royal Astronomical Society

The abundance, distribution, and physical nature of highly ionized oxygen O vi, O vii, and O viii in IllustrisTNG

artículo científico publicado en 2018

The colours of satellite galaxies in the Illustris simulation ⬇️

scholarly article

The dynamics of galaxy pairs in a cosmological setting

scholarly article

The evolution of the mass-metallicity relation and its scatter in IllustrisTNG

scholarly article

The formation of massive, compact galaxies at z = 2 in the Illustris simulation ⬇️

artículo científico publicado en 2015

The fraction of dark matter within galaxies from the IllustrisTNG simulations

artículo científico publicado en 2018

The illustris simulation: Public data release ⬇️

scholarly article

The impact of feedback on cosmological gas accretion ⬇️

artículo científico publicado en 2015

The impact of galactic feedback on the circumgalactic medium ⬇️

scholarly article

The incidence of low-metallicity Lyman-limit systems at z ~ 3.5: implications for the cold-flow hypothesis of baryonic accretion ⬇️

artículo científico publicado en 2015

The merger rate of galaxies in the Illustris simulation: a comparison with observations and semi-empirical models ⬇️

artículo científico publicado en 2015

The metallicity evolution of interacting galaxies ⬇️

artículo científico publicado en 2012

The neutral gas content of post-merger galaxies ⬇️

scholarly article

The slow flow model of dust efflux in local star-forming galaxies

scholarly article

The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation ⬇️

artículo científico publicado en 2015

Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions ⬇️

scholarly article

Lista de obras de Paul Torrey

A census of cool-core galaxy clusters in IllustrisTNG

A model for cosmological simulations of galaxy formation physics

A model for cosmological simulations of galaxy formation physics: multi-epoch validation

An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations ⬇️

An integral field study of abundance gradients in nearby luminous infrared galaxies ⬇️

Baryons in the Cosmic Web of IllustrisTNG – II. The connection among galaxies, haloes, their formation time, and their location in the Cosmic Web ⬇️

Can We Constrain Warm Dark Matter Masses with Individual Galaxies?

Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations

Damped Lyman α absorbers as a probe of stellar feedback ⬇️

Deep learning predictions of galaxy merger stage and the importance of observational realism

Early-type galaxy density profiles from IllustrisTNG – I. Galaxy correlations and the impact of baryons ⬇️

Early-type galaxy density profiles from IllustrisTNG – II. Evolutionary trend of the total density profile ⬇️

Empirical constraints for the magnitude and composition of galactic winds

Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction

Erratum: A model for cosmological simulations of galaxy formation physics

First results from the IllustrisTNG simulations: a tale of two elements – chemical evolution of magnesium and europium

First results from the IllustrisTNG simulations: matter and galaxy clustering

First results from the IllustrisTNG simulations: radio haloes and magnetic fields

First results from the IllustrisTNG simulations: the galaxy colour bimodality

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time

Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion

Galaxy mergers moulding the circum-galactic medium – I. The impact of a major merger

Galaxy mergers on a moving mesh: a comparison with smoothed particle hydrodynamics

Galaxy morphology and star formation in the Illustris Simulation atz = 0 ⬇️

Galaxy pairs in the Sloan Digital Sky Survey - V. Tracing changes in star formation rate and metallicity out to separations of 80 kpc

Galaxy pairs in the Sloan Digital Sky Survey - VI. The orbital extent of enhanced star formation in interacting galaxies

Galaxy pairs in the Sloan Digital Sky Survey – X. Does gas content alter star formation rate enhancement in galaxy interactions? ⬇️

Gas-phase metallicity gradients of TNG50 star-forming galaxies

H <i>α</i> emission in local galaxies: star formation, time variability, and the diffuse ionized gas

Halo mass and assembly history exposed in the faint outskirts: the stellar and dark matter haloes of Illustris galaxies ⬇️

High-redshift <i>JWST</i> predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves

High-redshift <i>JWST</i> predictions from IllustrisTNG: dust modelling and galaxy luminosity functions

High-redshift predictions from IllustrisTNG – III. Infrared luminosity functions, obscured star formation, and dust temperature of high-redshift galaxies

Hot gaseous Coronae around spiral galaxies: probing the illustris simulation ⬇️

Hydrogen reionization in the Illustris universe ⬇️

Interacting galaxies in the IllustrisTNG simulations – II: star formation in the post-merger stage

Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe ⬇️

Introducing the Illustris project: the evolution of galaxy populations across cosmic time ⬇️

Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG

Low- and High-velocity O vi in Milky Way-like Galaxies: The Role of Stellar Feedback

Mapping galaxy encounters in numerical simulations: the spatial extent of induced star formation ⬇️

Modelling galactic conformity with the colour–halo age relation in the Illustris simulation ⬇️

Moving-mesh cosmology: properties of gas discs

On the assembly of dwarf galaxies in clusters and their efficient formation of globular clusters ⬇️

On the cosmic evolution of Fe/Mg in QSO absorption line systems ⬇️

Properties of galaxies reproduced by a hydrodynamic simulation

Similar star formation rate and metallicity variability time-scales drive the fundamental metallicity relation

Simulating galactic dust grain evolution on a moving mesh

Supermassive black holes and their feedback effects in the IllustrisTNG simulation

Synthetic galaxy images and spectra from the Illustris simulation ⬇️

The Illustris simulation: the evolving population of black holes across cosmic time ⬇️

The abundance, distribution, and physical nature of highly ionized oxygen O vi, O vii, and O viii in IllustrisTNG

The colours of satellite galaxies in the Illustris simulation ⬇️

The dynamics of galaxy pairs in a cosmological setting

The evolution of the mass-metallicity relation and its scatter in IllustrisTNG

The formation of massive, compact galaxies at z = 2 in the Illustris simulation ⬇️

The fraction of dark matter within galaxies from the IllustrisTNG simulations

The illustris simulation: Public data release ⬇️

The impact of feedback on cosmological gas accretion ⬇️

The impact of galactic feedback on the circumgalactic medium ⬇️

The incidence of low-metallicity Lyman-limit systems at z ~ 3.5: implications for the cold-flow hypothesis of baryonic accretion ⬇️

The merger rate of galaxies in the Illustris simulation: a comparison with observations and semi-empirical models ⬇️

The metallicity evolution of interacting galaxies ⬇️

The neutral gas content of post-merger galaxies ⬇️

The slow flow model of dust efflux in local star-forming galaxies

The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation ⬇️

Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions ⬇️