Lista de obras - Annalisa Pillepich - Dominio Público Uruguay

A "Light," centrally concentrated Milky Way halo? ⬇️

artículo científico publicado en 2013

A Deep Learning Approach to Galaxy Cluster X-Ray Masses

scholarly article by M. Ntampaka et al published 7 May 2019 in The Astrophysical Journal

A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations

artículo científico publicado en 2019

A census of cool-core galaxy clusters in IllustrisTNG

scholarly article

A redshift-dependent IRX–β dust attenuation relation for TNG50 galaxies

artículo científico publicado en 2020

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

scholarly article

An off-center density peak in the Milky Way's dark matter halo? ⬇️

scholarly article

Atomic and molecular gas in IllustrisTNG galaxies at low redshift

artículo científico publicado en 2019

Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys

scholarly article

Baryons in the Cosmic Web of IllustrisTNG – I: gas in knots, filaments, sheets, and voids

scholarly article

Building late-type spiral galaxies by in-situ and ex-situ star formation ⬇️

artículo científico publicado en 2015

CANDELS visual classifications: scheme, data release, and first results ⬇️

article

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

Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST

scientific article published in 2022

Constraining primordial non-Gaussianity with future galaxy surveys

artículo científico publicado en 2012

ETHOS – an effective theory of structure formation: predictions for the high-redshift Universe – abundance of galaxies and reionization

scientific article published on 28 March 2018

Erratum: Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys

scholarly article published in Monthly Notices of the Royal Astronomical Society

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

Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering

artículo científico publicado en 2018

Formation and incidence of shell galaxies in the Illustris simulation

artículo científico publicado en 2018

Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion

scholarly article

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

artículo científico publicado en 2015

Gas-phase metallicity gradients of TNG50 star-forming galaxies

artículo científico publicado en 2021

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

artículo científico publicado en 2014

Halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditions

article

Hidden depths in the local Universe: The Stellar Stream Legacy Survey

artículo científico publicado en 2023

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

Ingredients for 21 cm Intensity Mapping

scientific article published in the Astrophysical Journal

Jellyfish galaxies with the IllustrisTNG simulations – I. Gas-stripping phenomena in the full cosmological context

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

Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations ⬇️

artículo científico publicado en 2017

Modeling the Atomic-to-molecular Transition in Cosmological Simulations of Galaxy Formation

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

artículo científico publicado en 2015

Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO and SFR data

artículo científico publicado en 2021

Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs

artículo científico publicado en 2019

On the Nature of Disks at High Redshift Seen by JWST/CEERS with Contrastive Learning and Cosmological Simulations

artículo científico publicado en 2024

On the Scatter of the Present-day Stellar Metallicity–Mass Relation of Cluster Dwarf Galaxies

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

artículo científico publicado en 2015

Shape of dark matter haloes in the Illustris simulation: effects of baryons

artículo científico publicado en 2019

Shock finding on a moving-mesh – II. Hydrodynamic shocks in the Illustris universe ⬇️

scholarly article

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

Simulating galaxy formation with black hole driven thermal and kinetic feedback ⬇️

scholarly article by Rainer Weinberger et al published 22 November 2016 in Monthly Notices of the Royal Astronomical Society

Simulating galaxy formation with the IllustrisTNG model

scholarly article

Subhalo demographics in the Illustris simulation: effects of baryons and halo-to-halo variation

artículo científico publicado en 2017

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 AGORA high-resolution galaxy simulations comparison project

scholarly article

The ALMA Spectroscopic Survey in the HUDF: the Molecular Gas Content of Galaxies and Tensions with IllustrisTNG and the Santa Cruz SAM

artículo científico publicado en 2019

The Bispectrum of Redshifted 21 Centimeter Fluctuations from the Dark Ages ⬇️

scientific article published in the Astrophysical Journal

The Fornax3D project: Discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427

scientific article published in 2022

The IllustrisTNG simulations: public data release

The MUSE Hubble Ultra Deep Field Survey

scientific article published in 2021

The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity

scholarly article by Pillepich A. et al published 2012 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 distribution of dark matter in the Milky Way's disk ⬇️

artículo científico publicado en 2014

The diverse evolutionary paths of simulated high-z massive, compact galaxies to z = 0 ⬇️

artículo científico publicado en 2016

The eROSITA Final Equatorial Depth Survey (eFEDS)

scientific article published in 2022

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 host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS ⬇️

artículo científico publicado en 2014

The illustris simulation: Public data release ⬇️

scholarly article

The information content of stellar halos: stellar population gradients and accretion histories in early-Type Illustris galaxies ⬇️

artículo científico publicado en 2016

The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disc survival through mergers

scientific article published in 2022

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

artículo científico publicado en 2015

The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations

artículo científico publicado en 2018

The role of mergers and halo spin in shaping galaxy morphology ⬇️

scholarly article

The size evolution of star-forming and quenched galaxies in the IllustrisTNG simulation

scholarly article

The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics

artículo científico publicado en 2019

The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars ⬇️

scholarly article

The stellar mass assembly of low-redshift, massive, central galaxies in SDSS and the TNG300 simulation

scientific article published in 2020

The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations

artículo científico publicado en 2017

UV to submillimetre luminosity functions of TNG50 galaxies

artículo científico publicado en 2022

Zooming in on accretion – I. The structure of halo gas ⬇️

scholarly article

Lista de obras de Annalisa Pillepich

A "Light," centrally concentrated Milky Way halo? ⬇️

A Deep Learning Approach to Galaxy Cluster X-Ray Masses

A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations

A census of cool-core galaxy clusters in IllustrisTNG

A redshift-dependent IRX–β dust attenuation relation for TNG50 galaxies

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

An off-center density peak in the Milky Way's dark matter halo? ⬇️

Atomic and molecular gas in IllustrisTNG galaxies at low redshift

Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys

Baryons in the Cosmic Web of IllustrisTNG – I: gas in knots, filaments, sheets, and voids

Building late-type spiral galaxies by in-situ and ex-situ star formation ⬇️

CANDELS visual classifications: scheme, data release, and first results ⬇️

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

Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of <i>JWST</i>

Constraining primordial non-Gaussianity with future galaxy surveys

ETHOS – an effective theory of structure formation: predictions for the high-redshift Universe – abundance of galaxies and reionization

Erratum: Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys

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

Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering

Formation and incidence of shell galaxies in the Illustris simulation

Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion

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

Gas-phase metallicity gradients of TNG50 star-forming galaxies

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

Halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditions

Hidden depths in the local Universe: The Stellar Stream Legacy Survey

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

Ingredients for 21 cm Intensity Mapping

Jellyfish galaxies with the IllustrisTNG simulations – I. Gas-stripping phenomena in the full cosmological context

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

Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations ⬇️

Modeling the Atomic-to-molecular Transition in Cosmological Simulations of Galaxy Formation

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

Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO and SFR data

Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs

On the Nature of Disks at High Redshift Seen by JWST/CEERS with Contrastive Learning and Cosmological Simulations

On the Scatter of the Present-day Stellar Metallicity–Mass Relation of Cluster Dwarf Galaxies

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

Shape of dark matter haloes in the Illustris simulation: effects of baryons

Shock finding on a moving-mesh – II. Hydrodynamic shocks in the Illustris universe ⬇️

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

Simulating galaxy formation with black hole driven thermal and kinetic feedback ⬇️

Simulating galaxy formation with the IllustrisTNG model

Subhalo demographics in the Illustris simulation: effects of baryons and halo-to-halo variation

Supermassive black holes and their feedback effects in the IllustrisTNG simulation

Synthetic galaxy images and spectra from the Illustris simulation ⬇️

The AGORA high-resolution galaxy simulations comparison project

The ALMA Spectroscopic Survey in the HUDF: the Molecular Gas Content of Galaxies and Tensions with IllustrisTNG and the Santa Cruz SAM

The Bispectrum of Redshifted 21 Centimeter Fluctuations from the Dark Ages ⬇️

The Fornax3D project: Discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427

The IllustrisTNG simulations: public data release

The MUSE <i>Hubble</i> Ultra Deep Field Survey

The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity

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 distribution of dark matter in the Milky Way's disk ⬇️

The diverse evolutionary paths of simulated high-z massive, compact galaxies to z = 0 ⬇️

The eROSITA Final Equatorial Depth Survey (eFEDS)

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 host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS ⬇️

The illustris simulation: Public data release ⬇️

The information content of stellar halos: stellar population gradients and accretion histories in early-Type Illustris galaxies ⬇️

The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disc survival through mergers

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

The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations

The role of mergers and halo spin in shaping galaxy morphology ⬇️

The size evolution of star-forming and quenched galaxies in the IllustrisTNG simulation

The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics

The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars ⬇️

The stellar mass assembly of low-redshift, massive, central galaxies in SDSS and the TNG300 simulation

The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations

UV to submillimetre luminosity functions of TNG50 galaxies