Lista de obras -

A Comparison of the Stellar, CO, and Dust-continuum Emission from Three Star-forming HUDF Galaxies at z ∼ 2

artículo científico publicado en 2020

A NOEMA Molecular Line Scan of the Hubble Deep Field North: Improved Constraints on the CO Luminosity Functions and Cosmic Density of Molecular Gas

artículo científico publicado en 2023

A Theory for the Variation of Dust Attenuation Laws in Galaxies

scientific article published in the Astrophysical Journal

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

artículo científico publicado en 2020

ALMA spectroscopic survey in the Hubble Ultra Deep Field: survey description ⬇️

artículo científico publicado en 2016

ALMACAL - III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H I-absorption-selected system

scholarly article

ALMACAL IX: Multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background

artículo científico publicado en 2022

ALMACAL V: absorption-selected galaxies with evidence for excited ISMs

Dissecting the IRX–β dust attenuation relation: exploring the physical origin of observed variations in galaxies

scholarly article

Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models

artículo científico publicado en 2022

PdBI COLD DUST IMAGING OF TWO EXTREMELY REDH– [4.5] > 4 GALAXIES DISCOVERED WITH SEDS AND CANDELS ⬇️

artículo científico publicado en 2014

Semi-analytic forecasts for JWST – II. Physical properties and scaling relations for galaxies at z = 4–10

artículo científico publicado en 2019

The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History

artículo científico publicado en 2020

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies

artículo científico publicado en 2019

The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy

artículo científico publicado en 2019

The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z ∼ 3

artículo científico publicado en 2020

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 ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Excitation and Atomic Carbon in Star-forming Galaxies at z = 1–3

artículo científico publicado en 2020

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Constraining the Molecular Content at log(M */M ⊙) ∼ 9.5 with CO Stacking of MUSE-detected z ∼ 1.5 Galaxies

artículo científico publicado en 2020

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies

artículo científico publicado en 2020

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: continuum number counts, resolved 1.2 mm extragalactic background, and properties of the faintest dusty star-forming galaxies ⬇️

artículo científico publicado en 2016

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: implications for spectral line intensity mapping at millimeter wavelengths and CMB spectral distortions ⬇️

scientific article published in the Astrophysical Journal

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: molecular gas reservoirs in high-redshift galaxies ⬇️

artículo científico publicado en 2016

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: search for [CII] line and dust emission in 6 < z < 8 galaxies ⬇️

artículo científico publicado en 2016

The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High Redshift

artículo científico publicado en 2022

The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years

artículo científico publicado en 2021

The art of modelling CO, [C i], and [C ii] in cosmological galaxy formation models

scholarly article

The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 <z< 3.0 ⬇️

scholarly article

Lista de obras de

A Comparison of the Stellar, CO, and Dust-continuum Emission from Three Star-forming HUDF Galaxies at <i>z</i> ∼ 2

A NOEMA Molecular Line Scan of the Hubble Deep Field North: Improved Constraints on the CO Luminosity Functions and Cosmic Density of Molecular Gas

A Theory for the Variation of Dust Attenuation Laws in Galaxies

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

ALMA spectroscopic survey in the Hubble Ultra Deep Field: survey description ⬇️

ALMACAL - III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H I-absorption-selected system

ALMACAL IX: Multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background

ALMACAL V: absorption-selected galaxies with evidence for excited ISMs

Dissecting the IRX–β dust attenuation relation: exploring the physical origin of observed variations in galaxies

Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models

PdBI COLD DUST IMAGING OF TWO EXTREMELY REDH– [4.5] > 4 GALAXIES DISCOVERED WITH SEDS AND CANDELS ⬇️

Semi-analytic forecasts for JWST – II. Physical properties and scaling relations for galaxies at z = 4–10

The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History

The ALMA Spectroscopic Survey in the <i>Hubble</i> Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies

The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy

The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to <i>z</i> ∼ 3

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

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Excitation and Atomic Carbon in Star-forming Galaxies at <i>z</i> = 1–3

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Constraining the Molecular Content at log(<i>M</i> <sub>*</sub>/<i>M</i> <sub>⊙</sub>) ∼ 9.5 with CO Stacking of MUSE-detected <i>z</i> ∼ 1.5 Galaxies

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: continuum number counts, resolved 1.2 mm extragalactic background, and properties of the faintest dusty star-forming galaxies ⬇️

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: implications for spectral line intensity mapping at millimeter wavelengths and CMB spectral distortions ⬇️

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: molecular gas reservoirs in high-redshift galaxies ⬇️

The ALMA spectroscopic survey in the Hubble Ultra Deep Field: search for [CII] line and dust emission in 6 < z < 8 galaxies ⬇️

The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High Redshift

The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years

The art of modelling CO, [C i], and [C ii] in cosmological galaxy formation models

The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 <z< 3.0 ⬇️