Lista de obras - Mauro Stefanon - Dominio Público Uruguay

A Path to the Stars: The Evolution of the Species

A Spectroscopic Follow-up Program of Very Massive Galaxies at 3 < z < 4: Confirmation of Spectroscopic Redshifts, and a High Fraction of Powerful AGNs

artículo científico publicado en 2017

A strongly lensed massive ultracompact quiescent galaxy at z ~ 2.4 in the COSMOS/UltraVISTA field ⬇️

artículo científico publicado en 2012

ALMA Measures Molecular Gas Reservoirs Comparable to Field Galaxies in a Low-mass Galaxy Cluster at z = 1.3

artículo científico publicado en 2022

ALMA as a Redshift Machine: Using [C II] to Efficiently Confirm Galaxies in the Epoch of Reionization

artículo científico publicado en 2023

CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip ⬇️

scholarly article

CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ∼ 2

artículo científico publicado en 2017

Discovery of a Dark, Massive, ALMA-only Galaxy at z ~ 5–6 in a Tiny 3 mm Survey

scholarly article published on 22 October 2019

Early Science with the Large Millimeter Telescope: Detection of Dust Emission in Multiple Images of a Normal Galaxy at z > 4 Lensed by a Frontier Fields Cluster ⬇️

artículo científico publicado en 2017

Extending the evolution of the stellar mass–size relation at z ≤ 2 to low stellar mass galaxies from HFF and CANDELS

artículo científico publicado en 2021

Galaxy Stellar Mass Functions from z ∼ 10 to z ∼ 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time

artículo científico publicado en 2021

HFF-DeepSpace Photometric Catalogs of the 12 Hubble Frontier Fields, Clusters, and Parallels: Photometry, Photometric Redshifts, and Stellar Masses

scholarly article

HST F160W Imaging of Very Massive Galaxies at 1.5 < z < 3.0: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates

article

HST Imaging of the Brightest z ∼ 8–9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function

artículo científico publicado en 2017

Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0

artículo científico publicado en 2017

Measuring the Average Molecular Gas Content of Star-forming Galaxies at z = 3–4

artículo científico publicado en 2021

Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 <z< 2.7 ⬇️

artículo científico publicado en 2017

Normal, dust-obscured galaxies in the epoch of reionization

artículo científico publicado en 2021

Observational Constraints on the Merger History of Galaxies since z ≈ 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields

artículo científico publicado en 2019

Optical-faint, far-infrared-bright Herschel sources in the CANDELS fields: ultra-luminous infrared galaxies at z > 1 and the effect of source blending

artículo científico publicado en 2014

Path to the stars: the evolution of the species in the hunting to the GRBs

Precise weak lensing constraints from deep high-resolution Ks images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2 J 232727.7−020437 at z = 0.70

artículo científico publicado en 2018

Properties of submillimeter galaxies in the CANDELS GOODS-South field ⬇️

artículo científico publicado en 2014

REM: Automatic for the People

REM: a fully robotic telescope for GRB observations

Spectroscopic confirmation of an ultra massive and compact galaxy at z = 3.35: a detailed look at an early progenitor of local giant ellipticals ⬇️

artículo científico publicado en 2015

Stellar mass functions of galaxies at 4 < z < 7 from an IRAC-selected sample in Cosmos/Ultravista: limits on the abundance of very massive galaxies ⬇️

scientific article published in the Astrophysical Journal

The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at z ≈ 7

artículo científico publicado en 2022

The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4

artículo científico publicado en 2022

The ALMA REBELS Survey: The Cosmic H i Gas Mass Density in Galaxies at z ≈ 7

artículo científico publicado en 2022

The ALMA REBELS survey: the dust content of z ∼ 7 Lyman break galaxies

artículo científico publicado en 2022

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 Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field

artículo científico publicado en 2019

The Mass, Color, and Structural Evolution of Today’s Massive Galaxies Since z ∼ 5 ⬇️

scientific article published in the Astrophysical Journal

The REM Observing Software

The Rest-frame Optical (900 nm) Galaxy Luminosity Function at z ∼ 4–7: Abundance Matching Points to Limited Evolution in the M STAR/M HALO Ratio at z ≥ 4

artículo científico publicado en 2017

The Software for the Robotization of the TROBAR Telescope

The Spitzer/IRAC Legacy over the GOODS Fields: Full-depth 3.6, 4.5, 5.8, and 8.0 μm Mosaics and Photometry for >9000 Galaxies at z ∼ 3.5–10 from the GOODS Reionization Era Wide-area Treasury from Spitzer (GREATS)

artículo científico publicado en 2021

The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at 7 < z < 8

artículo científico publicado en 2019

The evolution in the stellar mass of brightest cluster galaxies over the past 10 billion years ⬇️

artículo científico publicado en 2016

The evolution of the fractions of quiescent and star-forming galaxies as a function of stellar mass since z = 3: increasing importance of massive, dusty star-forming galaxies in the early universe ⬇️

scholarly article

The evolution of the stellar mass functions of star-forming and quiescent galaxies to z = 4 from the COSMOS/UltraVISTA survey ⬇️

artículo científico publicado en 2013

The progenitors of local ultra-massive galaxies across cosmic time: from dusty star-bursting to quiescent stellar populations ⬇️

artículo científico publicado en 2014

Ultra-deep K_s_-band imaging of the Hubble Frontier Fields ⬇️

Using cumulative number densities to compare galaxies across cosmic time ⬇️

z ∼ 2–9 Galaxies Magnified by the Hubble Frontier Field Clusters. I. Source Selection and Surface Density–Magnification Constraints from >2500 Galaxies

artículo científico publicado en 2022

Lista de obras de Mauro Stefanon

A Path to the Stars: The Evolution of the Species

A Spectroscopic Follow-up Program of Very Massive Galaxies at 3 < z < 4: Confirmation of Spectroscopic Redshifts, and a High Fraction of Powerful AGNs

A strongly lensed massive ultracompact quiescent galaxy at z ~ 2.4 in the COSMOS/UltraVISTA field ⬇️

ALMA Measures Molecular Gas Reservoirs Comparable to Field Galaxies in a Low-mass Galaxy Cluster at z = 1.3

ALMA as a Redshift Machine: Using [C II] to Efficiently Confirm Galaxies in the Epoch of Reionization

CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip ⬇️

CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ∼ 2

Discovery of a Dark, Massive, ALMA-only Galaxy at z ~ 5–6 in a Tiny 3 mm Survey

Early Science with the Large Millimeter Telescope: Detection of Dust Emission in Multiple Images of a Normal Galaxy at z > 4 Lensed by a Frontier Fields Cluster ⬇️

Extending the evolution of the stellar mass–size relation at <i>z</i> ≤ 2 to low stellar mass galaxies from HFF and CANDELS

Galaxy Stellar Mass Functions from z ∼ 10 to z ∼ 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time

HFF-DeepSpace Photometric Catalogs of the 12 Hubble Frontier Fields, Clusters, and Parallels: Photometry, Photometric Redshifts, and Stellar Masses

HST F160W Imaging of Very Massive Galaxies at 1.5 < z < 3.0: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates

HST Imaging of the Brightest z ∼ 8–9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function

Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0

Measuring the Average Molecular Gas Content of Star-forming Galaxies at z = 3–4

Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 <z< 2.7 ⬇️

Normal, dust-obscured galaxies in the epoch of reionization

Observational Constraints on the Merger History of Galaxies since z ≈ 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields

Optical-faint, far-infrared-bright Herschel sources in the CANDELS fields: ultra-luminous infrared galaxies at z > 1 and the effect of source blending

Path to the stars: the evolution of the species in the hunting to the GRBs

Precise weak lensing constraints from deep high-resolution Ks images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2 J 232727.7−020437 at z = 0.70

Properties of submillimeter galaxies in the CANDELS GOODS-South field ⬇️

REM: Automatic for the People

REM: a fully robotic telescope for GRB observations

Spectroscopic confirmation of an ultra massive and compact galaxy at z = 3.35: a detailed look at an early progenitor of local giant ellipticals ⬇️

Stellar mass functions of galaxies at 4 < z < 7 from an IRAC-selected sample in Cosmos/Ultravista: limits on the abundance of very massive galaxies ⬇️

The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at <i>z</i> ≈ 7

The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4

The ALMA REBELS Survey: The Cosmic H i Gas Mass Density in Galaxies at z ≈ 7

The ALMA REBELS survey: the dust content of <i>z</i> ∼ 7 Lyman break galaxies

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 Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field

The Mass, Color, and Structural Evolution of Today’s Massive Galaxies Since z ∼ 5 ⬇️

The REM Observing Software

The Rest-frame Optical (900 nm) Galaxy Luminosity Function at z ∼ 4–7: Abundance Matching Points to Limited Evolution in the M STAR/M HALO Ratio at z ≥ 4

The Software for the Robotization of the TROBAR Telescope

The Spitzer/IRAC Legacy over the GOODS Fields: Full-depth 3.6, 4.5, 5.8, and 8.0 μm Mosaics and Photometry for >9000 Galaxies at z ∼ 3.5–10 from the GOODS Reionization Era Wide-area Treasury from Spitzer (GREATS)

The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at 7 < z < 8

The evolution in the stellar mass of brightest cluster galaxies over the past 10 billion years ⬇️

The evolution of the fractions of quiescent and star-forming galaxies as a function of stellar mass since z = 3: increasing importance of massive, dusty star-forming galaxies in the early universe ⬇️

The evolution of the stellar mass functions of star-forming and quiescent galaxies to z = 4 from the COSMOS/UltraVISTA survey ⬇️

The progenitors of local ultra-massive galaxies across cosmic time: from dusty star-bursting to quiescent stellar populations ⬇️

Ultra-deep K_s_-band imaging of the Hubble Frontier Fields ⬇️

Using cumulative number densities to compare galaxies across cosmic time ⬇️

z ∼ 2–9 Galaxies Magnified by the Hubble Frontier Field Clusters. I. Source Selection and Surface Density–Magnification Constraints from &gt;2500 Galaxies

z ∼ 2–9 Galaxies Magnified by the Hubble Frontier Field Clusters. I. Source Selection and Surface Density–Magnification Constraints from >2500 Galaxies