Search Results - "Giavalisco, Mauro"
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Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon
Published in The Astrophysical journal (01-01-2023)“…Abstract We use the spectral energy distribution fitting code Prospector to reconstruct the nonparametric star formation history (SFH) of massive ( log M * >…”
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On the Stellar Populations of Galaxies at z = 9–11: The Growth of Metals and Stellar Mass at Early Times
Published in The Astrophysical journal (01-03-2022)“…We present a detailed stellar population analysis of 11 bright (H < 26.6) galaxies at z=9−11 (three spectroscopically confirmed) to constrain the chemical…”
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The Low-redshift Lyman Continuum Survey. I. New, Diverse Local Lyman Continuum Emitters
Published in The Astrophysical journal. Supplement series (21-04-2022)“…Abstract The origins of Lyman continuum (LyC) photons responsible for the reionization of the universe are as of yet unknown and highly contested. Detecting…”
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THE EVOLUTION OF THE GALAXY REST-FRAME ULTRAVIOLET LUMINOSITY FUNCTION OVER THE FIRST TWO BILLION YEARS
Published in The Astrophysical journal (01-09-2015)“…ABSTRACT We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity functions at z = 4-8. We use deep Hubble Space Telescope…”
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Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3
Published in The Astrophysical journal (01-02-2018)“…Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists…”
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CLEAR. II. Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift
Published in The Astrophysical journal (01-08-2020)“…The origin of the correlations between mass, morphology, quenched fraction, and formation history in galaxies is difficult to define, primarily due to the…”
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LYMAN-BREAK GALAXIES
Published in Annual review of astronomy and astrophysics (01-01-2002)“…In this paper we review the properties of Lyman-break galaxies, namely starburst galaxies at high redshifts, approximately in the range 2.5 < z < 5, identified…”
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Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5 < z < 2.5
Published in The Astrophysical journal (20-03-2017)“…In this paper, we investigate the relationship between star formation and structure, using a mass-complete sample of 27,893 galaxies at 0.5 < z < 2.5 selected…”
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The Differential Assembly History of the Centers and Outskirts of Main-sequence Galaxies at z ∼ 2.3
Published in The Astrophysical journal (01-03-2023)“…Abstract We present a study of spatially resolved star formation histories (SFHs) for 60 z ∼ 2.3 main-sequence, star-forming galaxies selected from the MOSDEF…”
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CLUMPY GALAXIES IN CANDELS. I. THE DEFINITION OF UV CLUMPS AND THE FRACTION OF CLUMPY GALAXIES AT 0.5 < z < 3
Published in The Astrophysical journal (10-02-2015)“…Although giant clumps of stars are thought to be crucial to galaxy formation and evolution, the most basic demographics of clumps are still uncertain, mainly…”
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Large-scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity
Published in The Astrophysical journal (10-02-2020)“…We present a robust method, weighted von Mises kernel density estimation, along with boundary correction to reconstruct the underlying number density field of…”
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Morphology Dependence of Stellar Age in Quenched Galaxies at Redshift ∼1.2:Massive Compact Galaxies Are Older than More Extended Ones
Published in The Astrophysical journal (01-04-2017)“…We report the detection of morphology-dependent stellar age in massive quenched galaxies (QGs) at z ∼ 1.2. The sense of the dependence is that compact QGs are…”
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Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
Published in The Astrophysical journal (01-03-2024)“…Abstract We explore the relationships between the [O/H] gas-phase metallicity radial gradients and multiple galaxy properties for 238 star-forming galaxies at…”
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THE EVOLUTION OF STAR FORMATION HISTORIES OF QUIESCENT GALAXIES
Published in The Astrophysical journal (20-11-2016)“…ABSTRACT Although there has been much progress in understanding how galaxies evolve, we still do not understand how and when they stop forming stars and become…”
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CLEAR: The Gas-phase Metallicity Gradients of Star-forming Galaxies at 0.6 < z < 2.6
Published in The Astrophysical journal (01-12-2021)“…Abstract We report on the gas-phase metallicity gradients of a sample of 238 star-forming galaxies at 0.6 < z < 2.6, measured through deep near-infrared Hubble…”
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The Intrinsic Characteristics of Galaxies on the SFR-M∗ Plane at 1.2 < z < 4: I. The Correlation between Stellar Age, Central Density, and Position Relative to the Main Sequence
Published in The Astrophysical journal (01-02-2018)“…We use the deep CANDELS observations in the GOODS North and South fields to revisit the correlations between stellar mass (M*), star formation rate (SFR) and…”
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The Low-redshift Lyman-continuum Survey: [S ii] Deficiency and the Leakage of Ionizing Radiation
Published in The Astrophysical journal (01-07-2021)“…Abstract The relationship between galaxy characteristics and the reionization of the universe remains elusive, mainly due to the observational difficulty in…”
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Evidence of Environmental Quenching at Redshift z 2
Published in The Astrophysical journal (01-08-2018)“…We report evidence of environmental quenching among galaxies at redshifts of 2, namely the probability that a galaxy quenches its star formation activity is…”
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Selection of Massive Evolved Galaxies at 3 ≤ z ≤ 4.5 in the CANDELS Fields
Published in The Astrophysical journal (01-07-2020)“…Using the CANDELS photometric catalogs for the Hubble Space Telescope/ACS and WFC3, we identified massive evolved galaxies at 3 < z < 4.5 employing three…”
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CLEAR: High-ionization [Ne v] λ3426 Emission-line Galaxies at 1.4 < z < 2.3
Published in The Astrophysical journal (01-05-2023)“…Abstract We analyze a sample of 25 [Ne v ] ( λ 3426) emission-line galaxies at 1.4 < z < 2.3 using Hubble Space Telescope/Wide Field Camera 3 G102 and G141…”
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