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A Statistical and Multi-Wavelength Study of Star Formation in Galaxies

Schreiber, Corentin

1st ed. 2016., 2016

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On the dust temperatures of high-redshift galaxies

Monthly notices of the Royal Astronomical Society, 2019-10, Vol.489 (1), p.1397-1422

2019

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THE SFR–M RELATION AND EMPIRICAL STAR FORMATION HISTORIES FROM ZFOURGE AT 0.5 < z < 4

The Astrophysical journal, 2016-02, Vol.817 (2), p.118

2016

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Revealing the Environmental Dependence of Molecular Gas Content in a Distant X-Ray Cluster at z = 2.51

Astrophysical journal. Letters, 2018-11, Vol.867 (2), p.L29

2018

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

The Astrophysical journal, 2017-03, Vol.837 (2), p.147

2017

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The MUSE Hubble Ultra Deep Field Survey

Astronomy and astrophysics (Berlin), 2018-11, Vol.619

2018

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The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day

Astronomy and astrophysics (Berlin), 2015-03, Vol.575, p.A74

2015

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A massive, quiescent galaxy at a redshift of 3.717

Nature (London), 2017-04, Vol.544 (7648), p.71-74

2017

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DISCOVERY OF A GALAXY CLUSTER WITH A VIOLENTLY STARBURSTING CORE AT z = 2.506

The Astrophysical journal, 2016-09, Vol.828 (1), p.56-56

2016

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Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation

Astronomy and astrophysics (Berlin), 2015-01, Vol.573, p.A113

2015

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The MUSE Hubble Ultra Deep Field Survey: XI. Constraining the low-mass end of the stellar mass – star formation rate relation at z < 1

Astronomy and astrophysics (Berlin), 2018-11, Vol.619, p.A27

2018

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ACTIVE GALACTIC NUCLEI EMISSION LINE DIAGNOSTICS AND THE MASS-METALLICITY RELATION UP TO REDSHIFT z ∼ 2: THE IMPACT OF SELECTION EFFECTS AND EVOLUTION

The Astrophysical journal, 2014-06, Vol.788 (1), p.1-26

2014

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A massive galaxy that formed its stars at z ≈ 11

Nature (London), 2024-04, Vol.628 (8007), p.277-281

2024

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A population of faint, old, and massive quiescent galaxies at 3<z<4 revealed by JWST NIRSpec Spectroscopy

Scientific reports, 2024-02, Vol.14 (1), p.3724, Article 3724

2024

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Low Star Formation Activity and Low Gas Content of Quiescent Galaxies at z = 3.5–4.0 Constrained with ALMA

The Astrophysical journal, 2022-09, Vol.936 (1), p.61

2022

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Consistent Dynamical and Stellar Masses with Potential Light IMF in Massive Quiescent Galaxies at 3 < z < 4 Using Velocity Dispersions Measurements with MOSFIRE

Astrophysical journal. Letters, 2021-02, Vol.908 (2), p.L35

2021

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A population of faint, old, and massive quiescent galaxies at [Formula: see text] revealed by JWST NIRSpec Spectroscopy

Scientific reports, 2024-02, Vol.14 (1), p.3724-3724

2024

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A population of faint, old, and massive quiescent galaxies at $$3 z 4$$ 3 z 4 revealed by JWST NIRSpec Spectroscopy

Scientific reports, 2024-02, Vol.14 (1), p.1-14

2024

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The MUSE Hubble Ultra Deep Field Survey. XI. Constraining the low-mass end of the stellar mass – star formation raterelation at z < 1

Astronomy and astrophysics (Berlin), 2018-11, Vol.619

2018

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Reaching the Distant Universe with ALMA

A Statistical and Multi-Wavelength Study of Star Formation in Galaxies, 2016, p.167-198

Schreiber, Corentin

2016

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The Main Sequence of Star-Forming Galaxies as Seen by Herschel

A Statistical and Multi-Wavelength Study of Star Formation in Galaxies, 2016, p.29-86

Schreiber, Corentin

2016

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Conclusions and Perspectives

A Statistical and Multi-Wavelength Study of Star Formation in Galaxies, 2016, p.199-203

Schreiber, Corentin

2016

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The Downfall of Massive Star-Forming Galaxies During the Last 10Gyr\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10\,\mathrm{Gyr}$$\end{document}

A Statistical and Multi-wavelength Study of Star Formation in Galaxies, 2016, p.127-166

Schreiber, Corentin

2016

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A Statistical and Multi-Wavelength Study of Star Formation in Galaxies

On the dust temperatures of high-redshift galaxies

THE SFR–M RELATION AND EMPIRICAL STAR FORMATION HISTORIES FROM ZFOURGE AT 0.5 < z < 4

Revealing the Environmental Dependence of Molecular Gas Content in a Distant X-Ray Cluster at z = 2.51

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

The MUSE Hubble Ultra Deep Field Survey

The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day

A massive, quiescent galaxy at a redshift of 3.717

DISCOVERY OF A GALAXY CLUSTER WITH A VIOLENTLY STARBURSTING CORE AT z = 2.506

Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation

The MUSE Hubble Ultra Deep Field Survey: XI. Constraining the low-mass end of the stellar mass – star formation rate relation at z < 1

ACTIVE GALACTIC NUCLEI EMISSION LINE DIAGNOSTICS AND THE MASS-METALLICITY RELATION UP TO REDSHIFT z ∼ 2: THE IMPACT OF SELECTION EFFECTS AND EVOLUTION

A massive galaxy that formed its stars at z ≈ 11

A population of faint, old, and massive quiescent galaxies at 3<z<4 revealed by JWST NIRSpec Spectroscopy

Low Star Formation Activity and Low Gas Content of Quiescent Galaxies at z = 3.5–4.0 Constrained with ALMA

Consistent Dynamical and Stellar Masses with Potential Light IMF in Massive Quiescent Galaxies at 3 < z < 4 Using Velocity Dispersions Measurements with MOSFIRE

A population of faint, old, and massive quiescent galaxies at [Formula: see text] revealed by JWST NIRSpec Spectroscopy

A population of faint, old, and massive quiescent galaxies at $$3 z 4$$ 3 z 4 revealed by JWST NIRSpec Spectroscopy

The MUSE Hubble Ultra Deep Field Survey. XI. Constraining the low-mass end of the stellar mass – star formation raterelation at z < 1

THE SFR-M RELATION AND EMPIRICAL STAR FORMATION HISTORIES FROM ZFOURGE AT 0.5 < z < 4 This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile

Reaching the Distant Universe with ALMA

The Main Sequence of Star-Forming Galaxies as Seen by Herschel

Conclusions and Perspectives

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