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One Percent Determination of the Primordial Deuterium Abundance

The Astrophysical journal, 2018-03, Vol.855 (2), p.102

2018

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The PHLEK Survey: A New Determination of the Primordial Helium Abundance

The Astrophysical journal, 2020-06, Vol.896 (1), p.77

2020

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MUSE Analysis of Gas around Galaxies (MAGG) – II: metal-enriched halo gas around z ∼ 1 galaxies

Monthly notices of the Royal Astronomical Society, 2020-11, Vol.499 (4), p.5022-5046

2020

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Searching for the Lowest-metallicity Galaxies in the Local Universe

The Astrophysical journal, 2018-08, Vol.863 (2), p.134

2018

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The Little Cub: Discovery of an Extremely Metal-poor Star-forming Galaxy in the Local Universe

Astrophysical journal. Letters, 2017-08, Vol.845 (2), p.L22

2017

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BIG BANG NUCLEOSYNTHESIS AND THE HELIUM ISOTOPE RATIO

Astrophysical journal. Letters, 2015-10, Vol.812 (1), p.1-5

Cooke, Ryan J.

2015

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THE PRIMORDIAL DEUTERIUM ABUNDANCE OF THE MOST METAL-POOR DAMPED Lyα SYSTEM

The Astrophysical journal, 2016-10, Vol.830 (2), p.148

2016

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CARBON-ENHANCED METAL-POOR STARS: RELICS FROM THE DARK AGES

The Astrophysical journal, 2014-08, Vol.791 (2), p.1-12

2014

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THE HISTORY OF R-PROCESS ENRICHMENT IN THE MILKY WAY

The Astrophysical journal, 2015-07, Vol.807 (2), p.1-10

2015

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THE MOST METAL-POOR DAMPED Lyα SYSTEMS: AN INSIGHT INTO DWARF GALAXIES AT HIGH-REDSHIFT

The Astrophysical journal, 2015-02, Vol.800 (1), p.1-17

2015

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Harvesting the Ly α forest with convolutional neural networks

Monthly notices of the Royal Astronomical Society, 2022-10, Vol.517 (1), p.755-775

2022

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MUSE Analysis of Gas around Galaxies (MAGG) – I: Survey design and the environment of a near pristine gas cloud at z ≈ 3.5

Monthly notices of the Royal Astronomical Society, 2020-01, Vol.491 (2), p.2057-2074

2020

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Origins of carbon-enhanced metal-poor stars

Monthly notices of the Royal Astronomical Society, 2018-01, Vol.473 (1), p.984-995

2018

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Primordial Helium-3 Redux: The Helium Isotope Ratio of the Orion Nebula

The Astrophysical journal, 2022-06, Vol.932 (1), p.60

2022

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MUSE Analysis of Gas around Galaxies (MAGG) – IV. The gaseous environment of z ∼ 3–4 Ly α emitting galaxies

Monthly notices of the Royal Astronomical Society, 2022-11, Vol.518 (1), p.305-331

2022

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PRECISION MEASURES OF THE PRIMORDIAL ABUNDANCE OF DEUTERIUM

The Astrophysical journal, 2014-01, Vol.781 (1), p.1-16

2014

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PRECISION MEASURES OF THE PRIMORDIAL ABUNDANCE OF DEUTERIUM

The Astrophysical journal, 2014-01, Vol.781 (1), p.31

2014

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Discovery of the most metal-poor damped Lyman α system

Monthly notices of the Royal Astronomical Society, 2017-05, Vol.467 (1), p.802-811

2017

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Exploring the Environment of the most powerful Explosions

Proceedings of the International Astronomical Union, 2015-08, Vol.11 (A29B), p.261-262

2015

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Primordial Helium-3 Redux: The Helium Isotope Ratio of the Orion Nebula Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO program(s) 107.22U1.001, 194.C-0833

The Astrophysical journal, 2022-06, Vol.932 (1)

2022

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One Percent Determination of the Primordial Deuterium Abundance Based on observations collected at the W.M. Keck Observatory which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation

The Astrophysical journal, 2018-03, Vol.855 (2)

2018

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THE PRIMORDIAL DEUTERIUM ABUNDANCE OF THE MOST METAL-POOR DAMPED Ly SYSTEM∗ ∗ Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere, Chile (VLT program ID: 093.A-0016(A)), and at the W.M. Keck Observatory which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financia

The Astrophysical journal, 2016-10, Vol.830 (2)

2016

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MUSE Analysis of Gas around Galaxies (MAGG) – IV. The gaseous environment of z ∼ 3–4 Ly α emitting galaxies

Monthly notices of the Royal Astronomical Society, 2022-10, Vol.518 (1)

2022

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Detection of two interstellar polycyclic aromatic hydrocarbons via spectral matched filtering

Science (American Association for the Advancement of Science), 2021-03, Vol.371 (6535), p.1265-1269

2021

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On the lack of correlation between [O iii ]/[O ii ] and Lyman continuum escape fraction

Monthly notices of the Royal Astronomical Society, 2019-03, Vol.483 (4), p.5223-5245

2019

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One Percent Determination of the Primordial Deuterium Abundance

The PHLEK Survey: A New Determination of the Primordial Helium Abundance

MUSE Analysis of Gas around Galaxies (MAGG) – II: metal-enriched halo gas around z ∼ 1 galaxies

Searching for the Lowest-metallicity Galaxies in the Local Universe

The Little Cub: Discovery of an Extremely Metal-poor Star-forming Galaxy in the Local Universe

BIG BANG NUCLEOSYNTHESIS AND THE HELIUM ISOTOPE RATIO

THE PRIMORDIAL DEUTERIUM ABUNDANCE OF THE MOST METAL-POOR DAMPED Lyα SYSTEM

CARBON-ENHANCED METAL-POOR STARS: RELICS FROM THE DARK AGES

THE HISTORY OF R-PROCESS ENRICHMENT IN THE MILKY WAY

THE MOST METAL-POOR DAMPED Lyα SYSTEMS: AN INSIGHT INTO DWARF GALAXIES AT HIGH-REDSHIFT

Harvesting the Ly α forest with convolutional neural networks

MUSE Analysis of Gas around Galaxies (MAGG) – I: Survey design and the environment of a near pristine gas cloud at z ≈ 3.5

Origins of carbon-enhanced metal-poor stars

Primordial Helium-3 Redux: The Helium Isotope Ratio of the Orion Nebula

MUSE Analysis of Gas around Galaxies (MAGG) – IV. The gaseous environment of z ∼ 3–4 Ly α emitting galaxies

PRECISION MEASURES OF THE PRIMORDIAL ABUNDANCE OF DEUTERIUM

PRECISION MEASURES OF THE PRIMORDIAL ABUNDANCE OF DEUTERIUM

Discovery of the most metal-poor damped Lyman α system

Exploring the Environment of the most powerful Explosions

Primordial Helium-3 Redux: The Helium Isotope Ratio of the Orion Nebula Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO program(s) 107.22U1.001, 194.C-0833

MUSE Analysis of Gas around Galaxies (MAGG) – IV. The gaseous environment of z ∼ 3–4 Ly α emitting galaxies

Detection of two interstellar polycyclic aromatic hydrocarbons via spectral matched filtering

On the lack of correlation between [O iii ]/[O ii ] and Lyman continuum escape fraction

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