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The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: the z = 9 luminosity function and further evidence for a smooth decline in ultraviolet luminosity density at z≥ 8

Monthly notices of the Royal Astronomical Society, 2016-07, Vol.459 (4), p.3812-3824

2016

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A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10

Monthly notices of the Royal Astronomical Society, 2020-04, Vol.493 (2), p.2059-2084

2020

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New redshift z ≃ 9 galaxies in the Hubble Frontier Fields: implications for early evolution of the UV luminosity density

Monthly notices of the Royal Astronomical Society, 2015-07, Vol.450 (3), p.3032-3044

2015

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Unveiling the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope

Monthly notices of the Royal Astronomical Society, 2017-04, Vol.466 (3), p.3612-3635

2017

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The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3

Monthly notices of the Royal Astronomical Society, 2019-11, Vol.490 (1), p.417-439

2019

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A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses, and star-formation histories

Monthly notices of the Royal Astronomical Society. Letters, 2022-11, Vol.518 (1), p.L45-L50

2022

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The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5

Monthly notices of the Royal Astronomical Society, 2022-05, Vol.513 (3), p.3510-3525

2022

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The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging

Monthly notices of the Royal Astronomical Society, 2023, Vol.518 (4), p.6011-6040

2023

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The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys

Monthly notices of the Royal Astronomical Society, 2021-05, Vol.503 (3), p.4413-4435

2021

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Obscured star formation in bright z ≃ 7 Lyman-break galaxies

Monthly notices of the Royal Astronomical Society, 2018-12, Vol.481 (2), p.1631-1644

2018

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The abundance of z ≳ 10 galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging

Monthly notices of the Royal Astronomical Society, 2023-02, Vol.520 (3), p.4554-4561

2023

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The evolution of the equivalent width of the Hα emission line and specific star formation rate in star-forming galaxies at 1 < z < 5

Monthly notices of the Royal Astronomical Society, 2016-08, Vol.460 (4), p.3587-3597

2016

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A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS

Monthly notices of the Royal Astronomical Society, 2023-02, Vol.520 (3), p.3974-3985

2023

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The ultraviolet continuum slopes (β) of galaxies at z ≃ 8-16 from JWST and ground-based near-infrared imaging

Monthly notices of the Royal Astronomical Society, 2023-03, Vol.520 (1), p.14-23

2023

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Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5

Monthly notices of the Royal Astronomical Society, 2020-07, Vol.496 (1), p.695-707

2020

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The relationship between dust and [C i ] at z = 1 and beyond

Monthly notices of the Royal Astronomical Society, 2019-01, Vol.482 (3), p.3135-3161

2019

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The evolution of the equivalent width of the Ha emission line and specific star formation rate in star-forming galaxies at 1 < z < 5

Monthly notices of the Royal Astronomical Society, 2016-08, Vol.460 (4), p.3587-3587

2016

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The galaxy UV luminosity function at z ≃ 11 from a suite of public JWST ERS, ERO, and Cycle-1 programs

Monthly notices of the Royal Astronomical Society, 2024-01, Vol.527 (3), p.5004-5022

2024

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The NIRVANDELS Survey: a robust detection of α-enhancement in star-forming galaxies at z ≃ 3.4

Monthly notices of the Royal Astronomical Society, 2021-07, Vol.505 (1), p.903-920

2021

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The VANDELS survey: the ionizing properties of star-forming galaxies at 3 ≤ z ≤ 5 using deep rest-frame ultraviolet spectroscopy

Monthly notices of the Royal Astronomical Society, 2023-05, Vol.522 (4), p.6295-6325

2023

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A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass, and age from z = 0.6 to z = 1.3

Monthly notices of the Royal Astronomical Society, 2022-03, Vol.512 (1), p.1262-1274

2022

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No evidence for Population III stars or a direct collapse black hole in the z = 6.6 Lyman α emitter ‘CR7’

Monthly notices of the Royal Astronomical Society, 2017-07, Vol.469 (1), p.448-458

2017

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Connecting the escape fraction of Lyman-alpha and Lyman-continuum photons in star-forming galaxies at z ≃ 4–5

Monthly notices of the Royal Astronomical Society, 2023-11, Vol.527 (2), p.4040-4051

2023

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The VANDELS survey: a strong correlation between Ly α equivalent width and stellar metallicity at 3 ≤ z ≤ 5

Monthly notices of the Royal Astronomical Society, 2020-06, Vol.495 (1), p.1501-1510

2020

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The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10

Monthly notices of the Royal Astronomical Society, 2024-05, Vol.531 (1), p.997-1020

2024

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The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: the z = 9 luminosity function and further evidence for a smooth decline in ultraviolet luminosity density at z≥ 8

A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10

New redshift z ≃ 9 galaxies in the Hubble Frontier Fields: implications for early evolution of the UV luminosity density

Unveiling the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope

The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3

A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses, and star-formation histories

The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5

The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging

The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys

Obscured star formation in bright z ≃ 7 Lyman-break galaxies

The abundance of z ≳ 10 galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging

The evolution of the equivalent width of the Hα emission line and specific star formation rate in star-forming galaxies at 1 < z < 5

A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS

The ultraviolet continuum slopes (β) of galaxies at z ≃ 8-16 from JWST and ground-based near-infrared imaging

Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5

The relationship between dust and [C i ] at z = 1 and beyond

The evolution of the equivalent width of the Ha emission line and specific star formation rate in star-forming galaxies at 1 < z < 5

The galaxy UV luminosity function at z ≃ 11 from a suite of public JWST ERS, ERO, and Cycle-1 programs

The NIRVANDELS Survey: a robust detection of α-enhancement in star-forming galaxies at z ≃ 3.4

The VANDELS survey: the ionizing properties of star-forming galaxies at 3 ≤ z ≤ 5 using deep rest-frame ultraviolet spectroscopy

A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass, and age from z = 0.6 to z = 1.3

No evidence for Population III stars or a direct collapse black hole in the z = 6.6 Lyman α emitter ‘CR7’

Connecting the escape fraction of Lyman-alpha and Lyman-continuum photons in star-forming galaxies at z ≃ 4–5

The VANDELS survey: a strong correlation between Ly α equivalent width and stellar metallicity at 3 ≤ z ≤ 5

The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10

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