Dr Harley Katz: Publications

Simulating the diversity of shapes of the Lyman-α line

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 523:3 (2023) 3749-3772

Authors:

Jérémy Blaizot, Thibault Garel, Anne Verhamme, Harley Katz, Taysun Kimm, Léo Michel-Dansac, Peter D Mitchell, Joakim Rosdahl, Maxime Trebitsch

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The physics of indirect estimators of Lyman Continuum escape and their application to high-redshift JWST galaxies

(2023)

Authors:

Nicholas Choustikov, Harley Katz, Aayush Saxena, Alex Cameron, Julien Devriendt, Adrianne Slyz, Joki Rosdahl, Jeremy Blaizot, Leo Michel-Dansac

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A novel approach to correcting Te-based mass–metallicity relations

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 522:1 (2023) l89-l94

Authors:

Alex J Cameron, Harley Katz, Martin P Rey

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Evidence for a Low Lyman Continuum Escape Fraction in Three Massive, Ultraviolet-bright Galaxies at z > 7

The Astrophysical Journal American Astronomical Society 944:1 (2023) 61

Authors:

Callum EC Witten, Nicolas Laporte, Harley Katz

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First insights into the ISM at z > 8 with JWST: possible physical implications of a high [O iii] λ4363/[O iii] λ5007

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 518:1 (2022) 592-603

Authors:

Harley Katz, Aayush Saxena, Alex J Cameron, Stefano Carniani, Andrew J Bunker, Santiago Arribas, Rachana Bhatawdekar, Rebecca AA Bowler, Kristan NK Boyett, Giovanni Cresci, Emma Curtis-Lake, Francesco D’Eugenio, Nimisha Kumari, Tobias J Looser, Roberto Maiolino, Hannah Übler, Chris Willott, Joris Witstok

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Dr Harley Katz

Sub department

Simulating the diversity of shapes of the Lyman-α line

Authors:

The physics of indirect estimators of Lyman Continuum escape and their application to high-redshift JWST galaxies

Authors:

A novel approach to correcting Te-based mass–metallicity relations

Authors:

Evidence for a Low Lyman Continuum Escape Fraction in Three Massive, Ultraviolet-bright Galaxies at z > 7

Authors:

First insights into the ISM at z > 8 with JWST: possible physical implications of a high [O iii] λ4363/[O iii] λ5007

Authors:

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