George D. Becker

First Constraints on Fuzzy Dark Matter from Lyman-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>α</mml:mi></mml:math> Forest Data and Hydrodynamical Simulations

Hydrogen reionization ends by <i>z</i> = 5.3: Lyman-α optical depth measured by the XQR-30 sample

A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems

The Evolution of O i over 3.2 &lt; z &lt; 6.5: Reionization of the Circumgalactic Medium

Discovery of Excess O<scp>i</scp>Absorption toward the \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=6.42$ \end{document} QSO SDSS J1148+5251

The XQR-30 metal absorber catalogue: 778 absorption systems spanning 2 ≲ <i>z</i> ≲ 6.5

Galaxies: Formation, Evolution, Phenomena

Astronomy and Astrophysical Research

Astrophysics and Star Formation Studies

Radio Astronomy Observations and Technology

Stellar, planetary, and galactic studies