Aaron Smith

Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift

The THESAN project: Lyman-alpha emitters as probes of ionized bubble sizes

The <scp>thesan-zoom</scp> project: mystery N/O more – uncovering the origin of peculiar chemical abundances and a not-so-fundamental metallicity relation at 3 &amp;lt; <i>z</i> &amp;lt; 12

The <scp>thesan-zoom</scp> project: The Hidden Neighbours of O  <scp>i</scp> Absorbers during Reionization

The <scp>thesan-zoom</scp> project: burst, quench, repeat – unveiling the evolution of high-redshift galaxies along the star-forming main sequence

The <scp>thesan-zoom</scp> project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe

The <scp>thesan-zoom</scp>  project: Population III star formation continues until the end of reionization

The <scp>thesan</scp> project: tracking the expansion and merger histories of ionized bubbles during the Epoch of Reionization

The <scp>thesan–zoom</scp> project: long-term imprints of external reionization on galaxy evolution

Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies

The <scp>thesan-zoom</scp> project: star formation efficiencies in high-redshift galaxies

The galaxy-IGM connection in THESAN: the physics connecting the IGM Lyman- <a:math xmlns:a="http://www.w3.org/1998/Math/MathML"> <a:mi>α</a:mi> </a:math> opacity and galaxy density in the reionization epoch

High-redshift AGN population in radiation-hydrodynamics simulations

RIGEL: Feedback-regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger

The <scp>thesan</scp> project: galaxy sizes during the epoch of reionization

The <scp>thesan</scp> project: public data release of radiation-hydrodynamic simulations matching reionization-era <i>JWST</i> observations

The <scp>thesan</scp> project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization

The nature of diffuse ionized gas in star-forming galaxies

Adapting <scp>arepo-rt</scp> for exascale computing: GPU acceleration and efficient communication

The MillenniumTNG project: the galaxy population at <i>z</i> ≥ 8

The <scp>thesan</scp> project: ionizing escape fractions of reionization-era galaxies

<scp>thesan-hr</scp>: galaxies in the Epoch of Reionization in warm dark matter, fuzzy dark matter, and interacting dark matter

<scp>thesan-hr</scp>: how does reionization impact early galaxy evolution?

Simulating ionization feedback from young massive stars: impact of numerical resolution

The <scp>thesan</scp> project: Lyman-α emitter luminosity function calibration

Bridging the Gap between Cosmic Dawn and Reionization Favors Models Dominated by Faint Galaxies

The<scp>thesan</scp>project: properties of the intergalactic medium and its connection to reionization-era galaxies

The<scp>thesan</scp>project: Lyman-α emission and transmission during the Epoch of Reionization

H<i>α</i>emission in local galaxies: star formation, time variability, and the diffuse ionized gas

The <scp>thesan</scp> project: predictions for multitracer line intensity mapping in the epoch of reionization