Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Reionization, Redshift, and Star formation.
Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST’s massive UV-bright galaxies
Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
The <scp>thesan</scp> project: environmental drivers of Local Group reionization
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 &lt; <i>z</i> &lt; 12
The <scp>thesan-zoom</scp> project: The Hidden Neighbours of O <scp>i</scp> Absorbers during Reionization
The <scp>thesan</scp> project: environmental drivers of Local Group reionization
Identifying Signatures of Inflow onto Face-on Galaxies Using the Balmer Decrement
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
High-redshift millennium and astrid galaxies in effective field theory at the field level
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 <scp>thesan-zoom</scp> project: star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
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 MillenniumTNG project: impact of massive neutrinos on the cosmic large-scale structure and the distribution of galaxies
Measuring the splashback feature: Dependence on halo properties and history
Evolution of cosmic filaments in the MTNG simulation
The boundary of cosmic filaments
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 impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0 &lt; <i>z</i> &lt; 7