Accelerated Reionization Era Simulations

High-performance, multithreaded C++ library with a Python interface designed for the rapid visualization of Smoothed Particle Hydrodynamics (SPH) simulations.

C++ and JavaScript N-body dark matter simulations testing the dark matter hypothesis through NFW halo concentration analysis and Baryons-only comparative modelling

Emerge - the smooth empirical model for galaxy formation

Mock cone facility for astrophysical applications

A model for core formation in dark matter haloes and ultra-diffuse galaxies by outflow episodes

A modular, data-agnostic toolkit for converting N-body simulation merger trees from various formats (ASCII, Binary, HDF5) and tool-chains (AHF, Rockstar, Subfind, Gadget-4) into SAGE-compatible HDF5 and binary files.

The inference code for our Nature paper about globular clusters in M31/Andromeda.

MPhys Thesis (Durham University, supervised by Prof. Richard Bower)

Fork of the public version of the GIZMO multi-physics massively-parallel code that includes primordial black hole evaporation feedback (PBHEF)

Orbit Super Position Modeling Package based off of Dr. Karl Gebhardt's fortran code and the code used in https://iopscience-iop-org.libweb.lib.utsa.edu/article/10.3847/2041-8213/ae0b4f/meta

A simple Python simulation of cosmic metallicity evolution using Astropy and Planck 2024 cosmology. Demonstrates exponential chemical enrichment, sensitivity to physical parameters, and galaxy metallicity gradients—educational tool for astrophysics and fine-tuning studies.

Code and data for the "entropy plateaus" paper (Altamura et al. 2025)

Analysis of the stellar-to-halo mass relation in synthetic central and satellite galaxies across redshifts z=0 to z=1 using the SHARK semi-analytic model.

James Webb Space Telescope Impossible Ancient Galaxies Resolution

Code for MSci Project "Powerful AGN outflows at cosmic noon can solve the S_8 tension?"

A collection of data and scripts for our analysis of the gas accretion rates in the Hestia simulations.

Código utilizado para generar (algunas de) las figuras mostradas en la charla "Historia de acreción de gas en los discos estelares de las galaxias tipo Vía Láctea de las simulaciones Auriga", presentada en la Reunión Anual de la Asociación Argentina de Astronomía durante septiembre de 2022.