Gravity Simulation (Galaxy Birth) in real time, N-Body and 1-Body
Dense Basis SED fitting
Zeus21: Lightning-fast simulations of cosmic dawn
sapphire is a JAX-based framework for modeling the dynamical phase space evolution of galaxy populations
Spherical Overdensity Aperture Processor: MPI parallel Python code to compute properties of halos in SWIFT n-body simulations
Estimating galaxy gas mass fractions using SDSS imaging
Learning astrophysics with top-k sparse feature networks (SFNets)
Using SDSS imaging to predict galaxy metallicity. Maintained by @jwuphysics @boada
The Meraxes semi-analytic galaxy formation model.
Flexible, fully bayesian stacking software for modelling of astronomical data sets
LLM-driven autonomous agent for automated spectral energy distribution (SED) modeling and interpretation of multi-band galaxy observations using CIGALE.
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
CCN UNet detector, intended to be applied to galaxy images to discover regions.
Implementation of the BarnesHut algorithm in Julia, with benchmark comparisons with the brute force algorithm.
A model for core formation in dark matter haloes and ultra-diffuse galaxies by outflow episodes
Parallelized direct N-body code in Python + Numba to simulate galaxy mergers with ~2×10⁵ particles
Quantifying the recoverable variance in star formation rate from 1.4 GHz radio continuum emission using VLA-COSMOS and MeerKAT data.
Implementation of starlight synthesis algorithms for galactic evolution analysis.
Systematic comparison of galaxies in cosmic voids versus dense "walls" using DESI DR1 data to investigate environmental quenching mechanisms in galaxy evolution.
Reproducible public-data stress tests of CO, [C I], and dust molecular-gas tracer calibrations using Dunne et al. (2022).
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