Open simulation tools are a core research output. They exist to make the phenomenology testable, and they are used by the neutrino-telescope community to model detectors that do not yet exist and the environments they will be built in. Listed here are the codes built for general use. Analysis code for individual papers lives on GitHub.
Neutrino-telescope effective areas from muon transport, without a detector simulation.
Solves high-energy muon transport analytically and turns the muon range into the volume a detector effectively watches, giving effective areas, event rates and single-track energies. One code serves IceCube, KM3NeT/ARCA, P-ONE, TRIDENT and Baikal-GVD, so published effective areas can be reproduced, explained and carried to detectors that have not been simulated yet. Author and maintainer.
Open-source, end-to-end simulation framework for neutrino telescopes.
Generates events and detection-module photon hits for user-defined detector geometries in water or ice. Lead developer and current maintainer. Released publicly (Comput. Phys. Commun. 2024) and adopted as a community baseline, including for the NuBench event-reconstruction benchmark.
Check a BibTeX file against INSPIRE and fix what is wrong.
Command-line tool that checks every entry of a .bib file against InspireHEP, flags missing or mismatched records, suggests canonical replacements and writes a corrected file. Author and maintainer.
Open tools for training students and running a research group.
A physics-first starting kit for early-career researchers.
Short guides, templates, examples and exercises in seven tracks. They cover reading arXiv papers, journal clubs, writing papers, Git and GitHub, coding practices, plotting, and working with LLMs. Used to onboard new students. Author and maintainer.
