MAGGPY
This tutorial introduces MAGGPY as a framework to connect BNS population models with short GRB observations. Users will learn how to generate synthetic GRB catalogs using different jet geometries and detector sensitivities (e.g. Fermi-GBM), infer jet launching efficiencies, and test the consistency of progenitor models. The tutorial also demonstrates how to interface MAGGPY catalogs with GWFish to make joint detection predictions for current and next-generation gravitational-wave observatories, highlighting applications and impact on multi-messenger studies
The material used in ACME tutorials is available here:

Funded by the European Union. Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or of the European Research Executive Agency (REA). Neither the European Union nor the granting authority can be held responsible for them. The ACME project has received funding from the European Union’s Horizon Europe Research and innovation programme under Grant Agreement No 101131928.
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