{ "cells": [ { "cell_type": "markdown", "id": "c256186f", "metadata": {}, "source": [ "# Converting Arepo snapshots to be usable by TARDIS" ] }, { "cell_type": "markdown", "id": "b4ffa8ca", "metadata": {}, "source": [ "### What is [Arepo](https://arepo-code.org/)?\n", "> *Arepo is a massively parallel gravity and magnetohydrodynamics code for astrophysics, designed for problems of large dynamic range. It employs a finite-volume approach to discretize the equations of hydrodynamics on a moving Voronoi mesh, and a tree-particle-mesh method for gravitational interactions. Arepo is originally optimized for cosmological simulations of structure formation, but has also been used in many other applications in astrophysics.*\n", "\n", "(Weinberger, 2020)" ] }, { "cell_type": "markdown", "id": "e3b3a256", "metadata": {}, "source": [ "This parser is intended for loading Arepo output files ('snapshots'), extracting the relevant (line-of-sight dependent) data and exporting it to `csvy` files, which can in turn be used in TARDIS models ([see CSVY model](../index.rst#csvy-model))." ] }, { "cell_type": "markdown", "id": "e3ea3fbc", "metadata": {}, "source": [ "