SOAP: A Python Package for Calculating the Properties of Galaxies and Halos Formed in Cosmological Simulations
Robert McGibbon, John C. Helly, Joop Schaye, Matthieu Schaller, Bert Vandenbroucke

TL;DR
SOAP is a Python package that efficiently computes detailed properties of galaxies and halos from cosmological simulation data, supporting multiple definitions and parallel processing for large datasets.
Contribution
We introduce SOAP, a versatile Python tool that enables consistent, parallel analysis of galaxy and halo properties across various simulation types and halo definitions.
Findings
Supports multiple halo definitions including spherical overdensities and fixed apertures.
Provides parallel processing capabilities for large datasets.
Compatible with dark matter-only and hydrodynamic simulations.
Abstract
Modern large scale cosmological hydrodynamic simulations require robust tools capable of analysing their data outputs in a parallel and efficient manner. We introduce SOAP (Spherical Overdensity and Aperture Processor), a Python package designed to compute halo and galaxy properties from SWIFT simulations after being post-processed with a subhalo finder. SOAP takes a subhalo catalogue as input and calculates a wide array of properties for each object. SOAP offers parallel processing capabilities via mpi4py for efficient handling of large datasets, and allows for consistent property calculation across multiple halo finders. SOAP supports various halo definitions, including spherical overdensities and fixed physical apertures, providing flexibility for diverse observational comparisons. The package is compatible with both dark matter-only and full hydrodynamic simulations, producing HDF5…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
