ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:2007.003] SPARTA: Subhalo and PARticle Trajectory Analysis

SPARTA is a post-processing framework for particle-based cosmological simulations. The code is written in pure, MPI-parallelized C and is optimized for high performance. The main purpose of SPARTA is to understand the formation of structure in a dynamical sense, namely by analyzing the trajectories (or orbits) of dark matter particles around their halos. Within this framework, the user can add analysis modules that operate on individual trajectories or entire halos. The initial goal of SPARTA was to compute the splashback radius of halos, but numerous other applications have been implemented as well, including spherical overdensity calculations and tracking subhalos via their constituent particles.

Code site:
http://www.benediktdiemer.com/code/sparta/ https://bitbucket.org/bdiemer/sparta
Described in:
https://ui.adsabs.harvard.edu/abs/2017ApJS..231....5D https://ui.adsabs.harvard.edu/abs/2020ApJS..251...17D
Bibcode:
2020ascl.soft07003D

Views: 2753

ascl:2007.003
Add this shield to your page
Copy the above HTML to add this shield to your code's website.