Rapid Stellar and Binary Population Synthesis with COMPAS
Abstract
Compact Object Mergers: Population Astrophysics and Statistics (COMPAS; https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of isolated stellar binaries under a set of parameterized assumptions in order to allow comparisons against observational data sets, such as those coming from gravitational-wave observations of merging compact remnants. It includes a number of tools for population processing in addition to the core binary evolution components. COMPAS is publicly available via the GitHub repository https://github.com/TeamCOMPAS/COMPAS/, and is designed to allow for flexible modifications as evolutionary models improve. This paper describes the methodology and implementation of COMPAS. It is a living document that will be updated as new features are added to COMPAS; the current document describes COMPAS v02.21.00.
- Publication:
-
The Astrophysical Journal Supplement Series
- Pub Date:
- February 2022
- DOI:
- 10.3847/1538-4365/ac416c
- arXiv:
- arXiv:2109.10352
- Bibcode:
- 2022ApJS..258...34R
- Keywords:
-
- 1622;
- 154;
- 1108;
- 162;
- Astrophysics - Instrumentation and Methods for Astrophysics;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- Code publicly available via https://compas.science . Minor updates to match version accepted to ApJS