%0 Generic %1 compas2021rapid %A COMPAS, Team %A :, %A Riley, Jeff %A Agrawal, Poojan %A Barrett, Jim W. %A Boyett, Kristan N. K. %A Broekgaarden, Floor S. %A Chattopadhyay, Debatri %A Gaebel, Sebastian M. %A Gittins, Fabian %A Hirai, Ryosuke %A Howitt, George %A Justham, Stephen %A Khandelwal, Lokesh %A Kummer, Floris %A Lau, Mike Y. M. %A Mandel, Ilya %A de Mink, Selma E. %A Neijssel, Coenraad %A Riley, Tim %A van Son, Lieke %A Stevenson, Simon %A Vigna-Gomez, Alejandro %A Vinciguerra, Serena %A Wagg, Tom %A Willcox, Reinhold %D 2021 %K library %T Rapid stellar and binary population synthesis with COMPAS %U http://arxiv.org/abs/2109.10352 %X COMPAS (Compact Object Mergers: Population Astrophysics and Statistics, https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of isolated stellar binaries under a set of parametrised 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 which will be updated as new features are added to COMPAS; the current document describes COMPAS v02.21.00.

@misc{compas2021rapid, abstract = {COMPAS (Compact Object Mergers: Population Astrophysics and Statistics, https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of isolated stellar binaries under a set of parametrised 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 which will be updated as new features are added to COMPAS; the current document describes COMPAS v02.21.00.}, added-at = {2021-09-23T12:12:07.000+0200}, author = {COMPAS, Team and : and Riley, Jeff and Agrawal, Poojan and Barrett, Jim W. and Boyett, Kristan N. K. and Broekgaarden, Floor S. and Chattopadhyay, Debatri and Gaebel, Sebastian M. and Gittins, Fabian and Hirai, Ryosuke and Howitt, George and Justham, Stephen and Khandelwal, Lokesh and Kummer, Floris and Lau, Mike Y. M. and Mandel, Ilya and de Mink, Selma E. and Neijssel, Coenraad and Riley, Tim and van Son, Lieke and Stevenson, Simon and Vigna-Gomez, Alejandro and Vinciguerra, Serena and Wagg, Tom and Willcox, Reinhold}, biburl = {https://www.bibsonomy.org/bibtex/21be9c067b7b74bc7d009f073e38baf3f/gpkulkarni}, description = {Rapid stellar and binary population synthesis with COMPAS}, interhash = {536d905e3546829a902b1270148b255b}, intrahash = {1be9c067b7b74bc7d009f073e38baf3f}, keywords = {library}, note = {cite arxiv:2109.10352Comment: Code publicly available via https://compas.science}, timestamp = {2021-09-23T12:12:07.000+0200}, title = {Rapid stellar and binary population synthesis with COMPAS}, url = {http://arxiv.org/abs/2109.10352}, year = 2021 }