ASCL Code Record
GWecc computes the pulsar timing array (PTA) signals induced by eccentric supermassive binaries. Written in C++, it computes the plus/cross polarizations as well as Earth and pulsar terms of the PTA signal given the binary parameters and the sky locations of the binary and the pulsar. A python wrapper is included through which GWecc can be used to simulate, search for and constrain gravitational wave-emitting eccentric supermassive binaries using packages such as ENTERPRISE (ascl:1912.015) and libstempo (ascl:2002.017).
GWecc is superseded by GWecc.jl and is no longer maintained.
- Code site:
- https://github.com/abhisrkckl/GWecc
- Described in:
- https://ui.adsabs.harvard.edu/abs/2020PhRvD.101d3022S https://ui.adsabs.harvard.edu/abs/2023CQGra..40o5014S
- Bibcode:
- 2020ascl.soft02013S
https://ui.adsabs.harvard.edu/abs/2020PhRvD.101d3022S , https://ui.adsabs.harvard.edu/abs/2023CQGra..40o5014S , https://ui.adsabs.harvard.edu/abs/2020ascl.soft02013S
