GYRE is a suite of stellar oscillation codes built on a new Magnus Multiple Shooting scheme, which is robust, accurate (up to 6th order in grid spacing), and makes efficient use of computational resources (multiple cores and/or cluster nodes). The suite is written in Fortran 2008, with an object oriented architecture that is simple, clean, modular and adherent to modern coding best practices. The code is described in detail in Townsend & Teitler (2013, MNRAS, 435, 3406).
For the most up-to-date information on GYRE's capabilities, please see the Capabilities page.
- Namelist Input Files
- Stellar Model Files
- Output Files
- Variables & Equations
- Frequently Asked Questions
- Release Notes
- Documentation for previous releases
- The GYRE discussion forums (for bug reports, etc)
- The MESA SDK Software Development Kit
- The MESA Stellar Evolution Code
- The Mercurial branching stragegy providing the basis for the GYRE development model
GYRE has been developed with support from the Astronomy & Astrophysics Grants (AAG) program of the National Science Foundation, through awards AST-0908688 and AST-0904607.