************* Preliminaries ************* Intended Audience ================= This manual is aimed at a broad audience --- whether you're a GYRE novice or a seasoned veteran, it provides you with the information you'll need to get the most out of GYRE. However, it does presume some experience with Unix command-line environments, and likewise some basic familiarity with the subject of stellar oscillations. If you need the former, then the Internet is your oyster; and for the latter, we recommend the following online resources: * Jørgen Christensen-Dalsgaard's `Lecture Notes on Stellar Oscillations `__; * Gerald Handler's `Asteroseismology `__ article. Obtaining GYRE ============== The source code for GYRE is hosted in the :git:`rhdtownsend/gyre` git repository on :git:`GitHub <>`. GYRE is free software: you can redistribute it and/or modify it under the terms of the `GNU General Public License `__ as published by the `Free Software Foundation `__, version 3. .. _citing-gyre: Citing GYRE =========== If you use GYRE in your research, please cite one or more of the relevant 'instrument' papers: * :ads_citet:`townsend:2013` describes the basic operation of the code; * :ads_citet:`townsend:2018` outlines capabilities for :ref:`non-adiabatic oscillation ` calculations; * :ads_citet:`goldstein:2020` describes the :ref:`contour method ` for finding non-adiabatic modes; * :ads_citet:`sun:2023` introduces the :ref:`gyre_tides frontend ` for evaluating tidal responses. If you find yourself using GYRE on a regular basis, you might consider contributing to the project to ensure its long-term success. Options include * contributing code to the project (e.g., via GitHub pull requests), to extend GYRE's capabilities; * contributing documentation and tutorials to the project, to make GYRE more user-friendly; * inviting the GYRE team to be co-authors on relevant papers; * inviting the GYRE team to be co-investigators on relevant grant applications. Development Team ================ GYRE remains under active development by the following team: * `Rich Townsend `__ (University of Wisconsin-Madison); project leader * `Warrick Ball `__ (University of Birmingham) * `Ritvik Narayan `__ (UW-Madison) * `Jarret Rosenberg `__ (University of Wisconsin-Madison) * `Meng Sun `__ (National Astronomical Observatories of Chinese Academy of Sciences) Former developers include: * `Earl Bellinger `__ (MPIA Garching) * Jacqueline Goldstein (MIT) * Zhao Guo (Cambridge University) * Rianna Kuenzi (University of Wisconsin-Madison) * Mathias Michielsen (KU-Leuven) * Joel Ong (University of Hawaii-Manoa) * Vincent Vanlaer (KU-Leuven) Also, the following people have made valuable contributions toward testing GYRE: * Siemen Burssens (KU Leuven) * Timothy Van Reeth (KU Leven) Related Links ============= * The `GYRE discussion forums `__, the place to post feature requests and bug reports (don't send emails!). * The `MESA Software Development Kit (SDK) `__, which provides the compilers and supporting libraries needed to build GYRE. * The `MESA Stellar Evolution Code `__, which can generate stellar models readable by GYRE. Acknowledgments ================ GYRE has been developed with financial support from the following grants: * NSF awards AST-0908688, AST-0904607, ACI-1339606, ACI-1663696, and AST-1716436; * NASA awards NNX14AB55G, NNX16AB97G, 80NSSC20K0515 and 80NSSC24K0895. GYRE has also benefited greatly from contributions (code, bug reports, feature requests) from the academic community. Thanks, folks!