@@ -44,5 +44,6 @@ If the program is run using the test input files supplied with DPI, the energy e
When using the DPI library please cite both the following references:
Turrini, D. (2015). DPI: Symplectic mapping for binary star systems for the Mercury software package. Astrophysics Source Code Library. ascl:1504.012
Turrini, D., Barbieri, M., Marzari, F., Thebault, P., Tricarico, P. (2005). Planetary Formation and Orbital Stability in Binary Star Systems. Memorie della Società Astronomica Italiana Supplementi 6, 172.
Turrini, D. (2015). DPI: Symplectic mapping for binary star systems for the Mercury software package. Astrophysics Source Code Library. [ascl:1504.012](http://ascl.net/1504.012). ADS Bibcode: [2015ascl.soft04012T](https://ui.adsabs.harvard.edu/abs/2015ascl.soft04012T/abstract)
Turrini, D., Barbieri, M., Marzari, F., Thebault, P., Tricarico, P. (2005). Planetary Formation and Orbital Stability in Binary Star Systems. Memorie della Società Astronomica Italiana Supplementi 6, 172. ADS Bibcode: [2005MSAIS...6..172T](https://ui.adsabs.harvard.edu/abs/2005MSAIS...6..172T/abstract)
