@@ -44,6 +44,5 @@ 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](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)
* 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)
