@@ -9,7 +9,7 @@ Note on this release: release 1.0 supplies the symplectic mapping for S-type bin
Disclaimer: the DPI library is supplied with a modified version of Mercury 6 for the convenience of the users; however, only those files whose name begins with "dpi" are property of the author and are released under GPL 3 license.
Disclaimer: the DPI library is supplied with a modified version of Mercury 6 for the convenience of the users; however, only those files whose name begins with "dpi" are property of the author and are released under GPL 3 license.
## USING DPI LIBRARY WITH MERCURY 6
## USING THE DPI LIBRARY WITH MERCURY 6
The use of DPI in conjunction with Mercury 6 should be straightforward for Mercury's users. Users not familiar with Mercury 6 are advised to first read Mercury's manual to get in touch with its working.
The use of DPI in conjunction with Mercury 6 should be straightforward for Mercury's users. Users not familiar with Mercury 6 are advised to first read Mercury's manual to get in touch with its working.
@@ -42,6 +42,7 @@ If the program is run using the test input files supplied with DPI, the energy e
## HOW TO CITE THE DPI LIBRARY
## HOW TO CITE THE DPI LIBRARY
When using the DPI library please cite it as:
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. (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.
