Update README.md

8e7ee7c6 · Diego Turrini · 8f0fa9f2 · 8e7ee7c6
Commit 8e7ee7c6 authored Dec 07, 2020 by Diego Turrini
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@@ -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)
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-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)