1 code implementation • 12 Jun 2018 • Benjamin E. Nelson, Eric B. Ford, Johannes Buchner, Ryan Cloutier, Rodrigo F. Díaz, João P. Faria, Vinesh M. Rajpaul, Surangkhana Rukdee
We found the dispersion in $\widehat{\mathcal{Z}}$ across different methods grew with increasing $n$-planet models: $\sim\,$3 for 0-planets, $\sim\,$10 for 1-planet, $\sim\,$$10^2$-$10^3$ for 2-planets, and $>\,$$10^4$ for 3-planets.
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics
