Cambridge University Press (CUP), Proceedings of the International Astronomical Union, A29A(11), p. 200-200, 2015
DOI: 10.1017/s1743921316002787
Full text: Unavailable
AbstractTransiting candidate validation is essentially a Bayesian model comparison problem: different models, all explaining the observations comparably well, compete for the support of the available data. The basic characteristics of the planet validation problem are discussed and the different approaches taken to tackle its difficulties are reviewed.