Prediction in the evolution of the logarithm of the Bayes factor in a real case of the KOBE experiment, assuming a planet at Ppeak = 94.13 d. The number of observations and the time it takes to detect the planet are compared using three different strategies: KOBEsim (K), KOBEsim beta (K_β), and spacing the observations in a fixed cadence (MC) of 6 d. Planet detection criterion: ln(B₁₀) > 6.