Stability maps as function of the mass and eccentricity of each of the planet of the HD 23472 system. The stability criterion is given in Eq. (2). Blue is short-term stable while red is short-term unstable. For each map, the parameters of the rest of the system are set to the nominal value given in Table 1, except for the eccentricities that are set to zero. The white dashed lines show the 0.16–0.84 quantiles oftheposterior of the mass of each planet. Only the 0.84 quantile is shown for planets d and f.