Left: comparison of the r₀₂ constraint with the models A3 and A4. Right: comparison of the r₁₀ constraint with the models A3 and A4. The data points seem clearly to agree with the model A3, a fact that was not established with the data of Bouchy & Carrier (2002). Indeed, all their points for the r₁₀ asteroseismic constraint were situated between the curves of the models A3 and A4 (see Miglio & Montalbán 2005).