Notes. The table corresponds to Fig. 10. The number of stars per bin, predicted for a uniform distribution, is given for the upper gray data (linear age, including upper limit data from vsini measurements), the upper black data (without data obtained from vsini), lower gray data (same as upper gray data for logarithmic age), and lower black data (without vsini data). The 0.05-confidence interval for each bin is given in the fourth column and the maximal value is shown for comparison. The maximal value indicates the peak of the concentration of coeval stars that is identified with the Her-Lyr association.