Figure 3.21: A comparison of the cosmic dispersion added for stars solved with
the stochastic solution in the old and the new solution. For new detections the F2
statistic is given for the old solution. These can be recognized as the horizontal
distributions in the lower part of the graph. To the left, these are mainly normal
5-parameters solutions (blue dots), t0 the right (blue-gree dots) are mainly 7- or
9-parameter solutions in the published data. The green dots represent solutions
classified as stochastic in both the published and the new reduction. The red dots
were classified as VIM solutions in the published data.