We fitted the Gaussian data and the
t 3 data separately and thus there were 1400 trials per data set (for each observer). We used a maximum likelihood procedure to find the best fits of the parameters, and we calculated the 95% confidence intervals of each parameter using bootstrap methods (Efron & Tibshirani,
1993).
The results of interest are the fits for the binned influences per dot on PSE for each of the two stimulus types.
Figure 6 shows the fits for each observer for each of the two stimulus types with bootstrapped 95% CI. The blue dashed diagonals connect the fits for the binned influences per dot on PSE for the simple center-of-gravity (COG) model. The figure also shows the mean influence of each bin across all observers (with 95% CI), for each of the two stimulus types.
In the results presented here, we divided the stimulus space into eight bins (four to the right of 0 and four to the left of 0), which, as noted above, means that we only fit and display four influence-per-dot parameters because of the symmetry assumption. As for the length of each bin, remember that we scaled the t 3 stimuli so that, on average, 90% of the dots appeared within the same region as 90% of the dots of the Gaussian stimuli. In the results presented here, we decided to divide the region that covers 90% of the dots into six bins and used two more bins, one on each side, to cover the remaining 10% of the dots. Thus, the length of each of the inner bins (labeled 1, 2, and 3), for both the Gaussian and the t 3 analyses, was 0.49°. There were six of these, three to the right of 0 (which are shown in the graph) and three to the left of 0 (which are not shown in the graph because they are defined symmetrically), and so the horizontal region covered by these bins was 2.9°. The length of the outermost bin (labeled 4) was 3.7°, extending from the end of bin 3 until the end of the display region, with the outermost bin on the left being defined symmetrically.
No difference was evident between observers who saw the Gaussian stimuli first (O1, O3, O4, O6, O7) and observers who saw the t 3 stimuli first (O2, O5). We ran two other observers who saw the t 3 stimuli first, but their precision (measured as the slope of the psychometric function) was much lower than the precision of the observers reported here. The fits for the influences-per-dot parameters for these two observers were similar to those of the seven observers whose results are shown, but with markedly larger confidence intervals. Hence, we omit them from the graphical summary of data.
Most observers' fits for the influence-per-dot parameters were not significantly different from that predicted by the COG model for either of the two stimulus types (p > 0.05 based on 95% bootstrapped CI). Only one observer (O2) had significantly less influence per dot for the outermost bin than that predicted by COG for both stimulus types (p < 0.05 based on 95% bootstrapped CI). One other observer (O6) had less influence per dot for the outermost bin than that predicted by COG only for the t 3 condition and not for the Gaussian condition.
An interesting result that we did not expect was the over-weighting of the outermost bin for the Gaussian stimuli by two observers (O5 and O7). One possibility is that these observers might be basing their estimate in part on the convex hull of the cluster (the smallest convex region containing all the dots of the cluster). Such a strategy could yield very high influences for the outermost bins when fitting the data with our GLM. (It has previously been shown that saccades to highly non-uniform dot clusters tend to land at the COG of the
shape implied by the dot cluster, rather than the COG of the dots themselves; see Melcher & Kowler,
1999.) These observers were evidently not using an outlier-robust method in estimating the center.
A second interesting result that we did not expect was the down-weighting of the innermost dots (bin 1) for many of the observers. We suspect that this is due to the fact that the cluster is very dense in the innermost bins. Hence, a decrease in influence per dot could occur due to crowding (McGowan et al.,
1998).