The data shown in
Figure 5 do not indicate lightness constancy. If the observers’ matches were lightness constant, each standard would always be matched with the same palette reflectance, leading to normalized relative match versus slant curves that consisted of horizontal lines (i.e.,
, red broken line in each panel). None of the observers’ data are well described by a horizontal line.
Another useful comparison for observer performance is the prediction obtained by assuming that observers make their matches in proportion to the luminance reflected from the standard (luminance matching). In this case, the data should be fit by a scaled version standard card luminance as a function of slant. The predictions for luminance matching are shown in
Figure 5 as blue, broken lines. For each observer, the predicted curve has been scaled to provide the best fit to that observer’s data.
Observer BST comes close to exhibiting luminance matching. The other observers all show deviations from luminance matching in the general direction of lightness constancy. The data from observers FGS and GYD come close to being constant over a range of standard object slants (−45° to +45°) but deviate substantially as the slant increases to +60°. Other observers exhibit behavior that varied between these extrema.
To provide a sense of how observers vary between luminance matching and lightness constancy, we derived a simple error-based constancy index. We found for each of the three sessions, the normalized relative matches for that session. Let
represent the sum of squared errors between the luminance matching prediction (blue broken lines in
Figure 5) and the individual session data for a single observer. Similarly, let
be the sum of squared errors for the constancy prediction (red broken lines in
Figure 5). then
is a constancy index that takes on a value of 0 when the data are perfectly characterized as luminance matches and a value of 1 when the data reveal perfect constancy. For
Experiment 1, the index ranges between 0.17 and 0.54, with a mean of 0.35 and median of 0.33.
Table 1 provides the index values for all experiments reported in this paper. Error-based constancy indices for each observer are provided in
Figure 5. Interpretation of the index should be tempered against the observation that the index definition is somewhat arbitrary and that no single number can capture the richness of the data. In the companion study, we present model-based summary measures of the individual variation.
The mean data (across observers) from
Experiment 1 are plotted in
Figure 7 below. This plot also reveals performance that is intermediate between luminance matching and lightness constancy, but it should again be emphasized that individual variation around the mean is large.