The predicted values of
were converted to MacLeod-Boynton coordinates and tested against the empirical matches. In
Figure 6 the empirical means (pluses) and the ±1
SD ellipses are replotted on the same axes as
Figure 5. The other symbols near the plusses show the model predictions for
n = 0 (inverted triangles representing the gray world model) and
n = 10 (upright triangle representing the brightness weighting model). Note that there are no free parameters in either model. The value of n that determines the selectivity of brightness weighting is fixed for each model. Two considerations apply in testing the models. First, any prediction that is more than 2
SD from the mean can be rejected as a good fit. By this criterion, hardly any of the predictions from either model are rejected. However, given the large sizes of the ellipses for this data set, this test is not very selective. The second consideration is that the pattern of predictions from a model should be close to the pattern of the empirical means. Both models do fairly well in this regard, and the brightness-weighted model (
n = 10) does not provide a significantly better explanation for illuminant color estimation. The predictions for
n = 1 were very similar to those for
n = 0, and the predictions for
n = 100 were very similar to those for
n = 10. The predominant discrepancy seems to be that the matched chromaticity is less saturated than the predicted chromaticity. This may be due to the desaturating effects of adaptation to chromatic variations, which, in this study, are present only on the side with the Standard filter (Krauskopf , Williams, & Heeley,
1982; Webster & Mollon,
1997; Zaidi, Spehar, & DeBonet,
1997,
1998). This possibility points out that a proper brightness-weighting model should incorporate better estimates of the brightness and color appearance of different surfaces, and both estimates are likely to be nonlinear functions of cone-absorptions.
Equations 9–
11 are just an approximation to this class of models. Note that, for the biased backgrounds, the model predictions are not good estimates of the veridical matches shown in
Figure 5. It is worth pointing out that for
n = ∞, we are explicitly not claiming that the brightest surface appears as the illumination source. Identification of the illumination source depends on geometric factors like fuzzy borders (Zavagno,
1999), which are not present in our displays. In their gamut matching simulations, Tominaga et al. (
2001) found it useful to scale the intensity of all images to keep them within similar ranges; in the human visual system, retinal processes like photoreceptor adaptation and center surround receptive fields provide automatic intensity scaling for later visual processing.