In one subject (BMS), we attempted to see whether the observed OFRs could be quantitatively accounted for by our subtractive model (
Equation 3). To obtain the data required for such an analysis, we ran
Experiments 1B through
1D using stimuli that all had the same total size (approximately 25° × 25°) but comprised abutting strips of variable height. Panel A of
Figure A1 shows the normalized TF tuning (like in
Experiment 1B) obtained for 0.5-cpd sinusoidal gratings arranged in 0.4°- (pink open diamonds), 1.6°- (blue open squares), or 6.2°- (green filled diamonds) high strips.
12 Although gratings' strip heights differed 16-fold, their tuning was similar: The response is a separable function of TF and strip height. The strongest OFRs were recorded at 18.6 cycles/s.
13 Panel B of
Figure A1 shows the SF tuning curves (like in
Experiment 1C) for filtered noise stimuli whose strip heights ranged from 0.1° to 25° in two-octave increments (see the
Figure A1 insert for symbol definition). All dependences were fit by skewed Gaussian functions (median
r2 = 0.998, range = 0.984–1.000; see
Supplementary Table S7 for the full list of fit parameters) and revealed that, as the strip height increased, the peaks of the dependencies shifted toward lower central SFs (similar to findings of Sheliga et al.,
2013). Panel C of
Figure A1 shows results of an experiment similar to
Experiment 1D but run using filtered noise stimuli whose strip heights ranged from 0.1° to 25° in two-octave increments. Recall that in this experiment the pattern on the screen was a sum of two filtered noise stimuli: The first moved with the near-optimal TF, whereas the second was a new randomly chosen filtered noise sample substituted each frame (i.e., flicker). Panel C shows that an addition of flickering stimuli (larger symbols) strongly reduced the OFRs compared with moving stimuli presented in isolation (smaller symbols; 0.25 cpd central SF, shown on the ordinate axis). This effect depended on SF but did not depend on strip height. The data were well fit by semilog Gaussians (median
r2 = 0.943, range = 0.908–0.987). See
Supplementary Table S8 for the full list of the best-fit Gaussian parameters. Constraining the Gaussian peak SF and sigma parameters to be the same for stimuli of different strip height had minor impact; it led to a 1.1% (range = 0.1%–4.4%) drop in
r2 values. The best-fitting Gaussian amplitudes, on the other hand, varied considerably with strip height (range = 0.033°–0.053°) and, in fact, were linearly related to the OFR amplitudes to moving stimuli of different strip heights when those were presented in isolation (
r2 = 0.978; not shown). The changes in the amplitude of attenuation may reflect changes in the effective SF components that drive flicker, parallel to the changes in drive. Using the data from panels A through C of
Figure A1, it was possible to use
Equation 3 to predict the data for subject BMS in
Experiment 4 data (
r2 = 0.957; the entire data set was evaluated by a single fitting procedure).
14 The model dependence between the optimal strip height and speed of motion is shown in panel D of
Figure A1 using a black dashed line. This figure also replots subject BMS's experimentally measured curve from
Figure 10D (filled circles and solid lines) along with its 95% confidence interval (gray shaded area). The model fit provides a good account of the data, although it underestimates the steepness of the rise at the largest speeds. We also show the result of using the model without incorporating the effect of flicker (black dotted line), which produces similar results over most of the range. This suggests that there is little change in the balance of flicker and drive with strip height so that the effects we demonstrated with 1D noise (
Experiments 1 through
3) seem to have similar effects across this range of 2D stimuli.