Visual stimuli were presented on a 21-inch CRT computer monitor. Each visual stimulus consisted of a 2 × 2 grid with three uniform gray homogeneous fields and one field with black-and-white square wave gratings (
Fig. 1). Each field was presented as a rectangular target easily distinguishable from the black background. All fields were the same size (8.2° × 6.15°), and the center of each field was 7.5° from the center of the screen (at a viewing distance of 83 cm). The separation between two adjacent targets was 4.6 cm (3.2°). Luminance was measured with a luminance meter (model LS-100; Minolta, Osaka, Japan). The black-white Michelson contrast of the gratings ranged from 96% to 97%. The luminance of the black stripes was 6.75 cd/m
2 (i.e., similar to the background), whereas the luminance of the white stripes, which was measured at three different positions, varied from 384 cd/m
2 to 405 cd/m
2 (average, 393 cd/m
2; 2.6 log cd/m
2). The luminance of the gray fields varied from a minimum of 190 cd/m
2 to a maximum of 210 cd/m
2 (average, 200 cd/m
2). The maximum difference between the space-average luminance of the three gray fields in each visual stimulus was <5%. For each visual stimulus, the space-average luminance of the field with the gratings was within 2% of the space-average luminance of the average of the three gray fields. Given that the differences in space average luminance among the plain fields were similar to or larger than the differences in space average luminance between the plain fields and the field with the gratings, subjects could not use luminance as a cue to determine the field with the gratings. The field with the gratings could appear randomly at 1 of 4 positions.
The 14 spatial frequencies used were 1.5, 2.3, 3.12, 4.68, 6.24, 9.36, 12.48, 14.62, 18.73, 21.06, 24.96, 29.25, 32.76, and 35.1 cyc/deg at a distance of 83 cm. This large range of frequencies was used to build the probability density functions (see Results). The range of spatial frequencies was similar to the range of spatial frequencies tested by the TAC at 55 cm (0.31, 0.42, 0.63 0.84, 1.30, 1.60, 2.40, 3.10, 4.70, 6.40, 9.60, 13.00, 19.00, 26.00, 38.00) with higher spatial frequencies added (21.06, 29.25, 32.76) and lower spatial frequencies deleted (0.31, 0.42, 0.63, 0.84). This was done to improve the resolution of the measurements when testing adults because their VA would lie in the higher spatial frequencies whereas the range provided by the TAC is sparse at these higher spatial frequencies. For graphic purposes, the spatial frequencies were converted from cycles per degree to the log of the minimum angle of resolution (logMAR). The minimum angle of resolution is expressed in minutes of arc (1 min arc = 1/60th of a degree); thus, logMAR = log (60/spatial frequency of gratings * 2).
A remote gaze-tracking system was used to monitor and estimate the subject's visual scanning parameters (Vision 2020; El-Mar Inc., Toronto, Canada). The gaze estimation system extracts eye features from video images and uses these features to estimate gaze position. The features extracted are the pupil center and two or more corneal reflexes. The corneal reflexes are virtual images of infrared light sources illuminating the eye and are created by the front surface of the cornea. The gaze-tracking system allows free head movements in a volume of 25 * 25 * 25 cm
3 and estimates gaze position at a rate of 30 Hz with accuracy better than 1°.
23 –25 The system was optimized to measure the point-of-gaze in infants and young children (i.e., calibration routine requires only one point).
The relative fixation time (RFT), which is defined as the percentage of fixation time on the field with the gratings over the sum of fixation times on all four fields, was used to quantify visual scanning behavior.