When measuring detection and resolution thresholds, we used the Octopus 201 perimeter (Haag-Streit International, Köniz, Switzerland) combined with the space synoptophore (a modified haploscope device) developed by Iwai
11 (Fig. 1) . In this modified device, the refraction mirrors of the standard haploscope were replaced with half mirrors. We used the space synoptophore to confirm the binocular condition by projecting fusion patterns on the front of the half mirrors. The fusion patterns used were a 3° square for each eye, a 135° line for the left eye, and a 45° line for the right eye
(Fig. 2) . To project the fusion patterns, we removed the projection lamp of the space synoptophore and used the background luminance of the Octopus 201 perimeter. A parallel-line target was then projected on the cupola of the Octopus 201 perimeter with a background luminance of 4 apostilb (asb) and stimulus duration of 100 ms. Thresholds were determined using a 4-2-1 dB bracketing staircase measurement procedure. Three parallel-line targets with various widths and distances between the lines of 10′, 2.5′, or 1.43′ angle of vision and a length of 1.724° were used
(Fig. 2) . This system enabled us to confirm the conditions of binocular vision when measuring the visual sensitivities of the right and left eyes separately and together
(Fig. 1) . Fixation was checked in two ways. One was for the examiner to monitor the pupils’ positions of both eyes with a small infrared video camera. The measurement was to be continued only when the subject fixed the central fixation point within the cupola of the Octopus 201 under the binocular condition. The other was for the subject to push the button continuously. The subjects were instructed in advance to discontinue the measurement by continuously pushing the button as soon as the fusion patterns were perceived to be broken. In other words, the measurement would be discontinued if the subject’s fixation had shifted or if the subject had continuously pushed the button.
The Sargon program is designed to project any test point in the Octopus 201 perimeter. With this program, we tested 27 points. Among the 27 points, 17 were located in the central 6° visual field and 10 on the horizontal meridian subtending 8°, 10°, 12°, 16°, and 20°.