Abstract
purpose. To develop a sensitive psychophysical test for detecting visual defects such as microscotomas.
methods. Frequency-of-seeing curves were measured with 0.75′ and 7.5′ spots. On each trial, from 0 to 4 stimuli were randomly presented at any of eight equally spaced loci 0.5° from fixation. By correcting the aberrations of the eye, adaptive optics produced retinal images of the 0.75′ spot that were 3.0 μm wide at half height, small enough to be almost entirely confined within the typical cone diameter at this eccentricity. Data were collected from a patient with deuteranopia (AOS1) whose retina, imaged with adaptive optics, suggested that ≈30% of his cones were missing or abnormal. Patients with protanomalous trichromacy (1 subject), deuteranopia (1 subject), and trichromacy (5 subjects) served as controls (all had normal cone density and complete cone mosaics). Psychophysical results were modeled by a Monte Carlo simulation incorporating measured properties of the cone mosaic.
results. Frequency-of-seeing curves for AOS1 obtained with 0.75′ spots showed lower asymptote, slope, and sensitivity than for controls. The 7.5′ results showed that these differences were the result of the small spot size, which on some trials was confined mostly to the locus of the putatively missing cones. A two-parameter model satisfactorily described the data and was highly sensitive to the proportion of missing cones simulated.
conclusions. Adaptive-optics microperimetry is a powerful psychophysical test for assessing the loss of neural elements, even in retinas that appear otherwise normal in standard clinical tests. This technique may prove useful in estimating the proportion of missing cones in different patients and in detecting other visual losses such as those associated with glaucoma.
Insults to the visual system are notoriously difficult to detect. For example, in human glaucomatous eyes, before a deficit in visual performance can be detected by standard automated perimetry, 25% to 35% of the ganglion cells are dead,
1 and many more may be nonfunctional or of reduced sensitivity. The redundancy of visual mechanisms explains part of the insensitivity of such tests
2 3 4 5 6 because the sensitivity profiles of many neurons overlap along the stimulus dimensions to which they respond, so that when one neuron dies or otherwise fails to respond to a given stimulus, the stimulus can nevertheless be detected through the response of neighboring neurons. Although newer techniques, such as short-wavelength automated perimetry,
7 frequency-doubling perimetry,
8 9 high-pass resolution perimetry,
10 and other techniques,
2 diminish the redundancy in the neural mechanisms, the stimuli themselves are redundant enough to cause correlated responses even in neurons whose sensitivities do not overlap. For example, the smallest spots used in clinical perimetry subtend 0.11°. Even without optical spread, the image of such a spot covers some 150 cones at the center of the fovea of an average retina.
11 This produces correlated responses not only among these 150 cones but also among the many other postreceptoral cells connected to them either directly or indirectly. One way to reduce the redundancy of the neural response is to reduce the component caused by the test stimulus itself. Normally, spread of the retinal image by the optics of the eye limits the amount by which one can reduce the stimulus size and hence the number of cones excited. Here we used adaptive optics to reduce the size of the retinal image close to the theoretical limit and thereby minimize the number of cones stimulated on any given presentation; we used these small test spots to detect missing cones in a retina in which larger spots used in clinical perimetry could not.
The person whose retina we tested (AOS1) represented a subclass of persons with dichromacy who carry genetic mutations that disrupt the function of one of the cone photopigments.
12 Previous results with high-resolution retinal imaging
13 have shown that the retina of AOS1 contained lacunae, equal in size to one or more cones, that the authors hypothesized represented the loci at which cones expressing the mutant gene have been severely damaged or lost. A micrograph of his retina is shown in the upper part of
Figure 1 ; for comparison, the retina of a healthy trichromat (AOS2) is shown below it. Note the relative sparseness of visible cones in the upper micrograph. Although the hypothesized missing cones occupy almost a third of the cone mosaic, ophthalmic examination revealed no abnormalities aside from the dichromacy. For example, visual acuity was 20/16 (−0.10 logMAR), standard visual fields were normal, and funduscopic examination results were unremarkable. Test stimuli used here were small enough to fall largely within the lacunae observed photographically and thereby made it possible to detect the associated microscotomas psychophysically. Use of large spots, approximating the size of those in clinical use, failed to produce the signs we attributed to the missing cones.
One drop each of phenylephrine hydrochloride (2.5%) and tropicamide (1%) dilated the subjects’ pupils and suspended accommodation in their right eyes. Their heads were stabilized by a bite bar containing their dental impression. Stimuli were 0.75′ or 7.5′ spots produced by a digital light–processing (DLP) video projector (MP1600; Compaq; Hewlett Packard, Mountain View, CA)
15 at any of eight equally spaced locations 0.5° from a dim, 2′ fixation target
(Fig. 2) . The light passed through an interference filter with a 10-nm pass band centered at 550 nm, a wavelength to which M and L cones are equally sensitive. At maximum, the test spot illuminated the retina at 5.06 log troland. The projector also provided a steady background field of 3.08 log troland (its minimum output) covering a circular region slightly greater than 1°. Sensitivity to the 7.5′ spot was so much greater than that to the 0.75′ spot that a 1.11 log filter was required in the projector beam to present spots dim enough to measure the low end of the frequency-of-seeing curve. This brought the maximum log troland value down to 3.95. Because the filter also reduced the background field, we added a steady, 550-nm background field that brought the total background field for the 7.5′ spots back up to 3.44 log troland, comparable to that for the 0.75′ spots.
The shortest duration flash allowed by the proprietary software of the projector delivered a train of six pulses of equal intensity: each pulse was 3 ms long, and each was separated from one another by 5.5 ms of darkness. Each of the 3-ms pulses was in turn composed of micropulses that were turned on and off by the projector’s software to vary the total amount of light contained by the six pulses over 256 steps. Troland values of the stimuli used for each subject are shown by the locations of the data points (see
3 Fig. 4 ).
A spectro-colorimeter (PR-650; Photograph Research, Chatsworth, CA) was used to calibrate luminous flux in the test stimuli, and a radiometer (IL 1700; International Light, Newport, MA) was used to measure the power of the background, which was numerically converted to trolands. These measurements were made in the plane of the subject’s pupil. A high-speed photodiode (PDA 155; Thorlabs, Newton, NJ) and oscilloscope were used to measure temporal properties of the DLP projector output.
Because the time available for testing AOS1 was limited, we increased the rate of data acquisition by simultaneously presenting 0, 1, 2, 3, or 4 stimuli with equal frequency as is sometimes done in clinical perimetry.
16 17 18 Although one can further increase efficiency by presenting four stimuli on a higher proportion of trials, we chose not to so as to avoid the response biases that might result. The subject’s task was to report, by a key-press, the number of stimuli presented. This increase in the number of stimuli and alternative responses only slightly delays the response
19 20 and has no noticeable effect on the reliability of detection
19 21 22 23 (our results also show no relationship between detection and number of stimuli). The subject’s response initiated the next trial.
The stimuli described were presented through an adaptive optical system that minimized optical aberrations.
24 25 Measured point-spread functions with and without adaptive optics are shown in
Figure 3 . Although cone sizes varied over the areas tested and among subjects, as a rough estimate, without adaptive optics approximately 9% of the incident light in a 0.75′ test spot fell within the geometric boundaries of a single cone, whereas with adaptive optics approximately 55% did, so that adaptive optics increased the amount of light in this area approximately sixfold. Because of the Gaussian shape of the cone entrance aperture, this optical correction increased the relative amount of light that actually entered the cone even more.
Preliminary observations established the range spanned by each observer’s frequency-of-seeing curve, and from five to eight points on the curve, spaced at 0.1 intervals on a log troland scale, were tested to describe the curve. A block of trials consisted of 50 trials at each stimulus magnitude, in random order, and each observer had four such blocks. Measurement and correction of the aberrations of each subject’s eye was performed between each block of trials, instead of during the blocks, to prevent the superluminescent diode used for wavefront sensing from affecting the subject’s sensitivity. Although the measurement took less than 800 ms, more than 1 minute was required for the subject’s eye to recover from exposure to the light from the diode.
To determine whether the differences between the 0.75′ data of AOS1 and of the control subjects could be explained on the basis of the evident differences in their retinal mosaic, we simulated the experiment with a model (implemented in MATLAB; MathWorks, Natick, MA) that incorporates the retinal mosaic and optical point-spread functions of AOS1 and that of one of the trichromatic subjects (AOS2).
The model consisted of a Monte Carlo simulation of 10,000 stimuli of varying energy, presented to a given subject’s retinal cone mosaic. For each stimulus presentation, the model used a set of detection rules to determine whether the stimulus was seen. The output of the model was a frequency-of-seeing curve.
According to the model, a given stimulus was detected if the visual excitation exceeded the response criterion for that flash. Visual excitation was calculated by summing the products of each point of the retinal image of the spot with the corresponding point of the sensitivity profile of the photoreceptor mosaic (i.e., by finding the inner product). The retinal image of the spot was found by convolving the geometric image of the stimulus with the subject’s own point spread function, measured at an eccentricity of 0.5°, after the aberrations of that subject’s eye had been optically compensated.
24 25
The sensitivity profile of the photoreceptor mosaic was obtained by convolving the optical aperture of the cones with a set of points representing locations of the observed centers of the cones in a patch of retina approximately 0.75° square that was imaged in vivo at 0.5° eccentricity by an adaptive optics ophthalmoscope.
26 Individual cones were assigned a spectral sensitivity based on the relative numbers of short-wavelength-sensitive (S), M, and L cones in the retina. Because these vary across healthy subjects, we used previous densitometry measurements with an adaptive optics ophthalmoscope
13 24 27 28 to determine the appropriate ratio of S-, M-, and L-cone assignments to use for each subject. In addition, the optical aperture of each cone was represented by a two-dimensional Gaussian profile with a width at half height of 0.615 times the intercone distance, on the basis of interferometric estimates.
29 30 31 32 We truncated the Gaussian at the physical boundary of the cone (meaning that light falling on the cone mosaic outside the cone’s physical aperture would not be absorbed by photopigment within that particular cone), but doing so had a negligible effect on the results (data not shown).
Because of fixational eye movements, the absolute location of a stimulus on the retina varied from trial to trial. Therefore, we incorporated fixational instability in the model to determine the location of the retinal mosaic on which the stimulus fell on each trial. The position of the retinal mosaic with respect to the retinal image of the spot was sampled randomly from a probability density function representing the statistics of eye position measurements. The two-dimensional distribution of fixations of AOS2 and four other subjects were observed by using high-resolution imaging with adaptive optics to record the absolute position of the retina while fixating.
24 The fixational patterns of AOS2 so obtained were used in the simulations of his psychophysical performance, whereas the mean of all five subjects was used in the simulation the performance of AOS1. Consistent with previous reports using a different methodology, in both cases the fixational patterns were elongated along the horizontal axis and had an SD of approximately 5′.
The model therefore yields on each trial an estimate of the relative amount of light absorbed by each cone in the vicinity of the test flash. Although previous models of the detection of small spots by the cone system
33 34 35 36 37 38 39 40 41 42 have assumed that each cone has a threshold, in the sense that stimulation of a cone below a fixed value makes no contribution to detection by the subject, we found such a threshold unnecessary; excluding it simplifies the model while improving the fit slightly (though not reliably). We assumed instead that the total number of photopigment molecules activated (
visual excitation) in all the cones sums linearly to determine whether the flash was seen: if the total number of activations exceeded a given value, the
response criterion, we assumed that the subject detected the stimulus. (Nonlinear summation of cone excitation, such as root-mean-square summation,
43 44 45 46 yields frequency-of-seeing curves with too great a slope.) To obtain frequency-of-seeing curves, we simply counted the proportion of trials on which the visual excitation exceeded the response criterion at each of the stimulus intensities.
The model thus has two free parameters that were separately adjusted to fit each subject’s data: the observer’s response criterion, just mentioned, and sensitivity, the proportion of quanta in the stimulus that ultimately activates a photopigment molecule. Sensitivity simply relates such visual excitation to the amount of light absorbed, and changing its value translates the frequency-of-seeing curve along the log intensity axis. The response criterion is the visual excitation required for the subject to respond to the stimulus; changing its value translates the frequency-of-seeing curve along the absolute intensity axis and varies the slope and shape of the frequency-of-seeing curve when plotted on semilog axes. Thus, in the model, two parameters serve where three were required for the curves in
Figure 4 .
In our simulations, variation in the locations of the spots relative to the cones produced by eye movements caused variation in visual excitation from trial to trial, depending on where the spots fell with respect to the cones and gaps between cones in the mosaic. Increasing the response criterion increased the number of trials in which too little light was absorbed to be detected. This affected both the height and the slope of the frequency-of-seeing curve. Hence, the topography of the individual’s retinal mosaic determined the trial-by-trial variability, and the subject’s response criterion determined the effect of that variability on the frequency-of-seeing curve.
The variability of light absorbed qualifies as noise, and so the model is based on the theory of signal detection.
47 48 49 However, in the experiments using the 7.5′ spot, the variability of absorbed light resulting from variation in spot location was negligible. The stochastic noise associated with quantal absorptions was also small, approximately 0.3% of the mean (SD). Hence, the trial-by-trial variability of the response has to be attributed to some other source, such as noise intrinsic to the visual system. For AOS2 this inferred noise was 22 times smaller than that for the smaller spot, and for AOS1 it was 115 times smaller. The contribution of such visual noise to detection of the small spot was therefore small relative to that associated with stimulus location. Nevertheless, for the sake of consistency, we included this noise in the model for detection of the small spot, assuming that the amount of intrinsic noise involved in detecting the small spot was the same as that for the large spot. This was incorporated into the model by adding a random sample from a Gaussian distribution to the total visual excitation on each trial.
The model is of course somewhat simplified. For example, although the intercone distances in our model faithfully reflected those of the individual retina tested, we assumed a fixed cone size. Similarly, the stimuli actually fell at eight locations, but our model represented the cone mosaic at only one location: there can be small differences in cone density on different meridians,
50 51 and the effects of any such asymmetries could be exaggerated by the tendency of observers to fixate off the anatomic center of the fovea.
24
The model also omitted absorption of light by the retinal blood vessels. Approximately 90% of the retina is covered with a capillary bed that absorbs some 40% of incident light.
52 Placing the stimuli 0.5° from fixation, an area that in most persons is devoid of retinal vasculature, mitigates this problem. However the size of this avascular zone varies widely, and its radius in healthy persons can be as small as 0.3°.
53 Indeed, retinal imaging reveals that subject AOS6 in this experiment has extensive invasion of the central fovea by retinal vessels (data not shown). Therefore, one would expect the slope of his frequency-of-seeing curve to be shallower than those of the other subjects and also shallower than predicted by the model. That this subject does have the shallowest frequency-of-seeing curve is evident in
Table 1and
Figure 4 , and it is significantly shallower than that generated by the model for his retina (data not shown).
Figure 4shows the results obtained with the small and large test spots, and
Table 1provides a summary of the relevant statistics. The curves in
Figure 4are maximum likelihood fits of a cumulative Gaussian curve to the data. The means, slopes at the means, and upper asymptotes of those curves are given in
Table 1 . The means are used as an estimate of each observer’s psychophysical threshold for detecting the test stimulus and, for the control subjects, are comparable to those in the literature.
54 55 56 False-positive rate, f +, for a particular subject is specified by the equation:
\[f_{{+}}\ {=}\ d_{\mathrm{r}}/(8N_{b}),\]
where
d r is the number of reported detections when no stimulus was presented,
N b is the number of trials on which no stimulus was presented (blank trials), and 8 is the number of possible locations for the stimulus on each trial. We assumed that the number of true detections,
d, is:
\[d\ {=}\ d_{\mathrm{r}}\ {-}\ f_{{+}}(8N\ {-}\ d),\]
where
N is the total number of trials. Here, the false-positive rate (
f +) is multiplied by the number of opportunities for a false positive, which is eight times the number of trials minus the number of true detections (
d). Dividing
d by the number of stimuli presented yields proportion correct, as plotted in
Figures 4to
5 6 .
Reliable differences (at the 0.01 probability level), as determined by
t tests on the means and standard errors given in
Table 1 , are as follows. (Identical conclusions follow from an analysis of the results in terms of
d′, a measure of sensitivity from the theory of signal detection that is free of the effects of response biases if the underlying assumptions are met.
47 57 ) When the 0.75′ test stimulus was used, the mean of frequency-of-seeing curve (i.e., the threshold) for AOS1 was higher than those of the control subjects, and the slope and asymptote are lower. However, only the small spot produced reliable differences between AOS1 and the control subjects in the slopes and asymptotes of the frequency-of-seeing curves, and this difference between the results with these two different spots is statistically reliable. Because the false-positive rates of AOS1 did not differ reliably from those of the control subjects, these thresholds are valid estimates of sensitivity.
The larger test spot produced a threshold difference between AOS1 and the control subjects that was 40% greater (P < 0.01) than for the smaller spot. Hence, AOS1 shows less spatial summation than the control subjects, possibly because of lack of a complete cone mosaic, but we cannot rule out other abnormalities of his visual system that are independent of this loss of cones.
The data from the other color-deficient control subjects (AOS7 and AOS8) do not differ reliably from those of the trichromatic subjects in any way. When AOS7 and AOS8 are compared with AOS1, only the asymptotes for the 0.75′ data and the means for the 7.5′ data differ reliably (t = 17.3 and 29.2, respectively; P < 0.05 in both cases); the decrease in the number of reliable differences may be due to the fact that the differences between AOS1 and two subjects (the two dichromats) must be greater to be statistically reliable than differences between AOS1 and seven subjects (all the control subjects).
These results show that some of the sensitivity differences between AOS1 and the control subjects show up only when small spots are used. Next we examined whether the difference could be accounted for on the basis of the differences in retinal topography.
The technique outlined here serves not only to detect the loss of cone function but holds promise as a means of measuring the amount of loss. Given that the shape of the frequency-of-seeing curve depends on the proportion of cones lost
(Fig. 6) , it can be used to estimate the magnitude of functional loss, perhaps with a precision within 5%. This might be valuable in trying to monitor progressive loss of cone function in patients with cone degeneration, especially in those in whom functional loss might precede visible signs of loss in retinal images. Note that by testing with a wavelength to which both M- and L-cones are equally sensitive, there is no difference between them as far as this test is concerned. Any cone loss, whether specific to a particular cone class or randomly distributed, should reveal itself to these test stimuli.
This technique may also hold promise as a means of detecting small scotomas caused by other anomalies, such as the loss of ganglion cells that occurs in glaucoma. We speculate here that most techniques for detecting missing cones are hampered by redundancy in the representation of the stimuli in the receptor layer. The detection of missing ganglion cells is hindered not only by the same source of redundancy but also by redundancy associated with overlapping receptive fields. If one ganglion cell is lost, others continue to respond. The total signal transmitted may be smaller, and the loss of a particular ganglion cell may change the properties of the signal transmitted, but the loss of a ganglion cell fails to produce a complete scotoma, as the loss of a single cone does. Nevertheless, the stimuli used here reduce the redundancy that limits the effectiveness of such tests and are likely to increase sensitivity to the loss of ganglion cell activity.
Present affiliation: Department of Ophthalmology, Medical College of Wisconsin, Milwaukee, Wisconsin.
Presented, in part, at the 2005 OSA Fall Vision Meeting in Tuscon, Arizona, October 21–23.
Supported by National Eye Institute Grants R01-EY04367, P30-EY01319, and F32-EY014749; and in part by the National Science Foundation Science and by the Technology Center for Adaptive Optics, managed by the University of California at Santa Cruz under Cooperative Agreement AST-9876783.
Submitted for publication September 7, 2005; revised February 23 and April 3, 2006; accepted July 3, 2006.
Disclosure:
W. Makous, None;
J. Carroll, None;
J.I. Wolfing, None;
J. Lin, None;
N. Christie, None;
D.R. Williams, P, C
The publication costs of this article were defrayed in part by page charge payment. This article must therefore be marked “
advertisement” in accordance with 18 U.S.C. §1734 solely to indicate this fact.
Corresponding author: Walter Makous, Center for Visual Science, University of Rochester, Box 270268, Rochester, NY 14627-0270;
walt@cvs.rochester.edu.
Table 1. Statistical Summary of Frequency-of-Seeing Data
Table 1. Statistical Summary of Frequency-of-Seeing Data
Subject | 0.75′ Spot | | | | 7.5′ Spot | | | |
| Mean | Slope | Asymptote | False+ | Mean | Slope | Asymptote | False+ |
AOS1 | 4.50* | 3.28* | 0.76, † | 0.0023 | 3.01, † | 7.81 | 0.95 | 0.0068 |
AOS2 | 4.12 | 6.53 | 0.93 | 0.0043 | 2.64 | 8.04 | 1.00 | 0.0026 |
AOS3 | 4.40 | 7.70 | 0.85 | 0.0000 | 2.80 | 7.55 | 0.93 | 0.0008 |
AOS4 | 4.37 | 6.27 | 0.97 | 0.0029 | 2.71 | 7.42 | 0.99 | 0.0008 |
AOS5 | 4.22 | 5.87 | 0.95 | 0.0045 | 2.72 | 10.11 | 0.95 | 0.0058 |
AOS6 | 4.42 | 3.81 | 0.94 | 0.0083 | 2.71 | 9.03 | 0.97 | 0.0107 |
AOS7 | 4.39 | 5.91 | 0.91 | 0.0018 | 2.65 | 9.97 | 0.99 | 0.0009 |
AOS8 | 4.33 | 3.89 | 0.89 | 0.0111 | 2.67 | 8.96 | 0.96 | 0.0120 |
Mean | 4.32 | 5.71 | 0.92 | 0.0047 | 2.70 | 8.72 | 0.97 | 0.0048 |
SE | 0.041 | 0.533 | 0.015 | 0.0014 | 0.021 | 0.414 | 0.010 | 0.0018 |
The authors thank Peter Bex (University College, London), Li Chen (University of Rochester), Mina Chung (University of Rochester), Syndee Givre (University of North Carolina), Jay Neitz (Medical College of Wisconsin), Maureen Neitz (Medical College of Wisconsin), and Jason Porter (University of Houston) for their assistance in this work.
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