Table 3.
Mean Threshold in Non-Stereoblind Adults, arcsec |
Population SD, log10 arcsec |
Bland-Altman 95% Limits of Agreement in log10 arcsec = 1.96 SD of Differences Between Test and Retest |
Spearman Correlation Between Test and Retest |
|
ASTEROID | 57 | 0.35 | ±0.64 (raw) | 0.63 |
±0.56 (quantized) | ||||
TNO | 5250 | 0.2150 | ±0.4550 | 0.5731 |
6031 | ±0.4831 | |||
Randot Preschool | 51 | 0.24 | ±0.5944 | |
Near Frisby | 2150 | 0.0650 | ±0.2444 | |
±0.2750 | ||||
Randot | 2950 | 0.1550 | ±0.3450 | |
Titmus | 4150 | 0.0550 | ±0.1350 |
Values reported without references are from the present study. The “quantized” Limits of Agreement reported for ASTEROID is after mapping the original thresholds to the closest available Randot Preschool stereotest score. This is essential for a fair comparison, since test-retest differences are naturally smaller where only a few discrete scores are available. Antona et al.50 reported values only in arcseconds. To convert to log arcseconds, we divided the range (standard deviation or limits of agreement) reported in arcseconds by the population mean threshold in arcseconds and by the natural logarithm of 10. For the means, we have reported the value in arcseconds corresponding to the mean of log10 arcsecond values. Antona et al.50 reported only the mean of the arcsecond, so we have used those values. Bosten et al.31 reported mean and median in arcseconds; we have taken the median of the values in arcseconds in the expectation that this will be closer to the mean of the log values.