Abstract
The ideal-observer performance, as measured by the area under the receiver’s operating characteristic curve, is computed for six examples of signal-detection tasks. Exact values for this quantity, as well as approximations based on the signal-to-noise ratio of the log likelihood and the likelihood-generating function, are found. The noise models considered are normal, exponential, Poisson, and two-sided exponential. The signal may affect the mean or the variance in each case. It is found that the approximation from the likelihood-generating function tracks well with the exact area, whereas the log-likelihood signal-to-noise approximation can fail badly. The signal--to-noise ratio of the likelihood ratio itself is also computed for each example to demonstrate that it is not a good measure of idealobserver performance.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1783-1793 |
| Number of pages | 11 |
| Journal | Applied optics |
| Volume | 39 |
| Issue number | 11 |
| DOIs | |
| State | Published - Apr 10 2000 |
ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics
- Engineering (miscellaneous)
- Electrical and Electronic Engineering