| Literature DB >> 32286438 |
Örjan Johansson1,2, Gustaf Samelius3,4, Ewa Wikberg4, Guillaume Chapron5, Charudutt Mishra3,6, Matthew Low7.
Abstract
Reliable assessments of animal abundance are key for successful conservation of endangered species. For elusive animals with individually-unique markings, camera-trap surveys are a benchmark standard for estimating local and global population abundance. Central to the reliability of resulting abundance estimates is the assumption that individuals are accurately identified from photographic captures. To quantify the risk of individual misidentification and its impact on population abundance estimates we performed an experiment under controlled conditions in which 16 captive snow leopards (Panthera uncia) were camera-trapped on 40 occasions and eight observers independently identified individuals and recaptures. Observers misclassified 12.5% of all capture occasions, resulting in systematically inflated population abundance estimates on average by one third (mean ± SD = 35 ± 21%). Our results show that identifying individually-unique individuals from camera-trap photos may not be as reliable as previously believed, implying that elusive and endangered species could be less abundant than current estimates indicate.Entities:
Mesh:
Year: 2020 PMID: 32286438 PMCID: PMC7156508 DOI: 10.1038/s41598-020-63367-z
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1Conceptual figure of the experiment and influence of different errors on the structure of the capture histories (CH) in photograph-based population abundance estimation. Here, the true CH contains an individual (A) who was captured twice using a camera-trap and another individual (B) who was captured once. Capture-recapture methods use the number of individuals and the proportion of captures (1) and non-captures (0) to estimate the population abundance; thus anything influencing either of these factors will influence the population estimate. A shift error moves a capture event from one individual to another, but does not change the total number of individuals or the number of 1’s and 0’s (middle left). A combination error combines the captures from two individuals into one, reducing the number of individuals and the total number of zeros (lower left). A splitting error splits the captures from one individual into two and creates a “ghost” individual, increasing the number of individuals and the total number of 0’s (top right). A capture exclusion where identification is possible, is a form of identification error that changes a 1 to 0 in that individual’s CH (bottom right). Population abundance estimates will be underestimated by combinations and overestimated by splits. In a conventional capture-recapture framework, shifts will largely not affect population estimates. Exclusions may over- or underestimate the abundance, depending on whether they result in the loss of individuals from the CH or if they are non-random relative to individual identity (bottom right). The image was created in the software OmniGraffle 7 (https://www.omnigroup.com/omnigraffle).
Figure 2Example of photographs used in this study to assess identification errors in camera-trap photographs of snow leopards. Note the right side of the cat is visible and the background has been removed to prevent observers identifying the cat based on visual information from the background.
Probabilities of identification errors while classifying each set of camera-trap photographs (capture event (CE) folders) of snow leopards (estimates are the mean ± SD of the posterior distribution of the expected mean error probability from Bayesian binomial models described in Appendix S1).
| Error | Overall | Non-expert | Expert | P(Non> Expert) |
|---|---|---|---|---|
| Split | 0.091 ± 0.016 | 0.098 ± 0.025 | 0.078 ± 0.021 | 0.709 |
| Combine | 0.016 ± 0.007 | 0.007 ± 0.007 | 0.019 ± 0.011 | 0.138 |
| Shift | 0.023 ± 0.008 | 0.042 ± 0.016 | 0.002 ± 0.001 | 1 |
| Total split | 0.111 ± 0.011 | 0.139 ± 0.028 | 0.078 ± 0.022 | 0.957 |
| Total combine | 0.037 ± 0.011 | 0.049 ± 0.017 | 0.019 ± 0.011 | 0.918 |
| Exclude | 0.087 ± 0.016 | 0.119 ± 0.027 | 0.053 ± 0.018 | 0.981 |
| Exclude* | 0.049 ± 0.013 | 0.044 ± 0.019 | 0.053 ± 0.018 | 0.344 |
| CE error | 0.125 ± 0.019 | 0.146 ± 0.029 | 0.099 ± 0.024 | 0.895 |
| CE error + | 0.208 ± 0.023 | 0.264 ± 0.036 | 0.151 ± 0.028 | 0.994 |
| CE error* + | 0.174 ± 0.023 | 0.191 ± 0.034 | 0.151 ± 0.028 | 0.782 |
Estimates are presented for the 8 observers (overall) and also divided according to their previous experience in snow leopard photo classification (non-expert vs. expert) with the probability that non-experts have greater errors than experts [P(non > expert) derived from the posterior distribution of the difference between observers]. Total split and total combine add the shift estimate to the split and combine estimates, respectively, since shifts involve a split and combination error. Capture event error (CE) relates to the total probability of a capture event being misclassified: this is presented for classification errors only (CE error) and when exclusions are considered as a classification error (CE error+). Because observer 2 excluded 30% of all capture events, some estimates are also presented where observer 2 has been removed from the analysis (*).
The types of identification errors and the number of individuals added to or lost from the capture history for each observer (Obs1–4 are non-experts and 5–8 are experts).
| Exclude | Split | Shift | Combine | Individuals lost in excluded CEs | Individuals lost in combination errors | Ghosts created in split errors | Number of individuals identified (true) | |
|---|---|---|---|---|---|---|---|---|
| Obs1 | 4 | 5 | 5 | 1 | 1 | 2 | 5 | 18 (15) |
| Obs2 | 12 | 2 | 0 | 0 | 3 | 0 | 2 | 15 (13) |
| Obs3 | 0 | 2 | 0 | 0 | 0 | 0 | 2 | 18 (16) |
| Obs4 | 1 | 4 | 1 | 0 | 0 | 0 | 4 | 20 (16) |
| Obs5 | 4 | 3 | 0 | 0 | 1 | 0 | 3 | 18 (15) |
| Obs6 | 1 | 4 | 0 | 0 | 0 | 0 | 4 | 20 (16) |
| Obs7 | 2 | 0 | 1 | 0 | 1 | 0 | 0 | 15 (15) |
| Obs8 | 1 | 3 | 0 | 3 | 0 | 1 | 3 | 18 (16) |
Exclude = capture events (CE) removed from classification for being too difficult to classify, split = CEs split from one individual to create two individuals, combine = CEs combined from two individuals into one individual, shift = CEs split from one individual and combined with another. These errors result in the loss of individuals when: (1) they are not considered because all CEs containing their photos were excluded [here they are not present in the capture history], or (2) they are combined with another individual [here they remain in the capture history, but are misclassified]. Errors also result in false individuals being created (ghosts) from splitting errors. Thus the ‘number of individuals identified’ in a capture history can have three meanings: (1) how many unique animals the observer thinks they saw and classified; this is the number of rows in the capture history and equals: the true number photographed – individuals lost (exclusion or combination) + ghosts created, (2) how many unique animals the observer actually saw and classified (true); this equals number of animals recorded in the capture history (true number photographed – individuals lost through CE exclusion), and (3) in a very broad sense it could be interpreted to mean the population abundance estimate, since the capture history also contains information about animals that were not seen (see Table 3).
Comparison of the structure of the capture histories (CH) derived from classification of snow leopard images by eight observers (Obs 1–4 were non-experts, Obs 5–8 were experts) with the true capture history (TRUE).
| CH structure | Population estimate | Bias in population estimate | ||||||
| 5 | 4 | 3 | 2 | 1 | True | Remaining | ||
| TRUE | 1 | 2 | 5 | 4 | 4 | 16.6 ± 0.9 | +3.7% | +3.7% |
| Obs1 | 0 | 2 | 3 | 6 | 7 | 20.3 ± 2.0 | +27% | +35% |
| Obs 2 | 1 | 1 | 1 | 4 | 8 | 23.9 ± 7.2 | +49% | +84% |
| Obs 3 | 1 | 2 | 3 | 6 | 6 | 21.0 ± 2.8 | +31% | +31% |
| Obs 4 | 0 | 2 | 2 | 9 | 7 | 22.8 ± 2.3 | +42% | +42% |
| Obs 5 | 1 | 1 | 3 | 5 | 8 | 23.5 ± 4.5 | +47% | +56% |
| Obs 6 | 0 | 3 | 2 | 6 | 9 | 22.8 ± 2.3 | +42% | +42% |
| Obs 7 | 2 | 0 | 5 | 5 | 3 | 16.1 ± 1.3 | +0.6% | +7% |
| Obs 8 | 3 | 0 | 2 | 5 | 8 | 23.2 ± 3.9 | +45% | +45% |
The CHs were based on 5 sampling occasions; CH structure shows how many times each snow leopard individual was seen (where the ‘5’ column indicates an individual was recorded in 5 capture events, and the ‘1’ column indicates an individual was only identified by the observer once). Based on each observer’s CH a population abundance estimate was derived using a closed capture-recapture model (mean ± SD; see methods). The bias in the mean estimate for the population is shown relative to the true population size (n = 16) and also relative to the number of unique individuals remaining in each observers’ CH after accounting for animals removed from consideration because of capture event exclusion (for observers 1, 2, 5 & 7 the number of unique individuals assessed was n = 15, 13, 15 & 15 respectively; see Table 1).
Figure 3How different rates of ghost-producing splitting errors (0.05–0.20) affect the population abundance estimate, based on camera-trapping data from a real-world snow leopard study in Mongolia[21] (where the population size = 12, capture occasions = 16, capture probability = 0.16). Estimates are derived from 1000 simulations at each error rate; the solid line is the median error and the grey shading the 95% quantile range. This is shown relative to the expected credible range of splitting errors (50% and 95% CIs as thick and thin lines respectively), from expert and non-expert observers (generated from the binomial likelihood of the model in Appendix S1; for splitting errors that create new individuals).