| Literature DB >> 23469083 |
Abstract
Many field studies of insects have focused on the adult stage alone, likely because immature stages are unknown in most insect species. Molecular species identification (e.g., DNA barcoding) has helped ascertain the immature stages of many insects, but larval developmental stages (instars) cannot be identified. The identification of the growth stages of collected individuals is indispensable from both ecological and taxonomic perspectives. Using a larval-adult body size relationship across species, I present a novel technique for identifying the instar of field-collected insect larvae that are identified by molecular species identification technique. This method is based on the assumption that classification functions derived from discriminant analyses, performed with larval instar as a response variable and adult and larval body sizes as explanatory variables, can be used to determine the instar of a given larval specimen that was not included in the original data set, even at the species level. This size relationship has been demonstrated in larval instars for many insects (Dyar's rule), but no attempt has been made to include the adult stage. Analysis of a test data set derived from the beetle family Carabidae (Coleoptera) showed that classification functions obtained from data sets derived from related species had a correct classification rate of 81-100%. Given that no reliable method has been established to identify the instar of field-collected insect larvae, these values may have sufficient accuracy as an analytical method for field-collected samples. The chief advantage of this technique is that the instar can be identified even when only one specimen is available per species if classification functions are determined for groups to which the focal species belongs. Similar classification functions should be created for other insect groups. By using those functions together with molecular species identification, future studies could include larval stages as well as adults.Entities:
Mesh:
Year: 2013 PMID: 23469083 PMCID: PMC3585218 DOI: 10.1371/journal.pone.0057836
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Figure 1Schematic diagram showing analyses of species with n larval instars.
On the adult size–larval size plane, “areas” of larval instars are not expected to overlap with each other (A) because among species, species with larger adult sizes have larger larval sizes (arrow 1), and within species, older larvae have larger body sizes (arrow 2). Using this adult size–larval size relationship (B), the instar of a larval sample that was not included in the data set can be identified based on larval size (measured from the specimen; arrow 3) and expected adult size (obtained from conspecific adult specimens or the literature) after molecular methods are used to identify the species of the larval sample; arrow 4). Dotted lines indicate boundaries between instar areas. Note that this diagram is conceptual; in practical analyses (discriminant analyses), the “area” of each larval instar cannot be represented two-dimensionally.
Correct classification rates (%) of linear (LDA) and Mahalanobis squared distance-based (MDA) discriminant analyses for various Carabidae taxa.
| Taxa |
| LDA | MDA | ||||||
| L1 | L2 | L3 | all | L1 | L2 | L3 | all | ||
| Data set 1 | |||||||||
| Overall Carabidae | 358/302/311 | 70.9 | 60.3 | 81.4 | 71.0 | 78.2 | 52.3 | 80.7 | 71.0 |
| Trechinae | 46/37/31 | 82.6 | 89.2 | 77.4 | 83.3 | 89.1 | 86.5 | 87.1 | 87.7 |
| Pterostichini | 93/88/87 | 86.0 | 84.1 | 90.8 | 86.9 | 88.2 | 83.0 | 90.8 | 87.3 |
| Zabrini* | 31/26/27 | 74.2 | 69.2 | 88.9 | 77.4 | 87.1 | 61.5 | 88.9 | 79.8 |
| Harpalini | 81/70/72 | 77.8 | 61.4 | 80.6 | 73.5 | 79.0 | 58.6 | 79.2 | 72.6 |
| Sphodrini* | 16/16/17 | 93.8 | 93.8 | 88.2 | 91.8 | 93.8 | 93.8 | 88.2 | 91.8 |
| Platynini* | 12/11/14 | 91.7 | 90.9 | 100.0 | 94.6 | 100.0 | 81.8 | 100.0 | 94.6 |
| Chlaeniini+Panagaeini+Oodini* | 15/14/16 | 93.3 | 85.7 | 100.0 | 93.3 | 93.3 | 85.7 | 100.0 | 93.3 |
| Lebiini+Cyclosomini* | 20/18/18 | 95.0 | 83.3 | 100.0 | 92.9 | 95.0 | 88.9 | 100.0 | 94.6 |
| Data set 2 | |||||||||
| Overall Carabidae | 173/94/136 | 72.3 | 56.4 | 83.1 | 72.2 | 76.3 | 56.4 | 81.6 | 73.4 |
| Trechinae | 13/9/11 | 92.3 | 100.0 | 81.8 | 90.9 | 100.0 | 88.9 | 100.0 | 97.0 |
| Pterostichini* | 33/23/26 | 84.8 | 78.3 | 84.6 | 82.9 | 90.9 | 65.2 | 92.3 | 84.1 |
| Zabrini | 16/3/13 | 75.0 | 66.7 | 92.3 | 81.2 | ― | ― | ― | ― |
| Harpalini | 45/24/41 | 80.0 | 83.3 | 87.8 | 83.6 | 86.7 | 87.5 | 90.2 | 88.2 |
| Sphodrini* | 8/8/7 | 100.0 | 100.0 | 85.7 | 95.5 | 87.5 | 100.0 | 100.0 | 95.5 |
| Platynini | 3/2/4 | 100.0 | 100.0 | 100.0 | 100.0 | ― | ― | ― | ― |
| Chlaeniini+Panagaeini+Oodini* | 15/13/13 | 100.0 | 76.9 | 100.0 | 92.7 | 86.7 | 92.3 | 100.0 | 92.7 |
| Lebiini+Cyclosomini | 15/6/13 | 93.3 | 83.3 | 100.0 | 94.1 | 73.3 | 83.3 | 100.0 | 85.3 |
Asterisks indicate taxa for which the homogeneity of the variance–covariance matrix of the data set was confirmed.
L1, L2, and L3 indicate first, second, and third instar larvae, respectively.
Results of GLMs that analyzed the effects of taxa and larval instar on the correct classification rates of linear (LDA) and Mahalanobis squared distance-based (MDA) discriminant analyses.
| Factors | LDA | MDA | ||||||
| Estimates | SE | z-value |
| Estimates | SE | z-value |
| |
| Data set 1 | ||||||||
| (Intercept) | 2.67 | 0.61 | 4.36 | <0.001 | 2.92 | 0.62 | 4.71 | <0.001 |
| Trechinae | –1.01 | 0.65 | –1.55 | 0.121 | –0.66 | 0.67 | –1.00 | 0.319 |
| Pterostichini | –0.73 | 0.63 | –1.17 | 0.242 | –0.70 | 0.63 | –1.12 | 0.264 |
| Zabrini | –1.41 | 0.65 | –2.16 | 0.031 | –1.29 | 0.66 | –1.95 | 0.051 |
| Harpalini | –1.62 | 0.62 | –2.62 | 0.009 | –1.70 | 0.62 | –2.73 | 0.006 |
| Sphodrini | –0.21 | 0.80 | –0.27 | 0.791 | –0.21 | 0.80 | –0.26 | 0.796 |
| Platynini | 0.21 | 0.94 | 0.23 | 0.822 | 0.21 | 0.95 | 0.22 | 0.824 |
| Lebiini+Cyclosomini | –0.06 | 0.79 | –0.08 | 0.939 | 0.25 | 0.85 | 0.29 | 0.770 |
| Second instar | –0.38 | 0.22 | –1.74 | 0.081 | –0.81 | 0.23 | –3.56 | <0.001 |
| Third instar | 0.33 | 0.24 | 1.36 | 0.173 | 0.12 | 0.26 | 0.46 | 0.643 |
| Data set 2 | ||||||||
| (Intercept) | 1.91 | 0.16 | 12.19 | <0.001 | 1.95 | 0.27 | 7.32 | <0.001 |
| Second instar | – | – | – | – | −0.37 | 0.40 | −0.94 | 0.346 |
| Third instar | – | – | – | – | 0.91 | 0.50 | 1.82 | 0.068 |
Model of each dataset was constructed from a full model (i.e., one containing all predictors, including the interactions) using the function stepAIC in the R package MASS.