| Literature DB >> 29445426 |
Takahiro Kyoya1, Rika Iwamoto2, Yuko Shimanura2, Megumi Terada1, Shuichi Masuda2.
Abstract
INTRODUCTION: The in vivo comet assay is a widely used genotoxicity test that can detect DNA damage in a range of organs. It is included in the Organisation for Economic Co-operation and Development Guidelines for the Testing of Chemicals. However, various protocols are still used for this assay, and several different image analyzers are used routinely to evaluate the results. Here, we verified a protocol that largely contributes to the equivalence of results, and we assessed the effect on the results when slides made from the same sample were analyzed using two different image analyzers (Comet Assay IV vs Comet Analyzer).Entities:
Keywords: % tail DNA; Comet analyzer; Comet assay IV; EMS; Image analyzer; Validation
Year: 2018 PMID: 29445426 PMCID: PMC5801904 DOI: 10.1186/s41021-017-0092-x
Source DB: PubMed Journal: Genes Environ ISSN: 1880-7046
Differences in the conditions of Studies 1, 2, and 3
Comet assay results for all studies
| Protocol | Analyzer | Test substance | Mean % tail DNA ± SD | ||
|---|---|---|---|---|---|
| Study 1 | Study 2 | Study 3 | |||
| Method 1 | Comet Assay IV | PS | 2.25 ± 0.58 | 1.48 ± 0.36 | 1.71 ± 0.76 |
| EMS | 46.36 ± 5.78## | 27.45 ± 11.89# | 27.03 ± 1.41** | ||
| Comet Analyzer | PS | 4.04 ± 0.13 | 3.51 ± 0.42 | 1.34 ± 0.18 | |
| EMS | 35.12 ± 6.66## | 18.54 ± 3.37## | 20.40 ± 4.41## | ||
| Method 2 | Comet Assay IV | PS | 6.53 ± 4.34 | 3.39 ± 3.59 | 2.78 ± 1.16 |
| EMS | 21.49 ± 13.05* | 12.54 ± 5.47* | 25.57 ± 7.92## | ||
| Comet Analyzer | PS | 4.19 ± 1.29 | 2.97 ± 0.52 | 4.37 ± 1.84 | |
| EMS | 8.56 ± 1.92** | 11.05 ± 3.08## | 15.34 ± 4.76** | ||
Statistical analyses were conducted between the EMS-treatment and negative control groups for each of the method/analyzer combinations
SD standard deviation, PS physiological saline, EMS ethyl methanesulfonate
*p < 0.05, **p < 0.01 (Student’s t-test)
#p < 0.05, ##p < 0.01 (Aspin-Welch’s t-test)
Fig. 1Typical comet images observed with SYBR Gold staining (Method 1)
Fig. 2Typical Comet images observed with EtBr staining (Method 2)