| Literature DB >> 22373412 |
Michael Agne1, Chien-Hsun Huang, Inchi Hu, Haitian Wang, Tian Zheng, Shaw-Hwa Lo.
Abstract
In this study, we analyze the Genetic Analysis Workshop 17 data to identify regions of single-nucleotide polymorphisms (SNPs) that exhibit a significant influence on response rate (proportion of subjects with an affirmative affected status), called the affected ratio, among rare variants. Under the null hypothesis, the distribution of rare variants is assumed to be uniform over case (affected) and control (unaffected) subjects. We attempt to pinpoint regions where the composition is significantly different between case and control events, specifically where there are unusually high numbers of rare variants among affected subjects. We focus on private variants, which require a degree of "collapsing" to combine information over several SNPs, to obtain meaningful results. Instead of implementing a gene-based approach, where regions would vary in size and sometimes be too small to achieve a strong enough signal, we implement a fixed-bin approach, with a preset number of SNPs per region, relying on the assumption that proximity and similarity go hand in hand. Through application of 100-SNP and 30-SNP fixed bins, we identify several most influential regions, which later are seen to contain some of the causal SNPs. The 100- and 30-SNP approaches detected seven and three causal SNPs among the most significant regions, respectively, with two overlapping SNPs located in the ELAVL4 gene, reported by both procedures.Entities:
Year: 2011 PMID: 22373412 PMCID: PMC3287865 DOI: 10.1186/1753-6561-5-S9-S3
Source DB: PubMed Journal: BMC Proc ISSN: 1753-6561
Figure 1Significance return frequency by region using the 100-SNP fixed-bin approach.
Figure 2Significance return frequency by region using the 30-SNP fixed-bin approach.
Return of the top 10 regions (fixed bin = 100)
| Region | Return frequency | True SNP |
|---|---|---|
| 26 | 120 | |
| 250 | 114 | |
| 179 | 109 | C14S1381 |
| 62 | 108 | |
| 6 | 98 | C1S3181, C1S3182, C1S2919 |
| 1 | 80 | |
| 5 | 64 | |
| 205 | 58 | C17S1009, C17S1030, C17S1056 |
| 10 | 54 | |
| 95 | 52 | |
| 805 | 131 | |
| 677 | 81 | |
| 701 | 75 | |
| 764 | 63 | |
| 811 | 63 | |
| 19 | 59 | C1S3181, C1S3182 |
| 84 | 53 | |
| 199 | 50 | C4S4935 |
| 724 | 47 | |
| 33 | 46 |