| Literature DB >> 35363835 |
Wenqian Song1, Nan Xiao1, Shihang Zhou1, Weijian Yu1, Ni Wang1, Linnan Shao1, Ying Duan1, Mei Chen1, Lingzi Pan1, Yuexin Xia1, Li Zhang1, Ming Liu2.
Abstract
OBJECTIVES: To assess the efficacy of Y-chromosome mini-STR-based next-generation sequencing (NGS) for non-invasive prenatal paternity testing (NIPPT).Entities:
Mesh:
Substances:
Year: 2022 PMID: 35363835 PMCID: PMC8974964 DOI: 10.1371/journal.pone.0266332
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Fig 1Schematic representation of library preparation and NGS.
Data for D3S1358 is shown as a representative example. (a) Amplification of the target sequence with barcoding primers. (b) Second PCR amplification adding specialized adapters and indexes to both ends. (c) Purification of the amplicon and pooling multiple libraries together. (d) Linearization of DNA libraries. (e) Loading DNA libraries onto the flow cell. (f) Bridge PCR amplification. (g) Cluster generation. (h) Paired-end sequencing. (i) Base calling, alignment and data analysis.
Fig 2Flow chart for experimental procedures and data analysis.
Fig 3The NGS sequencing reads per sample per locus of plasma DNA (range: 1068–140045 reads).
Fig 4Overview of target sequence length for all STR loci as per NGS and CE.
Target sequence indicates the PCR amplicon without barcoding and adapter primers.
The paternity testing parameters using cffDNA in the 14 cases with male fetuses.
| Case No. | Haplotype frequency | CPI | Probability of paternity |
|---|---|---|---|
| 1 | 0.001174 | 852 | 99.8828% |
| 2 | 0.017606 | 56.8 | 98.2699% |
| 3 | 0.001174 | 852 | 99.8828% |
| 4 | 0.003521 | 284 | 99.6491% |
| 5 | 0.005869 | 170.4 | 99.4166% |
| 6 | 0.001174 | 852 | 99.8828% |
| 7 | 0.003521 | 284 | 99.6491% |
| 8 | 0.001174 | 852 | 99.8828% |
| 9 | 0.001174 | 852 | 99.8828% |
| 10 | 0.003521 | 284 | 99.6491% |
| 11 | 0.001174 | 852 | 99.8828% |
| 12 | 0.001174 | 852 | 99.8828% |
| 13 | 0.002347 | 426 | 99.7658% |
| 14 | 0.003521 | 0.1747 | 14.8719% |
aThe case with a mutation at DYS393