| Literature DB >> 35758686 |
Abdelmajeed Nasereddin1, Hadar Golan Berman2, Dana G Wolf3, Esther Oiknine-Djian3, Sheera Adar2.
Abstract
COVID-19 is caused by SARS-CoV-2, several virulent variants of which have emerged since 2019. More than 529 million people have been infected, and at least 6 million have died. Our aim was to develop a fast, accurate, low-cost method for detecting and identifying newly emerging variants of concern (VOCs) that could pose a global threat. The 341-bp DNA sequence of a specific region of the SARS-CoV-2's spike protein was amplified by a one-step PCR on RNA samples from 46 patients. The product was sequenced using next-generation sequencing (NGS). DNA sequences from seven genomes, the original Wuhan isolate and six different representative variants obtained from the GISAID website, were used as references. Complete whole-genome sequences from local isolates were also obtained from the GISAID website, and their RNA was used for comparison. We used an amplicon-based NGS method (termed VOC-NGS) for genotyping and successfully identified all 46 samples. Fifteen (32.6%) were like the original isolate. Twenty-seven were VOCs: nine (19.5%) Alpha, eight (19%) Delta, six (14%) Beta, and four (8.7%) Omicron. Two were variants of interest (VOI): one (2%) Kappa and one (2%) Zeta. Two samples were mixtures of two variants, one of Alpha and Beta and one of Alpha and Delta. The Spearman correlation between whole-genome sequencing (WGS) and VOC-NGS was significant (P < 0.001) with perfect agreement (Kappa = 0.916) for 36/38 (94.7%) samples with VOC-NGS detecting all the known VOCs. Genotyping by VOC-NGS enables rapid screening of high-throughput clinical samples that includes the identification of VOCs and mixtures of variants, at lower cost than WGS. IMPORTANCE The manuscript described SARS-Cov-2 genotyping by VOC-NGS, which presents an ideal balance of accuracy, rapidity, and cost for detecting and globally tracking VOCs and some VOI of SARS-CoV-2. A large number of clinical samples can be tested together. Rapid introduction of new mutations at a specific site of the spike protein necessitates efficient strain detection and identification to enable choice of treatment and the application of vaccination, as well as planning public health policy.Entities:
Keywords: NGS; PCR; SARS-CoV-2; WGS; mutations; pandemic; variants of concern (VOC); variants of interest (VOI)
Mesh:
Substances:
Year: 2022 PMID: 35758686 PMCID: PMC9430688 DOI: 10.1128/spectrum.00736-22
Source DB: PubMed Journal: Microbiol Spectr ISSN: 2165-0497
The primers used in the study and the final concentration of each one
| Primer | Sequence 5′–3′ | Final conc. μM | Product MW |
|---|---|---|---|
| MutF1 |
| 0.5 | 421 |
| MutR1 |
| 0.5 | |
| HS478F |
| 0.125 | 213 |
MW, molecular weight.
FIG 1PCR amplification used in the study to obtain the two required fragments was done with a combination of three primers (MutF1, MutR1, and HS478F). 1: the optimized PCR using 0.5 μM of MutF1_MutR1 primers. In order to control the lower-molecular-weight product amplification, low concentration of 2nd forward primer HS478F (0.125 μM). 2: 0.5 μM used in all the primers sets.
The viral isolates used in this study, including the WGS mutations, lineages, and their mutations detected by VOC-NGS system
| No. or GISAID | Sample barcode |
| VOC-NGS | VOC-NGS mutations | WGS mutations | WSG linages | Collection date and location (mo.date.yr/city) |
|---|---|---|---|---|---|---|---|
| EPI_ISL_10550531 | AbedN | NA | Omicron | N440K, G446S, Q493R, G496S, Q498R, Y505H | A67V, T95I, Q321E, G339D, R346K, S371L, S373P, S375F, K417N, N440K, G446S, S477N, T478K, E484A, Q493R, G496S, Q498R, N501Y, Y505H, T547K, D614G, H655Y, N679K, P681H, N764K, D796Y, N856K, Q954H, N969K, L981F | BA.1 21K | 02.19.2022/Jerusalem |
| EPI_ISL_10550530 | Sila | NA | Omicron | N440K, G446S, Q493R, G496S, Q498R, Y505H | A67V, T95I, G339D, R346K, S371L, S373P, S375F, K417N, N440K, G446S, S477N, T478K, E484A, Q493R, G496S, Q498R, N501Y, Y505H, T547K, D614G, H655Y, N679K, P681H, N764K, D796Y, N856K, Q954H, N969K, L981F | BA.1 21K | 02.19.2022/Jerusalem |
| EPI_ISL_10550533 | JER5 | NA | Omicron | N440K, G446S, Q493R, G496S, Q498R, Y505H | A67V, T95I, G339D), S371L, S373P, S375F, K417N, N440K, G446S, S477N, T478K, E484A, Q493R, G496S, Q498R, N501Y, Y505H, T547K, D614G, H655Y, N679K, P681H, N764K, D796Y, N856K, Q954H, N969K, L981F | BA.1 21K | 02.05.2022/Jericho |
| EPI_ISL_10550532 | JER12 | NA | Omicron | N440K, G446S, Q493R, G496S, Q498R, Y505H | A67V, V70I, T95I, Y145D, Q321Z, G339D, R346K, S371L, S373P, S375F, K417N, N440K, G446S, S477N, T478K, E484A, Q493R, G496S, Q498R, N501Y, Y505H, T547K, D614G, H655Y, N679K, P681H, N764K, D796Y, N856K, Q954H, N969K, L981F | BA.1 21K | 02.05.2022/Jericho |
| EPI_ISL_2107518 | AAS6 | NA | Alpha | N501Y | A570D, D614G, D1118H, L5F, N501Y, P681H, S982A, T716I, V70I | B.1.1.7 | 10.24.2020/Jericho |
| EPI_ISL_1502573 | AAS53 | NA | Alpha | N501Y | A570D, D614G, D1118H, L5F, N501Y, P681H, S982A, T716I, V70I | B.1.1.7 | 05.02.2021/Salfit |
| EPI_ISL_2107510 | AAS81 | NA | Alpha | N501Y | A570D, D614G, D1118H, L5F, N501Y, N1098D, P681H, S982A, T716I, V70I | B.1.1.7 | 09.04.2021/Salfit |
| EPI_ISL_2107509 | AAS80 | NA | Alpha | N501Y | A570D, D614G, D1118H, F490S, L5F, N501Y, P681H, S982A, T716I, V70I | B.1.1.7 | 09.04.2021/Tubas |
| EPI_ISL_2107525 | AAS77 | NA | Alpha | N501Y | A570D, D614G, D1118H, L5F, N501Y, P681H, S982A, T716I, V70I | B.1.1.7 | 09.04.2021/Tubas |
| EPI_ISL_1273092 | AAS29 | NA | Original | Not detected | A520S, D614G | B.1.1.50 | 11.30.2020/Tubas |
| EPI_ISL_661272 | WB-AQU-P3 | NA | Original | Not detected | D614G | B | 11.07.2020/Jericho |
| EPI_ISL_1273087 | AAS20 | NA | Original | Not detected | D614G | B.1.1.50 | 11.30.2020/Nablus |
| EPI_ISL_1502569 | AAS48 | NA | Original | Not detected | A570D, D614G, D1118H | NONE | 02.05.2021/Nablus |
| EPI_ISL_1273095 | AAS36 | NA | Original | Not detected | D614G | B.1.1.50 | 11.30.2020/Jenin |
| 96 | 2648372 | NA | Epsilon | L452R | L18F, D80A, D215G, L242H, K417N, E484K, N501Y, D614G, A701V, A1020S, G1219C | B.1.351 | 02.09.2021/Jerusalem |
| 249 | 2576218 | NA | Beta | MIX E484K, N501Y | L452R, D614G, S929I, L1063F | B.1.362 | 01.25.2021/Jerusalem |
| 416 | 2674042 | NA | Zeta | E484K | L5F, P26S, T95I, D253G, E484K, D614G, A701V | B.1.526 | 04.25.2021/Jerusalem |
| 610 | 225383 | NA | Delta | L452R, T478K | T19R, T95I, E156G, L452R, T478K, D614G, P681R, D950N | B.1.617.2 | 05.? ?0.2021/Jerusalem |
| 616 | 824 | NA | Alpha_Beta | K417N, E484K, N501Y | H69S, E484K, N501Y, A570D, D614G, S640F, P681H, T716I, S982A, D1118H | B.1.1.7 | 05.12.2021/Jerusalem |
| 641 | 2672172 | NA | Delta | L452R, T478K | T19R, E156G, L452R, T478K, D614G, P681R, D950N | B.1.617.2 | 02.28.2021/Tel Aviv |
| 721 | S1 | NA | Beta | K417N, E484K, N501Y | D80A, D215G, L242H, K417N, E484K, N501Y, D614G, A701V | B.1.351 | 10.03.2021/Jerusalem |
| 722 | S2 | NA | Alpha | N501Y | N74K, N501Y, A570D, D614G, P681H, T716I, S982A, D1118H | B.1.1.7 | 10.? ?0.2021/Jerusalem |
| 723 | S3 | NA | Original | Not detected | T95I, S477N, D614G, A831S | B.1.160 | 10.? ?0.2021/Jerusalem |
| 724 | S4 | NA | Original | Not detected | S477N, D614G | B.1.160 | 10.03.2021/Jerusalem |
| 725 | S5 | NA | Original | Not detected | S477N, D614G | B.1.160.16 | 10.? ?0.2021/Jerusalem |
| 726 | 835 | NA | Beta | K417N, E484K, N501Y | D614G | B.1 | 10.? ?0.2021/Jerusalem |
| 727 | 839 | NA | Original | Not detected | None | NA | 10.? ?0.2021/Jerusalem |
| 728 | S8 | NA | Beta | K417N, E484K, N501Y | V70F, D80A, D215G, L242H, K417N, E484K, N501Y, D614G, A701V | B.1.351 | 10.? ?0.2021/Jerusalem |
| 729 | S9 | NA | Beta | K417N, E484K, N501Y | NA | 10.03.2021/Jerusalem | |
| 730 | 829 | NA | Alpha | N501Y | N501Y, A570D, D614G, P681H, T716I, S982A, D1118H | B.1.1.7 | 10.? ?0.2021/Jerusalem |
| 731 | S11 | NA | Alpha | N501Y | N501Y, A570D, D614G, P681H, T716I, S982A, D1118H | B.1.1.7 | 10.? ?0.2021/Jerusalem |
| 732 | 848 | NA | Original | Not detected | S477N, D614G, A831S | B.1.160 | 10.? ?0.2021/Jerusalem |
| 733 | S13 | Original | Not detected | S477N, D614G | B.1.160 | 10.03.2021/Jerusalem | |
| 734 | S14 | Original | Not detected | S477N, D614G, A831S | B.1.160 | 10.03.2021/Jerusalem | |
| 735 | S15 | Original | Not detected | N439K, D614G | B.1.258 | 10.03.2021/Jerusalem | |
| 736 | S16 | Original | Not detected | N74K, N501Y, A570D, D614G, P681H, T716I, S982A, D1118H | B.1.1.7 | 10.03.2021/Jerusalem | |
| 740 | 2667065 | 29 | Delta | L452R, T478K | T19R, L452R, T478K, D614G, P681R, T791I, D950N | B.1.617.2 | 07.12.2021/Jerusalem |
| 741 | 845 | 33 | Alpha_Delta | L452R, T478K, N501Y | V3G, L5F, F140L, G142D, L242H, N501Y, A570D, D614G, P681H, T716I, S982A, D1118H | B.1.1.7 | 07.? ?0.2021/Jerusalem |
| 742 | 2665422 | 15 | Delta | L452R, T478K | T19R, E156G, L452R, T478K, D614G, P681R, D950N | B.1.617.2 | 07.13.2021/Jerusalem |
| 743 | 2672449 | 15 | Delta | L452R, T478K | L5F, T19R, E156G, L452R, T478K, D614G, P681R, D950N | B.1.617.2 | 07.? ?0.2021/Jerusalem |
| 744 | 2665453 | 18 | Delta | L452R, T478K | T19R, E156G, L452R, T478K, D614G, P681R, T791I, D950N | B.1.617.2 | 07.? ?0.2021/Jerusalem |
| 745 | 2672564 | 22 | Delta | L452R, T478K | T19R, E156G, L452R, T478K, D614G, P681R, D950N | B.1.617.2 | 07.16.2021/Jerusalem |
| 746 | 2672568 | 20 | Delta | L452R, T478K | T19R, E156G, L452R, T478K, D614G, P681R, D950N | B.1.617.2 | 07.16.2021/Jerusalem |
| 747 | 2672569 | 35 | Delta | L452R, T478K | Did not work due to high | NONE | 07.16.2021/Jerusalem |
, threshold cycle; NA, not available.
FIG 2Multiple alignment of spike HSR DNA sequences from representative patients with COVID-19 and reference sequences for different VOCs from the GISAID website (Table 2). The 341-bp DNA sequence from the spike HSR region was aligned, using a free online multiple sequence alignment program (35). Representative clinical samples used in the figure are 848, 824, 829, 839, 835, and Sila. The red dots indicate those nucleotides identical to those of the DNA sequence of the Wuhan isolate. The blue and black letters present the changes that have occurred in the nucleotide sequence compared to that of the Wuhan isolate. The black/blue letters indicate the position of nucleotide substitution/deletion. The black N portions showed no sequenced region by the Nextseq machine since the sequence kit could not reach beyond 150 bp from one direction. Clearly, the VOC-NGS system was able to identify Omicron’s six unique mutations (N440K, G446S, Q493R, G496S, Q498R, and Y505H) in the target region. Ns: Any nucleotide.
FIG 3IGV results of galaxy mapping at positions 232 and 283, showing, respectively, the mutations E484K with the nucleotide G changed significantly to A at 65% coinfection-contamination and N501Y with the nucleotide A almost fully changed significantly to T at 98%.
FIG 4The target region for amplicon sequencing (341 bp) from the Wuhan isolate. Bold black arrows indicate the positions of the primers. Highlighted: sequences used for primers in this study. Bold red: the nucleotide conversions. Bold black font: the corresponding amino acid conversions. * indicates mutations found in the recent Omicron variant.
FIG 5Schematic overview of the study workflow.