UNOISE2: improved error-correction for Illumina 16S and ITS amplicon sequencing
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Citations
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References
Introducing mothur: Open-Source, Platform-Independent, Community-Supported Software for Describing and Comparing Microbial Communities
Search and clustering orders of magnitude faster than BLAST
DADA2: High-resolution sample inference from Illumina amplicon data
UCHIME improves sensitivity and speed of chimera detection
UPARSE: highly accurate OTU sequences from microbial amplicon reads
Related Papers (5)
QIIME allows analysis of high-throughput community sequencing data.
Frequently Asked Questions (16)
Q2. What is the way to ensure that reads of the same template have the same length?
If multiple primers were used which do not bind to the same locus, then trimming is required to ensure that reads of the same template amplified by different primers start and end at the same position in the biological sequence.
Q3. Why is denoising more effective with quality-filtered reads?
denoising is more effective with quality-filtered reads because sequencing error bias can cause some errors to have sufficiently high abundances that they could be mistaken for biological variants, and these often have lower quality scores.
Q4. How many different 16S sequences are in the reference database?
the reference database for the HMP mock community (21 strains) has 115 different 16S sequences, an average of 5.5 distinct 16S sequences per strain.
Q5. Why is it problematic to cut the sequences?
Global trimming and defining abundance Calculating unique sequence abundance is problematic when reads of the same template sequence vary in length, e.g. because reads are truncated when the quality score drops below a threshold.
Q6. What is the way to classify a sequence as non-chimeric?
A sequence cannot be reliably classified as nonchimeric unless it is identical to a reference sequence(Edgar, 2016), and amplicons with uncorrected point errors therefore cannot be reliably classified.
Q7. How many chimeras will have abundance ratios 2?
If fluctuations in the abundance ratio are equally likely to give values <2 and >2, then approximately half of the chimeras formed in the first round will have abundance ratio <2, i.e. 1/(2N).
Q8. What are some examples of microbial tag sequencing experiments?
Recent examples of microbial tag sequencing experiments include the Human Microbiome Project(HMP Consortium, 2012) and a survey of the Arabidopsis root microbiome(Lundberg et al., 2012).
Q9. What is the probability that many of the UCHIME2 predictions are also false positives?
Given that UCHIME2 agrees with 400/657 of the DADA2 chimera predictions with ratios >2, it seems likely that many of the UCHIME2 predictions are also false positives, despite using more stringent parameters (no differences allowed in the model, abundance ratio ≥2).
Q10. Why is the abundance of a given sequence lost?
Some low-abundance variants may be lost that would be correctly identified by pooling, e.g., because they are singletons in some of the samples where they occur.
Q11. What is the protocol for amplification followed by sequencing?
The experimental protocol in such studies includes amplification by PCR followed by sequencing, which introduces errors in several ways.
Q12. What is the probability of false positive chimeras?
I believe that false positive chimeras will have a much higher frequency than uncorrected point errors, given the high accuracy of DADA2 on most of the mock datasets and the observation that fake chimeric models are very common, especially when differences are allowed(Edgar, 2016).
Q13. What is the maximum skew allowed for a member with d differences?
If skew(M, C) ≤ β(d) then M is a valid member of a cluster defined by C; i.e., βis the maximum skew allowed for a member with d differences.
Q14. What is the way to avoid the problems of global trimming?
These problems are avoided by ensuring that reads of the same template sequence have the same length (global trimming, implying that reads of the same template should be globally alignable, though more distantly related sequences need not be).
Q15. What is the way to define a sequence with high abundance?
With (1), a given template sequence with high abundance in the amplicons will typically have many different unique sequences with low abundances because its reads are truncated to many different lengths.
Q16. What is the name of the first amplicon sequencing error correction method?
The first amplicon sequencing error-correction methods were designed for pyrosequencing flowgrams(Quince et al., 2011, 2009; Reeder and Knight, 2010; Rosen et al., 2013).