Abstract
Section Flavi encompasses both harmful and beneficial Aspergillus species, such as Aspergillus oryzae, used in food fermentation and enzyme production, and Aspergillus flavus, food spoiler and mycotoxin producer. Here, we sequence 19 genomes spanning section Flavi and compare 31 fungal genomes including 23 Flavi species. We reassess their phylogenetic relationships and show that the closest relative of A. oryzae is not A. flavus, but A. minisclerotigenes or A. aflatoxiformans and identify high genome diversity, especially in sub-telomeric regions. We predict abundant CAZymes (598 per species) and prolific secondary metabolite gene clusters (73 per species) in section Flavi. However, the observed phenotypes (growth characteristics, polysaccharide degradation) do not necessarily correlate with inferences made from the predicted CAZyme content. Our work, including genomic analyses, phenotypic assays, and identification of secondary metabolites, highlights the genetic and metabolic diversity within section Flavi.
Original language | English |
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Article number | 1106 |
Number of pages | 12 |
Journal | Nature Communications |
Volume | 11 |
Issue number | 1 |
DOIs | |
Publication status | Published - 27 Feb 2020 |
Funding
Genome sequencing was kindly supported by Joint BioEnergy Institute and Joint Genome Institute. M.R.A., J.L.N., S.T. and T.C.V. gratefully acknowledge funding from the Villum Foundation, Grant VKR023437. M.R.A. and T.C.V. further acknowledge funding from the Danish National Research Foundation, grant number DNRF137. M.R.A. further acknowledges support from the Jorck Foundation. The work conducted by the US Department of Energy Joint Genome Institute, a US Department of Energy Office of Science User Facility, is supported by the Office of Science of the US Department of Energy under Contract No. DE-AC02-05CH11231. The US Department of Energy Joint BioEnergy Institute (www.jbei.org) is supported by the US Department of Energy, Office of Science, and Office of Biological and Environmental Research, through Contract DE-AC02-05CH11231 between Lawrence Berkeley National Laboratory and the US Department of Energy.