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Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation

It is commonly assumed that increasing the number of characters has the potential to resolve evolutionary radiations. Here, we studied photosynthetic stramenopiles (Ochrophyta) using alignments of heterogeneous origin mitochondrion, plastid, and nucleus. Surprisingly while statistical support for th...

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Autores principales: Di Franco, Arnaud, Baurain, Denis, Glöckner, Gernot, Melkonian, Michael, Philippe, Hervé
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Oxford University Press 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8763130/
https://www.ncbi.nlm.nih.gov/pubmed/34694402
http://dx.doi.org/10.1093/molbev/msab300
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author Di Franco, Arnaud
Baurain, Denis
Glöckner, Gernot
Melkonian, Michael
Philippe, Hervé
author_facet Di Franco, Arnaud
Baurain, Denis
Glöckner, Gernot
Melkonian, Michael
Philippe, Hervé
author_sort Di Franco, Arnaud
collection PubMed
description It is commonly assumed that increasing the number of characters has the potential to resolve evolutionary radiations. Here, we studied photosynthetic stramenopiles (Ochrophyta) using alignments of heterogeneous origin mitochondrion, plastid, and nucleus. Surprisingly while statistical support for the relationships between the six major Ochrophyta lineages increases when comparing the mitochondrion (6,762 sites) and plastid (21,692 sites) trees, it decreases in the nuclear (209,105 sites) tree. Statistical support is not simply related to the data set size but also to the quantity of phylogenetic signal available at each position and our ability to extract it. Here, we show that this ability for current phylogenetic methods is limited, because conflicting results were obtained when varying taxon sampling. Even though the use of a better fitting model improved signal extraction and reduced the observed conflicts, the plastid data set provided higher statistical support for the ochrophyte radiation than the larger nucleus data set. We propose that the higher support observed in the plastid tree is due to an acceleration of the evolutionary rate in one short deep internal branch, implying that more phylogenetic signal per position is available to resolve the Ochrophyta radiation in the plastid than in the nuclear data set. Our work therefore suggests that, in order to resolve radiations, beyond the obvious use of data sets with more positions, we need to continue developing models of sequence evolution that better extract the phylogenetic signal and design methods to search for genes/characters that contain more signal specifically for short internal branches.
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spelling pubmed-87631302022-01-18 Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation Di Franco, Arnaud Baurain, Denis Glöckner, Gernot Melkonian, Michael Philippe, Hervé Mol Biol Evol Discoveries It is commonly assumed that increasing the number of characters has the potential to resolve evolutionary radiations. Here, we studied photosynthetic stramenopiles (Ochrophyta) using alignments of heterogeneous origin mitochondrion, plastid, and nucleus. Surprisingly while statistical support for the relationships between the six major Ochrophyta lineages increases when comparing the mitochondrion (6,762 sites) and plastid (21,692 sites) trees, it decreases in the nuclear (209,105 sites) tree. Statistical support is not simply related to the data set size but also to the quantity of phylogenetic signal available at each position and our ability to extract it. Here, we show that this ability for current phylogenetic methods is limited, because conflicting results were obtained when varying taxon sampling. Even though the use of a better fitting model improved signal extraction and reduced the observed conflicts, the plastid data set provided higher statistical support for the ochrophyte radiation than the larger nucleus data set. We propose that the higher support observed in the plastid tree is due to an acceleration of the evolutionary rate in one short deep internal branch, implying that more phylogenetic signal per position is available to resolve the Ochrophyta radiation in the plastid than in the nuclear data set. Our work therefore suggests that, in order to resolve radiations, beyond the obvious use of data sets with more positions, we need to continue developing models of sequence evolution that better extract the phylogenetic signal and design methods to search for genes/characters that contain more signal specifically for short internal branches. Oxford University Press 2021-10-25 /pmc/articles/PMC8763130/ /pubmed/34694402 http://dx.doi.org/10.1093/molbev/msab300 Text en © The Author(s) 2021. Published by Oxford University Press on behalf of the Society for Molecular Biology and Evolution. https://creativecommons.org/licenses/by-nc/4.0/This is an Open Access article distributed under the terms of the Creative Commons Attribution-NonCommercial License (https://creativecommons.org/licenses/by-nc/4.0/), which permits non-commercial re-use, distribution, and reproduction in any medium, provided the original work is properly cited. For commercial re-use, please contact journals.permissions@oup.com
spellingShingle Discoveries
Di Franco, Arnaud
Baurain, Denis
Glöckner, Gernot
Melkonian, Michael
Philippe, Hervé
Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation
title Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation
title_full Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation
title_fullStr Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation
title_full_unstemmed Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation
title_short Lower Statistical Support with Larger Data Sets: Insights from the Ochrophyta Radiation
title_sort lower statistical support with larger data sets: insights from the ochrophyta radiation
topic Discoveries
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8763130/
https://www.ncbi.nlm.nih.gov/pubmed/34694402
http://dx.doi.org/10.1093/molbev/msab300
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