↓ Skip to main content

PLOS

Molecular Phylogeny of the Astrophorida (Porifera, Demospongiaep) Reveals an Unexpected High Level of Spicule Homoplasy

Overview of attention for article published in PLOS ONE, April 2011
Altmetric Badge

Mentioned by

wikipedia
4 Wikipedia pages

Citations

dimensions_citation
70 Dimensions

Readers on

mendeley
109 Mendeley
Title
Molecular Phylogeny of the Astrophorida (Porifera, Demospongiaep) Reveals an Unexpected High Level of Spicule Homoplasy
Published in
PLOS ONE, April 2011
DOI 10.1371/journal.pone.0018318
Pubmed ID
Authors

Paco Cárdenas, Joana R. Xavier, Julie Reveillaud, Christoffer Schander, Hans Tore Rapp

Abstract

The Astrophorida (Porifera, Demospongiae(p)) is geographically and bathymetrically widely distributed. Systema Porifera currently includes five families in this order: Ancorinidae, Calthropellidae, Geodiidae, Pachastrellidae and Thrombidae. To date, molecular phylogenetic studies including Astrophorida species are scarce and offer limited sampling. Phylogenetic relationships within this order are therefore for the most part unknown and hypotheses based on morphology largely untested. Astrophorida taxa have very diverse spicule sets that make them a model of choice to investigate spicule evolution.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 109 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
United States 2 2%
Germany 2 2%
Portugal 1 <1%
Mexico 1 <1%
Norway 1 <1%
Unknown 102 94%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 25 23%
Researcher 21 19%
Student > Master 18 17%
Student > Bachelor 14 13%
Student > Doctoral Student 6 6%
Other 12 11%
Unknown 13 12%
Readers by discipline Count As %
Agricultural and Biological Sciences 57 52%
Environmental Science 12 11%
Biochemistry, Genetics and Molecular Biology 9 8%
Earth and Planetary Sciences 3 3%
Immunology and Microbiology 2 2%
Other 10 9%
Unknown 16 15%