Paraxynobius van Achterberg, 2004

Taxonomic History / Nomenclature
Paraxynobius van Achterberg, 2004: 314, 317. Type species: Xynobius (Paraxynobius) granulatus van Achterberg, 2004 (original designation).

Type locality of type species: Christchurch, New Zealand; holotype female in RMNH (Leiden).

Originally described as a subgenus of Xynobius, and as of mid 2015 has not been treated since the original description. Valid subgenus within Opiinae. Wharton (2006) treats Xynobius as a subgenus of Eurytenes but Li et al. (2013) retain it as a separate genus.

Paraxynobius was based on two species from New Zealand characterized by a granulate mesopleuron (Fig. 9), fore wing r arising distad the midpoint of the very broad, somewhat wedge-shape stigma (Fig. 1, 11), fore wing 2Rs about equal in length to 3RSa, and the mesoscutual midpit not well developed (Figs 7, 8). It was placed in Xynobius largely on the basis of the presence of a dorsope and absence of a laterope on the first metasomal tergite (T1) and the exposed labrum. The occipital carina is complete dorsally (Fig. 7).
1. Paraxynobius habitus...
2.Paraxynobius face
3.Paraxynobius face
4. Paraxynobius head latera...
5.Paraxynobius mandible
6. Paraxynobius head dorsal...
7. Paraxynobius head and me...
8. Paraxynobius head and me...
9.Paraxynobius mesosoma
10.Paraxynobius propodeum
11.Paraxynobius wings
12. Paraxynobius metasoma...
13.Paraxynobius metasoma
No referenced distribution records have been added to the database for this OTU.

There are no specimens currently determined for this OTU, or those specimens determined for this OTU are not yet mappable.

This page was assembled by Bob Wharton and Danielle Restuccia. It is part of a review of the genera of World Opiinae, conducted at Texas A&M University. We are particularly grateful to Xanthe Shirley, Andrew Ly, Patricia Mullins, Trent Hawkins, Lauren Ward, Cheryl Hyde, Karl Roeder, and Andrea Walker, who did nearly all of the imaging (together with Danielle) for this project. Matt Yoder and Istvan Miko provided guidance on databasing issues associated with our use of mx and HAO respectively. This project would not have been possible without the kindness of many curators at museums throughout the world who gave generously of their time to Bob Wharton and his students. In particular, I thank Henry Townes (deceased) and David Wahl (American Entomological Institute, Gainesville), Gordon Nishida (Bernice P. Bishop Museum, Honolulu), Norm Penny, and Bob Zuparko (California Academy of Sciences, San Francisco), Bill Mason (deceased), Mike Sharkey, Andrew Bennett, and Henri Goulet (Canadian National Collection, Ottawa), Paul Dessart (deceased) (Institut Royal des Sciences Naturelles de Belgique, Brussels), Marc De Meyer (Koninklijk Museum voor Midden-Afrika, Tervuren), Axel Bachmann (Museo Argentino de Ciencias Natureles, Buenos Aires), Eberhard Koenigsmann (deceased) and Frank Koch (Museum fuer Naturkunde der Humboldt-Universitaet, Berlin), J. Casevitz Weulersse and Claire Villemant (Museum National d’Historie Naturelle, Paris), James O’Connor (National Museum of Ireland, Dublin), Jenö Papp (National Museum of Natural History, Budapest), Kees van Achterberg (National Museum of Natural History, Leiden), Max Fischer, Herb Zettel, and Dominique Zimmermann (Naturhistorisches Museum, Wien), Per Persson and Lars-Åke Janzon (Naturhistoriska Riksmuseet, Stockholm), Ermenegildo Tremblay (Silvestri Collection, Portici), Erasmus Haeselbarth (Staatliche Naturwissenschaftliche Sammlungen Bayerns, Munich), Tom Huddleston and Gavin Broad (The Natural History Museum, London), Paul Marsh and Robert Kula (USDA Systematic Research Laboratory and US National Museum of Natural History, Washington, D. C.), Vladimir Tobias (deceased) and Sergey Belokobylskij (Zoological Institute, Academy of Sciences, St. Petersburg), and Roy Danielsson (Zoological Institute, Department of Systematics, Lund) for facilitating loans and general assistance associated with examination of holotypes and other material in their care. This work was supported largely by NSF/PEET DEB 0328922 and 0949027, with REU supplements 0723663, 1026618, 1213790, and 1313933 (to Wharton). Page last updated June, 2015. The material on this page is freely available, but should be acknowledged if used elsewhere.

This material is based upon work supported by the National Science Foundation under Grant Numbers DEB 9300517, DEB (PEET) 9712543, DEB (PEET) 0328922 with REU supplements 0723663 and 1026618 and DEB 0949027 with REU supplements 1213790 and 1313933. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.