Biophthora Foerster, 1862

Taxonomic History / Nomenclature
Biophthora Foerster, 1862. Type species: Opius bajulus Haliday, 1837 (monobasic and original designation).

Type locality of type species apparently England (van Achterberg 1997); holotype female in National Museum of Ireland, Dublin, labelled as male by Stelfox, no doubt because it was described as a male by Haliday. Problem of correctly identifying the sex of the holotype noted by Koenig (1972) and van Achterberg (1997).

Treated as a synonym of the subgenus Xynobius by Fischer (1972) or as a synonym of the genus Xynobius by van Achterberg (2004). Wharton (2006), however, treated it as a separate genus (see remarks section).

Remarks
As noted by Wharton (2006), the type species of Biophthora, bajulus, is similar in many respects to the type species of Xynobius because of the sculptured scutellum, mesoscutal midpit, and T1 dorsope. Wharton (2006) argued against treatment of Biophthora as a synonym of Xynobius because of the differences in placement of the T2 spiracle in caelatus (type species of Xynobius). In bajulus, the spiracle is more dorsally placed relative to the more laterally place spiracle of caelatus. Other differences include wing venation (in bajulus, m-cu is postfurcal, the stigma is wedge-shaped, and the second submarginal cell is weakly narrowed distally), head (clypeus is flat and truncate ventrally, with the labrum weakly exposed; mandibles are more slender and more nearly parallel-sided in bajulus), and T1 sculpture (Wharton 2006). Wharton (2006) also treated bajulus as a senior subjective synonym of Sternaulopius beieri Fischer, 1968 and noted that there were few differences other than the sculptured scutellum of bajulus that separate the type species of Biophthora from the type species of Sternaulopius.
Diagnosis and Relationships
The type species is characterized by the presence of both a true sternaulus and a more dorsally placed precoxal sulcus. It is similar in this respect to the genus Sternaulopius, but differs from the latter by the presence of a sculptured scutellum (Figs 6, 9, 10). Other notable features include a relatively flattened clypeus with labrum narrowly exposed below the truncate ventral margin (Fig. 3), presence of a true sternaulus (Fig. 3) in addition to the more dorsally placed precoxal sulcus (Figs 4, 5), presence of a mesoscutal midpit (Figs 2, 6, 8-10), crenulate but short notaulus (Fig. 6), fore wing as in Figs 1 and 11 (with postfurcal m-cu, distally narrowing second submarginal cell, wedge-shaped stigma, with r arising basal midpoint), hind wing as in Fig. 12, T1 with deep dorsope (Fig. 15), T2 with spiracles positioned dorsal-laterally (Fig. 14).
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1. Biophthora bajulus later...
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2. Biophthora bajulus dorsa...
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3. Biophthora bajulus face ...
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4. Biophthora bajulus basal...
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5. Biophthora bajulus later...
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6. Biophthora bajulus...
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7. Biophthora bajulus...
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8. Biophthora bajulus...
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9. Biophthora bajulus dorsa...
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10. Biophthora bajulu...
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11.Biophthora bajulus wings
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12. Biophthora bajulus hind wing...
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13. Biophthora bajulus metas...
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14. Biophthora bajulus metas...
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15. Biophthora bajulus T...
 
Distribution
No referenced distribution records have been added to the database for this OTU.
Map

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

Acknowledgements
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 July, 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.