Antrops orbitalis (KITS & MARSHALL, 2013)
publication ID |
https://doi.org/ 10.11646/zootaxa.3704.1.1 |
publication LSID |
lsid:zoobank.org:pub:341ED5F6-2DCA-4E73-83D6-389DF0DD347F |
persistent identifier |
https://treatment.plazi.org/id/03A18780-C673-FFB8-0DD3-DAB4FB87F892 |
treatment provided by |
Felipe |
scientific name |
Antrops orbitalis |
status |
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Antrops orbitalis group
The Antrops orbitalis group is a clade of 15 species, 13 of which were previously undescribed. This clade was keyed as the Archiborborus orbitalis View in CoL group by Marshall and Buck (2010), who suggested that it represented an unnamed subgenus. Although this group is highly distinct within the subfamily, the phylogeny of Kits et al. (2013) suggests it belongs within the genus Antrops View in CoL . Members of the group are small (<3 mm), entirely black to dark brown, and usually almost entirely shiny ( Fig. 9 View FIGURES 7–12 ). Species occur exclusively in the Andes and the Venezuelan coastal ranges, from approximately 1200 m to over 4000 m ASL. Several species occur in the dry puna of northern Argentina and Chile to Peru, while other species occur in moister páramo and cloud forest habitats from Bolivia north to Venezuela.
The A. orbitalis View in CoL group is clearly monophyletic. Synapomorphies for the clade (states found in other Archiborborinae in parentheses) include 1) the nearly uniform structure of the male fifth sternite ( Fig. 121 View FIGURES 119–124 ), broad and parallel-sided at the base with the apical portion narrowed triangularly (various, but never exactly as above); 2) the characteristic ventral tooth of the surstylus ( Fig. 86 View FIGURES 85–91 ) (surstylus entire, not toothed); 3) entirely brown halter (halter predominately white); 4) interfrontal plates darker than orbital and frontal plates, shiny, and striate (interfrontal plates usually smooth and/or microtomentose, if shiny and striate then paler than orbital and interfrontal plates); 5) gena entirely shiny (gena with at least some microtomentum). The extensively shiny appearance of all members of the group except the male of A. guandera View in CoL sp. nov. is also distinctive, and combined with the unmarked wings this group is readily recognizable. Within the species group, A. guandera View in CoL is likely the sister group to the remaining species, based on the plesiomorphic retention of extensive microtomentum and 6 acrostichal rows in the male. The A. nitidicollis complex is derived within the group, with the greatest reduction of microtomentum and partial loss of the microtrichia at the base of the wing ( Fig. 14 View FIGURES 13–18 ) as derived characters for the clade.
Many specific characters for identification depend in part on the form of the surstylus. Descriptive terms for the parts of the surstylus referred to in descriptions are illustrated in Figure 86 View FIGURES 85–91 .
No known copyright restrictions apply. See Agosti, D., Egloff, W., 2009. Taxonomic information exchange and copyright: the Plazi approach. BMC Research Notes 2009, 2:53 for further explanation.
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Antrops orbitalis
KITS, JOEL H. & MARSHALL, STEPHEN A. 2013 |
Antrops orbitalis
KITS & MARSHALL 2013 |
A. guandera
KITS & MARSHALL 2013 |
A. guandera
KITS & MARSHALL 2013 |
A. nitidicollis
KITS & MARSHALL 2013 |
Archiborborus orbitalis
Duda 1921 |
A. orbitalis
Duda 1921 |
Antrops
Enderlein 1909 |