Calisto obscura subsp. grannus
publication ID |
https://doi.org/ 10.11646/zootaxa.4317.1.1 |
publication LSID |
lsid:zoobank.org:pub:D92F7Bb8-A6D5-4530-83Ba-14D5A50A29Fb |
DOI |
https://doi.org/10.5281/zenodo.6029783 |
persistent identifier |
https://treatment.plazi.org/id/0148B602-FFD1-FF98-FF17-FBD815DFFF51 |
treatment provided by |
Plazi |
scientific name |
Calisto obscura subsp. grannus |
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The C. grannus View in CoL populations
We analyzed 58 sequences belonging to the eight taxa included in the former C. grannus complex or species group due its genitalic morphology and the possession of two circled ocelli with central pupils at the under surface of HW ( Schwartz & Gali 1984, Gonzalez 1987). Some were originally described as separate species from localities separated a few kilometers at the major mountain range of Hispaniola, the Cordillera Central ( C. grannus grannus M. Bates, 1939 , C. grannus dilemma González, 1987 , C. grannus phoinix González, 1987 , C. grannus amazona González, 1987 , C. grannus micheneri Clench, 1944 ) whereas others were discovered at more distant places of the C. Central ( C. grannus dystacta González, 1987 ), the middle Sierra de Neiba ( C. grannus micrommata Schwartz & Gali, 1984 ) or the southern Sierra de Bahoruco ( C. grannus sommeri Schwartz & Gali, 1984 ) ( Fig. 19 View FIGURES 19 – 20. 19 ). Sourakov & Zakharov (2011), based on COI barcode sequences obtained from 28 specimens, lowered the status of most of these taxa from species to subspecies level using mitochondrial DNA as evidence of low divergence level between them. We did not include sequences from the latter study in our analysis as they lacked precise geographical data, with the exception of six sequences representing C. grannus sommeri , which we included in our dataset.
No Bayesian, Maximum Likelihood or Neighbor Joining produced a single cluster formed only by specimens from the same locality or belonging to a single taxon with most clades weakly supported ( Fig. 18 View FIGURE 18 ). K2P pairwise distances values were between 0 and 2.1%, or 0 to 12 differences, with intra-taxon minimum pairwise distances ranging from 0 ( C. grannus micrommata ) to 1.1% ( C. grannus phoinix ) and intertaxa minimum pairwise distances from 0.3 ( C. grannus micrommata – C. grannus sommeri ) to 1.2% ( C. grannus amazona – C. grannus micheneri ).
The species identification methods recovered a single entity (all PTP variants, ABGD, BIN) or two and as much as 14 entities, GMYC single and multiple threshold respectively ( Fig. 18 View FIGURE 18 ). The later method also mixed specimens from different named populations mixed within the delimited entities.
The Median Joining haplotype network shed some light on the relationships of these populations ( Fig. 20 View FIGURES 19 – 20. 19 ). The analysis identified 36 haplotypes. Calisto grannus sommeri and C. grannus micrommata were represented by 8, 18 sequences, and 2, 4 sequences, haplotypes respectively. These haplotypes are unique from their respective geographic ranges, Sierra de Bahoruco and Sierra de Neiba. Populations of the northern Cordillera Central included 26 haplotypes, 36 sequences, 19 of them represented by unique sequences. Four haplotypes of these populations are shared by two or three named populations ( Fig. 20 View FIGURES 19 – 20. 19 ).
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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Satyrinae |
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