cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15468/wjhhur
title: Redescription of Aspidogaster limacoides Diesing, 1834 (Aspidogastrea: Aspidogastridae) from freshwater fishes of northern Germany

description: This dataset contains the digitized treatments in Plazi based on the original journal article Suthar, Jaydipbhai, Al-Jufaili, Sarah, Bray, Rodney A., Frank, Marcus, Theisen, Stefan, Palm, Harry W. (2021): Redescription of Aspidogaster limacoides Diesing, 1834 (Aspidogastrea: Aspidogastridae) from freshwater fishes of northern Germany. Parasitology Research (3405) 120 (10): 3405-3416, DOI: 10.1007/s00436-021-07253-1, URL: http://dx.doi.org/10.1007/s00436-021-07253-1AbstractAspidogaster limacoides Diesing, 1834 (Aspidogastridae) is redescribed based on light and scanning electron microscopy of specimens from the stomach and intestine of Abramis brama, Rutilus rutilus and Scardinius erythrophthalmus (Actinopterygii: Cyprinidae). The fishes were sampled during 2018 and 2019 at Lake Tollense in Mecklenburg-Western Pomerania, Germany. The prevalence of A. limacoides was highest in R. rutilus (61.7%) followed by Scardinius erythrophthalmus (7.7%) and A. brama (2.9%), while it was absent in Perca fluviatilis from the same lake. The following structures of A. limacoides are described for the first time: a depression on the ventral side of the neck, variations in the number and the arrangement of alveoli, numerous pits scattered all over the body surface, the presence of a few papillae-like structures posterior lateral to the mouth, the number of marginal organs represented by openings of exocrine multicellular glands as shown in histology and the subterminal position of the excretory pore. These characters can be used to distinguish three species of Aspidogaster, namely, A. ijimai, A. conchicola and A. limacoides, suggesting that SEM is a useful and promising tool in differentiating Aspidogaster species. Comparison of molecular data of the ITS1-5.8S-ITS2 regions showed a 94% similarity to A. limacoides from the European part of Russia. Phylogenetic analysis showed that the present specimens clustered in the same clade with A. limacoides sensu stricto, forming a distinct group to the exclusion of congeners.
DOI: 10.15468/xvwu33
title: A new species of Coronatella Dybowski & Grochowski, 1984 (Cladocera: Chydoridae) endemic to Jeju Island (Republic of Korea)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Sinev, Artem Y., Lee, Wonchoel, Kotov, Alexey A. (2022): A new species of Coronatella Dybowski & Grochowski, 1984 (Cladocera: Chydoridae) endemic to Jeju Island (Republic of Korea). Zootaxa 5159 (4): 571-582, DOI: 10.11646/zootaxa.5159.4.6AbstractRecently particular attention of cladocerologists has focussed on a subtropical-southern temperate zone of the Far East of Eurasia comprising a center of water flea (Crustacea: Cladocera) endemism. Two endemic taxa were described previously from Jeju Island (Republic of Korea), but still the cladocerans of this island are poorly known. The aim of this communication is to describe a new species of Coronatella (Coronatella) Dybowski & Grochowski, 1894 (Anomopoda: Chydoridae) and discuss diagnostic characters of this taxon with reference to their diagnostic value in other cladoceran groups. Surprisingly, all characters discriminating C. (C.) jejuana sp. nov. from closest C. (C.) rectangula (Sars, 1862) are from the set suggested for chydorid species delimitation by Nikolai Smirnov more than 50 years ago. Therefore, a search for diagnostic characters of a potentially new taxon could concentrate on just some potentially important structures. However, a program of detailed redescriptions of previously established taxa is necessary for an adequate description of new taxa which are congeners of the former, and such comprehensive work is still in its infancy.
DOI: 10.15468/m437eb
title: Molecular phylogeny of Hipparchia Fabricius, 1807 (Lepidoptera: Nymphalidae: Satyrinae) with description of an overlooked species from the Zagros mountains, Iran

description: This dataset contains the digitized treatments in Plazi based on the original journal article Naderi, Alireza, Hagen, Wolfgang Ten, Nazari, Vazrick (2025): Molecular phylogeny of Hipparchia Fabricius, 1807 (Lepidoptera: Nymphalidae: Satyrinae) with description of an overlooked species from the Zagros mountains, Iran. Zootaxa 5636 (2): 361-375, DOI: 10.11646/zootaxa.5636.2.9, URL: https://doi.org/10.11646/zootaxa.5636.2.9AbstractUsing sequence data from four nuclear genes alongside DNA barcodes, we reconstructed the evolutionary history of genus Hipparchia Fabricius, 1807. Our phylogeny supported the previously proposed subgeneric classification for the genus and revealed an overlooked taxon close to H. fatua (Freyer, 1845) from the Zagros mountain range in Western Iran, here described as a new species, Hipparchia lunulata sp. nov. We also confirm that the range of H. fatua sichaea (Lederer, 1857), originally described from Beirut, extends to the westernmost part of the Zagros mountains in Iran.
DOI: 10.15468/qq4g4m
title: A new long-snouted Corydoras (Siluriformes: Callichthyidae) from the rio Xingu and rio Tapajós basins, Brazilian Amazon

description: This dataset contains the digitized treatments in Plazi based on the original journal article Tencatt, Luiz Fernando Caserta, Couto, Ondina Lillan Pinto do, Santos, Sérgio Alexandre dos, Sousa, Leandro Melo de (2024): A new long-snouted Corydoras (Siluriformes: Callichthyidae) from the rio Xingu and rio Tapajós basins, Brazilian Amazon. Neotropical Ichthyology (e 230112) 22 (1): 1-30, DOI: 10.1590/1982-0224-2023-0112, URL: http://dx.doi.org/10.1590/1982-0224-2023-0112
DOI: 10.15468/dl.24abwz
title: Occurrence Download

description: A dataset containing 0 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is one of (Amphibia)",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "Year is greater than or equal to 1980",
 "OccurrenceStatus is Present",
 {
 "not" : {
 "BasisOfRecord" : [
 "is one of (Fossil, Living Specimen)"
 ]
 }
 },
 "Geometry POLYGON((-135 7.5,-127.5 7.5,-127.5 15,-135 15,-135 7.5))"
 ]
}

 The dataset includes 0 records from 0 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0041207-251009101135966/datasets/export for details.
DOI: 10.15468/dl.fss7xt
title: Occurrence Download

description: A dataset containing 331303 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is one of (Rhus typhina, Parthenocissus quinquefolia, Spiraea billardii, Prunus laurocerasus, Rosa rugosa, Spiraea alba, Pistia stratiotes, Solidago gigantea, Rubus armeniacus, Robinia pseudoacacia, Acer negundo, Ailanthus altissima, Alternanthera philoxeroides, Aponogeton distachyos, Arundo donax, Asclepias syriaca, Azolla filiculoides, Baccharis halimifolia, Cabomba caroliniana, Carpobrotus, Cotoneaster horizontalis, Egeria densa, Eichhornia crassipes, Elaeagnus angustifolia, Elodea canadensis, Elodea nuttallii, Fallopia baldschuanica, Fraxinus pennsylvanica, Gymnocoronis spilanthoides, Helianthus tuberosus, Helianthus laetiflorus, Heracleum mantegazzianum, Hydrilla verticillata, Hydrocotyle ranunculoides, Impatiens capensis, Impatiens glandulifera, Koenigia polystachya, Laburnum anagyroides, Lagarosiphon major, Lemna minuta, Lemna turionifera, Limnobium laevigatum, Reynoutria japonica, Myriophyllum rubricaule, Prunus serotina, Parthenocissus tricuspidata, Mahonia aquifolium, Parthenocissus inserta, Spiraea tomentosa, Spiraea douglasii, Reynoutria bohemica, Salvinia molesta, Myriophyllum heterophyllum, Rudbeckia laciniata, Ludwigia grandiflora, Reynoutria sachalinensis, Spiraea salicifolia, Solidago canadensis, Myriophyllum aquaticum, Ludwigia peploides, Zizania latifolia)",
 "Country is Belgium",
 "Year is greater than or equal to 2013",
 "HasCoordinate is true",
 "OccurrenceStatus is Present"
 ]
}

 The dataset includes 331303 records from 42 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0041182-251009101135966/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.qhcwgj
title: Occurrence Download

description: A dataset containing 6631 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is Angola",
 "IucnRedListCategory is one of (CR, EN, VU)"
 ]
}

 The dataset includes 6631 records from 137 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0041208-251009101135966/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/csc2.obs.08234
title: Chandra X-ray Observatory ObsId 08234

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.11087
title: Chandra X-ray Observatory ObsId 11087

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.12439
title: Chandra X-ray Observatory ObsId 12439

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.14586
title: Chandra X-ray Observatory ObsId 14586

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.02677
title: Chandra X-ray Observatory ObsId 02677

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.05372
title: Chandra X-ray Observatory ObsId 05372

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.09606
title: Chandra X-ray Observatory ObsId 09606

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.21679
title: Chandra X-ray Observatory ObsId 21679

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.03662
title: Chandra X-ray Observatory ObsId 03662

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.12438
title: Chandra X-ray Observatory ObsId 12438

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.22504
title: Chandra X-ray Observatory ObsId 22504

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.14987
title: Chandra X-ray Observatory ObsId 14987

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.10064
title: Chandra X-ray Observatory ObsId 10064

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.07517
title: Chandra X-ray Observatory ObsId 07517

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.08156
title: Chandra X-ray Observatory ObsId 08156

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.10360
title: Chandra X-ray Observatory ObsId 10360

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.17691
title: Chandra X-ray Observatory ObsId 17691

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.13730
title: Chandra X-ray Observatory ObsId 13730

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.23047
title: Chandra X-ray Observatory ObsId 23047

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.07739
title: Chandra X-ray Observatory ObsId 07739

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.14453
title: Chandra X-ray Observatory ObsId 14453

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.03507
title: Chandra X-ray Observatory ObsId 03507

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.10289
title: Chandra X-ray Observatory ObsId 10289

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.10891
title: Chandra X-ray Observatory ObsId 10891

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.09568
title: Chandra X-ray Observatory ObsId 09568

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.19599
title: Chandra X-ray Observatory ObsId 19599

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.03795
title: Chandra X-ray Observatory ObsId 03795

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.11041
title: Chandra X-ray Observatory ObsId 11041

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.16676
title: Chandra X-ray Observatory ObsId 16676

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.12547
title: Chandra X-ray Observatory ObsId 12547

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.08033
title: Chandra X-ray Observatory ObsId 08033

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.19601
title: Chandra X-ray Observatory ObsId 19601

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.22060
title: Chandra X-ray Observatory ObsId 22060

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.04128
title: Chandra X-ray Observatory ObsId 04128

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.17318
title: Chandra X-ray Observatory ObsId 17318

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.21366
title: Chandra X-ray Observatory ObsId 21366

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.01047
title: Chandra X-ray Observatory ObsId 01047

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.12284
title: Chandra X-ray Observatory ObsId 12284

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.08984
title: Chandra X-ray Observatory ObsId 08984

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.05561
title: Chandra X-ray Observatory ObsId 05561

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.03794
title: Chandra X-ray Observatory ObsId 03794

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.10520
title: Chandra X-ray Observatory ObsId 10520

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.07825
title: Chandra X-ray Observatory ObsId 07825

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.04548
title: Chandra X-ray Observatory ObsId 04548

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".