cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.stk.acisfj0106419m715738_001
title: Chandra X-ray Observatory Stack acisfJ0106419m715738_001

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.stk.acisfj0102393m715033_001
title: Chandra X-ray Observatory Stack acisfJ0102393m715033_001

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.stk.acisfj0102009m720113_001
title: Chandra X-ray Observatory Stack acisfJ0102009m720113_001

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.stk.acisfj0156268p053622_001
title: Chandra X-ray Observatory Stack acisfJ0156268p053622_001

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.stk.acisfj0200121m093120_001
title: Chandra X-ray Observatory Stack acisfJ0200121m093120_001

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.stk.acisfj0102059m720441_001
title: Chandra X-ray Observatory Stack acisfJ0102059m720441_001

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.stk.acisfj0126435p331311_001
title: Chandra X-ray Observatory Stack acisfJ0126435p331311_001

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.stk.acisfj0224181m043940_001
title: Chandra X-ray Observatory Stack acisfJ0224181m043940_001

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.stk.acisfj0151006m003444_001
title: Chandra X-ray Observatory Stack acisfJ0151006m003444_001

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.stk.acisfj0209377p522648_001
title: Chandra X-ray Observatory Stack acisfJ0209377p522648_001

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.stk.acisfj0223086p425913_001
title: Chandra X-ray Observatory Stack acisfJ0223086p425913_001

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.stk.acisfj0225046m244716_001
title: Chandra X-ray Observatory Stack acisfJ0225046m244716_001

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.stk.acisfj0126109m052910_001
title: Chandra X-ray Observatory Stack acisfJ0126109m052910_001

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.stk.acisfj0226009p030318_001
title: Chandra X-ray Observatory Stack acisfJ0226009p030318_001

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.stk.acisfj0102378m720453_001
title: Chandra X-ray Observatory Stack acisfJ0102378m720453_001

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.stk.acisfj0206225m060953_001
title: Chandra X-ray Observatory Stack acisfJ0206225m060953_001

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.stk.acisfj0201217p195844_001
title: Chandra X-ray Observatory Stack acisfJ0201217p195844_001

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.stk.acisfj0205398m582557_001
title: Chandra X-ray Observatory Stack acisfJ0205398m582557_001

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.stk.acisfj0224387p891406_001
title: Chandra X-ray Observatory Stack acisfJ0224387p891406_001

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.stk.acisfj0109261p354300_001
title: Chandra X-ray Observatory Stack acisfJ0109261p354300_001

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.stk.acisfj0120378m724525_001
title: Chandra X-ray Observatory Stack acisfJ0120378m724525_001

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.stk.acisfj0159535m084820_001
title: Chandra X-ray Observatory Stack acisfJ0159535m084820_001

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.stk.acisfj0152597m134305_001
title: Chandra X-ray Observatory Stack acisfJ0152597m134305_001

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.stk.acisfj0112050p492826_001
title: Chandra X-ray Observatory Stack acisfJ0112050p492826_001

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.stk.acisfj0155415p312504_001
title: Chandra X-ray Observatory Stack acisfJ0155415p312504_001

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.stk.acisfj0228149p311823_001
title: Chandra X-ray Observatory Stack acisfJ0228149p311823_001

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.stk.acisfj0229576p002803_001
title: Chandra X-ray Observatory Stack acisfJ0229576p002803_001

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.stk.acisfj0258200p132652_001
title: Chandra X-ray Observatory Stack acisfJ0258200p132652_001

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.stk.acisfj0109487p613327_001
title: Chandra X-ray Observatory Stack acisfJ0109487p613327_001

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.stk.acisfj0206518p121549_001
title: Chandra X-ray Observatory Stack acisfJ0206518p121549_001

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.stk.acisfj0102500m222122_001
title: Chandra X-ray Observatory Stack acisfJ0102500m222122_001

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.stk.acisfj0123363p331535_001
title: Chandra X-ray Observatory Stack acisfJ0123363p331535_001

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.stk.acisfj0215238m034313_001
title: Chandra X-ray Observatory Stack acisfJ0215238m034313_001

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: 10.15468/dl.rp3juj
title: Occurrence Download

description: A dataset containing 128 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((-99.39471 -13.41260,-56.95013 -13.41260,-56.95013 3.55796,-99.39471 3.55796,-99.39471 -13.41260))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Cestrum auriculatum L'Hér."
 ]
}

 The dataset includes 128 records from 19 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010696-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/csc2.stk.acisfj0155294p434602_001
title: Chandra X-ray Observatory Stack acisfJ0155294p434602_001

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.stk.acisfj0102484m023141_001
title: Chandra X-ray Observatory Stack acisfJ0102484m023141_001

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.stk.acisfj0205182m023259_001
title: Chandra X-ray Observatory Stack acisfJ0205182m023259_001

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.stk.acisfj0236212m522822_001
title: Chandra X-ray Observatory Stack acisfJ0236212m522822_001

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.stk.acisfj0205432p644935_001
title: Chandra X-ray Observatory Stack acisfJ0205432p644935_001

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.stk.acisfj0110179p314715_001
title: Chandra X-ray Observatory Stack acisfJ0110179p314715_001

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.stk.acisfj0157097p285142_001
title: Chandra X-ray Observatory Stack acisfJ0157097p285142_001

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: 10.15468/dl.n3zqer
title: Occurrence Download

description: A dataset containing 12029 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Crotalaria pallida Aiton"
 ]
}

 The dataset includes 12029 records from 431 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010695-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5281/zenodo.18045304
title: Efficient simulation of low-entanglement bosonic Gaussian states in polynomial time

description: dataset and code for arXiv: 2512.10643.
DOI: 10.5281/zenodo.18045305
title: Efficient simulation of low-entanglement bosonic Gaussian states in polynomial time

description: dataset and code for arXiv: 2512.10643.
DOI: 10.15468/vzsw3x
title: Cheirostylis barbata, a new species Orchidaceae (Goodyerinae) from Yunnan, China

description: This dataset contains the digitized treatments in Plazi based on the original journal article Wu, Xun-Feng, Liu, Qiang, Li, Jin-Long, Tang, Zong-Ying, Xing, Xiao-Ke (2020): Cheirostylis barbata, a new species Orchidaceae (Goodyerinae) from Yunnan, China. Phytotaxa 436 (3): 293-297, DOI: 10.11646/phytotaxa.436.3.7, URL: http://dx.doi.org/10.11646/phytotaxa.436.3.7AbstractCheirostylis barbata, a new species of Orchidaceae, is described and illustrated from Yunnan Province, China. It is morphological similar to C. griffthii, but it can be easily distinguished from the latter in having densely villous inflorescence, floral bracts 1.2–1.4 cm, significantly longer than ovary, lobes of lip deeply laciniate with 7–9 divisions, each lacinae randomly oriented, 6.0– 7.5 mm long, hypochile containing 2 callus, each callus 4-toothed. A preliminary assessment of extinction risk, according to the IUCN Red List Categories and Criteria, is also provided.
DOI: 10.15468/v4hq8s
title: Wing pattern variation and DNA barcodes defy taxonomic splitting in the New Zealand Pimelea Looper Notoreas perornata (Walker) (Lepidoptera: Geometridae: Larentiinae): the importance of populations as conservation units

description: This dataset contains the digitized treatments in Plazi based on the original journal article Hoare, Robert J. B., Patrick, Brian H., Buckley, Thomas R., Brav-Cubitt, Talia (2023): Wing pattern variation and DNA barcodes defy taxonomic splitting in the New Zealand Pimelea Looper Notoreas perornata (Walker) (Lepidoptera: Geometridae: Larentiinae): the importance of populations as conservation units. Zootaxa 5346 (1): 1-27, DOI: 10.11646/zootaxa.5346.1.1, URL: http://dx.doi.org/10.11646/zootaxa.5346.1.1AbstractThe endemic Notoreas perornata (Walker, 1863) complex (Lepidoptera: Geometridae: Larentiinae) from the North Island and northern South Island of New Zealand is reviewed. Larvae feed on Pimelea spp. (Thymelaeaceae), frequently in highly fragmented and threatened shrubland habitats. Allopatric populations tend to differ in size and wing pattern characteristics, but not in genitalia; moreover extensive variation renders recognition of subspecies / allopatric species based on any species concept problematic. A mitochondrial DNA gene tree is not congruent with morphology and indicates rapid recent divergence that has not ‘settled’ into diagnosable lineages. Based on our results, we synonymise Notoreas simplex Hudson, 1898 with N. perornata (Walker, 1863), and retain N. perornata as a single, highly diverse but monotypic species. All known populations are illustrated to display variation. For conservation purposes, we recommend the continued recognition within the species of 10 populations or groups of populations that appear to be on the way to diverging at subspecific level based on morphological and/or DNA data. The conservation status of all these populations is reviewed. One conservation unit, comprising the populations from Westland, has not been seen since 1998 and is feared possibly extinct.
DOI: 10.15468/z6srqh
title: Morphological and molecular evidence for a new species from China: Dendrobium yongjiaense (Orchidaceae: Malaxideae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Zhou, Zhuang, Zhang, Sai, Yang, Yan-Ping, Ma, Liang, Lan, Si-Ren (2020): Morphological and molecular evidence for a new species from China: Dendrobium yongjiaense (Orchidaceae: Malaxideae). Phytotaxa 441 (2): 203-210, DOI: 10.11646/phytotaxa.441.2.7, URL: http://dx.doi.org/10.11646/phytotaxa.441.2.7AbstractA new orchid species, Dendrobium yongjiaense, from Zhejiang, China, is described and illustrated here. Detailed morphological study indicates that D. yongjiaense is similar to D. monticola and D. strongylanthum, but it differs in the shape and size of leaf, flower size, and a mid-lobe of the lip with densly distinct crystalline papillae and wrinkled 3–5 crest lines in middle. Molecular phylogeny analyses based on the nrITS and plastid DNA (matK and trnL-F) reveal that D. yongjiaense is a member of sect. Stachyobium, and genetically similar to D. monticola.
DOI: 10.15468/qpn84b
title: Nothobranchius balamaensis (Cyprinodontiformes: Nothobranchiidae), a new species of annual killifish from northern Mozambique

description: This dataset contains the digitized treatments in Plazi based on the original journal article Bragança, Pedro H. N., Bellstedt, Dirk U., Merwe, P. De Wet Van Der, Cotterill, Fenton P. D., Watters, Brian R., Chakona, Albert (2022): Nothobranchius balamaensis (Cyprinodontiformes: Nothobranchiidae), a new species of annual killifish from northern Mozambique. Zootaxa 5174 (5): 508-524, DOI: 10.11646/zootaxa.5174.5.2AbstractA new seasonal killifish of the genus Nothobranchius is described from the Montepuez River system in northern Mozambique. The new species, Nothobranchius balamaensis Bragança & Chakona, is differentiated from congeners by its characteristic colour pattern and molecular data further support its taxonomic distinctiveness. Phylogenetic results based on two mitochondrial and three nuclear genes confirms N. balamaensis is closely related to N. kirki and N. wattersi; all three belonging to the Coastal-Inland Clade. The new species is most similar in colour pattern to N. kirki sharing the characteristic of a deep red-orange colouration in the basal, proximal, and medial zones of the caudal and anal fins that grades to orange in the distal zone. This is a key feature that distinguishes these two species from all other Nothobranchius. The main distinguishing features between the new species and N. kirki is the presence of a light blue to white band or series of irregular markings in the proximal zone of the anal fin in N. kirki, versus the absence of such a colour pattern element in N. balamaensis, as well as differences in the dorsal fin pattern. When compared to all population groups of N. wattersi, the colour pattern of N. balamaensis is distinctive. Nothobranchius balamaensis is a relatively slender member of the genus, a characteristic that clearly distinguishes it from both N. kirki and N. wattersi. Nothobranchius balamaensis is currently only known from a few specimens from the type locality.