cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.stk.acisfj0051128p002053_001
title: Chandra X-ray Observatory Stack acisfJ0051128p002053_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.acisfj0103510m715920_001
title: Chandra X-ray Observatory Stack acisfJ0103510m715920_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.acisfj0147092p463026_001
title: Chandra X-ray Observatory Stack acisfJ0147092p463026_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.acisfj0212008p042213_001
title: Chandra X-ray Observatory Stack acisfJ0212008p042213_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.acisfj0103564m720109_001
title: Chandra X-ray Observatory Stack acisfJ0103564m720109_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.acisfj0137242m454108_001
title: Chandra X-ray Observatory Stack acisfJ0137242m454108_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.acisfj0214306m051813_001
title: Chandra X-ray Observatory Stack acisfJ0214306m051813_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.acisfj0213571p275422_001
title: Chandra X-ray Observatory Stack acisfJ0213571p275422_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.acisfj0236389p593856_002
title: Chandra X-ray Observatory Stack acisfJ0236389p593856_002

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.acisfj0050399m732234_001
title: Chandra X-ray Observatory Stack acisfJ0050399m732234_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.acisfj0107381m721504_001
title: Chandra X-ray Observatory Stack acisfJ0107381m721504_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.acisfj0136403p154817_001
title: Chandra X-ray Observatory Stack acisfJ0136403p154817_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.acisfj0208565m074857_001
title: Chandra X-ray Observatory Stack acisfJ0208565m074857_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.acisfj0216454p703528_001
title: Chandra X-ray Observatory Stack acisfJ0216454p703528_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.acisfj0050558p293311_001
title: Chandra X-ray Observatory Stack acisfJ0050558p293311_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.acisfj0104256m720640_001
title: Chandra X-ray Observatory Stack acisfJ0104256m720640_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.dcsxck
title: Occurrence Download

description: A dataset containing 11503 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Cosmos sulphureus Cav."
 ]
}

 The dataset includes 11503 records from 402 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010691-250127130748423/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.acisfj0229507m293815_001
title: Chandra X-ray Observatory Stack acisfJ0229507m293815_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.acisfj0139577m055334_001
title: Chandra X-ray Observatory Stack acisfJ0139577m055334_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.acisfj0217439m034504_001
title: Chandra X-ray Observatory Stack acisfJ0217439m034504_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.acisfj0111051m455823_001
title: Chandra X-ray Observatory Stack acisfJ0111051m455823_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.acisfj0216093m115551_001
title: Chandra X-ray Observatory Stack acisfJ0216093m115551_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.acisfj0217106m050940_001
title: Chandra X-ray Observatory Stack acisfJ0217106m050940_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.acisfj0104071m715031_001
title: Chandra X-ray Observatory Stack acisfJ0104071m715031_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.acisfj0136466p412408_001
title: Chandra X-ray Observatory Stack acisfJ0136466p412408_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.acisfj0145495m043207_001
title: Chandra X-ray Observatory Stack acisfJ0145495m043207_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.acisfj0215133m084608_001
title: Chandra X-ray Observatory Stack acisfJ0215133m084608_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.acisfj0108398p013452_001
title: Chandra X-ray Observatory Stack acisfJ0108398p013452_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.acisfj0053546m000235_001
title: Chandra X-ray Observatory Stack acisfJ0053546m000235_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.acisfj0146262p614519_001
title: Chandra X-ray Observatory Stack acisfJ0146262p614519_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.acisfj0055076m374214_001
title: Chandra X-ray Observatory Stack acisfJ0055076m374214_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.acisfj0055021m374558_001
title: Chandra X-ray Observatory Stack acisfJ0055021m374558_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.acisfj0147361p021945_001
title: Chandra X-ray Observatory Stack acisfJ0147361p021945_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.acisfj0220551m015638_001
title: Chandra X-ray Observatory Stack acisfJ0220551m015638_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.acisfj0148124p000207_001
title: Chandra X-ray Observatory Stack acisfJ0148124p000207_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.acisfj0107389m113914_001
title: Chandra X-ray Observatory Stack acisfJ0107389m113914_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.acisfj0104475m221701_001
title: Chandra X-ray Observatory Stack acisfJ0104475m221701_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.acisfj0104539p020834_001
title: Chandra X-ray Observatory Stack acisfJ0104539p020834_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: 10.3886/e241562v1
title: Sociocultural Attitudes Towards Appearance

description: data :the Sociocultural Attitudes Towards Appearance Scale in
Chinese college students
description: Response Rates: likert sacle
description: Presence of Common Scales: The Sociocultural Attitudes
Towards Appearance Scale-4
DOI: 10.15468/4dab5m
title: Lesteva (s. str.) amica sp. n., a new species from Yunnan, China (Coleoptera: Staphylinidae: Omaliinae: Anthophagini)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Shavrin, Alexey V. (2022): Lesteva (s. str.) amica sp. n., a new species from Yunnan, China (Coleoptera: Staphylinidae: Omaliinae: Anthophagini). Zootaxa 5195 (3): 293-295, DOI: 10.11646/zootaxa.5195.3.8
DOI: 10.15468/fk6abg
title: Life-cycle of the Afrotropical snail-killing fly Sepedon (Parasepedon) ruficeps Becker, 1923

description: This dataset contains the digitized treatments in Plazi based on the original journal article Gbedjissi, Ghélus Louis, Vala, Jean-Claude (2014): Life-cycle of the Afrotropical snail-killing fly Sepedon (Parasepedon) ruficeps Becker, 1923. African Invertebrates 55 (1): 1, DOI: 10.5733/afin.055.0102, URL: http://www.bioone.org/doi/abs/10.5733/afin.055.0102ABSTRACTSepedon ruficeps is a widespread species among Sciomyzidae in the Afrotropical Region. Its general distribution, and more specifically that in Benin, is mapped. The complete life-cycle, from egg to adult, and descriptions of all immature stages are presented. Larval predation of freshwater molluscs is analyzed, with the main objective of discovering biological control agents for snail intermediate hosts of trematodes, principally Schistosoma and Fasciola species which affect man and domestic animals. The results reported here relate to Radix natalensis, snail host of Fasciola gigantea. In the absence of sufficient mollusc-prey, however, the fly larvae show alternative predation at the expense of the freshwater snail Aulophorus furcatus. This particularity could allow intensive laboratory rearing, before release of all stages of the fly in the field for biocontrol of distomiasis. S. ruficeps is undoubtedly polyphagous and multivoltine.KEY WORDS: Immature stages, larval feeding behaviour, larval predation, biological control agent, oligochaete, fascioliasis, Radix natalensis.
DOI: 10.15468/6uxpsv
title: Is the North Atlantic Geodia barretti (Porifera, Tetractinellida, Geodiidae) present on the Southwest Indian Ridge?

description: This dataset contains the digitized treatments in Plazi based on the original journal article Periasamy, Rengaiyan, Cárdenas, Paco, Kurian, Palayil John, Ingole, Baban, Samaai, Toufiek (2023): Is the North Atlantic Geodia barretti (Porifera, Tetractinellida, Geodiidae) present on the Southwest Indian Ridge? Zootaxa 5380 (5): 461-474, DOI: 10.11646/zootaxa.5380.5.3, URL: https://www.mapress.com/zt/article/download/zootaxa.5380.5.3/52400AbstractThere are currently 163 species of Geodia Lamarck, 1815 described worldwide, many of which are found in deep waters, but none of which have been recorded from the Southwest Indian Ridge (SWIR). Spicule morphology and barcodes (Folmer COI, 28S (C2–D2), partial 18S) suggest that a specimen of Geodia collected on the SWIR at a depth of 2236 m is closely comparable to Geodia barretti Bowerbank, 1858. Geodia barretti is the most studied and thus well-known deep-sea Geodia species, due to its wide North Atlantic distribution and key role in boreal sponge grounds. This unexpected and markedly disjunct record would extend the distribution range of this species considerably, consequently challenging our knowledge about interoceanic deep-sea sponges.
DOI: 10.15468/ghyagv
title: A new species of Bauhinia ser. Cansenia (Cercidoideae, Leguminosae) endemic to the Atlantic Forest in the state of Bahia, Brazil

description: This dataset contains the digitized treatments in Plazi based on the original journal article Dos Santos, Antonio C. B., De Queiroz, Luciano P., Paula, Antonio P. O., Carvalho, Reginaldo De (2022): A new species of Bauhinia ser. Cansenia (Cercidoideae, Leguminosae) endemic to the Atlantic Forest in the state of Bahia, Brazil. Phytotaxa 568 (2): 213-220, DOI: 10.11646/phytotaxa.568.2.6, URL: http://dx.doi.org/10.11646/phytotaxa.568.2.6AbstractThe genus Bauhinia belongs to the subfamily Cercidoideae (Leguminosae) and includes ca. 230 species with pantropical distribution. Sixty-two species are recorded in Brazil, 20 of which occur in the northeastern Brazilian state of Bahia. The genus is classified in eight sections, with sect. Pauletia being the most diverse. This article describes Bauhinia arleneae, a new species from this section, restricted to the humid forests of the central-eastern region of the state of Bahia. The new species is morphologically similar to B. cinnamomea, with both species sharing entire and elliptical leaves with acuminate apex and flowers paired along the pseudoracemes. B. arleneae differs from B. cinnamomea by the slender and flexuous multi-stemmed shrub or treelet habit, with glabrous leaves with 3 to 5 primary veins and fruit with coriaceous-woody, reticulate valves. We provide a description, illustrations, and a distribution map for the new species.
DOI: 10.15468/2g57sw
title: Aspidistra saccata (Asparagaceae), a new species with erect stem from limestone areas in Guangxi, China

description: This dataset contains the digitized treatments in Plazi based on the original journal article Huang, Xue-Yan, Peng, Yu-De, Nong, Dong-Xin, Huang, Bao-You, Yu, Li-Ying (2022): Aspidistra saccata (Asparagaceae), a new species with erect stem from limestone areas in Guangxi, China. Phytotaxa 541 (3): 297-300, DOI: 10.11646/phytotaxa.541.3.10, URL: http://dx.doi.org/10.11646/phytotaxa.541.3.10
DOI: 10.15468/jubav3
title: Hidden diversity in Daptomys (Rodentia: Cricetidae): a new species from lower montane forests of central Peru

description: This dataset contains the digitized treatments in Plazi based on the original journal article Pacheco, Víctor, Sánchez-Vendizú, Pamela, Fajardo, Úrsula, Cossíos, Daniel, Cadenillas, Richard (2025): Hidden diversity in Daptomys (Rodentia: Cricetidae): a new species from lower montane forests of central Peru. Zootaxa 5696 (4): 451-481, DOI: 10.11646/zootaxa.5696.4.1, URL: https://doi.org/10.11646/zootaxa.5696.4.1AbstractDaptomys Anthony, 1929, comprises at least five species, distributed in lower and premontane Neotropical forests from Venezuela to Bolivia, but its real diversity is likely underestimated. During recent expeditions to Tingo María National Park, Huánuco Department, in central Peru, we collected two specimens of Daptomys in premontane forest, that represent a new lineage. Here, we present an integrative approach combining coalescent phylogenetic analyses (based on cytochrome b and three nuclear gene sequences), along with morphological and morphometric data, to support the recognition of the Huánuco specimens as a new species of Daptomys, which we describe in this paper. The new species can be distinguished from other congeners by a unicolored tail ending in a distinct pencil of white hairs, a very small toothrow, anteriorly expanded nasals, a very short incisive foramina, a long palate with a prominent median process, and a large postglenoid foramen. In addition, the species delimitation methods recovered D. musseri as a valid species which is supported also by morphological and morphometric differentiation and distribution pattern.
DOI: 10.15468/yjurfp
title: Remarks on the type of the Linnaean name Asplenium marinum (Aspleniaceae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Ferrer-Gallego, P. Pablo (2016): Remarks on the type of the Linnaean name Asplenium marinum (Aspleniaceae). Phytotaxa 260 (1): 98-100, DOI: 10.11646/phytotaxa.260.1.12, URL: http://dx.doi.org/10.11646/phytotaxa.260.1.12