cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15468/ttvnn2
title: Lilium evansii (Liliaceae), a new species from Yunnan, China, formed by ancient hybridization and subsequent isolation

description: This dataset contains the digitized treatments in Plazi based on the original journal article Wang, Jing-Bo, Yuan, Yu-Mei, Ma, Wei-Yin, Yan, Mao-Lin, Yang, Chun-Meng, Pai, Zao-Zha, Li, Hai-Tao, Gao, Yun-Dong (2025): Lilium evansii (Liliaceae), a new species from Yunnan, China, formed by ancient hybridization and subsequent isolation. Phytotaxa 693 (3): 205-220, DOI: 10.11646/phytotaxa.693.3.2, URL: https://doi.org/10.11646/phytotaxa.693.3.2AbstractA new species, Lilium evansii (Liliaceae family), was recently discovered in Yunnan Province, China. Although its range is nearest that of L. henrici, it exhibits the greatest morphological similarity to L. mackliniae, native to the isolated region of Manipur, India, from which it is separated by the vast Kachin Plains. By integration of morphological features and molecular phylogenetic analyses, we clarify the taxonomic placement of L. evansii. The observed discordance between nuclear ribosomal ITS and plastid analyses in resolving the phylogenetic position of this species coupled with its distribution in the Hengduan Mountains points to incomplete lineage sorting or ancient hybridization events and subsequent geographic isolation as key factors in the emergence of this species. Comparative studies using molecular phylogenetics underscore the importance of this discovery for enhancing our understanding of evolutionary processes in the Lilium-Nomocharis complex, a group that thrives in the biodiversity hotspot spanning the Hengduan Mountains and adjacent Himalayan regions.
DOI: 10.15468/m5kthr
title: Cyclodinus humilis (Germar, 1824) neu für die Fauna der Schweiz (COleOptera: Anthicidae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Straumann, Tobias (2020): Cyclodinus humilis (Germar, 1824) neu für die Fauna der Schweiz (COleOptera: Anthicidae). Entomo Helvetica 13: 163-164, DOI: 10.5169/seals-985898Abstract: First record of Cyclodinus humilis (Germar, 1824) in Switzerland (Coleoptera: Anthicidae). − In 2019, Cyclodinus humilis was detected for the first time in Switzerland, in Sisseln, in the canton of Aargau, near a stream.Zusammenfassung: 2019 wurde Cyclodinus humilis erstmals in der Schweiz, in Sisseln im Kanton Aargau, an einem Bach festgestellt.
DOI: 10.15468/aasuq7
title: Anthurium tacotalpense (Araceae), a new species from Mexico

description: This dataset contains the digitized treatments in Plazi based on the original journal article Pérez-Farrera, Miguel Ángel, Jiménez, Pedro Díaz, Croat, Thomas B., Hentrich, Heiko, Vega, José Padilla, Aguilar-Rodríguez, Pedro A. (2022): Anthurium tacotalpense (Araceae), a new species from Mexico. Phytotaxa 538 (1): 74-78, DOI: 10.11646/phytotaxa.538.1.6AbstractAnthurium tacotalpense a new species of genus Anthurium sect. Andiphilum from Tabasco, Mexico is described and illustrated. The new species is morphologically similar to Anthurium cerrobaulense but it differs from that species in having adaxially flattened petioles, spadix up to twice as long and immature berries green, orange when mature.
DOI: 10.15468/zrxtew
title: First Instar Larva Of Atractocerus Brasiliensis (Lepeletier & Audinet-Serville, 1825) (Lymexylidae, Atractocerinae

description: This dataset contains the digitized treatments in Plazi based on the original journal article Casari, Ymexylidae Tractocerinae Sônia A., Albertoni, Fabiano F. (2013): First Instar Larva Of Atractocerus Brasiliensis (Lepeletier & Audinet-Serville, 1825) (Lymexylidae, Atractocerinae. Papéis Avulsos de Zoologia 53 (27): 359-372, DOI: 10.1590/S0031-10492013002700001ABSTRACTThe first instar larva of Atractocerus brasiliensis (Lepetelier & Audinet-Serville, 1825) from state of Goiás, Brazil, and reared in laboratory, is described and illustrated. This is the second species with known first instar larva for the genus and the third for the family. Comparisons with mature larva of this species and with the other known first instar larvae are presented. Illustrations of first instar and mature larvae are also included.KEY-WORDS: Coleoptera; Hylecoetus; Immature; Mature larva; Neotropical region.
DOI: 10.15468/hbtpqm
title: Addendum to the description of the new species Ramphotyphlops mollyozakiae Wallach, 2020 (Serpentes: Typhlopidae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Wallach, Van (2021): Addendum to the description of the new species Ramphotyphlops mollyozakiae Wallach, 2020 (Serpentes: Typhlopidae). Pod @ rcis 12 (2): 22-23, DOI: 10.5281/zenodo.15594380
DOI: 10.25574/csc2.stk.acisfj1701122m300640_001
title: Chandra X-ray Observatory Stack acisfJ1701122m300640_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.acisfj1701169m300433_001
title: Chandra X-ray Observatory Stack acisfJ1701169m300433_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.acisfj1702445p340226_001
title: Chandra X-ray Observatory Stack acisfJ1702445p340226_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.acisfj1757468p044433_001
title: Chandra X-ray Observatory Stack acisfJ1757468p044433_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.acisfj1719297m410018_001
title: Chandra X-ray Observatory Stack acisfJ1719297m410018_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.acisfj1748144m360743_001
title: Chandra X-ray Observatory Stack acisfJ1748144m360743_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.acisfj1659317m370703_001
title: Chandra X-ray Observatory Stack acisfJ1659317m370703_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.acisfj1748349m281519_001
title: Chandra X-ray Observatory Stack acisfJ1748349m281519_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.acisfj1747485m284314_001
title: Chandra X-ray Observatory Stack acisfJ1747485m284314_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.acisfj1748289m283852_001
title: Chandra X-ray Observatory Stack acisfJ1748289m283852_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.acisfj1702496m484657_001
title: Chandra X-ray Observatory Stack acisfJ1702496m484657_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.acisfj1754172p662647_001
title: Chandra X-ray Observatory Stack acisfJ1754172p662647_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.acisfj1800440m414716_001
title: Chandra X-ray Observatory Stack acisfJ1800440m414716_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.acisfj1748577m293407_001
title: Chandra X-ray Observatory Stack acisfJ1748577m293407_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.acisfj1754192p673733_001
title: Chandra X-ray Observatory Stack acisfJ1754192p673733_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.acisfj1722311p655130_001
title: Chandra X-ray Observatory Stack acisfJ1722311p655130_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.acisfj1754349p680010_001
title: Chandra X-ray Observatory Stack acisfJ1754349p680010_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.acisfj1748194m285233_001
title: Chandra X-ray Observatory Stack acisfJ1748194m285233_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.acisfj1822179m160425_001
title: Chandra X-ray Observatory Stack acisfJ1822179m160425_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.acisfj1801380m265008_001
title: Chandra X-ray Observatory Stack acisfJ1801380m265008_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.acisfj1756313p400613_001
title: Chandra X-ray Observatory Stack acisfJ1756313p400613_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.acisfj1720271p273334_001
title: Chandra X-ray Observatory Stack acisfJ1720271p273334_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.acisfj1754109p663929_001
title: Chandra X-ray Observatory Stack acisfJ1754109p663929_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.acisfj1755229p662701_001
title: Chandra X-ray Observatory Stack acisfJ1755229p662701_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.acisfj1819346m134702_001
title: Chandra X-ray Observatory Stack acisfJ1819346m134702_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.acisfj1730238m201548_001
title: Chandra X-ray Observatory Stack acisfJ1730238m201548_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.acisfj1749033m293800_001
title: Chandra X-ray Observatory Stack acisfJ1749033m293800_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.acisfj1810167m314536_001
title: Chandra X-ray Observatory Stack acisfJ1810167m314536_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.acisfj1722304m361241_001
title: Chandra X-ray Observatory Stack acisfJ1722304m361241_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.acisfj1701445m405141_001
title: Chandra X-ray Observatory Stack acisfJ1701445m405141_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.acisfj1833510m103150_001
title: Chandra X-ray Observatory Stack acisfJ1833510m103150_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.acisfj1819332m145753_001
title: Chandra X-ray Observatory Stack acisfJ1819332m145753_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.acisfj1722400m345912_001
title: Chandra X-ray Observatory Stack acisfJ1722400m345912_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.acisfj1749087m291150_001
title: Chandra X-ray Observatory Stack acisfJ1749087m291150_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.acisfj1750247m212555_001
title: Chandra X-ray Observatory Stack acisfJ1750247m212555_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.acisfj1704153p783957_001
title: Chandra X-ray Observatory Stack acisfJ1704153p783957_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.acisfj1721106m193530_001
title: Chandra X-ray Observatory Stack acisfJ1721106m193530_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.acisfj1808397m202515_001
title: Chandra X-ray Observatory Stack acisfJ1808397m202515_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.acisfj1722433p654657_001
title: Chandra X-ray Observatory Stack acisfJ1722433p654657_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.acisfj1750127m064233_001
title: Chandra X-ray Observatory Stack acisfJ1750127m064233_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.acisfj1750139m293408_001
title: Chandra X-ray Observatory Stack acisfJ1750139m293408_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.acisfj1704597m013213_001
title: Chandra X-ray Observatory Stack acisfJ1704597m013213_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.acisfj1723297m342043_001
title: Chandra X-ray Observatory Stack acisfJ1723297m342043_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.acisfj1755547p181859_001
title: Chandra X-ray Observatory Stack acisfJ1755547p181859_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.acisfj1709474m442943_001
title: Chandra X-ray Observatory Stack acisfJ1709474m442943_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.acisfj1755243p663908_001
title: Chandra X-ray Observatory Stack acisfJ1755243p663908_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.acisfj1749146m284412_001
title: Chandra X-ray Observatory Stack acisfJ1749146m284412_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.acisfj1750227m305447_001
title: Chandra X-ray Observatory Stack acisfJ1750227m305447_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.acisfj1757190m273143_001
title: Chandra X-ray Observatory Stack acisfJ1757190m273143_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.acisfj1756338p663401_001
title: Chandra X-ray Observatory Stack acisfJ1756338p663401_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".