cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.stk.acisfj1229590p133711_001
title: Chandra X-ray Observatory Stack acisfJ1229590p133711_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.acisfj1129595p363858_001
title: Chandra X-ray Observatory Stack acisfJ1129595p363858_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.acisfj1218100p281053_001
title: Chandra X-ray Observatory Stack acisfJ1218100p281053_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.acisfj1220057m002510_001
title: Chandra X-ray Observatory Stack acisfJ1220057m002510_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.acisfj1120487p232410_001
title: Chandra X-ray Observatory Stack acisfJ1120487p232410_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.acisfj1218495p142516_001
title: Chandra X-ray Observatory Stack acisfJ1218495p142516_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.acisfj1225557p181307_001
title: Chandra X-ray Observatory Stack acisfJ1225557p181307_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.acisfj1218219p401402_001
title: Chandra X-ray Observatory Stack acisfJ1218219p401402_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.acisfj1121487m131301_001
title: Chandra X-ray Observatory Stack acisfJ1121487m131301_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.acisfj1133202p470130_001
title: Chandra X-ray Observatory Stack acisfJ1133202p470130_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.acisfj1222061p090215_001
title: Chandra X-ray Observatory Stack acisfJ1222061p090215_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.acisfj1229490p132618_001
title: Chandra X-ray Observatory Stack acisfJ1229490p132618_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.acisfj1219115p042859_001
title: Chandra X-ray Observatory Stack acisfJ1219115p042859_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.acisfj1219232p055022_001
title: Chandra X-ray Observatory Stack acisfJ1219232p055022_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.acisfj1228054p283639_001
title: Chandra X-ray Observatory Stack acisfJ1228054p283639_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.acisfj1221311p491509_001
title: Chandra X-ray Observatory Stack acisfJ1221311p491509_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.acisfj1121527p564715_001
title: Chandra X-ray Observatory Stack acisfJ1121527p564715_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.acisfj1124439p191946_001
title: Chandra X-ray Observatory Stack acisfJ1124439p191946_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.acisfj1218499m010220_001
title: Chandra X-ray Observatory Stack acisfJ1218499m010220_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.acisfj1219283p505352_001
title: Chandra X-ray Observatory Stack acisfJ1219283p505352_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.acisfj1219406p293620_001
title: Chandra X-ray Observatory Stack acisfJ1219406p293620_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.acisfj1123574p213220_001
title: Chandra X-ray Observatory Stack acisfJ1123574p213220_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.acisfj1126586p294442_001
title: Chandra X-ray Observatory Stack acisfJ1126586p294442_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.acisfj1222582p154753_001
title: Chandra X-ray Observatory Stack acisfJ1222582p154753_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.acisfj1123086p053034_001
title: Chandra X-ray Observatory Stack acisfJ1123086p053034_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.acisfj1220059p291548_001
title: Chandra X-ray Observatory Stack acisfJ1220059p291548_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.acisfj1226550m005216_001
title: Chandra X-ray Observatory Stack acisfJ1226550m005216_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.acisfj1221166p043626_001
title: Chandra X-ray Observatory Stack acisfJ1221166p043626_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.acisfj1226355p035819_001
title: Chandra X-ray Observatory Stack acisfJ1226355p035819_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.acisfj1221053p113736_001
title: Chandra X-ray Observatory Stack acisfJ1221053p113736_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.acisfj1221538p042753_001
title: Chandra X-ray Observatory Stack acisfJ1221538p042753_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.acisfj1225592p154000_001
title: Chandra X-ray Observatory Stack acisfJ1225592p154000_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.acisfj1220356p334725_001
title: Chandra X-ray Observatory Stack acisfJ1220356p334725_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.acisfj1222405p075716_001
title: Chandra X-ray Observatory Stack acisfJ1222405p075716_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.acisfj1229074p020337_001
title: Chandra X-ray Observatory Stack acisfJ1229074p020337_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.acisfj1225542p073258_001
title: Chandra X-ray Observatory Stack acisfJ1225542p073258_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.acisfj1220015p291707_001
title: Chandra X-ray Observatory Stack acisfJ1220015p291707_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.acisfj1220170p752232_001
title: Chandra X-ray Observatory Stack acisfJ1220170p752232_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.acisfj1229425p081444_001
title: Chandra X-ray Observatory Stack acisfJ1229425p081444_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.acisfj1219448p124809_001
title: Chandra X-ray Observatory Stack acisfJ1219448p124809_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.acisfj1220233p053430_001
title: Chandra X-ray Observatory Stack acisfJ1220233p053430_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.acisfj1222187p144552_001
title: Chandra X-ray Observatory Stack acisfJ1222187p144552_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.acisfj1230431p080453_001
title: Chandra X-ray Observatory Stack acisfJ1230431p080453_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.acisfj1124538m591537_001
title: Chandra X-ray Observatory Stack acisfJ1124538m591537_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.acisfj1128206m011423_001
title: Chandra X-ray Observatory Stack acisfJ1128206m011423_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.acisfj1224275p420632_001
title: Chandra X-ray Observatory Stack acisfJ1224275p420632_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.acisfj1224147p083155_001
title: Chandra X-ray Observatory Stack acisfJ1224147p083155_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.acisfj1125352p542304_001
title: Chandra X-ray Observatory Stack acisfJ1125352p542304_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.emajss
title: Occurrence Download

description: A dataset containing 155767 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Cynodon dactylon (L.) Pers."
 ]
}

 The dataset includes 155767 records from 1924 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010734-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/6cekgg
title: Nachweis von Dinoderus minutus (Fabricius, 1775) in der Schweiz (Coleoptera: Bostrichidae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Marggi, Werner, Germann, Christoph (2018): Nachweis von Dinoderus minutus (Fabricius, 1775) in der Schweiz (Coleoptera: Bostrichidae). Entomo Helvetica 11: 157-160, DOI: 10.5169/seals-986033Abstract: Record of the Bamboo Borer Dinoderus minutus (Fabricius, 1775) in Switzerland (Coleoptera: Bostrichidae). − Three living specimens were found in bamboo Mikado sticks. While this pantropical species is not capable of establishing wild populations in Switzerland, it has the potential to inflict considerable damage in the warm season. A short overview of the Swiss Bostrichidae is provided and a key to the Dinoderus species occurring in Switzerland is given.Zusammenfassung: Drei lebende Exemplare wurden in Mikado-Stäbchen aus Bambus gefunden. Die pantropisch verbreitete Art kann sich bei uns nicht im Freien etablieren, könnte jedoch hohes Schadpotenzial während der warmen Monate zeigen. Eine kurze Übersicht über die schweizerischen Bostrichidae und ein kurzer Schlüssel zu den bisher bei uns gemeldeten Dinoderus -Arten wird gegeben.
DOI: 10.15468/b6g6xm
title: Phedimus yangshanicus (Crassulaceae), a new species from limestone hills in Guangdong, China

description: This dataset contains the digitized treatments in Plazi based on the original journal article Chao, Zhi (2020): Phedimus yangshanicus (Crassulaceae), a new species from limestone hills in Guangdong, China. Phytotaxa 429 (2): 148-156, DOI: 10.11646/phytotaxa.429.2.5, URL: http://dx.doi.org/10.11646/phytotaxa.429.2.5AbstractThe author describes a new species of Crassulaceae, Phedimus yangshanicus, growing on limestone rocks or hills in Guangdong, China. Morphologically unique in the genus, this plant is distinguished from the other species by its dimorphic leaves. The plant shows obviously pseudopetiolated big basal leaves, which appear nearly opposite due to shortening of the nodes and are persistent at anthesis, and has alternate small leaves on the flowering stem.
DOI: 10.15468/dl.7pdkea
title: Occurrence Download

description: A dataset containing 134 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is one of (Anacropora puertogalerae, Anacropora matthaii, Anacropora reticulata, Anacropora spinosa)",
 "HasCoordinate is true"
 ]
}

 The dataset includes 134 records from 12 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0064653-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/8hdg32
title: A new Sobralia (Orchidaceae: Sobralieae) from Panama

description: This dataset contains the digitized treatments in Plazi based on the original journal article Serracín, Zuleika, Samudio, Zabdy, Bogarín, Diego (2022): A new Sobralia (Orchidaceae: Sobralieae) from Panama. Phytotaxa 559 (1): 81-87, DOI: 10.11646/phytotaxa.559.1.9, URL: http://dx.doi.org/10.11646/phytotaxa.559.1.9AbstractIn Panama, the Orchidaceae comprise 187 genera, of which one of the most conspicuous is Sobralia. The flowers of Sobralia are mostly ephemeral but colorful, often fragrant, and of variable sizes. Despite being a prominent group, its taxonomy is still underdeveloped in most neotropical countries. To continue with taxonomic studies in the Orchidaceae of Panama, we investigated a species of Sobralia, which differs from any recorded species of the genus. We documented the species with digital images and compared it with morphologically similar taxa. This paper describes and illustrates a new Sobralia from the Bosque Protector Palo Seco in the Fortuna area, Panama. Sobralia rinconiana differs from all other species recorded in Panama by the combination of a large plant size that reaches up to 120 cm high and the larger and broader, ellipticallanceolate leaves (30–35 × 14–16 cm). Sobralia rinconiana is most similar to S. carazoi but differs in the spreading flowers with reflexed petals and the infundibuliform, cream-yellow lip, the wider, longer sepals and petals, and the longer, suberect column. The accurate estimate of the number of Sobralia species in Panama is still uncertain. Its diversity may increase as new areas are explored or species complexes are resolved.
DOI: 10.15468/em3m7m
title: Neotypification of the Linnaean name Iris aphylla (Iridaceae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Boltenkov, Eugeny V. (2016): Neotypification of the Linnaean name Iris aphylla (Iridaceae). Phytotaxa 273 (2): 141-143, DOI: 10.11646/phytotaxa.273.1.7, URL: http://dx.doi.org/10.11646/phytotaxa.273.1.7