cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15468/dl.wvt2ep
title: Occurrence Download

description: A dataset containing 112 species occurrences available in GBIF matching the query:
{
 "and" : [
 "BasisOfRecord is Specimen",
 "TaxonKey is Eschweilera punctata S.A.Mori"
 ]
}

 The dataset includes 112 records from 12 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010733-250127130748423/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.acisfj0856406p424240_001
title: Chandra X-ray Observatory Stack acisfJ0856406p424240_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.acisfj0945131m623014_001
title: Chandra X-ray Observatory Stack acisfJ0945131m623014_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.acisfj0944161p541125_001
title: Chandra X-ray Observatory Stack acisfJ0944161p541125_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.acisfj0955017m012939_001
title: Chandra X-ray Observatory Stack acisfJ0955017m012939_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.acisfj0859527p131059_001
title: Chandra X-ray Observatory Stack acisfJ0859527p131059_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.acisfj0858105p275206_001
title: Chandra X-ray Observatory Stack acisfJ0858105p275206_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.acisfj0955134p694113_001
title: Chandra X-ray Observatory Stack acisfJ0955134p694113_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.acisfj0904229p130928_001
title: Chandra X-ray Observatory Stack acisfJ0904229p130928_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.acisfj0946460p392704_001
title: Chandra X-ray Observatory Stack acisfJ0946460p392704_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.acisfj0946200p030332_001
title: Chandra X-ray Observatory Stack acisfJ0946200p030332_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.acisfj1010224p141303_001
title: Chandra X-ray Observatory Stack acisfJ1010224p141303_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.acisfj0857368m772002_001
title: Chandra X-ray Observatory Stack acisfJ0857368m772002_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.acisfj0901375m641639_001
title: Chandra X-ray Observatory Stack acisfJ0901375m641639_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.acisfj0944177p093036_001
title: Chandra X-ray Observatory Stack acisfJ0944177p093036_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.acisfj0906510p495201_001
title: Chandra X-ray Observatory Stack acisfJ0906510p495201_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.acisfj0955442p694142_002
title: Chandra X-ray Observatory Stack acisfJ0955442p694142_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.acisfj0900078m455042_002
title: Chandra X-ray Observatory Stack acisfJ0900078m455042_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.acisfj0955263p693735_001
title: Chandra X-ray Observatory Stack acisfJ0955263p693735_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.acisfj0955334p180840_001
title: Chandra X-ray Observatory Stack acisfJ0955334p180840_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.acisfj0955510p694032_001
title: Chandra X-ray Observatory Stack acisfJ0955510p694032_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.acisfj0948088p161405_001
title: Chandra X-ray Observatory Stack acisfJ0948088p161405_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.acisfj1012091p324414_001
title: Chandra X-ray Observatory Stack acisfJ1012091p324414_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.acisfj0946500p661131_001
title: Chandra X-ray Observatory Stack acisfJ0946500p661131_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.acisfj0947054p542951_001
title: Chandra X-ray Observatory Stack acisfJ0947054p542951_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.acisfj0903322p502842_001
title: Chandra X-ray Observatory Stack acisfJ0903322p502842_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.acisfj0955082p693910_001
title: Chandra X-ray Observatory Stack acisfJ0955082p693910_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.acisfj0904426m322237_002
title: Chandra X-ray Observatory Stack acisfJ0904426m322237_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.acisfj0949520p731410_001
title: Chandra X-ray Observatory Stack acisfJ0949520p731410_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.acisfj0903033p402540_001
title: Chandra X-ray Observatory Stack acisfJ0903033p402540_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.acisfj0953407m453923_001
title: Chandra X-ray Observatory Stack acisfJ0953407m453923_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.acisfj0948037p315556_001
title: Chandra X-ray Observatory Stack acisfJ0948037p315556_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.acisfj0949323p553437_001
title: Chandra X-ray Observatory Stack acisfJ0949323p553437_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.acisfj0902435m481156_001
title: Chandra X-ray Observatory Stack acisfJ0902435m481156_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.acisfj0956291p694145_001
title: Chandra X-ray Observatory Stack acisfJ0956291p694145_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.acisfj1015484p094659_001
title: Chandra X-ray Observatory Stack acisfJ1015484p094659_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.acisfj0904495m573535_001
title: Chandra X-ray Observatory Stack acisfJ0904495m573535_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.acisfj0952421p515108_001
title: Chandra X-ray Observatory Stack acisfJ0952421p515108_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.acisfj0956489m653749_001
title: Chandra X-ray Observatory Stack acisfJ0956489m653749_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.acisfj0906438m520548_001
title: Chandra X-ray Observatory Stack acisfJ0906438m520548_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.acisfj0957597p021843_001
title: Chandra X-ray Observatory Stack acisfJ0957597p021843_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.acisfj0955338p690321_001
title: Chandra X-ray Observatory Stack acisfJ0955338p690321_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.acisfj0907400m004140_001
title: Chandra X-ray Observatory Stack acisfJ0907400m004140_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.acisfj1043556m595939_001
title: Chandra X-ray Observatory Stack acisfJ1043556m595939_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.acisfj0906340p045143_001
title: Chandra X-ray Observatory Stack acisfJ0906340p045143_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.acisfj0959285p633433_001
title: Chandra X-ray Observatory Stack acisfJ0959285p633433_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.acisfj0951225p263456_001
title: Chandra X-ray Observatory Stack acisfJ0951225p263456_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.acisfj0956019p411028_001
title: Chandra X-ray Observatory Stack acisfJ0956019p411028_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.kjhdsj
title: Occurrence Download

description: A dataset containing 170114 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is one of (Prunus serotina Ehrh., Cerasus serotina var. cartilaginea Lehm., Prunus capollin var. prophyllosa Donn.Sm., Cerasus capollin Ser. ex DC., Cerasus longifolius Nutt. ex Torr. & A.Gray, Prunus hirsuta Elliott, Prunus cartilaginea Lehm., Cerasus serotina var. cartilaginea Lehm. ex G.Kirchn., Prunus serotina f. typica Schwer., Prunus virginiana DuRoi, Cerasus serotina var. asplenifolia G.Kirchn., Cerasus serotina var. montana Small, Prunus serotina var. neomontana Sudw., Cerasus serotina var. retusa Ser., Prunus serotina f. pyramidalis Zabel, Prunus serotina var. pendula Ed.Otto, Prunus serotina var. variegata L.H.Bailey, Prunus serotina Roth, Prunus novoleontis Standl., Padus hirsuta (Elliot) M.Roem., Prunus serotina subsp. hirsuta (Elliott) McVaugh, Prunus serotina subsp. hirsuta (Elliott) Mc Vaugh, Padus serotina var. cartilaginea (Lehm.) Belozor, Prunus serotina f. cartilaginea (Lehm.) Schwer., Prunus serotina subsp. cartilaginea (Lehm.) Asch. & Graebn., Prunus serotina var. cartilaginea (Lehm.) Dippel, Padus cartilaginea (Lehm.) M.Roem., Padus serotina f. cartilaginea (Lehm.) C.K.Schneid., Cerasus virginiana (L.) Michx., Prunus serotina subsp. asplenifolia (G.Kirchn.) Asch. & Graebn., Cerasus asplenifolia (G.Kirchn.) K.Koch, Prunus serotina var. asplenifolia (G.Kirchn.) Dippel, Padus serotina f. asplenifolia (G.Kirchn.) C.K.Schneid., Prunus serotina f. asplenifolia (G.Kirchn.) Schwer., Padus serotina var. asplenifolia (G.Kirchn.) Belozor, Prunus serotina var. smallii Britton, 1897, Prunus serotina var. montana (Small) Britton, Padus serotina f. neomontana (Sudw.) S.Ya.Sokolov, Padus serotina subsp. neomontana (Sudw.) Small, Padus retusa (Ser. ex DC.) M.Roem., Prunus serotina subsp. pyramidalis (Zabel) Asch. & Graebn., Padus serotina var. pyramidalis (Zabel) Belozor, Prunus serotina f. pendula (Ed.Otto) Schwer., Padus serotina var. pendula (Dippel) Belozor, Padus serotina f. pendula (Ed.Otto) C.K.Schneid., Prunus serotina subsp. pendula (Ed.Otto) Asch. & Graebn., Cerasus serotina (Ehrh.) Poit. & Turpin, Padus serotina (Ehrh.) J.Agardh., Padus serotina (Ehrh.) Borkh., Prunus virginiana var. serotina (Ehrh.) Merrem, Cerasus serotina (Ehrh.) Loisel.)",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "Year is greater than or equal to 2000"
 ]
}

 The dataset includes 170114 records from 570 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010706-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.13144/lil-1204
title: Fichier des prénoms - Edition 2017

description: Les fichiers des prénoms contiennent les prénoms attribués aux enfants nés en France (métropole et départements d'Outre-Mer) et les effectifs par sexe associés à chaque prénom entre 1900 et 2016 (et ce, dans les 2 fichiers -national et départemental- comme depuis 2014). Le répertoire n'est pas exhaustif notamment pour les personnes nées avant 1946. L'édition 2017 ne recense pas les prénoms des personnes vivantes une année donnée, mais les naissances enregistrées à l'état civil sur les bulletins de naissance ; sont exclues les personnes nées à l'étranger. Les prénoms doivent respecter 2 conditions pour figurer dans le fichier : ils doivent avoir été attribués au moins 20 fois, et pour une année donnée le prénom doit avoir été attribué au moins 3 fois. Les prénoms qui ne remplissent pas ces conditions sont regroupés dans un champ "prénoms rares". Les données sont accessibles au niveau national et départemental, les départements d'Outre-Mer étant regroupés (code 97).
DOI: 10.6084/m9.figshare.26838265
title: Preferential fluids ascent paths revealed by coupling chemical, electrical and magnetic methods: insights for risk mitigation in a long-dormant volcanic province (Monts Dore, France) [Dataset]

description: This study focuses on the dormant volcanic province of the Monts Dore in France, and in particular, around the Lake Pavin, in order to identify the preferential pathways by which volcanic fluids (water, gas, magma) can ascend. By combining data on soil CO<sub>2</sub> flux with geophysical information (magnetism, electrical resistivity tomography), fluid circulation routes were mapped. The results highlighted two potential sites of fluid emission likely to affect inhabited areas, since simulations of potential lava flow propagation were also carried out on the basis of the identification of these high permeability areas. As a result, potential risks maps were drawn up to show the feasibility of identifying exposed areas to natural hazards even in long-term quiescent volcanic provinces. This research provides new methodological elements in order to assess volcanic risk and develop an adapted urban planning in long-dormant volcanic areas as the Monts Dore.