cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.stk.acisfj0313451p044637_001
title: Chandra X-ray Observatory Stack acisfJ0313451p044637_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.acisfj0338396p100026_001
title: Chandra X-ray Observatory Stack acisfJ0338396p100026_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.acisfj0120021p142131_001
title: Chandra X-ray Observatory Stack acisfJ0120021p142131_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.acisfj0312281p413634_001
title: Chandra X-ray Observatory Stack acisfJ0312281p413634_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.acisfj0237035m613742_001
title: Chandra X-ray Observatory Stack acisfJ0237035m613742_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.acisfj0323070m212246_001
title: Chandra X-ray Observatory Stack acisfJ0323070m212246_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.acisfj0118551m010149_001
title: Chandra X-ray Observatory Stack acisfJ0118551m010149_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.acisfj0111104m724351_001
title: Chandra X-ray Observatory Stack acisfJ0111104m724351_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.acisfj0214143p602024_001
title: Chandra X-ray Observatory Stack acisfJ0214143p602024_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.acisfj0237254m263241_001
title: Chandra X-ray Observatory Stack acisfJ0237254m263241_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.acisfj0113388p005222_001
title: Chandra X-ray Observatory Stack acisfJ0113388p005222_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.acisfj0147218m091623_001
title: Chandra X-ray Observatory Stack acisfJ0147218m091623_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.acisfj0333058m282919_001
title: Chandra X-ray Observatory Stack acisfJ0333058m282919_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.acisfj0228559p002810_001
title: Chandra X-ray Observatory Stack acisfJ0228559p002810_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.acisfj0145161m094442_001
title: Chandra X-ray Observatory Stack acisfJ0145161m094442_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.acisfj0304551m273032_001
title: Chandra X-ray Observatory Stack acisfJ0304551m273032_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.acisfj0119088m082913_001
title: Chandra X-ray Observatory Stack acisfJ0119088m082913_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.acisfj0215314m521351_001
title: Chandra X-ray Observatory Stack acisfJ0215314m521351_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.acisfj0315000p420159_001
title: Chandra X-ray Observatory Stack acisfJ0315000p420159_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.acisfj0238338p023318_001
title: Chandra X-ray Observatory Stack acisfJ0238338p023318_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.acisfj0215386m125928_001
title: Chandra X-ray Observatory Stack acisfJ0215386m125928_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.acisfj0319499m260342_001
title: Chandra X-ray Observatory Stack acisfJ0319499m260342_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.acisfj0243263p372106_002
title: Chandra X-ray Observatory Stack acisfJ0243263p372106_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.acisfj0259296p134347_001
title: Chandra X-ray Observatory Stack acisfJ0259296p134347_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.acisfj0306566p010819_001
title: Chandra X-ray Observatory Stack acisfJ0306566p010819_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.nr2h87
title: Occurrence Download

description: A dataset containing 51322 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Pusa hispida (Schreber, 1775)"
 ]
}

 The dataset includes 51322 records from 116 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010701-250127130748423/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.acisfj0317127m075906_001
title: Chandra X-ray Observatory Stack acisfJ0317127m075906_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.acisfj0216487m050940_001
title: Chandra X-ray Observatory Stack acisfJ0216487m050940_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.acisfj0149021m145619_001
title: Chandra X-ray Observatory Stack acisfJ0149021m145619_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.acisfj0303379m153832_001
title: Chandra X-ray Observatory Stack acisfJ0303379m153832_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.acisfj0328329m214314_001
title: Chandra X-ray Observatory Stack acisfJ0328329m214314_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.acisfj0303463p645418_001
title: Chandra X-ray Observatory Stack acisfJ0303463p645418_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.acisfj0243514m593030_001
title: Chandra X-ray Observatory Stack acisfJ0243514m593030_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.acisfj0123147m020836_001
title: Chandra X-ray Observatory Stack acisfJ0123147m020836_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.acisfj0305254p034812_001
title: Chandra X-ray Observatory Stack acisfJ0305254p034812_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.acisfj0240305p191536_001
title: Chandra X-ray Observatory Stack acisfJ0240305p191536_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.acisfj0319411m192423_001
title: Chandra X-ray Observatory Stack acisfJ0319411m192423_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.acisfj0152482p005753_001
title: Chandra X-ray Observatory Stack acisfJ0152482p005753_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.t96qgx
title: Occurrence Download

description: A dataset containing 546 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Cryptostegia madagascariensis Bojer"
 ]
}

 The dataset includes 546 records from 56 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010705-250127130748423/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.acisfj0333380m391836_001
title: Chandra X-ray Observatory Stack acisfJ0333380m391836_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.acisfj0150488p004200_001
title: Chandra X-ray Observatory Stack acisfJ0150488p004200_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.acisfj0242407m000123_002
title: Chandra X-ray Observatory Stack acisfJ0242407m000123_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.acisfj0152486m032636_001
title: Chandra X-ray Observatory Stack acisfJ0152486m032636_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.acisfj0223024m043614_001
title: Chandra X-ray Observatory Stack acisfJ0223024m043614_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.acisfj0309466p271750_001
title: Chandra X-ray Observatory Stack acisfJ0309466p271750_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.acisfj0331114p435406_001
title: Chandra X-ray Observatory Stack acisfJ0331114p435406_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.acisfj0248159p602140_001
title: Chandra X-ray Observatory Stack acisfJ0248159p602140_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.acisfj0151337m595708_001
title: Chandra X-ray Observatory Stack acisfJ0151337m595708_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: 10.13144/lil-1162
title: Recensement de la population 2014 : fichier détail mobilités professionnelles

description: Le fichier détail "Mobilités professionnelles" du recensement de la population de 2014 porte sur les déplacements quotidiens pour aller travailler (déplacements domicile-travail), les principales caractéristiques sociodémographiques, ainsi que celles du ménage auquel l'individu appartient. Les variables y sont disponibles avec des modalités détaillées, y compris les variables à diffusion restreinte (nationalité, pays de naissance, ancienneté d'arrivée en France). A partir de ce fichier, il est donc possible de faire des analyses exploratoires de données, de modéliser des comportements, ou simplement de tabuler sur une sous-population particulière définie selon certains critères : appartenance à une zone géographique et/ou unité statistique présentant certaines caractéristiques.
DOI: 10.13144/lil-1164
title: Recensement de la population 2014 : fichier détail migrations résidentielles des individus entre communes

description: Le fichier détail du recensement de la population de 2014 "Migrations résidentielles des individus entre communes" est de nouveau diffusé après quatre ans de suspension (entre 2009 et 2012) suite à un changement de questionnaire. Ce fichier détail fait désormais référence à la résidence antérieure des personnes recensées 1 an avant leur interrogation (contre 5 ans pour les recensements de la population 2006, 2007 et 2008). Il porte sur la résidence actuelle et antérieure des individus, leurs principales caractéristiques sociodémographiques, ainsi que celles du ménage auquel ils appartiennent. Les variables y sont disponibles avec des modalités détaillées, y compris les variables à diffusion restreinte (nationalité, pays de naissance, ancienneté d'arrivée en France). A partir de ce fichier, il est donc possible de faire des analyses exploratoires de données, de modéliser des comportements, ou simplement de tabuler sur une sous-population particulière définie selon certains critères : appartenance à une zone géographique et/ou unité statistique présentant certaines caractéristiques.
DOI: 10.5281/zenodo.10599896
title: 'Dietary change is not a prerequisite for effective biodiversity conservation but reduces socioeconomic obstacles' - model outputs

description: Archive of output reports produced for the MAgPIE v4.6.11 paper 'Dietary change is not a prerequisite for effective biodiversity conservation but reduces socioeconomic obstacles'.

The data contain the MAgPIE model and post-processing outputs of all assessed scenarios. The data is displayed in the main text in Figs. 1-5, in the Extended Data Figs 2-6 and in Supplementary Figs. 3, 4, & 6-23.

The model code of the MAgPIE and SEALS models can be accessed via:

MAgPIE model code: https://doi.org/10.5281/zenodo.8318615 and https://github.com/magpiemodel/magpie

MAgPIE model documentation: https://rse.pik-potsdam.de/doc/magpie/4.6.11/
DOI: 10.5281/zenodo.14243700
title: 'Dietary change is not a prerequisite for effective biodiversity conservation but reduces socioeconomic obstacles' - model outputs

description: Archive of output reports produced for the MAgPIE v4.8.2 paper 'Dietary change is not a prerequisite for effective biodiversity conservation but reduces socioeconomic obstacles'.

The data contain the MAgPIE model and post-processing outputs of all assessed scenarios. The data is displayed in the main text in Figs. 1-5, in Supplementary Figs. 4-34.

The model code of the MAgPIE and SEALS models can be accessed via:

MAgPIE model code:

https://doi.org/10.5281/zenodo.13833444 and https://github.com/magpiemodel/magpie

MAgPIE model documentation:

https://rse.pik-potsdam.de/doc/magpie/4.8.2/

SEALS model code:

https://github.com/jandrewjohnson/seals_dev/releases/tag/v1.0.0

SEALS mode documentation:

https://justinandrewjohnson.com/earth_economy_devstack/seals_overview.html