cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.obs.21182
title: Chandra X-ray Observatory ObsId 21182

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.obs.15074
title: Chandra X-ray Observatory ObsId 15074

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.obs.18630
title: Chandra X-ray Observatory ObsId 18630

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.obs.11447
title: Chandra X-ray Observatory ObsId 11447

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.obs.11688
title: Chandra X-ray Observatory ObsId 11688

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.obs.17583
title: Chandra X-ray Observatory ObsId 17583

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.obs.07870
title: Chandra X-ray Observatory ObsId 07870

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.obs.20924
title: Chandra X-ray Observatory ObsId 20924

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.obs.18159
title: Chandra X-ray Observatory ObsId 18159

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.obs.22212
title: Chandra X-ray Observatory ObsId 22212

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.obs.17255
title: Chandra X-ray Observatory ObsId 17255

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.obs.03059
title: Chandra X-ray Observatory ObsId 03059

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.obs.17256
title: Chandra X-ray Observatory ObsId 17256

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.obs.17585
title: Chandra X-ray Observatory ObsId 17585

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.obs.01636
title: Chandra X-ray Observatory ObsId 01636

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.obs.02402
title: Chandra X-ray Observatory ObsId 02402

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.obs.15146
title: Chandra X-ray Observatory ObsId 15146

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.obs.17093
title: Chandra X-ray Observatory ObsId 17093

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.obs.02060
title: Chandra X-ray Observatory ObsId 02060

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.obs.04493
title: Chandra X-ray Observatory ObsId 04493

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.obs.11689
title: Chandra X-ray Observatory ObsId 11689

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.du7nba
title: Occurrence Download

description: A dataset listing the 146 species recorded in GBIF matching the query:
{
 "and" : [
 "GbifRegion is Latin America and the Caribbean",
 "Locality is one of (Girardota, Girardota, Antioquia, Girardota, Girardota Antioquia, Girardota-La Sapera, Girardota--Vereda Portachuelos, Girardota, Antioquia, CO-45a2-45a92 Diagonal 56 - , Girardota, Antioquia, CO (6.389, -75.439), Girardota, Antioquia, CO (6.353, -75.455), Girardota, Antioquia, CO (6.352, -75.455), Girardota Rio Medellin, Girardota - Vía Juan Cojo, Girardota - Vía Juan Cojo - El Totumo, Girardota nr. Medellin; Colombia, Girardota, Antioquia, CO-14173-14355 Calle 12a - 6)"
 ]
}

 The dataset's 146 records were derived from 8 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010525-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/csc2.obs.04925
title: Chandra X-ray Observatory ObsId 04925

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.obs.17193
title: Chandra X-ray Observatory ObsId 17193

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.obs.07638
title: Chandra X-ray Observatory ObsId 07638

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.obs.18891
title: Chandra X-ray Observatory ObsId 18891

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.obs.20441
title: Chandra X-ray Observatory ObsId 20441

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.obs.21026
title: Chandra X-ray Observatory ObsId 21026

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.obs.17497
title: Chandra X-ray Observatory ObsId 17497

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.obs.02135
title: Chandra X-ray Observatory ObsId 02135

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.obs.12286
title: Chandra X-ray Observatory ObsId 12286

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.obs.18097
title: Chandra X-ray Observatory ObsId 18097

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.obs.10136
title: Chandra X-ray Observatory ObsId 10136

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.obs.17036
title: Chandra X-ray Observatory ObsId 17036

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.obs.08500
title: Chandra X-ray Observatory ObsId 08500

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.obs.00927
title: Chandra X-ray Observatory ObsId 00927

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.obs.14969
title: Chandra X-ray Observatory ObsId 14969

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.obs.17257
title: Chandra X-ray Observatory ObsId 17257

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.obs.10361
title: Chandra X-ray Observatory ObsId 10361

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.obs.13378
title: Chandra X-ray Observatory ObsId 13378

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.obs.10863
title: Chandra X-ray Observatory ObsId 10863

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.obs.10996
title: Chandra X-ray Observatory ObsId 10996

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.obs.21137
title: Chandra X-ray Observatory ObsId 21137

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.obs.18199
title: Chandra X-ray Observatory ObsId 18199

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.obs.10152
title: Chandra X-ray Observatory ObsId 10152

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.obs.23138
title: Chandra X-ray Observatory ObsId 23138

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.obs.15337
title: Chandra X-ray Observatory ObsId 15337

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.obs.14401
title: Chandra X-ray Observatory ObsId 14401

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.5d897w
title: Occurrence Download

description: A dataset containing 91159 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Lepus timidus Linnaeus, 1758"
 ]
}

 The dataset includes 91159 records from 296 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010541-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.hqy4mf
title: Occurrence Download

description: A dataset containing 613 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is Ethiopia",
 "OccurrenceStatus is Present",
 "TaxonKey is Lychnis abyssinica (Hochst.) Lidén"
 ]
}

 The dataset includes 613 records from 2 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0003576-241107131044228/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.4q9btd
title: Occurrence Download

description: A dataset containing 96 species occurrences available in GBIF matching the query:
{
 "and" : [
 "BasisOfRecord is Specimen",
 "Continent is North America",
 "Country is United States of America",
 "OccurrenceStatus is Present",
 "TaxonKey is Vicia faba L."
 ]
}

 The dataset includes 96 records from 35 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0003580-241107131044228/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.sykvt3
title: Occurrence Download

description: A dataset containing 0 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is one of (Aves)",
 "HasCoordinate is one of (true)",
 "Geometry POLYGON((-59.5159778937861 -18.0807442601035,-59.1147859472389 -18.0807442601035,-59.1147859472389 -17.6460510295733,-59.5159778937861 -17.6460510295733,-59.5159778937861 -18.0807442601035))"
 ]
}

 The dataset includes 0 records from 0 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0003581-241107131044228/datasets/export for details.
DOI: 10.5281/zenodo.13952338
title: Data of the article "Predicting the 2023/24 El Niño from a multi-scale and global perspective" that published in Communications Earth & Environment

description: MATLAB data of the article "Predicting the 2023/24 El Niño from a multi-scale and global perspective" that published in Communications Earth & Environment.

The article is available on the Communications Earth & Environment at https://www.nature.com/articles/s43247-024-01867-w.

These data include ocean temperature, current, atmosphere wind, pressure, precipitation, heat flux, and more, that from reanalysis data and coupled model outputs. Additionaly, there are four figures of the article.

The related MATLAB codes can be accessed from  https://github.com/HRKsince1993/COMMSENV-24-1347.git

If these data are helpful to you, please cite our article or acknowledge us in your publication, e. g.

Hu, R. et al. Predicting the 2023/24 El Niño from a multi-scale and global perspective. Commun. Earth Environ. 5, 675 (2024). 

If you have any questions, please contact Tao Lian (liantao@sio.org.cn) and/or Dake Chen (dchen@sio.org.cn) and/or me.

  

Best wishes

Ruikun Hu

Ph.D of physical oceanography

State Key Laboratory of Satellite Ocean Environment Dynamics,

Second Institute of Oceanography, Ministry of Natural Resources, Hangzhou, China

ruikunhu@sio.org.cn

October 18, 2024

Updated on November 8, 2024
DOI: 10.5281/zenodo.13952339
title: Data of the article "Predicting the 2023/24 El Niño from a multi-scale and global perspective" that published in Communications Earth & Environment

description: MATLAB data of the article "Predicting the 2023/24 El Niño from a multi-scale and global perspective" that published in Communications Earth & Environment.

The article is available on the Communications Earth & Environment at https://www.nature.com/articles/s43247-024-01867-w.

These data include ocean temperature, current, atmosphere wind, pressure, precipitation, heat flux, and more, that from reanalysis data and coupled model outputs. Additionaly, there are four figures of the article.

The related MATLAB codes can be accessed from  https://github.com/HRKsince1993/COMMSENV-24-1347.git

If these data are helpful to you, please cite our article or acknowledge us in your publication, e. g.

Hu, R. et al. Predicting the 2023/24 El Niño from a multi-scale and global perspective. Commun. Earth Environ. 5, 675 (2024). 

If you have any questions, please contact Tao Lian (liantao@sio.org.cn) and/or Dake Chen (dchen@sio.org.cn) and/or me.

  

Best wishes

Ruikun Hu

Ph.D of physical oceanography

State Key Laboratory of Satellite Ocean Environment Dynamics,

Second Institute of Oceanography, Ministry of Natural Resources, Hangzhou, China

ruikunhu@sio.org.cn

October 18, 2024

Updated on November 8, 2024
DOI: 10.5281/zenodo.14057295
title: How to discipline financial markets: reputation is not enough

description: This package contains the data, programs and instructions to replicate manuscript "How to discipline financial markets: reputation is not enough" by Maria Bigoni, Gabriele Camera and Marco Casari forthcoming at JEEA.
DOI: 10.5281/zenodo.14057296
title: How to discipline financial markets: reputation is not enough

description: This package contains the data, programs and instructions to replicate manuscript "How to discipline financial markets: reputation is not enough" by Maria Bigoni, Gabriele Camera and Marco Casari forthcoming at JEEA.
DOI: 10.5281/zenodo.14055611
title: Verification of library complexity in the HEK-Cas9 sublibraries - sequence data of the generated sublibraries A and B

description: Sequence data of the generated HEK-Cas9 sublibraries A and B, linked to the manuscript 10.1128/mbio.01925-24: The Bordetella effector protein BteA induces host cell death by disruption of calcium homeostasis by Martin Zmuda, Eliska Sedlackova, Barbora Pravdova, Monika Cizkova, Marketa Dalecka, Ondrej Cerny, Tania Romero Allsop, Tomas Grousl, Ivana Malcova, and Jana Kamanova
DOI: 10.5281/zenodo.14055612
title: Verification of library complexity in the HEK-Cas9 sublibraries - sequence data of the generated sublibraries A and B

description: Sequence data of the generated HEK-Cas9 sublibraries A and B, linked to the manuscript 10.1128/mbio.01925-24: The Bordetella effector protein BteA induces host cell death by disruption of calcium homeostasis by Martin Zmuda, Eliska Sedlackova, Barbora Pravdova, Monika Cizkova, Marketa Dalecka, Ondrej Cerny, Tania Romero Allsop, Tomas Grousl, Ivana Malcova, and Jana Kamanova
DOI: 10.5281/zenodo.14057297
title: DT-LEMBAS cell line specific models

description: This contains 33 ensembles of 50 DT-LEMBAS models each. The models were trained on 33 cell line transcriptomic data from the L1000 dataset.