cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.obs.05424
title: Chandra X-ray Observatory ObsId 05424

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.15503
title: Chandra X-ray Observatory ObsId 15503

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.04156
title: Chandra X-ray Observatory ObsId 04156

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.11097
title: Chandra X-ray Observatory ObsId 11097

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.14669
title: Chandra X-ray Observatory ObsId 14669

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.02948
title: Chandra X-ray Observatory ObsId 02948

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.04983
title: Chandra X-ray Observatory ObsId 04983

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.01881
title: Chandra X-ray Observatory ObsId 01881

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.15968
title: Chandra X-ray Observatory ObsId 15968

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.22848
title: Chandra X-ray Observatory ObsId 22848

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.15156
title: Chandra X-ray Observatory ObsId 15156

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.06830
title: Chandra X-ray Observatory ObsId 06830

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.00855
title: Chandra X-ray Observatory ObsId 00855

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.07155
title: Chandra X-ray Observatory ObsId 07155

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.05784
title: Chandra X-ray Observatory ObsId 05784

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.04703
title: Chandra X-ray Observatory ObsId 04703

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.11096
title: Chandra X-ray Observatory ObsId 11096

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.20965
title: Chandra X-ray Observatory ObsId 20965

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.07327
title: Chandra X-ray Observatory ObsId 07327

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.13459
title: Chandra X-ray Observatory ObsId 13459

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.11982
title: Chandra X-ray Observatory ObsId 11982

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.04180
title: Chandra X-ray Observatory ObsId 04180

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.04702
title: Chandra X-ray Observatory ObsId 04702

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.04831
title: Chandra X-ray Observatory ObsId 04831

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.13679
title: Chandra X-ray Observatory ObsId 13679

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.04698
title: Chandra X-ray Observatory ObsId 04698

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.14668
title: Chandra X-ray Observatory ObsId 14668

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.02243
title: Chandra X-ray Observatory ObsId 02243

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.09883
title: Chandra X-ray Observatory ObsId 09883

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.02247
title: Chandra X-ray Observatory ObsId 02247

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: 10.6084/m9.figshare.27885213
title: Benthic macroinvertebrate dynamics and responses to environmental factors in spring habitats of Kashmir Himalaya

description: Understanding the dynamics of the macroinvertebrate community and the environmental influences is crucial for effective management and conservation of springs. This study examines diversity and spatio-temporal variation in macroinvertebrate assemblages across 12 spring habitats in the South Kashmir Himalayas. Macroinvertebrates were collected, sorted, identified, and enumerated from spring habitats on a seasonal basis from 2013 to 2015, and subjected to various statistical tests. Through statistical tests, significant distinctions are observed among springs and seasons. Permutational analysis of variance showed significant differences in macroinvertebrate assemblages across springs and seasons using both abundance and presence–absence data. Alpha diversity metrics depict variations in richness and Shannon’s H across springs. β-diversity evaluation reveals significant differences in macroinvertebrate assemblages across springs based on abundance and presence–absence data. So, the spring sites present homogeneity in group dispersion (composition varies similarly) while having significantly different compositions. Physicochemical factors like temperature, dissolved oxygen, sulphate, nitrate-nitrogen, and substrate heterogeneity strongly influence the assemblage. In addition, substrate heterogeneity, perennial flow, and spring size also played an important role in explaining the assemblage patterns. The present study provides important information on the impact of environmental factors on the ecological characteristics of macroinvertebrate assemblages vital for effective conservation and monitoring.
DOI: 10.6084/m9.figshare.27885213.v1
title: Benthic macroinvertebrate dynamics and responses to environmental factors in spring habitats of Kashmir Himalaya

description: Understanding the dynamics of the macroinvertebrate community and the environmental influences is crucial for effective management and conservation of springs. This study examines diversity and spatio-temporal variation in macroinvertebrate assemblages across 12 spring habitats in the South Kashmir Himalayas. Macroinvertebrates were collected, sorted, identified, and enumerated from spring habitats on a seasonal basis from 2013 to 2015, and subjected to various statistical tests. Through statistical tests, significant distinctions are observed among springs and seasons. Permutational analysis of variance showed significant differences in macroinvertebrate assemblages across springs and seasons using both abundance and presence–absence data. Alpha diversity metrics depict variations in richness and Shannon’s H across springs. β-diversity evaluation reveals significant differences in macroinvertebrate assemblages across springs based on abundance and presence–absence data. So, the spring sites present homogeneity in group dispersion (composition varies similarly) while having significantly different compositions. Physicochemical factors like temperature, dissolved oxygen, sulphate, nitrate-nitrogen, and substrate heterogeneity strongly influence the assemblage. In addition, substrate heterogeneity, perennial flow, and spring size also played an important role in explaining the assemblage patterns. The present study provides important information on the impact of environmental factors on the ecological characteristics of macroinvertebrate assemblages vital for effective conservation and monitoring.
DOI: 10.15468/dl.c2dqje
title: Occurrence Download

description: A dataset containing 6796 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((-80.70261 46.6688,-77.0632 43.975,-74.31496 44.89431,-70.91416 44.8943,-69.93998 46.46107,-68.62091 47.31686,-66.53918 47.87959,-65.03081 47.62585,-63.54617 48.14854,-61.62533 46.87851,-61.28078 48.86633,-58.20976 50.58523,-57.39987 51.26812,-54.43676 51.98723,-55.60657 54.09665,-59.74587 56.20424,-63.61522 60.6716,-66.76469 60.71564,-73.2457 62.9166,-80.56527 62.69912,-80.70261 46.6688))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "Month is November",
 "OccurrenceStatus is Present",
 "Year 2024-2024"
 ]
}

 The dataset includes 6796 records from 4 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010415-250127130748423/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.13458
title: Chandra X-ray Observatory ObsId 13458

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.16019
title: Chandra X-ray Observatory ObsId 16019

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.04704
title: Chandra X-ray Observatory ObsId 04704

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.12210
title: Chandra X-ray Observatory ObsId 12210

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.04707
title: Chandra X-ray Observatory ObsId 04707

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.16227
title: Chandra X-ray Observatory ObsId 16227

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.09427
title: Chandra X-ray Observatory ObsId 09427

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.04699
title: Chandra X-ray Observatory ObsId 04699

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.15578
title: Chandra X-ray Observatory ObsId 15578

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.03233
title: Chandra X-ray Observatory ObsId 03233

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.14671
title: Chandra X-ray Observatory ObsId 14671

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.sd7ukn
title: Occurrence Download

description: A dataset containing 9588 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Plumeria rubra L."
 ]
}

 The dataset includes 9588 records from 390 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010417-250127130748423/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.02179
title: Chandra X-ray Observatory ObsId 02179

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.12721
title: Chandra X-ray Observatory ObsId 12721

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.13773
title: Chandra X-ray Observatory ObsId 13773

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.05480
title: Chandra X-ray Observatory ObsId 05480

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.07205
title: Chandra X-ray Observatory ObsId 07205

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.18090
title: Chandra X-ray Observatory ObsId 18090

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.14895
title: Chandra X-ray Observatory ObsId 14895

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.00865
title: Chandra X-ray Observatory ObsId 00865

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.15501
title: Chandra X-ray Observatory ObsId 15501

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.nfqxuk
title: Occurrence Download

description: A dataset containing 1678 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Podocarpus elatus R.Br. ex Endl."
 ]
}

 The dataset includes 1678 records from 74 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010418-250127130748423/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.04710
title: Chandra X-ray Observatory ObsId 04710

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.00082
title: Chandra X-ray Observatory ObsId 00082

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.02055
title: Chandra X-ray Observatory ObsId 02055

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.02244
title: Chandra X-ray Observatory ObsId 02244

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".