cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15468/dl.54rpqs
title: Occurrence Download

description: A dataset containing 949 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Wolffiella gladiata (Hegelm.) Hegelm."
 ]
}

 The dataset includes 949 records from 112 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0026501-241024112534372/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48512/xcv8502232
title: Supplemental Materials Tables for Cultural Landscape Studies Help Match Cultural Resource Identification and Assessment Efforts Article

description: Supplemental Material Tables for the Advances in Archaeological Practice article entitled Cultural Landscape Studies Help Match Cultural Resource Identification and Assessment Efforts to Undertaking Size and Complexity in the Section 106 Process
DOI: 10.15468/dl.2n9tay
title: Occurrence Download

description: A dataset containing 46730 species occurrences available in GBIF matching the query:
{
 "GenusKey" : [
 "is Taxodium Rich."
 ]
}

 The dataset includes 46730 records from 667 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0026489-241024112534372/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.7dvtym
title: Occurrence Download

description: A dataset containing 30 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is one of (China, Hong Kong, Macao, Chinese Taipei)",
 "TaxonKey is Cyperus pygmaeus Rottb."
 ]
}

 The dataset includes 30 records from 7 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0026503-241024112534372/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.6084/m9.figshare.24872034.v3
title: The tectonic responses in the overriding plate during the Tethyan convergence and the progressive extrusion process in Sundaland: insights from the Wuliangshan massif, SE Tibetan Plateau

description: We present the results of zircon U-Pb and Hf isotope analyses for the Wuliangshan metamorphic complex in the southeast Tibetan Plateau. According to this data, we reveal that the Wuliangshan metamorphic complex reflects the tectonic events of rapid subsidence and deposition that occurred within a short period from 260-250 Ma in a back-arc tectonic setting. Then, statistics of <sup>40</sup>Ar/<sup>39</sup>Ar age data from the Red River Fault, the Chongshan-Lancang River Fault, and the Gaoligong Fault are presented to discuss the tectonic extrusion process of the Sundaland.
DOI: 10.15468/dl.cuec5f
title: Occurrence Download

description: A dataset containing 525 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Actinodaphne mushaensis (Hayata) Hayata"
 ]
}

 The dataset includes 525 records from 20 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0026504-241024112534372/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.992eee
title: Occurrence Download

description: A dataset containing 1 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Natrix natrix corsa (Hecht, 1930)",
 "HasCoordinate is true",
 "Year is greater than or equal to 2013",
 "Year is less than or equal to 2018",
 "CoordinateUncertaintyInMeters is less than or equal to 1000"
 ]
}

 The dataset includes 1 records from 1 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0026505-241024112534372/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.znn534
title: Occurrence Download

description: A dataset containing 670 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Wolffiella lingulata (Hegelm.) Hegelm."
 ]
}

 The dataset includes 670 records from 99 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0026506-241024112534372/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.5d9j53
title: Occurrence Download

description: A dataset containing 71945 species occurrences available in GBIF matching the query:
{
 "GenusKey" : [
 "is Thuja L."
 ]
}

 The dataset includes 71945 records from 881 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0026492-241024112534372/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.57760/sciencedb.26728
title: Investigation on repetition-rate division dynamics in a high-power high-repetition-rate 2-μm Q-switched Ho:YLF laser
title: Investigation on repetition-rate division dynamics in a high-power high-repetition-rate 2-μm Q-switched Ho:YLF laser

description: We demonstrated a high-power, high-efficiency 2-μm Ho:YLF laser and investigated the repetition-rate division phenomenon in high-repetition-rate Q-switched mode of operation. The Ho:YLF laser produced 135 W of output power with an optical conversion efficiency of 68.3% in CW regime and over 55 W of average power in Q-switched regime, which, to the best of our knowledge, represent the highest power values achieved for both CW and Q-switched regimes of Ho:YLF lasers. Notably, a regular repetition-rate division phenomenon was observed when operating at high repetition rate of 10-30 kHz, i.e., the pulse repetition frequency shows an integer division of the set frequency, which is attributed to the insufficient energy storage during individual Q-switched cycles. To elucidate the underlying dynamics, we proposed a Q-switched laser model based on quasi-three-level rate equations, specifically tailored to the Ho:YLF gain medium. Theoretical analysis demonstrates that increasing the pump intensity is an effective approach to overcome the frequency division phenomenon. This study could provide practical design guidelines for achieving stable pulsed outputs in high-repetition-rate quasi-three-level Q-switched lasers.
description: We demonstrated a high-power, high-efficiency 2-μm Ho:YLF laser and investigated the repetition-rate division phenomenon in high-repetition-rate Q-switched mode of operation. The Ho:YLF laser produced 135 W of output power with an optical conversion efficiency of 68.3% in CW regime and over 55 W of average power in Q-switched regime, which, to the best of our knowledge, represent the highest power values achieved for both CW and Q-switched regimes of Ho:YLF lasers. Notably, a regular repetition-rate division phenomenon was observed when operating at high repetition rate of 10-30 kHz, i.e., the pulse repetition frequency shows an integer division of the set frequency, which is attributed to the insufficient energy storage during individual Q-switched cycles. To elucidate the underlying dynamics, we proposed a Q-switched laser model based on quasi-three-level rate equations, specifically tailored to the Ho:YLF gain medium. Theoretical analysis demonstrates that increasing the pump intensity is an effective approach to overcome the frequency division phenomenon. This study could provide practical design guidelines for achieving stable pulsed outputs in high-repetition-rate quasi-three-level Q-switched lasers.
DOI: 10.25574/csc2.obs.15634
title: Chandra X-ray Observatory ObsId 15634

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.18797
title: Chandra X-ray Observatory ObsId 18797

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.16822
title: Chandra X-ray Observatory ObsId 16822

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.04185
title: Chandra X-ray Observatory ObsId 04185

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.14410
title: Chandra X-ray Observatory ObsId 14410

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.21036
title: Chandra X-ray Observatory ObsId 21036

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.22693
title: Chandra X-ray Observatory ObsId 22693

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.06356
title: Chandra X-ray Observatory ObsId 06356

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.05781
title: Chandra X-ray Observatory ObsId 05781

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.09714
title: Chandra X-ray Observatory ObsId 09714

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.12887
title: Chandra X-ray Observatory ObsId 12887

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.05822
title: Chandra X-ray Observatory ObsId 05822

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.03003
title: Chandra X-ray Observatory ObsId 03003

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.22694
title: Chandra X-ray Observatory ObsId 22694

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.02210
title: Chandra X-ray Observatory ObsId 02210

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.19280
title: Chandra X-ray Observatory ObsId 19280

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.02164
title: Chandra X-ray Observatory ObsId 02164

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.15024
title: Chandra X-ray Observatory ObsId 15024

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.07922
title: Chandra X-ray Observatory ObsId 07922

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.09545
title: Chandra X-ray Observatory ObsId 09545

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.19497
title: Chandra X-ray Observatory ObsId 19497

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.21246
title: Chandra X-ray Observatory ObsId 21246

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.15065
title: Chandra X-ray Observatory ObsId 15065

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.05685
title: Chandra X-ray Observatory ObsId 05685

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.04774
title: Chandra X-ray Observatory ObsId 04774

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: 10.18434/mds2-3665
title: 1,2,3,4-Tetrahydrophenanthrene: Experimental and Derived Thermodynamic Properties
DOI: 10.25574/csc2.obs.07901
title: Chandra X-ray Observatory ObsId 07901

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.10427
title: Chandra X-ray Observatory ObsId 10427

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.12836
title: Chandra X-ray Observatory ObsId 12836

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.05823
title: Chandra X-ray Observatory ObsId 05823

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.22649
title: Chandra X-ray Observatory ObsId 22649

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.10745
title: Chandra X-ray Observatory ObsId 10745

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.24854
title: Chandra X-ray Observatory ObsId 24854

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.10921
title: Chandra X-ray Observatory ObsId 10921

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.18237
title: Chandra X-ray Observatory ObsId 18237

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.11334
title: Chandra X-ray Observatory ObsId 11334

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.12679
title: Chandra X-ray Observatory ObsId 12679

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.21069
title: Chandra X-ray Observatory ObsId 21069

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.19909
title: Chandra X-ray Observatory ObsId 19909

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.08188
title: Chandra X-ray Observatory ObsId 08188

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.10426
title: Chandra X-ray Observatory ObsId 10426

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.18275
title: Chandra X-ray Observatory ObsId 18275

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.07860
title: Chandra X-ray Observatory ObsId 07860

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.14406
title: Chandra X-ray Observatory ObsId 14406

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.04088
title: Chandra X-ray Observatory ObsId 04088

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.16126
title: Chandra X-ray Observatory ObsId 16126

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.14412
title: Chandra X-ray Observatory ObsId 14412

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.06098
title: Chandra X-ray Observatory ObsId 06098

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".