cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/20005
title: Chandra X-ray Observatory ObsId 20005

description: The NLSy1 IRAS17020+4544: dissecting the first low ionization sub-relativistic black hole wind with LETG and HST/COS
DOI: 10.25574/20006
title: Chandra X-ray Observatory ObsId 20006

description: The NLSy1 IRAS17020+4544: dissecting the first low ionization sub-relativistic black hole wind with LETG and HST/COS
DOI: 10.25574/20008
title: Chandra X-ray Observatory ObsId 20008

description: A Hig-Resolution Spectrum of the Black Hole GRS 1716-249
DOI: 10.25574/20019
title: Chandra X-ray Observatory ObsId 20019

description: Can Planets Affect Coronal Abundances?
DOI: 10.25574/20020
title: Chandra X-ray Observatory ObsId 20020

description: Can Planets Affect Coronal Abundances?
DOI: 10.25574/20073
title: Chandra X-ray Observatory ObsId 20073

description: A deep LETGS observation of Proxima Centauri
DOI: 10.25574/20080
title: Chandra X-ray Observatory ObsId 20080

description: A deep LETGS observation of Proxima Centauri
DOI: 10.25574/20084
title: Chandra X-ray Observatory ObsId 20084

description: A deep LETGS observation of Proxima Centauri
DOI: 10.25574/20098
title: Chandra X-ray Observatory ObsId 20098

description: The longest AMXP outburst: looking for pulsation in MAXI J0911-655 after 450 days
DOI: 10.25574/20130
title: Chandra X-ray Observatory ObsId 20130

description: Coronal Properties at the Edge of Coronal Viability
DOI: 10.25574/20165
title: Chandra X-ray Observatory ObsId 20165

description: THE EXTREME ULTRAVIOLET FLUX OF VERY LOW MASS STARS
DOI: 10.25574/20166
title: Chandra X-ray Observatory ObsId 20166

description: THE EXTREME ULTRAVIOLET FLUX OF VERY LOW MASS STARS
DOI: 10.25574/20167
title: Chandra X-ray Observatory ObsId 20167

description: THE EXTREME ULTRAVIOLET FLUX OF VERY LOW MASS STARS
DOI: 10.25574/20168
title: Chandra X-ray Observatory ObsId 20168

description: THE EXTREME ULTRAVIOLET FLUX OF VERY LOW MASS STARS
DOI: 10.25574/20169
title: Chandra X-ray Observatory ObsId 20169

description: Exploring Disks and Winds in Stellar-Mass Black Holes
DOI: 10.25574/20203
title: Chandra X-ray Observatory ObsId 20203

description: An Integrated Approach to Winds, Jets, and State Transitions
DOI: 10.25574/20204
title: Chandra X-ray Observatory ObsId 20204

description: An Integrated Approach to Winds, Jets, and State Transitions
DOI: 10.25574/20205
title: Chandra X-ray Observatory ObsId 20205

description: An Integrated Approach to Winds, Jets, and State Transitions
DOI: 10.25574/20206
title: Chandra X-ray Observatory ObsId 20206

description: An Integrated Approach to Winds, Jets, and State Transitions
DOI: 10.5281/zenodo.6908624
title: Morphing of Stiffness-Heterogeneous Liquid Crystal Elastomers Via Mechanical Training and Locally Controlled Photopolymerization

description: This dataset contains experimental and simulation data that support the findings of the study. Experimental data: stress-strain tests of highly crosslinked and lightly crosslinked liquid crystal elastomers. Simulation data: Codes (user element subroutine, .inp files) used for the finite element modeling of liquid crystal elastomer structures using the commercial software ABAQUS/Implicit.
DOI: 10.5281/zenodo.6908623
title: Morphing of Stiffness-Heterogeneous Liquid Crystal Elastomers Via Mechanical Training and Locally Controlled Photopolymerization

description: This dataset contains experimental and simulation data that support the findings of the study. Experimental data: stress-strain tests of highly crosslinked and lightly crosslinked liquid crystal elastomers. Simulation data: Codes (user element subroutine, .inp files) used for the finite element modeling of liquid crystal elastomer structures using the commercial software ABAQUS/Implicit.
DOI: 10.6084/m9.figshare.20685301.v1
title: ASV tables generated during sequence processing

description: These are ASV tables generated during processing of raw .fastq files. The first steps, error correction, chimaera removal, and taxonomic assignment, are carried out wtih DADA2, and result in the file ps_object_after_dada2.rds. Next steps include removing non-target sequences and samples with abnormally low numbers of sequences, and applying a prevalence filter, resulting in the final ASV table, phyloseq_after_pruning_filtering.rds. Both these files are phyloseq objects saved as R data files (.rds). They can be loaded into R using the readRDS function. <br> To run the R scripts from the github repository associated with the Legionella microbiome paper, these .rds files should be saved in the folder /data/process/.
DOI: 10.6084/m9.figshare.20685301
title: ASV tables generated during sequence processing

description: These are ASV tables generated during processing of raw .fastq files. The first steps, error correction, chimaera removal, and taxonomic assignment, are carried out wtih DADA2, and result in the file ps_object_after_dada2.rds. Next steps include removing non-target sequences and samples with abnormally low numbers of sequences, and applying a prevalence filter, resulting in the final ASV table, phyloseq_after_pruning_filtering.rds. Both these files are phyloseq objects saved as R data files (.rds). They can be loaded into R using the readRDS function. <br> To run the R scripts from the github repository associated with the Legionella microbiome paper, these .rds files should be saved in the folder /data/process/.
DOI: 10.25574/20259
title: Chandra X-ray Observatory ObsId 20259

description: Precise Localization of Transient Low-Mass X-ray Binaries
DOI: 10.6084/m9.figshare.20685370
title: Breakaway and ALDEx2 outputs

description: These are the outputs from running breakaway and ALDEx2 on the Legionella microbiome ASV table. <br> To run the manuscript.Rmd file from the github repo without having to compute these (which takes time), these files should be saved in the /data/process/ folder.
DOI: 10.6084/m9.figshare.20685370.v1
title: Breakaway and ALDEx2 outputs

description: These are the outputs from running breakaway and ALDEx2 on the Legionella microbiome ASV table. <br> To run the manuscript.Rmd file from the github repo without having to compute these (which takes time), these files should be saved in the /data/process/ folder.
DOI: 10.5281/zenodo.7026971
title: Dataset from Nature Catalysis paper: Unriddling the role of alkali metal cations and Pt-surface hydroxide in alkaline hydrogen evolution reaction

description: Dataset of the article "Unriddling the role of alkali metal cations and Pt-surface hydroxide in alkaline hydrogen evolution reaction" accepted in Nature Catalysis. The optimized geometries (in VASP format) and full 100-ps AIMD trajectories (in xyz format) of Pt(111)/water interface with alkali metal cations (Li+, Na+, K+) and with or without surface *OH.
DOI: 10.5281/zenodo.7026970
title: Dataset from Nature Catalysis paper: Unriddling the role of alkali metal cations and Pt-surface hydroxide in alkaline hydrogen evolution reaction

description: Dataset of the article "Unriddling the role of alkali metal cations and Pt-surface hydroxide in alkaline hydrogen evolution reaction" accepted in Nature Catalysis. The optimized geometries (in VASP format) and full 100-ps AIMD trajectories (in xyz format) of Pt(111)/water interface with alkali metal cations (Li+, Na+, K+) and with or without surface *OH.
DOI: 10.25919/ertt-8t73
title: Parkes observations for project P595 semester 2022APRS_11

description: We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the space missions, other observations supplement the P456 Pulsar Timing Array project and the remainder were chosen in order to make a detailed analysis of pulsar timing irregularities and intermittency.
DOI: 10.25919/tqpr-0r75
title: Parkes observations for project P456 semester 2022APRS_10

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. We are now in an exciting regime where a signal detected in our (and other data sets) has the form expected for a gravitational wave background. We are therefore now attempting to confirm, or deny, this exciting result. With this proposal we aim to maintain our pre-eminent position in the field. Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.6084/m9.figshare.20683870
title: larus_argentatus_decontaminated_FSCR.fasta.gz

description: ........
DOI: 10.6084/m9.figshare.20666529.v1
title: Supplemental Table S2

description: GWAS calls for each gene in the C. trachomatis chromosome. Locus tags are indicated for each gene in both the C. trachomatis D/UW3 and LGV/434 genome notation system. Coordinates for each gene are based on the sequence that can be found through NCBI accession # SAMN28177743. Genes that had no GWAS-predicted snps are not included in the table.
DOI: 10.6084/m9.figshare.20666529
title: Supplemental Table S2

description: GWAS calls for each gene in the C. trachomatis chromosome. Locus tags are indicated for each gene in both the C. trachomatis D/UW3 and LGV/434 genome notation system. Coordinates for each gene are based on the sequence that can be found through NCBI accession # SAMN28177743. Genes that had no GWAS-predicted snps are not included in the table.
DOI: 10.6084/m9.figshare.20666529.v3
title: Supplemental Table S2

description: GWAS calls for each gene in the C. trachomatis chromosome. Locus tags are indicated for each gene in both the C. trachomatis D/UW3 and LGV/434 genome notation system. Coordinates for each gene are based on the sequence that can be found through NCBI accession # SAMN28177743. Genes that had no GWAS-predicted snps are not included in the table.
DOI: 10.6084/m9.figshare.20666529.v2
title: Supplemental Table S2

description: GWAS calls for each gene in the C. trachomatis chromosome. Locus tags are indicated for each gene in both the C. trachomatis D/UW3 and LGV/434 genome notation system. Coordinates for each gene are based on the sequence that can be found through NCBI accession # SAMN28177743. Genes that had no GWAS-predicted snps are not included in the table.
DOI: 10.6084/m9.figshare.20666409
title: Supplemental Table S1

description: List of strains used for genomic analysis of MSM rectal tissue tropism.
DOI: 10.6084/m9.figshare.20666409.v2
title: Supplemental Table S1

description: List of strains used for genomic analysis of MSM rectal tissue tropism.
DOI: 10.6084/m9.figshare.20666409.v1
title: Supplemental Table S1

description: List of strains used for genomic analysis of MSM rectal tissue tropism.
DOI: 10.6084/m9.figshare.17645570.v4
title: Species data used in "Evaluating the robustness of Bergmann’s and Rapoport’s rules to different range sources and pattern approaches in New World Pit Vipers"

description: Species ranges estimated by experts, from ENMs and the phylogenies used in our analyses
DOI: 10.6084/m9.figshare.20685865
title: Custer County Nebraska 1880 Federal Census

description: Data consist of a digital transcription of the 1880 Custer County, Nebraska federal census. Data were transcribed from a microfilm of the census manuscript pages by an unknown volunteer at the Custer County (Nebraska) Historical Society and imported into a spreadsheet by the author. The author cross-checked and corrected these data using the manuscript pages accessible via FamilySearch.org. <br> <br> Source:<br> "United States Census, 1880." Database with images. <em>FamilySearch</em>. https://FamilySearch.org : 18 July 2022. Citing NARA microfilm publication T9. Washington, D.C.: National Archives and Records Administration, n.d.
DOI: 10.6084/m9.figshare.20685865.v1
title: Custer County Nebraska 1880 Federal Census

description: Data consist of a digital transcription of the 1880 Custer County, Nebraska federal census. Data were transcribed from a microfilm of the census manuscript pages by an unknown volunteer at the Custer County (Nebraska) Historical Society and imported into a spreadsheet by the author. The author cross-checked and corrected these data using the manuscript pages accessible via FamilySearch.org. <br> <br> Source:<br> "United States Census, 1880." Database with images. <em>FamilySearch</em>. https://FamilySearch.org : 18 July 2022. Citing NARA microfilm publication T9. Washington, D.C.: National Archives and Records Administration, n.d.
DOI: 10.6084/m9.figshare.20685361
title: Custer_County_1880_Enumerators_Eqi_Credible.csv

description: Data consist of duplicated entries in the 1880 Custer County, Nebraska federal census coming from equi-credible but different enumerators. Data were derived from source accessible via FamilySearch.org. Author manually scanned 1880 Custer County Census data to find duplicated entries. Additional information comes from inquiries to Family Search and Find A Grave to locate information on individual vital statistics. <br> Source: "United States Census, 1880." Database with images. <em>FamilySearch</em>. https://FamilySearch.org : 18 July 2022. Citing NARA microfilm publication T9. Washington, D.C.: National Archives and Records Administration, n.d.
DOI: 10.6084/m9.figshare.20685361.v1
title: Custer_County_1880_Enumerators_Eqi_Credible.csv

description: Data consist of duplicated entries in the 1880 Custer County, Nebraska federal census coming from equi-credible but different enumerators. Data were derived from source accessible via FamilySearch.org. Author manually scanned 1880 Custer County Census data to find duplicated entries. Additional information comes from inquiries to Family Search and Find A Grave to locate information on individual vital statistics. <br> Source: "United States Census, 1880." Database with images. <em>FamilySearch</em>. https://FamilySearch.org : 18 July 2022. Citing NARA microfilm publication T9. Washington, D.C.: National Archives and Records Administration, n.d.
DOI: 10.17632/cg38djj8y5.1
title: Sensors-on-Paper: Fabrication of Graphite Thermal Sensor Arrays on Cellulose Paper for Large Area Temperature Mapping 

description: This paper reports on a fabrication method to obtain multiple thermal sensors by employing an array of graphite thermocouple patterns on commonly available Xerox paper. The graphite thermocouples are patterned using two different grade graphite pencils, which show a stable and reproducible thermal sensitivity. The fabricated paper devices with multiple thermocouple arrays are capable of producing temperature mapping of the desired area. Different thermal conditions were applied to test and confirm the working of these devices. The present study shows that simple graphite trace patterns can convert a piece of paper into a thermal mapping device.
DOI: 10.17632/cg38djj8y5.2
title: Sensors-on-Paper: Fabrication of Graphite Thermal Sensor Arrays on Cellulose Paper for Large Area Temperature Mapping 

description: This paper reports on a fabrication method to obtain multiple thermal sensors by employing an array of graphite thermocouple patterns on commonly available Xerox paper. The graphite thermocouples are patterned using two different grade graphite pencils, which show a stable and reproducible thermal sensitivity. The fabricated paper devices with multiple thermocouple arrays are capable of producing temperature mapping of the desired area. Different thermal conditions were applied to test and confirm the working of these devices. The present study shows that simple graphite trace patterns can convert a piece of paper into a thermal mapping device.
DOI: 10.6084/m9.figshare.20110430.v1
title: Diversification of Phlyctinus in the Cape region

description: <strong>This item contains:</strong> - Fasta alignment of concatenated dataset. - Seven treefiles from ML analyses on 2 mitochondrial and 4 nuclear genes as well as on the concatenated dataset. - Four xml files used to run BEAST analyses. - Excel table containg the calculation of match ratios. <br> <strong>Abstract of the study related: </strong> The Cape Floristic Region in the Republic of South Africa is a well-recognized hotspot of biodiversity. Although this region is mostly known for its high level of plant diversity and endemicity, it also hosts an understudied and likely diverse arthropod fauna. Here we investigate the evolutionary history and timing of diversification of the apterous weevil genus <em>Phlyctinus</em> (Curculionidae: Entiminae), which is endemic to the coastal area and adjacent mountain ranges of the Cape floristic region and generally associated with sunflower plants (Asteraceae). We use a diverse array of molecular analyses (phylogenetic inference, molecular species delimitation and dating analyses) to analyse a novel molecular dataset of 202 weevil specimens (including 170 <em>Phlyctinus</em> sampled in 60 sites), and sequenced for two mitochondrial and four nuclear gene fragments. Phylogenetic and dating analyses indicate that the genus started diversifying in the late Miocene, with contrasting diversification dynamics for the three inferred clades, which present disjunct distributions. Host plant records and the lack of relatedness of species living in sympatry indicate that the diversification of <em>Phlyctinus</em> was predominantly driven by allopatric (geographic) speciation. We hypothesize that the interplay between topography and recurring cycles of coastline-habitat fragmentation resulting from sea level oscillations spurred the diversification of the most speciose clade, whereas in the two remaining clades populations likely remained connected thus hampering allopatric speciation. Interestingly, this pattern echoes with the role of sea level oscillations as an important driver of the radiation of several lineages in the coastline ecosystems of the Cape Floristic Region.
DOI: 10.25574/20632
title: Chandra X-ray Observatory ObsId 20632

description: The late outburst evolution of Nova Lup 2016: a likely solution of nova 'mysteries'
DOI: 10.6084/m9.figshare.20110430
title: Diversification of Phlyctinus in the Cape region

description: <strong>This item contains:</strong> - Fasta alignment of concatenated dataset. - Seven treefiles from ML analyses on 2 mitochondrial and 4 nuclear genes as well as on the concatenated dataset. - Four xml files used to run BEAST analyses. - Excel table containg the calculation of match ratios. <br> <strong>Abstract of the study related: </strong> The Cape Floristic Region in the Republic of South Africa is a well-recognized hotspot of biodiversity. Although this region is mostly known for its high level of plant diversity and endemicity, it also hosts an understudied and likely diverse arthropod fauna. Here we investigate the evolutionary history and timing of diversification of the apterous weevil genus <em>Phlyctinus</em> (Curculionidae: Entiminae), which is endemic to the coastal area and adjacent mountain ranges of the Cape floristic region and generally associated with sunflower plants (Asteraceae). We use a diverse array of molecular analyses (phylogenetic inference, molecular species delimitation and dating analyses) to analyse a novel molecular dataset of 202 weevil specimens (including 170 <em>Phlyctinus</em> sampled in 60 sites), and sequenced for two mitochondrial and four nuclear gene fragments. Phylogenetic and dating analyses indicate that the genus started diversifying in the late Miocene, with contrasting diversification dynamics for the three inferred clades, which present disjunct distributions. Host plant records and the lack of relatedness of species living in sympatry indicate that the diversification of <em>Phlyctinus</em> was predominantly driven by allopatric (geographic) speciation. We hypothesize that the interplay between topography and recurring cycles of coastline-habitat fragmentation resulting from sea level oscillations spurred the diversification of the most speciose clade, whereas in the two remaining clades populations likely remained connected thus hampering allopatric speciation. Interestingly, this pattern echoes with the role of sea level oscillations as an important driver of the radiation of several lineages in the coastline ecosystems of the Cape Floristic Region.
DOI: 10.25574/20654
title: Chandra X-ray Observatory ObsId 20654

description: AO-19 Calibration Observations of HZ43
DOI: 10.25574/20655
title: Chandra X-ray Observatory ObsId 20655

description: AO-19 Calibration Observations of HZ43
DOI: 10.25574/20659
title: Chandra X-ray Observatory ObsId 20659

description: AO-19 Measurements of the optical/UV Transmission of the HRC Filters.
DOI: 10.25574/20660
title: Chandra X-ray Observatory ObsId 20660

description: AO-19 Measurements of the optical/UV Transmission of the HRC Filters.
DOI: 10.25574/20661
title: Chandra X-ray Observatory ObsId 20661

description: AO-19 Measurements of the optical/UV Transmission of the HRC Filters.
DOI: 10.25574/20662
title: Chandra X-ray Observatory ObsId 20662

description: AO-19 Measurements of the optical/UV Transmission of the HRC Filters.
DOI: 10.25574/20694
title: Chandra X-ray Observatory ObsId 20694

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20695
title: Chandra X-ray Observatory ObsId 20695

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20696
title: Chandra X-ray Observatory ObsId 20696

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20697
title: Chandra X-ray Observatory ObsId 20697

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20698
title: Chandra X-ray Observatory ObsId 20698

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20699
title: Chandra X-ray Observatory ObsId 20699

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20700
title: Chandra X-ray Observatory ObsId 20700

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20701
title: Chandra X-ray Observatory ObsId 20701

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20702
title: Chandra X-ray Observatory ObsId 20702

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20703
title: Chandra X-ray Observatory ObsId 20703

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20704
title: Chandra X-ray Observatory ObsId 20704

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20705
title: Chandra X-ray Observatory ObsId 20705

description: AO-19 Calibration Observations to Monitor the Spatial Variations in the HRC-S Gain
DOI: 10.25574/20706
title: Chandra X-ray Observatory ObsId 20706

description: AO-19 LETG/HRC-S Calibration Observations of HZ43
DOI: 10.25574/20707
title: Chandra X-ray Observatory ObsId 20707

description: AO-19 LETG/HRC-S Calibration Observations of HZ43
DOI: 10.25574/20708
title: Chandra X-ray Observatory ObsId 20708

description: AO-19 LETG/HRC-S Calibration Observations of HZ43
DOI: 10.25574/20712
title: Chandra X-ray Observatory ObsId 20712

description: AO-19 Calibration Observations of Mkn421
DOI: 10.25574/20714
title: Chandra X-ray Observatory ObsId 20714

description: AO-19 Calibration Observations of Mkn421